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100644 Master/texmf-dist/doc/latex/latex-web-companion/xmlstyle/wrong.xml delete mode 100644 Master/texmf-dist/doc/latex/latex-web-companion/xmlstyle/xml.dcl delete mode 100644 Master/texmf-dist/doc/latex/latex-web-companion/xmlstyle/xslexa1.xsl (limited to 'Master/texmf-dist/doc/latex/latex-web-companion') diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apa/README.apa b/Master/texmf-dist/doc/latex/latex-web-companion/apa/README.apa index 0b972b5b1aa..c011a1f118c 100644 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apa/README.apa +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apa/README.apa @@ -1,4 +1,4 @@ -Files in Appendix A of the LaTeX Web Companion +Files in Appendix A of the LaTeX Graphics Companion Section A.1 +++++++++++ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apa/latexexa.ltx b/Master/texmf-dist/doc/latex/latex-web-companion/apa/latexexa.ltx deleted file mode 100644 index 2e334aa4cc5..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apa/latexexa.ltx +++ /dev/null @@ -1,109 +0,0 @@ -\documentclass{article} -\usepackage{graphicx} -\usepackage{url} -\title{Simulation of Energy Loss Straggling} -\author{Maria Physicist} -\newcommand{\Emax}{\ensuremath{E_{\mathrm{max}}}} -\newcommand{\GEANT}{\texttt{GEANT}} -\begin{document} -\maketitle - -\section{Introduction} - -Due to the statistical nature of ionisation energy loss, large -fluctuations can occur in the amount of energy deposited by a particle -traversing an absorber element. Continuous processes such as multiple -scattering and energy loss play a relevant role in the longitudinal -and lateral development of electromagnetic and hadronic -showers, and in the case of sampling calorimeters the -measured resolution can be significantly affected by such fluctuations -in their active layers. The description of ionisation fluctuations is -characterised by the significance parameter $\kappa$, which is -proportional to the ratio of mean energy loss to the maximum allowed -energy transfer in a single collision with an atomic electron -\[ -\kappa =\frac{\xi}{\Emax} -\] -\Emax{} -is the maximum transferable energy in a single collision with -an atomic electron. - -....... - -\section{Vavilov theory} -\label{vavref} - -Vavilov\cite{bib-VAVI} derived a more accurate straggling distribution -by introducing the kinematic limit on the maximum transferable energy -in a single collision, rather than using $ \Emax = \infty $. -Now we can write\cite{bib-SCH1}: -\begin{eqnarray*} -f \left ( \epsilon, \delta s \right ) & = & \frac{1}{\xi} \phi_{v} -\left ( \lambda_{v}, \kappa, \beta^{2} \right ) -\end{eqnarray*} -where -\begin{eqnarray*} -\phi_{v} \left ( \lambda_{v}, \kappa, \beta^{2} \right ) & = & -\frac{1}{2 \pi i} \int^{c+i\infty}_{c-i\infty}\phi \left( s \right ) -e^{\lambda s} ds \hspace{2cm} c \geq 0 \\ -\phi \left ( s \right ) & = & -\exp \left [ \kappa ( 1 + \beta^{2}\gamma ) \right ] -~ \exp \left [ \psi \left ( s \right ) \right ], \\ -\psi \left ( s \right ) & = & s \ln \kappa + ( s + \beta^{2} \kappa ) -\left [ \ln (s/\kappa) + E_{1} (s/\kappa) \right ] - \kappa e^{-s/\kappa}, -\end{eqnarray*} -and -\begin{eqnarray*} -E_{1}(z) & = & \int^{\infty}_{z} t^{-1} e^{-t} dt -\mbox{\hspace{1cm} (the exponential integral)} \\ -\lambda_v & = & \kappa \left [ \frac{\epsilon - \bar{\epsilon}}{\xi} -- \gamma' - \beta^2 \right] -\end{eqnarray*} - -The Vavilov parameters are simply related to the Landau parameter by -$\lambda_L = \lambda_v/\kappa - \ln\kappa $. It can be shown that as -$\kappa \rightarrow 0$, the distribution of the variable $\lambda_L$ -approaches that of Landau. For $\kappa \leq 0.01$ the two -distributions are already practically identical. Contrary to what many -textbooks report, the Vavilov distribution \emph{does not} approximate -the Landau distribution for small $\kappa$, but rather the -distribution of $\lambda_L$ defined above tends to the distribution of -the true $\lambda$ from the Landau density function. Thus the routine -\texttt{GVAVIV} samples the variable $\lambda_L$ rather than -$\lambda_v$. For $\kappa \geq 10$ the Vavilov distribution tends to a -Gaussian distribution (see next section). -.... - -\begin{thebibliography}{10} -\bibitem{bib-LAND} -L.Landau. -\newblock On the Energy Loss of Fast Particles by Ionisation. -\newblock Originally published in \emph{J. Phys.}, 8:201, 1944. -\newblock Reprinted in D.ter Haar, Editor, \emph{L.D.Landau, Collected - papers}, page 417. Pergamon Press, Oxford, 1965. - -\bibitem{bib-SCH1} -B.Schorr. -\newblock Programs for the Landau and the Vavilov distributions and the - corresponding random numbers. -\newblock \emph{Comp. Phys. Comm.}, 7:216, 1974. - -\bibitem{bib-SELT} -S.M.Seltzer and M.J.Berger. -\newblock Energy loss straggling of protons and mesons. -\newblock In \emph{Studies in Penetration of Charged Particles in - Matter}, Nuclear Science Series~39, Nat. Academy of Sciences, - Washington DC, 1964. - -\bibitem{bib-TALM} -R.Talman. -\newblock On the statistics of particle identification using ionization. -\newblock \emph{Nucl. Inst. Meth.}, 159:189, 1979. - -\bibitem{bib-VAVI} -P.V.Vavilov. -\newblock Ionisation losses of high energy heavy particles. -\newblock \emph{Soviet Physics JETP}, 5:749, 1957. -\end{thebibliography} - -\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apb/README.apb b/Master/texmf-dist/doc/latex/latex-web-companion/apb/README.apb index 0a6bb120150..fdd467caf1a 100644 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apb/README.apb +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apb/README.apb @@ -1,4 +1,4 @@ -Files in Appendix B of the LaTeX Web Companion +Files in Appendix B of the LaTeX Graphics Companion Section B.4 +++++++++++ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apb/invitation.sty b/Master/texmf-dist/doc/latex/latex-web-companion/apb/invitation.sty index e401c6b3ed5..68dedd1c10b 100644 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apb/invitation.sty +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apb/invitation.sty @@ -47,3 +47,4 @@ \ProcessOptions \endinput + diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apb/makelatex.sh b/Master/texmf-dist/doc/latex/latex-web-companion/apb/makelatex.sh new file mode 100755 index 00000000000..5ab25f55e50 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apb/makelatex.sh @@ -0,0 +1,14 @@ +#!/bin/sh +# makelatex.sh Generate latex from xml and xsl +# Author: M.Goossens / IT +# Last mod: Jan 24 1999 + +DIR=/afs/cern.ch/project/tex/java +#old CLASSPATH=$DIR/xt.jar:$DIR/xp.jar:$DIR/sax.jar:$CLASSPATH +CLASSPATH=$DIR/xtnew/xt.jar:$DIR/xp.jar:$DIR/xtnew/sax.jar:$CLASSPATH +export CLASSPATH +java com.jclark.xsl.sax.Driver minilatexexa.xml minilatex.xsl \ + | sed -e 's/>/>/g'\ + -e 's/</ a.tex +utf82latin1.sh a.tex minilatexexa.tex diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apb/minilatex.dtd b/Master/texmf-dist/doc/latex/latex-web-companion/apb/minilatex.dtd index 3bb7530819a..271a51e2bdb 100644 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apb/minilatex.dtd +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apb/minilatex.dtd @@ -30,7 +30,7 @@ - + @@ -55,7 +55,6 @@ - @@ -86,9 +85,9 @@ - + - + - - - - - + diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apb/minilatexexa.tex b/Master/texmf-dist/doc/latex/latex-web-companion/apb/minilatexexa.tex index 720477f73db..f92effe7a5b 100644 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apb/minilatexexa.tex +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apb/minilatexexa.tex @@ -64,7 +64,7 @@ in den Text aufgenommen. \begin{figure}\centering -\includegraphics[width=3cm, scale=.5]{colorcir} +\includegraphics[width=3cm, scale=.5]{colorcir.eps} \caption{Ein EPS Bild\label{fig-psfig}} \end{figure} \subsection{Beispiel einer Tabelle} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apb/minilatexexa.xml b/Master/texmf-dist/doc/latex/latex-web-companion/apb/minilatexexa.xml index 5b6f67fd551..787c60e3d1e 100644 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apb/minilatexexa.xml +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apb/minilatexexa.xml @@ -71,7 +71,7 @@ Abbildung  wurde mit dem Befehl in den Text aufgenommen.
- + Ein EPS Bild
diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apc/README.apc b/Master/texmf-dist/doc/latex/latex-web-companion/apc/README.apc index da64d7a3624..0e42d1eaaa0 100644 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apc/README.apc +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apc/README.apc @@ -1,4 +1,4 @@ -Files in Appendix C of the LaTeX Web Companion +Files in Appendix C of the LaTeX Graphics Companion Section C.3.1 +++++++++++++ @@ -8,9 +8,12 @@ invitationfr.dtd Corresponding DTD invlat1fr.xsl XSL file to transform the above to LaTeX -invitationfr.tex Resulting LaTeX file (Latin 1) +invitationfrraw.tex Raw (UTF-8) resulting LaTeX file after running with xt +invitationfr.tex Filtered resulting LaTeX file (Latin 1) invitation.sty Augmented package file to run the above with LaTeX +utf8tolatin1.java A java program to translate a UTF-8 file into Latin 1 + (used to invitationfrraw.tex -> invitationfr.tex) Section C.3.2 +++++++++++++ @@ -18,7 +21,13 @@ For the following a Unicode editor is, such as Yudit on Linux, is useful to visualize the files. utf8.xml XML example with UTF8 characters -utf8.xsl Accompanying XSL file to generate HTML output -ISOcyr1.pen Entity definitions for Cyrillic in utf8.xml +utf8.xsl accompanying XSL file to generate HTML output +ISOcyr1.pen entity definitions for Cyrillic in utf8.xml + +utf8raw.html resulting HTML file (after xt) +utf8.html HTML file after processing utf8raw.html with tidy + "tidy -utf8 utf8raw.html utf8.html" + + + -utf8.html Resulting HTML file (after xt) diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apc/invitation.sty b/Master/texmf-dist/doc/latex/latex-web-companion/apc/invitation.sty index f66dd78463d..a27c8a05fc2 100644 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apc/invitation.sty +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apc/invitation.sty @@ -43,4 +43,4 @@ \newcommand{\Where}[1]{\gdef\@Where{#1}} \newcommand{\Why}[1]{\gdef\@Why{#1}} \newcommand{\Signature}[1]{\gdef\@Sig{#1}} -\ProcessOptions \ No newline at end of file +\ProcessOptions diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apc/invitationfr.sty b/Master/texmf-dist/doc/latex/latex-web-companion/apc/invitationfr.sty deleted file mode 100644 index f66dd78463d..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apc/invitationfr.sty +++ /dev/null @@ -1,46 +0,0 @@ -% invitation.sty -% Package to format invitation.xml -\setlength{\textwidth}{22pc} -\setlength{\parskip}{1ex} -\setlength{\parindent}{0pt} -\pagestyle{empty}%% Turn off page numbering -\RequirePackage{array,calc} -\newcommand{\ToTitle}{To whom} -\newcommand{\WhyTitle}{Occasion} -\newcommand{\WhereTitle}{Venue} -\newcommand{\DateTitle}{When} -\newcommand{\SignatureTitle}{From} -\DeclareOption{francais}{% French text for fixed texts - \renewcommand{\ToTitle}{À} - \renewcommand{\WhyTitle}{À l'occasion de} - \renewcommand{\WhereTitle}{Où} - \renewcommand{\DateTitle}{Quand} - \renewcommand{\SignatureTitle}{De la part de}} -\newenvironment{Front}% - {\begin{center} - \Huge\sffamily INVITATION - \end{center} - } - {\begin{flushleft} - \rule{\linewidth}{1pt}\\[2mm] - \begin{tabular}{@{}>{\bfseries}ll@{}} - \ToTitle: & \@To \\ - \WhyTitle: & \@Why \\ - \WhereTitle: & \@Where \\ - \DateTitle: & \@Date - \end{tabular}\\[2mm] - \rule{\linewidth}{1pt} - \end{flushleft} - } -\newenvironment{Body}{\vspace*{\parskip}}{\vspace*{\parskip}} -\newenvironment{Back} - {\begin{flushleft}} - {\hspace*{.5\linewidth}\fbox{\SignatureTitle: \emph{\@Sig}} - \end{flushleft} - } -\newcommand{\To}[1]{\gdef\@To{#1}} -\newcommand{\Date}[1]{\gdef\@Date{#1}} -\newcommand{\Where}[1]{\gdef\@Where{#1}} -\newcommand{\Why}[1]{\gdef\@Why{#1}} -\newcommand{\Signature}[1]{\gdef\@Sig{#1}} -\ProcessOptions \ No newline at end of file diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apc/invitationfrraw.tex b/Master/texmf-dist/doc/latex/latex-web-companion/apc/invitationfrraw.tex new file mode 100644 index 00000000000..36a8f1a300a --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apc/invitationfrraw.tex @@ -0,0 +1,25 @@ +\documentclass[francais]{article} +\usepackage{invitation} +\usepackage[T1]{fontenc} +\begin{document} +\begin{Front} +\To{Anna, Bernard, Didier, Johanna} +\Date{Vendredi prochain à 20 heures} +\Where{Le Café du Web} +\Why{Mon premier bébé XML} +\end{Front} +\begin{Body} +\par +J'ai le plaisir de vous inviter à la célébration +de la naissance d'\emph{Invitation}, mon +premier enfant document XML. +\par +S'il vous plaît, faites tout votre possible pour me rejoindre +vendredi prochain. Et n'oubliez pas d'emmener vos amis. +\par +Je me réjouis \emph{vraiment} d'avance de votre présence. +\end{Body} +\begin{Back} +\Signature{Michel} +\end{Back} +\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apc/invlat1fr.xsl b/Master/texmf-dist/doc/latex/latex-web-companion/apc/invlat1fr.xsl index 9f5165fc4ed..fce6e7f64cf 100644 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apc/invlat1fr.xsl +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apc/invlat1fr.xsl @@ -1,15 +1,13 @@ - - - - - - + \documentclass[francais]{article} -\usepackage{invitationfr} +\usepackage{invitation} \usepackage[T1]{fontenc} \begin{document} @@ -18,7 +16,7 @@ - + \begin{Front} \To{ @@ -36,7 +34,7 @@ - + \begin{Body} @@ -44,18 +42,18 @@ - + \par - + \emph{ } - + \begin{Back} \Signature{ @@ -65,3 +63,4 @@ + diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8.html b/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8.html index 8709c70b120..51858d102a8 100644 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8.html +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8.html @@ -1,36 +1,39 @@ - -UTF8 file +UTF8 files

Handling UTF-8 files

-

The word Russian (РуÑÑкий) in Cyrillic:
-Using ISO Cyrillic set: -РуÑÑкий
-Using XML Unicode entities: -РуÑÑкий -

+ +

The word Russian (РуÑÑкий) in Cyrillic: +
+Using ISO Cyrillic set: РуÑÑкий +
+ Using XML Unicode entities: РуÑÑкий

+

Russian-English correspondence

-

â—†  Ъ ÑŠ Э Ñ Ð• е Р Ñ€ Т Ñ‚ Й й У у И и О о П п

+

◆  Ъ ÑŠ Э Ñ Ð• е Р Ñ€ Т Ñ‚ Й й У у И и О о П п

+ +

◆  Ра С Ñ Ð” д Ф Ñ„ Г г Ð¥ Ñ… J j К к Л л

-

â—†  Ра С Ñ Ð” д Ф Ñ„ Г г Ð¥ Ñ… J j К к Л л

+

◆  З з Ы ы Ь ь В в Б б Рн М м

-

â—†  З з Ы Ñ‹ Ь ÑŒ Ð’ в Б б Рн Ðœ м

+

◆  Я РЮ Э Ñ Ñ‘ ÑŽ Ñ Ñ‡ Ч ш Ш ц Ц щ Щ

-

â—†  Я РЮ Э Ñ Ñ‘ ÑŽ Ñ Ñ‡ Ч ш Ш ц Ц щ Щ

Greek-English correspondence

-

â— Q q Ω ω Ε ε Ρ Ï Î¤ Ï„ Î¥ Ï… Ι ι Ο ο Π Ï€

+

â— Q q Ω ω Ε ε Ρ Ï Î¤ Ï„ Î¥ Ï… Ι ι Ο ο Π Ï€

-

◠Α α Σ σ Δ δ Φ φ Γ γ Η η J j Κ κ Λ λ

+

â— Α α Σ σ Δ δ Φ φ Γ γ Η η J j Κ κ Λ λ

+ +

â— Ζ ζ Ξ ξ Χ χ V v Î’ β Πν Îœ μ

-

◠Ζ ζ Ξ ξ Χ χ V v Β β Πν Μ μ

Math characters

-

And here is one of Maxwell's equations: -∇·B=0

+ +

And here is one of Maxwell's equations: ∇·B=0

+ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8.xml b/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8.xml index 6863b87c29f..fd2cf40c58d 100644 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8.xml +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8.xml @@ -1,4 +1,4 @@ - + diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8.xsl b/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8.xsl index de6b5bfaf4c..4ca722afb02 100644 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8.xsl +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8.xsl @@ -1,11 +1,13 @@ - - - + + - + - UTF8 file + UTF8 files +

Handling UTF-8 files

@@ -34,3 +36,4 @@

â— 

+ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8raw.html b/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8raw.html new file mode 100644 index 00000000000..7fe4b5ea656 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8raw.html @@ -0,0 +1,35 @@ + + + +UTF8 files + + + +

Handling UTF-8 files

+

The word Russian (Русский) in Cyrillic:
+Using ISO Cyrillic set: +Русский
+Using XML Unicode entities: +Русский +

+

Russian-English correspondence

+ +

◆  Ъ ъ Э э Е е Р р Т т Й й У у И и О о П п

+ +

◆  А а С с Д д Ф ф Г г Х х J j К к Л л

+ +

◆  З з Ы ы Ь ь В в Б б Н н М м

+ +

◆  Я Ё Ю Э я ё ю э ч Ч ш Ш ц Ц щ Щ

+

Greek-English correspondence

+ +

● Q q Ω ω Ε ε Ρ ρ Τ τ Υ υ Ι ι Ο ο Π π

+ +

● Α α Σ σ Δ δ Φ φ Γ γ Η η J j Κ κ Λ λ

+ +

● Ζ ζ Ξ ξ Χ χ V v Β β Ν ν Μ μ

+

Math characters

+

And here is one of Maxwell's equations: +∇·B=0

+ + diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8tei.xml b/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8tei.xml deleted file mode 100644 index 6f24ea62bac..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/apc/utf8tei.xml +++ /dev/null @@ -1,48 +0,0 @@ - - -%ISOcyr1; -]> - - - - - TEI-lite, XSL and UTF8 - - - - - -Playing with Cyrillic -

The word Russian in Cyrillic is written: РуÑÑкий.

-

Using ISO Cyrillic set: -Русский .

-

Using XML Unicode entities: -Русский .

-
-Russian-English correspondence -

Q q W w E e R r T t Y y U u I i O o P p

-

Ъ ÑŠ Э Ñ Ð• е Р Ñ€ Т Ñ‚ Й й У у И и О о П п

-

A a S s D d F f G g H h J j K k L l

-

Ра С Ñ Ð” д Ф Ñ„ Г г Ð¥ Ñ… J j К к Л л

-

Z z X x C c V v B b N n M m

-

З з Ы ы Ь ь В в Б б Рн М м

-

YA YO YU EE ya yo yu ee ch CH sh SH ts TS shch SHCH

-

Я РЮ Э Ñ Ñ‘ ÑŽ Ñ Ñ‡ Ч ш Ш ц Ц щ Щ

-
-Greek-English correspondence -

Q q W w E e R r T t Y y I i O o P p

-

Q q Ω ω Ε ε Ρ Ï Î¤ Ï„ Î¥ Ï… Ι ι Ο ο Π Ï€

-

A a S s D d F f G g H h J j K k L l

-

Α α Σ σ Δ δ Φ φ Γ γ Η η J j Κ κ Λ λ

-

Z z X x C c V v B b N n M m

-

Ζ ζ Ξ ξ Χ χ V v Β β Πν Μ μ

-
-Math characters -

And here is one of Maxwell's equations: -∇·B=0

-
- -
-
diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch2/latexexa.aux b/Master/texmf-dist/doc/latex/latex-web-companion/ch2/latexexa.aux new file mode 100644 index 00000000000..7df7d7030da --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch2/latexexa.aux @@ -0,0 +1,55 @@ +\relax +\ifx\hyper@anchor\@undefined +\global \let \oldcontentsline\contentsline +\gdef \contentsline#1#2#3#4{\oldcontentsline{#1}{#2}{#3}} +\global \let \oldnewlabel\newlabel +\gdef \newlabel#1#2{\newlabelxx{#1}#2} +\gdef \newlabelxx#1#2#3#4#5#6{\oldnewlabel{#1}{{#2}{#3}}} +\AtEndDocument{\let \contentsline\oldcontentsline +\let \newlabel\oldnewlabel} +\else +\global \let \hyper@last\relax +\fi + +\@writefile{toc}{\contentsline {section}{\numberline {1}Introduction}{1}{section.1}} +\citation{bib-LAND} +\@writefile{toc}{\contentsline {section}{\numberline {2}Landau theory}{2}{section.2}} +\newlabel{sec:phys332-1}{{2}{2}{Landau theory\relax }{section.2}{}} +\@writefile{brf}{\backcite{bib-LAND}{{2}{2}{section.2}}} +\citation{bib-TALM} +\@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces The variable $\xi /I_0$ can be used to measure the validity range of the Landau theory. It depends on the type and energy of the particle, $Z$, $A$ and the ionisation potential of the material and the layer thickness. }}{3}{figure.1}} +\newlabel{fg:phys332-1}{{1}{3}{Introduction\relax }{figure.1}{}} +\@writefile{toc}{\contentsline {subsection}{\numberline {2.1}Restrictions}{3}{subsection.2.1}} +\@writefile{brf}{\backcite{bib-TALM}{{3}{2}{Item.4}}} +\citation{bib-VAVI} +\citation{bib-SCH1} +\citation{bib-SELT} +\@writefile{toc}{\contentsline {section}{\numberline {3}Vavilov theory}{5}{section.3}} +\newlabel{vavref}{{3}{5}{Vavilov theory\relax }{section.3}{}} +\@writefile{brf}{\backcite{bib-VAVI}{{5}{3}{section.3}}} +\@writefile{brf}{\backcite{bib-SCH1}{{5}{3}{section.3}}} +\@writefile{toc}{\contentsline {section}{\numberline {4}Gaussian Theory}{5}{section.4}} +\@writefile{brf}{\backcite{bib-SELT}{{5}{4}{section.4}}} +\@writefile{lof}{\contentsline {figure}{\numberline {2}{\ignorespaces Energy loss distribution for a 3 GeV electron in Argon as given by standard \texttt {GEANT}. The width of the layers is given in centimeters.}}{6}{figure.2}} +\newlabel{fg:phys332-2}{{2}{6}{Urb\'an model\relax }{figure.2}{}} +\@writefile{toc}{\contentsline {section}{\numberline {5}Urb\'an model}{6}{section.5}} +\newlabel{urban}{{5}{6}{Urb\'an model\relax }{section.5}{}} +\newlabel{eq:sigex}{{2}{6}{Urb\'an model\relax }{equation.2}{}} +\newlabel{eq:sigion}{{3}{6}{Urb\'an model\relax }{equation.3}{}} +\newlabel{eq:fisum}{{4}{7}{Urb\'an model\relax }{equation.4}{}} +\newlabel{eq:flnsum}{{5}{7}{Urb\'an model\relax }{equation.4}{}} +\@writefile{toc}{\contentsline {subsection}{\numberline {5.1}Fast simulation for $n_3 \geq 16$}{8}{subsection.5.1}} +\newlabel{eq:phys332-5}{{13}{8}{Fast simulation for $n_3 \geq 16$\relax }{equation.13}{}} +\newlabel{eq:phys332-1}{{16}{8}{Fast simulation for $n_3 \geq 16$\relax }{equation.16}{}} +\newlabel{eq:phys332-2}{{17}{8}{Fast simulation for $n_3 \geq 16$\relax }{equation.16}{}} +\newlabel{eq:phys332-3}{{18}{8}{Fast simulation for $n_3 \geq 16$\relax }{equation.18}{}} +\newlabel{eq:phys332-4}{{19}{8}{Fast simulation for $n_3 \geq 16$\relax }{equation.18}{}} +\newlabel{eq:phys332-6}{{22}{9}{Fast simulation for $n_3 \geq 16$\relax }{equation.22}{}} +\newlabel{eq:phys332-7}{{23}{9}{Fast simulation for $n_3 \geq 16$\relax }{equation.22}{}} +\newlabel{eq:phys332-8}{{24}{9}{Fast simulation for $n_3 \geq 16$\relax }{equation.22}{}} +\bibcite{bib-LAND}{1} +\bibcite{bib-SCH1}{2} +\bibcite{bib-SELT}{3} +\bibcite{bib-TALM}{4} +\bibcite{bib-VAVI}{5} +\@writefile{toc}{\contentsline {subsection}{\numberline {5.2}Special sampling for lower part of the spectrum}{10}{subsection.5.2}} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch2/latexexa.brf b/Master/texmf-dist/doc/latex/latex-web-companion/ch2/latexexa.brf new file mode 100644 index 00000000000..dc4d5c318ee --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch2/latexexa.brf @@ -0,0 +1,5 @@ +\backcite {bib-LAND}{{2}{2}{section.2}} +\backcite 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[1]{section.1}{Introduction}{} +\BOOKMARK [1]{section.2}{Landau theory}{} +\BOOKMARK [2]{subsection.2.1}{Restrictions}{section.2} +\BOOKMARK [1]{section.3}{Vavilov theory}{} +\BOOKMARK [1]{section.4}{Gaussian Theory}{} +\BOOKMARK [1]{section.5}{Urb\341n model}{} +\BOOKMARK [2]{subsection.5.1}{Fast simulation for n3 16}{section.5} +\BOOKMARK [2]{subsection.5.2}{Special sampling for lower part of the spectrum}{section.5} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch2/latexexa.pdf b/Master/texmf-dist/doc/latex/latex-web-companion/ch2/latexexa.pdf new file mode 100644 index 00000000000..19c6a108f19 Binary files /dev/null and b/Master/texmf-dist/doc/latex/latex-web-companion/ch2/latexexa.pdf differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch2/latexexa.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch2/latexexa.tex new file mode 100644 index 00000000000..21cf0c8b4cd --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch2/latexexa.tex @@ -0,0 +1,569 @@ +\documentclass{article} +\usepackage{graphicx} +\usepackage{url} +\title{Simulation of Energy Loss Straggling} +\author{Maria Physicist} +\usepackage{ae} +\usepackage[T1]{fontenc} +\usepackage[latin1]{inputenc} +\usepackage{fancyhdr,pifont} +\pagestyle{fancy} +\cfoot{\NavigationBar} +\def\NavigationBar{{\Large + \Acrobatmenu{FontsInfo}{\reflectbox{\ding{227}}} + \Acrobatmenu{NextPage}{\ding{227}} + \Acrobatmenu{FirstPage}{\reflectbox{\ding{224}}} + \Acrobatmenu{LastPage}{\ding{224}} + \Acrobatmenu{GoBack}{\reflectbox{\ding{249}}} + \Acrobatmenu{Quit}{\ding{54}}% +}} +\usepackage[colorlinks, backref, + pdfpagemode=FullScreen, + pdfauthor={Maria Physicist}, + pdftitle={Simulation of Energy Loss Straggling}, + pdfcreator={pdfTeX}, + pdfsubject={Energy Loss}, + pdfkeywords={physics,energy}, + pdfpagetransition={Blinds /Dm /V} +]{hyperref} +\newcommand{\Emax}{\ensuremath{E_{\mathrm{max}}}} +\newcommand{\GEANT}{\texttt{GEANT}} +\begin{document} +\maketitle + +\section{Introduction} + +Due to the statistical nature of ionisation energy loss, large +fluctuations can occur in the amount of energy deposited by a particle +traversing an absorber element. Continuous processes such as multiple +scattering and energy loss play a relevant role in the longitudinal +and lateral development of electromagnetic and hadronic +showers, and in the case of sampling calorimeters the +measured resolution can be significantly affected by such fluctuations +in their active layers. The description of ionisation fluctuations is +characterised by the significance parameter $\kappa$, which is +proportional to the ratio of mean energy loss to the maximum allowed +energy transfer in a single collision with an atomic electron +\[ +\kappa =\frac{\xi}{\Emax} +\] +\Emax{} +is the maximum transferable energy in a single collision with +an atomic electron. +\[ +\Emax =\frac{2 m_e \beta^2\gamma^2 } +{1 + 2\gamma m_e/m_x + \left ( m_e/m_x\right)^2}, +\] +where $\gamma = E/m_x$, $E$ is energy and +$m_x$ the mass of the incident particle, +$\beta^2 = 1 - 1/\gamma^2$ and $m_e$ is the electron mass. +$\xi$ comes from the Rutherford scattering cross section +and is defined as: +\begin{eqnarray*} \xi = \frac{2\pi z^2 e^4 N_{Av} Z \rho \delta x} + {m_e \beta^2 c^2 A} = 153.4 \frac{z^2} {\beta^2} \frac{Z}{A} + \rho \delta x \quad\mathrm{keV}, +\end{eqnarray*} +where + +\begin{tabular}{ll} +$z$ & charge of the incident particle \\ +$N_{Av}$ & Avogadro's number \\ +$Z$ & atomic number of the material \\ +$A$ & atomic weight of the material \\ +$\rho$ & density \\ +$ \delta x$ & thickness of the material \\ +\end{tabular} + +$\kappa$ measures the contribution of the collisions with energy +transfer close to \Emax. For a given absorber, $\kappa$ tends +towards large values if $\delta x$ is large and/or if $\beta$ is +small. Likewise, $\kappa$ tends towards zero if $\delta x $ is small +and/or if $\beta$ approaches 1. + +The value of $\kappa$ distinguishes two regimes which occur in the +description of ionisation fluctuations : + +\begin{enumerate} +\item A large number of collisions involving the loss of all or most + of the incident particle energy during the traversal of an absorber. + + As the total energy transfer is composed of a multitude of small + energy losses, we can apply the central limit theorem and describe + the fluctuations by a Gaussian distribution. This case is + applicable to non-relativistic particles and is described by the + inequality $\kappa > 10 $ (i.e. when the mean energy loss in the + absorber is greater than the maximum energy transfer in a single + collision). + +\item Particles traversing thin counters and incident electrons under + any conditions. + + The relevant inequalities and distributions are $ 0.01 < \kappa < 10 + $, Vavilov distribution, and $\kappa < 0.01 $, Landau distribution. +\end{enumerate} + +An additional regime is defined by the contribution of the collisions +with low energy transfer which can be estimated with the relation +$\xi/I_0$, where $I_0$ is the mean ionisation potential of the atom. +Landau theory assumes that the number of these collisions is high, and +consequently, it has a restriction $\xi/I_0 \gg 1$. In \GEANT{} +(see URL \url{http://wwwinfo.cern.ch/asdoc/geant/geantall.html}), the +limit of Landau theory has been set at $\xi/I_0 = 50$. Below this +limit special models taking into account the atomic structure of the +material are used. This is important in thin layers and gaseous +materials. Figure \ref{fg:phys332-1} shows the behaviour of $\xi/I_0$ +as a function of the layer thickness for an electron of 100 keV and 1 +GeV of kinetic energy in Argon, Silicon and Uranium. + +\begin{figure} + \centering + \includegraphics[width=.6\linewidth]{phys332-1} + \caption{The variable $\xi/I_0$ can be used to measure the + validity range of the Landau theory. It depends + on the type and energy of the particle, $Z$, $A$ + and the ionisation potential of the material and + the layer thickness. + } + \label{fg:phys332-1} +\end{figure} + +In the following sections, the different theories and models for the +energy loss fluctuation are described. First, the Landau theory and +its limitations are discussed, and then, the Vavilov and Gaussian +straggling functions and the methods in the thin layers and gaseous +materials are presented. + +\section{Landau theory} +\label{sec:phys332-1} + +For a particle of mass $m_x$ traversing a thickness of material +$\delta x $, the Landau probability distribution may be written in +terms of the universal Landau function $\phi(\lambda)$ +as\cite{bib-LAND}: +\begin{eqnarray*} +f( \epsilon , \delta x ) & = &\frac{1}{\xi} \phi ( \lambda ) +\end{eqnarray*} +where +\begin{eqnarray*} +\phi(\lambda )& = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty} +\exp \left ( u \ln u + \lambda u \right ) du \hspace{2cm} c \geq 0 \\ +\lambda & = & \frac{\epsilon -\bar{\epsilon} }{\xi} + - \gamma' - \beta^2 - \ln \frac{\xi}{\Emax} \\ +\gamma' & = & 0.422784\dots = 1 - \gamma \\ +\gamma & = & 0.577215\dots \mbox{(Euler's constant)} \\ +\bar{\epsilon} & = & \mbox{average energy loss} \\ +\epsilon & = & \mbox{actual energy loss} +\end{eqnarray*} + +\subsection{Restrictions} + +The Landau formalism makes two restrictive assumptions : +\begin{enumerate} +\item The typical energy loss is small compared to the maximum energy + loss in a single collision. This restriction is removed in the + Vavilov theory (see section \ref{vavref}). +\item The typical energy loss in the absorber should be large compared + to the binding energy of the most tightly bound electron. For + gaseous detectors, typical energy losses are a few keV which is + comparable to the binding energies of the inner electrons. In such + cases a more sophisticated approach which accounts for atomic energy + levels\cite{bib-TALM} is necessary to accurately simulate data + distributions. In \GEANT, a parameterised model by L. Urb\'{a}n is + used (see section \ref{urban}). +\end{enumerate} + +In addition, the average value of the Landau distribution is infinite. +Summing the Landau fluctuation obtained to the average energy from the +$dE/dx$ tables, we obtain a value which is larger than the one coming +from the table. The probability to sample a large value is small, so +it takes a large number of steps (extractions) for the average +fluctuation to be significantly larger than zero. This introduces a +dependence of the energy loss on the step size which can affect +calculations. + +A solution to this has been to introduce a limit on the value of the +variable sampled by the Landau distribution in order to keep the +average fluctuation to 0. The value obtained from the \texttt{GLANDO} +routine is: +\[ +\delta dE/dx = \epsilon - \bar{\epsilon} = \xi ( \lambda - \gamma' ++\beta^2 +\ln \frac{\xi}{\Emax}) +\] +In order for this to have average 0, we must impose that: +\[ +\bar{\lambda} = -\gamma' - \beta^2 -\ln \frac{\xi}{\Emax} +\] + +This is realised introducing a $\lambda_{\mathrm{max}}(\bar{\lambda})$ +such that if only values of $\lambda \leq \lambda_{\mathrm{max}}$ are +accepted, the average value of the distribution is $\bar{\lambda}$. + +A parametric fit to the universal Landau distribution has been +performed, with following result: +\[ +\lambda_{\mathrm{max}} = 0.60715 + + 1.1934\bar{\lambda}+(0.67794+0.052382\bar{\lambda}) + \exp(0.94753+0.74442\bar{\lambda}) +\] +only values smaller than $\lambda_{\mathrm{max}}$ are accepted, otherwise the +distribution is resampled. + + + +\newpage +\section{Vavilov theory} +\label{vavref} + +Vavilov\cite{bib-VAVI} derived a more accurate straggling distribution +by introducing the kinematic limit on the maximum transferable energy +in a single collision, rather than using $ \Emax = \infty $. +Now we can write\cite{bib-SCH1}: +\begin{eqnarray*} +f \left ( \epsilon, \delta s \right ) & = & \frac{1}{\xi} \phi_{v} +\left ( \lambda_{v}, \kappa, \beta^{2} \right ) +\end{eqnarray*} +where +\begin{eqnarray*} +\phi_{v} \left ( \lambda_{v}, \kappa, \beta^{2} \right ) & = & +\frac{1}{2 \pi i} \int^{c+i\infty}_{c-i\infty}\phi \left( s \right ) +e^{\lambda s} ds \hspace{2cm} c \geq 0 \\ +\phi \left ( s \right ) & = & +\exp \left [ \kappa ( 1 + \beta^{2}\gamma ) \right ] +~ \exp \left [ \psi \left ( s \right ) \right ], \\ +\psi \left ( s \right ) & = & s \ln \kappa + ( s + \beta^{2} \kappa ) +\left [ \ln (s/\kappa) + E_{1} (s/\kappa) \right ] - \kappa e^{-s/\kappa}, +\end{eqnarray*} +and +\begin{eqnarray*} +E_{1}(z) & = & \int^{\infty}_{z} t^{-1} e^{-t} dt +\mbox{\hspace{1cm} (the exponential integral)} \\ +\lambda_v & = & \kappa \left [ \frac{\epsilon - \bar{\epsilon}}{\xi} +- \gamma' - \beta^2 \right] +\end{eqnarray*} + +The Vavilov parameters are simply related to the Landau parameter by +$\lambda_L = \lambda_v/\kappa - \ln\kappa $. It can be shown that as +$\kappa \rightarrow 0$, the distribution of the variable $\lambda_L$ +approaches that of Landau. For $\kappa \leq 0.01$ the two +distributions are already practically identical. Contrary to what many +textbooks report, the Vavilov distribution \emph{does not} approximate +the Landau distribution for small $\kappa$, but rather the +distribution of $\lambda_L$ defined above tends to the distribution of +the true $\lambda$ from the Landau density function. Thus the routine +\texttt{GVAVIV} samples the variable $\lambda_L$ rather than +$\lambda_v$. For $\kappa \geq 10$ the Vavilov distribution tends to a +Gaussian distribution (see next section). + +\section{Gaussian Theory} + +Various conflicting forms have been proposed for Gaussian straggling +functions, but most of these appear to have little theoretical or +experimental basis. However, it has been shown\cite{bib-SELT} that +for $\kappa \geq 10 $ the Vavilov distribution can be replaced by a +Gaussian of the form : +\begin{eqnarray*} +f( \epsilon , \delta s) \approx \frac{1} +{\xi \sqrt{\frac{2 \pi}{\kappa} \left( 1 - \beta^2/2 \right)}} + \exp \left [ \frac{( \epsilon - \bar{\epsilon} )^2}{2} \frac{\kappa} + {\xi^2 (1- \beta^2/2)}\right ] +\end{eqnarray*} +thus implying +\begin{eqnarray*} +\mathrm{mean} & = & \bar{\epsilon} \\ +\sigma^2 & = & \frac{\xi^2}{\kappa} (1-\beta^2/2) = \xi + \Emax (1-\beta^2/2) +\end{eqnarray*} + +\section{Urb\'an model} +\label{urban} + +The method for computing restricted energy losses with $\delta$-ray +production above given threshold energy in \GEANT{} is a Monte +Carlo method that can be used for thin layers. It is fast and it can +be used for any thickness of a medium. Approaching the limit of the +validity of Landau's theory, the loss distribution approaches smoothly +the Landau form as shown in Figure \ref{fg:phys332-2}. +\begin{figure} + \centering + \includegraphics[width=.6\linewidth]{phys332-2} + \caption{Energy loss distribution for a 3 GeV electron in + Argon as given by standard \GEANT. The width of the layers is + given in centimeters.} + \label{fg:phys332-2} +\end{figure} + +It is assumed that the atoms have only two energy levels with binding +energy $E_1$ and $E_2$. The particle--atom interaction will then be +an excitation with energy loss $E_1$ or $E_2$, or an ionisation with +an energy loss distributed according to a function $g(E) \sim 1/E^2$: +\begin{equation} +g(E) = \frac{(\Emax + I)I}{\Emax} \frac{1}{E^2} +\end{equation} + +The macroscopic cross-section for excitations ($i=1,2$) is +\begin{equation} +\label{eq:sigex} +\Sigma_i = C \frac{f_i}{E_i} \frac{\ln (2 m \beta^2 \gamma^2/E_i) - \beta^2} + {\ln (2 m \beta^2 \gamma^2/ I) - \beta^2}(1-r) +\end{equation} +and the macroscopic cross-section for ionisation is +\begin{equation} +\label{eq:sigion} +\Sigma_3 = C \frac{\Emax}{I(\Emax+I) \ln(\frac{\Emax+I}{I})} + ~ r +\end{equation} +\Emax{} is the \GEANT{} cut for $\delta$-production, or the maximum +energy transfer minus mean ionisation energy, if it is smaller than +this cut-off value. The following notation is used: + +\begin{tabular}{ll} +$r, C$ & parameters of the model \\ +$E_i$ & atomic energy levels \\ +$I$ & mean ionisation energy \\ +${f_i}$ & oscillator strengths +\end{tabular} + +The model has the parameters $f_i$, $E_i$, $C$ and $r ~(0\leq r\leq +1)$. The oscillator strengths $f_i$ and the atomic level energies +$E_i$ should satisfy the constraints +\begin{eqnarray} +f_1 + f_2 & = & 1 \label{eq:fisum}\\ +f_1 \ln E_1 + f_2 \ln E_2 & = & \ln I \label{eq:flnsum} +\end{eqnarray} +The parameter $C$ can be defined with the help of the mean energy loss +$dE/dx$ in the following way: The numbers of collisions ($n_i$, i = +1,2 for the excitation and 3 for the ionisation) follow the Poisson +distribution with a mean number $ \langle n_i \rangle $. In a step +$\Delta x$ the mean number of collisions is +\begin{equation} +\langle n_i \rangle = \Sigma_i \Delta x +\end{equation} +The mean energy loss $dE/dx$ in a step is the sum of the excitation +and ionisation contributions +\begin{equation} +\frac{dE}{dx} \Delta x = \left[ \Sigma_1 E_1 + \Sigma_2 E_2 + + \Sigma_3 \int_{I}^{\Emax+I} E~g(E)~dE \right] + \Delta x +\end{equation} +From this, using the equations (\ref{eq:sigex}), (\ref{eq:sigion}), +(\ref{eq:fisum}) and (\ref{eq:flnsum}), one can define the parameter +$C$ +\begin{equation} +C = \frac{dE}{dx} +\end{equation} + +The following values have been chosen in \GEANT{} for the other +parameters: +\[ +\begin{array}{lcl} +f_2 = \left\{ \begin{array}{ll} + 0 & \mathrm{if}\, Z \leq 2 \\ + 2/Z & \mathrm{if}\, Z > 2 \\ + \end{array} \right. & \Rightarrow & f_1 = 1 - f_2 \\ +E_2 = 10 Z^2 \mathrm{eV} & \Rightarrow & E_1 = \left(\frac{I}{E_{2}^{f_2}} + \right)^{\frac{1}{f_1}} \\ +r = 0.4 & & \\ +\end{array} +\] +With these values the atomic level $E_2$ corresponds approximately +the K-shell energy of the atoms and $Zf_2$ the number of K-shell +electrons. $r$ is the only variable which can be tuned freely. It +determines the relative contribution of ionisation and +excitation to the energy loss. + +The energy loss is computed with the assumption that the step length +(or the relative energy loss) is small, and---in consequence---the +cross-section can be considered constant along the path length. The +energy loss due to the excitation is +\begin{equation} +\Delta E_e = n_1 E_1 + n_2 E_2 +\end{equation} +where $n_1$ and $n_2$ are sampled from Poisson distribution as +discussed above. The loss due to the ionisation can be generated from +the distribution $g(E)$ by the inverse transformation method: +\begin{eqnarray} +u = F(E) & = & \int_{I}^E g(x) dx \nonumber \\ +E = F^{-1}(u) & = & \frac{I}{1 - u \frac {\Emax}{\Emax+I}} \\ +\end{eqnarray} +where $u$ is a uniform random number between $F(I)=0$ and +$F(\Emax+I)=1$. The contribution from the ionisations will be +\begin{equation} +\Delta E_i = \sum_{j=1}^{n_3} \frac{I} + {1 - u_j \frac {\Emax}{\Emax + I}} +\end{equation} +where $n_3$ is the number of ionisation (sampled from Poisson +distribution). The energy loss in a step will then be $\Delta E = +\Delta E_e + \Delta E_i$. + +\subsection{Fast simulation for $n_3 \geq 16$} + +If the number of ionisation $n_3$ is bigger than 16, a faster sampling +method can be used. The possible energy loss interval is divided in +two parts: one in which the number of collisions is large and the +sampling can be done from a Gaussian distribution and the other in +which the energy loss is sampled for each collision. Let us call the +former interval $[I, \alpha I]$ the interval A, and the latter +$[\alpha I,\Emax]$ the interval B. $\alpha$ lies between 1 and +$\Emax/I$. A collision with a loss in the interval A happens with +the probability +\begin{equation} +\label{eq:phys332-5} +P(\alpha) = \int_I^{\alpha I} g(\!E\!) \, dE = + \frac {( \Emax + I) (\alpha - 1)}{\Emax \alpha} +\end{equation} +The mean energy loss and the standard deviation for this type +of collision are +\begin{equation} +\langle \Delta E(\alpha) \rangle = \frac{1}{P(\alpha)} + \int_I^{\alpha I} E \, g(\!E\!) \, dE = + \frac{I \alpha \ln \alpha}{\alpha - 1} +\end{equation} +and +\begin{equation} +\sigma^2(\alpha) = \frac{1}{P(\alpha)} + \int_I^{\alpha I} E^2 \, g(\!E\!) \, dE = + I^2 \alpha \left( 1 - \frac{\alpha \ln \! ^2 \alpha}{(\alpha - 1)^2} \right) +\end{equation} +If the collision number is high , we assume that the number of the +type A collisions can be calculated from a Gaussian distribution +with the following mean value and standard deviation: +\begin{eqnarray} +\label{eq:phys332-1} +\langle n_A \rangle & = & n_3 P(\alpha) \\ +\label{eq:phys332-2} +\sigma_A^2 & = & n_3 P(\alpha) ( 1 - P(\alpha)) +\end{eqnarray} +It is further assumed that the energy loss in these collisions +has a Gaussian distribution with +\begin{eqnarray} +\label{eq:phys332-3} +\langle \Delta E_A \rangle & = & n_A \langle \Delta E(\alpha) \rangle \\ +\label{eq:phys332-4} +\sigma_{E,A}^2 & = & n_A \sigma^2(\alpha) +\end{eqnarray} +The energy loss of these collision can then be sampled from the +Gaussian distribution. + +The collisions where the energy loss is in the interval B are sampled +directly from +\begin{equation} +\Delta E_B = \sum_{i=1}^{n_3 - n_A} \frac{\alpha I} + {1 - u_i \frac{\Emax + I - \alpha I}{\Emax + I}} +\end{equation} +The total energy loss is the sum of these two types of collisions: +\begin{equation} +\Delta E = \Delta E_A + \Delta E_B +\end{equation} + +The approximation of equations ((\ref{eq:phys332-1}), +(\ref{eq:phys332-2}), (\ref{eq:phys332-3}) and (\ref{eq:phys332-4}) +can be used under the following conditions: +\begin{eqnarray} +\label{eq:phys332-6} +\langle n_A \rangle - c \, \sigma_A & \geq & 0 \\ +\label{eq:phys332-7} +\langle n_A \rangle + c \, \sigma_A & \leq & n_3 \\ +\label{eq:phys332-8} +\langle \Delta E_A \rangle - c \, \sigma_{E,A} & \geq & 0 +\end{eqnarray} +where $c \geq 4$. From the equations (\ref{eq:phys332-5}), +(\ref{eq:phys332-1}) and (\ref{eq:phys332-3}) and from the conditions +(\ref{eq:phys332-6}) and (\ref{eq:phys332-7}) the following limits can +be derived: +\begin{equation} +\alpha_{\mathrm{min}} = \frac{(n_3 + c^2)(\Emax+I)} + {n_3 (\Emax + I) + c^2 I} \; \leq \alpha \; \leq +\alpha_{\mathrm{max}} = \frac{(n_3 + c^2)(\Emax+I)} + {c^2 (\Emax + I) + n_3 I} +\end{equation} +This conditions gives a lower limit to number of the ionisations $n_3$ +for which the fast sampling can be done: +\begin{equation} +n_3 \; \geq \; c^2 +\end{equation} +As in the conditions (\ref{eq:phys332-6}), (\ref{eq:phys332-7}) and +(\ref{eq:phys332-8}) the value of $c$ is as minimum 4, one gets $n_3 +\; \geq 16$. In order to speed the simulation, the maximum value is +used for $\alpha$. + +The number of collisions with energy loss in the interval B (the +number of interactions which has to be simulated directly) increases +slowly with the total number of collisions $n_3$. The maximum number +of these collisions can be estimated as +\begin{equation} +n_{B,max} = n_3 - n_{A,min} \approx n_3 (\langle n_A \rangle + - \sigma_A) +\end{equation} +From the previous expressions for $\langle n_A \rangle$ and $\sigma_A$ +one can derive the condition +\begin{equation} +n_B \; \leq \; n_{B,max} = \frac{2 n_3 c^2}{n_3+c^2} +\end{equation} +The following values are obtained with $c=4$: + +\begin{tabular}{llcrr} +$n_3$ & $n_{B,max}$ & & $n_3$ & $n_{B,max}$\\ \hline +16 & 16 & & 200 & 29.63\\ +20 & 17.78 & & 500 & 31.01 \\ +50 & 24.24 & & 1000 & 31.50 \\ +100 & 27.59 & & $\infty$ & 32.00 +\end{tabular} + +\subsection{Special sampling for lower part of the spectrum} + +If the step length is very small ($\leq 5$ mm in gases, $\leq$ 2-3 +$\mu$m in solids) the model gives 0 energy loss for some events. To +avoid this, the probability of 0 energy loss is computed +\begin{equation} +P( \Delta E=0) = e^{-( \langle n_1 \rangle + \langle n_2 \rangle + + \langle n_3 \rangle )} +\end{equation} +If the probability is bigger than 0.01 a special sampling is done, +taking into account the fact that in these cases the projectile +interacts only with the outer electrons of the atom. An energy level +$E_0 = 10$ eV is chosen to correspond to the outer electrons. The mean +number of collisions can be calculated from +\begin{equation} +\langle n \rangle = \frac{1}{E_0} \frac{dE}{dx} \Delta x +\end{equation} +The number of collisions $n$ is sampled from Poisson distribution. +In the case of the thin layers, all the collisions are considered as +ionisations and the energy loss is computed as +\begin{equation} +\Delta E = \sum_{i=1}^n \frac{E_0} + {1 - \frac {\Emax}{\Emax + E_0} u_i} +\end{equation} + +\begin{thebibliography}{10} +\bibitem{bib-LAND} +L.Landau. +\newblock On the Energy Loss of Fast Particles by Ionisation. +\newblock Originally published in \emph{J. Phys.}, 8:201, 1944. +\newblock Reprinted in D.ter Haar, Editor, \emph{L.D.Landau, Collected + papers}, page 417. Pergamon Press, Oxford, 1965. + +\bibitem{bib-SCH1} +B.Schorr. +\newblock Programs for the Landau and the Vavilov distributions and the + corresponding random numbers. +\newblock \emph{Comp. Phys. Comm.}, 7:216, 1974. + +\bibitem{bib-SELT} +S.M.Seltzer and M.J.Berger. +\newblock Energy loss straggling of protons and mesons. +\newblock In \emph{Studies in Penetration of Charged Particles in + Matter}, Nuclear Science Series~39, Nat. Academy of Sciences, + Washington DC, 1964. + +\bibitem{bib-TALM} +R.Talman. +\newblock On the statistics of particle identification using ionization. +\newblock \emph{Nucl. Inst. Meth.}, 159:189, 1979. + +\bibitem{bib-VAVI} +P.V.Vavilov. +\newblock Ionisation losses of high energy heavy particles. +\newblock \emph{Soviet Physics JETP}, 5:749, 1957. +\end{thebibliography} + +\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch2/phys332-1.pdf b/Master/texmf-dist/doc/latex/latex-web-companion/ch2/phys332-1.pdf new file mode 100644 index 00000000000..bbc8ac5dfa5 Binary files /dev/null and b/Master/texmf-dist/doc/latex/latex-web-companion/ch2/phys332-1.pdf differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch2/phys332-2.pdf b/Master/texmf-dist/doc/latex/latex-web-companion/ch2/phys332-2.pdf new file mode 100644 index 00000000000..a058beb73f2 Binary files /dev/null and b/Master/texmf-dist/doc/latex/latex-web-companion/ch2/phys332-2.pdf differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/Makefile.ex2 b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/Makefile.ex2 new file mode 100644 index 00000000000..c84db2a0f15 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/Makefile.ex2 @@ -0,0 +1,10 @@ +# Makefile for Example 2 +LTX = latex +L2H2 = latex2html -init_file myinit.pl -info "External_links_test" + +ex2 : ex21.aux ex22.aux + $(L2H2) ex2bib ex21 ex22 ex20 +ex21.aux : + $(LTX) ex21.tex +ex22.aux : + $(LTX) ex22.tex diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/Makefile.ex3 b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/Makefile.ex3 new file mode 100644 index 00000000000..896b004a5aa --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/Makefile.ex3 @@ -0,0 +1,62 @@ +# Makefile for Example 3 +L2H = $(L2HNEW)/latex2html -link 4 +L2HTOP = $(L2HNEW)/latex2html -split 0 +LTX = latex +EX = ex3 +HTML = .html +TX = .tex +TEXES = $(EX)*$(TX) +TOP = ex30 +BIB = $(EX)bib +TEXTOP = $(TOP)$(TX) +INT = internals.pl +BIBREF = '\#BIBLIO' +# Directories containing the segments +EX30 = ../$(TOP)/$(TOP) +EX31 = ../$(EX)1/$(EX)1 +EX32 = ../$(EX)2/$(EX)2 +EX3b = ../$(TOP)/$(TOP)$(HTML) +# Titles for navigation to the segments +EX30t = Exemple_d\'un_document_segmenté +EX31t = Une_figure_EPS +EX32t = Exemple_d\'un_tableau +EX3bt = Références + +COMMON = -info 0 -split 1 -link 4 -no_auto_link -biblio $(EX3b) -external_file $(TOP) \ + -up_url $(EX30)$(HTML) -up_title $(EX30t) -index $(EX3b) -index_in_navigation +update: $(TOP).ind + make $(TOP)/$(INT) $(EX)2/$(INT) $(EX)1/$(INT); make $(TOP)/$(INT) +fresh: + rm $(EX)*/$(INT) $(TOP).aux; make $(TOP).ind; + make $(TOP)$(HTML) $(EX)2$(HTML) $(EX)1$(HTML); make $(TOP)$(HTML) +$(TOP)$(HTML) : + $(L2HTOP) -down_url $(EX31)$(HTML) -down_title $(EX31t) -biblio $(BIBREF) $(TOP) +$(TOP)/$(INT) : $(TEXTOP) $(BIB)$(TX) $(EX)1/$(INT) $(EX)2/$(INT) + make $(TOP)$(HTML) +$(EX)1$(HTML) : + $(L2H) $(COMMON) -t $(EX31t) -prev_url $(EX30)$(HTML) -prev_title $(EX30t) \ + -down_url $(EX32)$(HTML) -down_title $(EX32t) $(EX)1 +$(EX)1/$(INT) : $(EX)1$(TX) + make $(EX)1$(HTML) +$(EX)2$(HTML) : + $(L2H) $(COMMON) -t $(EX32t) -prev_url $(EX31)$(HTML) -prev_title $(EX31t) \ + -down_url $(EX3b)$(BIBREF) -down_title $(EX3bt) $(EX)2 +$(EX)2/$(INT) : $(EX)2$(TX) + make $(EX)2$(HTML) + +# handle LaTeX/dvips/makeindex etc. +$(TOP).aux: $(TEXES) + make dvi +$(TOP).dvi: + make dvi +dvi: + $(LTX) $(TEXTOP); $(LTX) $(TEXTOP); make $(TOP).ind +$(TOP).ind: $(TOP).aux + makeindex $(TOP).idx; $(LTX) $(TEXTOP); touch $(TOP).ind +ps: + make $(TOP).ps +$(TOP).ps: $(TOP).dvi + dvips $(TOP).dvi -o +clean: + rm *.ps *.dvi *.log *.ilg + diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/README.ch3 b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/README.ch3 new file mode 100644 index 00000000000..5af34ae103b --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/README.ch3 @@ -0,0 +1,72 @@ +Source files for examples in Chapter 3 of the LaTeX Graphics Companion + +File for Section 3.2.1 +++++++++++++++++++++++ + +l2hexa.tex Latex source +colorcir.eps EPS file used by several examples +tac2dim.eps " " + +Files for Section 3.3 ++++++++++++++++++++++ + +sampleAMS.tex Latex sources +sampleMath.tex " +sampleAMS.css CSS style file for use with sampleAMS + see Section 3.3.4 + (copy into the sampleAMS directory) + +sampleMathImages.tex Special source files for Section 3.3.5 +sampleMathThumb.tex + +Section 3.4 ++++++++++++ + +Installing the necessary bits for running the examples is a little +complicated. You need to have the correct fonts + the pre-processors +and edit the .perl files to give the paths. + +In any case, the sources are in the folowing subdirectories: + http://www-texdev.mpce.mq.edu.au/l2h/indic/Indica/ + http://www-texdev.mpce.mq.edu.au/l2h/indic/ITRANS/ + +The LWC examples are from: + +Figure 3.14: + http://www-texdev.mpce.mq.edu.au/l2h/indic/Indica/indicadocs.doc +(This is a document by Yannis Haralambous, for Sinhala-TeX.) + + +Figure 3.15 is from there also. + + +Figures 3.16 and 3.17 + are from Avinash Chopde's documentation for ITRANS. + You can get the files from: + + http://www-texdev.mpce.mq.edu.au/l2h/indic/ITRANS/ + vnehru.itx (or vnehru.tex if you preprocess it) + vnehru/ has the Web document; + sample.itx (or sample.tex) + sample/ has the Web document; + +Files for Section 3.5.6 ++++++++++++++++++++++++ + +Makefile.ex2 Makefile for running the example + (rename to Makefile to run) +ex20.tex Latex sources +ex21.tex " +ex22.tex " +ex2bib.tex " +myinit.pl LaTeX2html customization file + +Files for Section 3.5.7.3 ++++++++++++++++++++++++++ + +Makefile.ex3 Makefile for running the example + (rename to Makefile to run) +ex30.tex Latex sources +ex31.tex " +ex32.tex " +ex3bib.tex " diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/colorcir.eps b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/colorcir.eps new file mode 100644 index 00000000000..149d0c170fb --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/colorcir.eps @@ -0,0 +1,109 @@ +%! +%%BoundingBox: 19 164 581 636 +0.0 setlinewidth + +/hsvcircle { +gsave + /h 0.0 def + 0 4 360 { + pop + gsave + 0.5 0.0 translate + + newpath + 0.0 0.0 moveto + 0.1 0.0 lineto + 0.1 0.02 lineto + 0.0 0.02 lineto + closepath + h 1.0 1.0 sethsbcolor + fill + + %newpath + %0.0 0.0 moveto + %0.1 0.0 lineto + %0.1 0.02 lineto + %0.0 0.02 lineto + %closepath + %0.0 setgray + %stroke + + grestore + /h h 4 360 div add def + 4 rotate + } for +grestore +} def + +/graycircle { +gsave + /h -1.0 def + 0 4 360 { + pop + gsave + 0.5 0.0 translate + + newpath + 0.0 0.0 moveto + 0.1 0.0 lineto + 0.1 0.02 lineto + 0.0 0.02 lineto + closepath + + h abs setgray + fill + + %newpath + %0.0 0.0 moveto + %0.1 0.0 lineto + %0.1 0.02 lineto + %0.0 0.02 lineto + %closepath + %0.0 setgray + %stroke + grestore + + /h h 8 360 div add def + 4 rotate + } for +grestore +} def + +0.0 setlinewidth +0.0 setgray +300 400 translate +500 500 scale + +30 rotate +1.0 0.7 scale +-30 rotate + +hsvcircle +0.8 0.8 scale +graycircle +0.8 0.8 scale +hsvcircle +0.8 0.8 scale +graycircle +0.8 0.8 scale +hsvcircle +0.8 0.8 scale +graycircle +0.8 0.8 scale +hsvcircle +0.8 0.8 scale +graycircle +0.8 0.8 scale +hsvcircle +0.8 0.8 scale +graycircle +0.8 0.8 scale +hsvcircle +0.8 0.8 scale +graycircle +0.8 0.8 scale +hsvcircle +0.8 0.8 scale +graycircle + +showpage diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex20.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex20.tex new file mode 100644 index 00000000000..6ff0504b594 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex20.tex @@ -0,0 +1,25 @@ +\documentclass{article} +\usepackage{html} +%begin{latexonly} +\usepackage[T1]{fontenc} +%end{latexonly} +\usepackage[dvips]{graphicx} +\usepackage{francais} +\begin{document} +\begin{center}\Large + Exemple d'un document composé\\ +\end{center} + +\htmladdnormallink{Les Images}{../ex21/ex21.html} + +\externallabels{../ex21}{../ex21/labels.pl} +Référence à une figure externe~\externalref{Fpsfig}. + +\htmladdnormallink{Les tableaux}{../ex22/ex22.html} + +\externallabels{../ex22}{../ex22/labels.pl} +Référence à un tableau externe~\externalref{tab-exa}. + +\htmladdnormallink{La bibliographie}% + {../ex2bib/ex2bib.html} +\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex21.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex21.tex new file mode 100644 index 00000000000..9b6bc130524 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex21.tex @@ -0,0 +1,27 @@ +\documentclass{article} +\usepackage{html} +%begin{latexonly} +\usepackage[T1]{fontenc} +%end{latexonly} +\usepackage[dvips]{graphicx} +\usepackage{francais} +\makeindex +\begin{document} +\section{Une figure EPS} +\label{sec-figure} +Cette section montre comment inclure une figure +\externallabels{../ex2bib}{../ex2bib/labels.pl}% +PostScript\externalref{bibPS} dans un document \LaTeX. +La \hyperref{figure}{figure }{}{Fpsfig} +est insérée dans le texte à l'aide de la commande +\verb!\includegraphics{colorcir}!. +\begin{figure} +\htmlimage{thumbnail=0.4} +\centering + \begin{tabular}{c@{\qquad}c} + \includegraphics[width=3cm]{colorcir} & + \includegraphics[width=3cm]{tac2dim} + \end{tabular} + \caption{Deux images EPS}\label{Fpsfig} +\end{figure} +\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex22.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex22.tex new file mode 100644 index 00000000000..ff97376b120 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex22.tex @@ -0,0 +1,29 @@ +\documentclass{article} +\usepackage{html} +%begin{latexonly} +\usepackage[T1]{fontenc} +%end{latexonly} +\usepackage[dvips]{graphicx} +\usepackage{francais} +\newcommand{\Lcs}[1]{\texttt{\symbol{'134}#1}} +\begin{document} +\section{Exemple d'un tableau} +\label{sec-tableau} +Le \hyperref{tableau}{tableau }{}{tab-exa} montre +l'utilisation de l'environnement \texttt{table}. +\begin{table} +\centering + \begin{tabular}{cccccc} + \Lcs{primo} & \primo & \Lcs{secundo} & \secundo & + \Lcs{tertio} & \tertio \\ + \Lcs{quatro} & \quatro& 1\Lcs{ier} & 1\ier & + 1\Lcs{iere} & 1\iere \\ + \Lcs{fprimo)}&\fprimo)& \Lcs{No} 10 & \No 10 & + \Lcs{no} 15 & \no 15 \\ + \Lcs{og} a \Lcs{fg}&\og a \fg&3\Lcs{ieme}&3\ieme & + 10\Lcs{iemes}& 10\iemes + \end{tabular} +\caption{Quelques commandes de l'option + \texttt{french} de \texttt{babel}}\label{tab-exa} +\end{table} +\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex2bib.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex2bib.tex new file mode 100644 index 00000000000..f691e5acfc9 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex2bib.tex @@ -0,0 +1,16 @@ +\documentclass{article} +\usepackage{html} +%begin{latexonly} +\usepackage[T1]{fontenc} +%end{latexonly} +\usepackage[dvips]{graphicx} +\usepackage{francais} +\makeindex +\begin{document} +\begin{thebibliography}{99} +\bibitem{bib-PS}\label{bibPS} +Adobe Inc. +\emph{PostScript, manuel de référence (2ième édition)} +InterÉditions (France), 1992 +\end{thebibliography} +\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex30.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex30.tex new file mode 100644 index 00000000000..0b1b755235f --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex30.tex @@ -0,0 +1,43 @@ +\documentclass{article} +\usepackage[dvips]{graphicx} +\usepackage{francais} +\usepackage{html} +\usepackage{makeidx} +%begin{latexonly} +\usepackage[T1]{fontenc} +%end{latexonly} + +\internal{../ex31/} +\internal[sections]{../ex31/} +%\internal[contents]{../ex31/} +\internal[figure]{../ex31/} +\internal[index]{../ex31/} + +\internal{../ex32/} +\internal[sections]{../ex32/} +%\internal[contents]{../ex32/} +\internal[table]{../ex32/} +\internal[index]{../ex32/} + +\makeindex +\title{Exemple d'un document segmenté} +\author{Ross Moore \& Michel Goossens} + +\begin{document} +\maketitle\htmlrule +\tableofchildlinks\htmlrule +%begin{latexonly} +\tableofcontents +%end{latexonly} +\listoffigures\listoftables\htmlrule + +\segment{ex31}{section}{Une figure EPS} +\endsegment[section] +\html{Référence à figure~\ref{Fpsfig}.} + +\segment{ex32}{section}{Exemple d'un tableau} +\endsegment[section] +\html{Référence à tableau~\ref{tab-exa}.} +\htmlrule \input{ex3bib} +\htmlrule \printindex \htmlrule +\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex31.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex31.tex new file mode 100644 index 00000000000..1f5c97339f3 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex31.tex @@ -0,0 +1,27 @@ +\begin{htmlonly} +\documentclass{article} +\usepackage{makeidx,html} +\usepackage[T1]{fontenc} +\usepackage[dvips]{graphicx} +\usepackage{francais} +\input ex31.ptr +\end{htmlonly} +\startdocument +\index{section!figure} + +Cette section montre comment inclure une figure +PostScript\cite{bib-PS} dans un document \LaTeX. +La \hyperref{figure}{figure }{}{Fpsfig} +est insérée dans le texte à l'aide de la commande +\verb!\includegraphics{colorcir}!. +\index{figure} +\index{PostScript} +\begin{figure}[h] +\htmlimage{thumbnail=0.4} +\centering + \begin{tabular}{c@{\qquad}c} + \includegraphics[width=3cm]{colorcir} & + \includegraphics[width=3cm]{tac2dim} + \end{tabular} + \caption{Deux images EPS}\label{Fpsfig} +\end{figure} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex32.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex32.tex new file mode 100644 index 00000000000..293d66f4650 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex32.tex @@ -0,0 +1,27 @@ +\begin{htmlonly} +\usepackage{makeidx,html} +\usepackage{francais} +\input ex32.ptr +\end{htmlonly} +\newcommand{\Lcs}[1]{\texttt{\symbol{'134}#1}} +\startdocument +\index{section!tableau} + +Le \hyperref{tableau}{tableau }{}{tab-exa} +montre l'utilisation de l'environnement \texttt{table}. +\begin{table}[h] +\centering + \begin{tabular}{cccccc} + \Lcs{primo} & \primo & \Lcs{secundo} & \secundo + & \Lcs{tertio} & \tertio \\ + \Lcs{quatro} & \quatro& 1\Lcs{ier} & 1\ier + & 1\Lcs{iere} & 1\iere \\ + \Lcs{fprimo)}&\fprimo)& \Lcs{No} 10 & \No 10 + & \Lcs{no} 15 & \no 15 \\ + \Lcs{og} a \Lcs{fg}&\og a \fg&3\Lcs{ieme}&3\ieme + & 10\Lcs{iemes}& 10\iemes + \end{tabular} +\caption{Quelques commandes de l'option \texttt{french} + de \texttt{babel}}\label{tab-exa} +\index{tableau} +\end{table} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex3bib.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex3bib.tex new file mode 100644 index 00000000000..12e197babf2 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/ex3bib.tex @@ -0,0 +1,6 @@ +\begin{thebibliography}{99} +\label{BIBLIO}\index{références} +\bibitem{bib-PS} +Adobe Inc. \emph{PostScript, manuel de référence + (2ième édition)} InterÉditions (France), 1992 +\end{thebibliography} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/l2hexa.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/l2hexa.tex new file mode 100644 index 00000000000..817ffbe7f1d --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/l2hexa.tex @@ -0,0 +1,62 @@ +\documentclass{article} +\usepackage{graphicx} +\usepackage{francais} +\usepackage{makeidx} +\newcommand{\Lcs}[1]{\texttt{\symbol{'134}#1}} +\makeindex +\title{Exemple d'un article en fran\c{c}ais} +\author{Michel Goossens} +\begin{document} +\maketitle +\tableofcontents +\listoffigures +\listoftables +\section{Une figure EPS} +\index{section} +Cette section montre comment inclure une figure PostScript\cite{bib-PS} +dans un document \LaTeX. La figure~\ref{Fpsfig} +est ins\'er\'ee dans le texte \`a l'aide de la commande + \verb!\includegraphics{colorcir.eps}!. +\index{figure} +\index{PostScript} +\begin{figure} + \begin{center} + \begin{tabular}{c@{\qquad}c} + \includegraphics[width=3cm]{colorcir} & + \includegraphics[width=3cm]{tac2dim} + \end{tabular} + \end{center} + \caption{Deux images EPS} + \label{Fpsfig} +\end{figure} + +\section{Exemple d'un tableau} + +Le tableau~\ref{tab:exa} \`a la page \pageref{tab:exa} +montre l'utilisation de l'environnement \texttt{table}. + +\begin{table} + \begin{center} + \begin{tabular}{cccccc} + \Lcs{primo} & \primo & \Lcs{secundo} & \secundo & \Lcs{tertio} & \tertio \\ + \Lcs{quatro} & \quatro& 1\Lcs{ier} & 1\ier & 1\Lcs{iere} & 1\iere \\ + \Lcs{fprimo)}&\fprimo)& \Lcs{No} 10 & \No 10 & \Lcs{no} 15 & \no 15 \\ + \Lcs{og} a \Lcs{fg}&\og a \fg&3\Lcs{ieme}&3\ieme & 10\Lcs{iemes}& 10\iemes + \end{tabular} + \end{center} + \caption{Quelques commandes de l'option \texttt{francais} de \texttt{babel}} + \label{tab:exa} + \index{tableau} +\end{table} + +\begin{thebibliography}{99} +\index{r\'ef\'erences} +\bibitem{bib-PS} +Adobe Inc. +\emph{PostScript, manuel de r\'ef\'erence (2\ieme \'edition)} +Inter\'Editions (France), 1992 +\end{thebibliography} +\printindex +\index{index} +\end{document} +% End of document. diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/myinit.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/myinit.pl new file mode 100644 index 00000000000..b24da780bf5 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/myinit.pl @@ -0,0 +1,8 @@ +# File myinit.pl +$ADDRESS = "Michel Goossens
" . + "Division IT
" . + "Tél. 767.5028
" . + "$address_data[1]
"; +$MAX_SPLIT_DEPTH = 0; # do not split document +$NO_NAVIGATION = 1; # no navigation panel +1; # Mandatory last line diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleAMS.css b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleAMS.css new file mode 100644 index 00000000000..daee915b4dd --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleAMS.css @@ -0,0 +1,4 @@ +H2 { border : 2pt solid brown ; color : maroon ; padding : 5pt } +TD.eqno {color : green ; fontweight : 700 } /* equation-number cells */ +TABLE.subequations { background-color : #E0E0E0 ; } +P { line-height : 18pt ; } diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleAMS.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleAMS.tex new file mode 100644 index 00000000000..7a0f0ea4629 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleAMS.tex @@ -0,0 +1,54 @@ +\documentclass[a4paper,twoside]{article} +\usepackage{html} +\usepackage{amsmath} + +\renewcommand{\d}{\partial}\providecommand{\bm}[1]{\mathbf{#1}} +\providecommand{\Range}{\mathcal{R}}\providecommand{\Ker}{\mathcal{N}} +\providecommand{\Quat}{\vec{\mathbf{Q}}} + +\newcommand{\StAndrews}{\htmlurl{http://www-groups.dcs.st-and.ac.uk/~history}}% +\newcommand{\Pythagorians}{\htmladdnormallink + {Pythagorians}{\StAndrews/Mathematicians/Pythagoras.html}} +\newcommand{\Fermat}{\htmladdnormallink + {Fermat, c.1637}{\StAndrews/HistTopics/Fermat's_last_theorem.html}} +\newcommand{\Wiles}{\htmladdnormallink + {Wiles, 1995}{\htmlurl{http://www.pbs.org:80/wgbh/nova/proof}}} + +\begin{document} +\htmlhead[center]{section}{Math examples} +\begin{eqnarray} + \phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty} + \exp \left( u \ln u + \lambda u \right ) du \hspace{1cm}\mbox{for } c \geq 0 \\ + \lambda & = & \frac{\epsilon -\bar{\epsilon} }{\xi} + - \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}} \\ + \gamma & = & 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)} \\ + \gamma' & = & 0.422784\dots = 1 - \gamma \\ + \epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss} +\end{eqnarray} + +Since~\eqref{eqn:stress-sr} or~\eqref{gdef} should hold for arbitrary $\delta\bm{c}$% +-vectors, it is clear that $\Ker(A) = \Range(B)$ and that when $y=B(x)$ one has...\\ +...the \Pythagorians{} knew infinitely many solutions in integers to $a^2+b^2=c^2$. +That no non-trivial integer solutions exist for $a^n+b^n=c^n$ with integers $n>2$ has long +been suspected (\Fermat). Only during the current decade has this been proved (\Wiles). + +\begin{eqnarray}\label{eqn:stress-sr} + V \bm{\pi}^{sr} & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i + + \sum_i \sum_{j>i} \bm{R}_{ij} \bm{F}_{ij}\right> \\ \nonumber + & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i + + \sum_{i}\sum_{j>i}\sum_\alpha\sum_\beta \bm{r}_{i\alpha j\beta}\bm{f}_{i\alpha j\beta} + - \sum_i \sum_\alpha \bm{p}_{i\alpha} \bm{f}_{i\alpha} \right> +\end{eqnarray} + +\begin{subequations}\label{bgdefs} +\begin{align} B_{ij}^\alpha & = + \left(B_{ij}^\alpha\right)_0 + \left(B_{ij}^\alpha\right)_a \label{bdef} \\ + \left(B_{ij}^\alpha\right)_0 & = \frac{1}{2}\left(\frac{\d N_i^\alpha}{\d X_j} + + \frac{\d N_j^\alpha} {\d X_i} \right) \label{b0def} \\ + \left(B_{ij}^\alpha\right)_a & = H_{ij}^{\alpha \beta} a^\beta \label{budef} \\ + H_{ij}^{\alpha \beta} & = + \frac{1}{2}\left( \frac{\d N_k^\alpha}{\d X_i} \frac{\d N_k^\beta}{\d X_j} + + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right) \label{gdef} +\end{align} +\end{subequations} +\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleMath.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleMath.tex new file mode 100644 index 00000000000..26ab42edddc --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleMath.tex @@ -0,0 +1,54 @@ +\documentclass[a4paper,twoside]{article} +\usepackage{html} +%\usepackage{amsmath} + +\renewcommand{\d}{\partial}\providecommand{\bm}[1]{\mathbf{#1}} +\providecommand{\Range}{\mathcal{R}}\providecommand{\Ker}{\mathcal{N}} +\providecommand{\Quat}{\vec{\mathbf{Q}}} + +\newcommand{\StAndrews}{\htmlurl{http://www-groups.dcs.st-and.ac.uk/~history}}% +\newcommand{\Pythagorians}{\htmladdnormallink + {Pythagorians}{\StAndrews/Mathematicians/Pythagoras.html}} +\newcommand{\Fermat}{\htmladdnormallink + {Fermat, c.1637}{\StAndrews/HistTopics/Fermat's_last_theorem.html}} +\newcommand{\Wiles}{\htmladdnormallink + {Wiles, 1995}{\htmlurl{http://www.pbs.org:80/wgbh/nova/proof}}} + +\begin{document} +\htmlhead[center]{section}{Math examples} +\begin{eqnarray} + \phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty} + \exp \left( u \ln u + \lambda u \right ) du \hspace{1cm}\mbox{for } c \geq 0 \\ + \lambda & = & \frac{\epsilon -\bar{\epsilon} }{\xi} + - \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}}\label{xiEmax} \\ + \gamma & = & 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)} \\ + \gamma' & = & 0.422784\dots = 1 - \gamma \\ + \epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss} +\end{eqnarray} + +Since~\ref{xiEmax} and \ref{eqn:stress-sr} hold for arbitrary $\delta\bm{c}$-vectors, +it is clear that $\Ker(A) = \Range(B)$ and that when $y=B(x)$ one has...\\ +...the \Pythagorians{} knew infinitely many solutions in integers to $a^2+b^2=c^2$. +That no non-trivial integer solutions exist for $a^n+b^n=c^n$ with integers $n>2$ has long +been suspected (\Fermat). Only during the current decade has this been proved (\Wiles). + +\begin{eqnarray}\label{eqn:stress-sr} + V \bm{\pi}^{sr} & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i + + \sum_i \sum_{j>i} \bm{R}_{ij} \bm{F}_{ij}\right> \\ \nonumber + & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i + + \sum_{i}\sum_{j>i}\sum_\alpha\sum_\beta \bm{r}_{i\alpha j\beta}\bm{f}_{i\alpha j\beta} + - \sum_i \sum_\alpha \bm{p}_{i\alpha} \bm{f}_{i\alpha} \right> +\end{eqnarray} +\end{document} +\begin{subequations}\label{bgdefs} +\begin{align} B_{ij}^\alpha & = + \left(B_{ij}^\alpha\right)_0 + \left(B_{ij}^\alpha\right)_a \label{bdef} \\ + \left(B_{ij}^\alpha\right)_0 & = \frac{1}{2}\left(\frac{\d N_i^\alpha}{\d X_j} + + \frac{\d N_j^\alpha} {\d X_i} \right) \label{b0def} \\ + \left(B_{ij}^\alpha\right)_a & = H_{ij}^{\alpha \beta} a^\beta \label{budef} \\ + H_{ij}^{\alpha \beta} & = + \frac{1}{2}\left( \frac{\d N_k^\alpha}{\d X_i} \frac{\d N_k^\beta}{\d X_j} + + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right) \label{gdef} +\end{align} +\end{subequations} +\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleMathImages.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleMathImages.tex new file mode 100644 index 00000000000..cca8e754e57 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleMathImages.tex @@ -0,0 +1,64 @@ +\documentclass[a4paper,twoside]{article} +\usepackage{html} +\usepackage{amsmath} + +\renewcommand{\d}{\partial}\providecommand{\bm}[1]{\mathbf{#1}} +\providecommand{\Range}{\mathcal{R}}\providecommand{\Ker}{\mathcal{N}} +\providecommand{\Quat}{\vec{\mathbf{Q}}} + +\newcommand{\StAndrews}{\url{http://www-groups.dcs.st-and.ac.uk/~history}}% +\newcommand{\Pythagorians}{\htmladdnormallink + {Pythagorians}{\StAndrews/Mathematicians/Pythagoras.html}} +\newcommand{\Fermat}{\htmladdnormallink + {Fermat, c.1637}{\StAndrews/HistTopics/Fermat's_last_theorem.html}} +\newcommand{\Wiles}{\htmladdnormallink + {Wiles, 1995}{http://www.pbs.org:80/wgbh/nova/proof}} + +\begin{document} +\htmlhead[center]{section}{Math examples} +\begin{flushright} +\begin{makeimage} +\begin{eqnarray} + \phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty} + \exp \left( u \ln u + \lambda u \right ) du \hspace{1cm}\mbox{for } c \geq 0 \\ + \lambda & = & \frac{\epsilon -\bar{\epsilon} }{\xi} + - \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}} \\ + \gamma & = & 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)} \\ + \gamma' & = & 0.422784\dots = 1 - \gamma \\ + \epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss} +\end{eqnarray} +\end{makeimage} +\end{flushright} + +Since~\eqref{eqn:stress-sr} or~\eqref{gdef} should hold for arbitrary $\delta\bm{c}$% +-vectors, it is clear that $\Ker(A) = \Range(B)$ and that when $y=B(x)$ one has...\\ +...the \Pythagorians{} knew infinitely many solutions in integers to $a^2+b^2=c^2$. +That no non-trivial integer solutions exist for $a^n+b^n=c^n$ with integers $n>2$ has long +been suspected (\Fermat). Only during the current decade has this been proved (\Wiles). + +\begin{flushright} +\begin{eqnarray}\htmlimage{} +\label{eqn:stress-sr} + V \bm{\pi}^{sr} & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i + + \sum_i \sum_{j>i} \bm{R}_{ij} \bm{F}_{ij}\right> \\ \nonumber + & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i + + \sum_{i}\sum_{j>i}\sum_\alpha\sum_\beta \bm{r}_{i\alpha j\beta}\bm{f}_{i\alpha j\beta} + - \sum_i \sum_\alpha \bm{p}_{i\alpha} \bm{f}_{i\alpha} \right> +\end{eqnarray} +\end{flushright} + +\begin{flushright} +\begin{subequations}\htmlimage{} +\label{bgdefs} +\begin{align} B_{ij}^\alpha & = + \left(B_{ij}^\alpha\right)_0 + \left(B_{ij}^\alpha\right)_a \label{bdef} \\ + \left(B_{ij}^\alpha\right)_0 & = \frac{1}{2}\left(\frac{\d N_i^\alpha}{\d X_j} + + \frac{\d N_j^\alpha} {\d X_i} \right) \label{b0def} \\ + \left(B_{ij}^\alpha\right)_a & = H_{ij}^{\alpha \beta} a^\beta \label{budef} \\ + H_{ij}^{\alpha \beta} & = + \frac{1}{2}\left( \frac{\d N_k^\alpha}{\d X_i} \frac{\d N_k^\beta}{\d X_j} + + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right) \label{gdef} +\end{align} +\end{subequations} +\end{flushright} +\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleMathThumb.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleMathThumb.tex new file mode 100644 index 00000000000..b6c61782721 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/sampleMathThumb.tex @@ -0,0 +1,64 @@ +\documentclass[a4paper,twoside]{article} +\usepackage{html} +\usepackage{amsmath} + +\renewcommand{\d}{\partial}\providecommand{\bm}[1]{\mathbf{#1}} +\providecommand{\Range}{\mathcal{R}}\providecommand{\Ker}{\mathcal{N}} +\providecommand{\Quat}{\vec{\mathbf{Q}}} + +\newcommand{\StAndrews}{\url{http://www-groups.dcs.st-and.ac.uk/~history}}% +\newcommand{\Pythagorians}{\htmladdnormallink + {Pythagorians}{\StAndrews/Mathematicians/Pythagoras.html}} +\newcommand{\Fermat}{\htmladdnormallink + {Fermat, c.1637}{\StAndrews/HistTopics/Fermat's_last_theorem.html}} +\newcommand{\Wiles}{\htmladdnormallink + {Wiles, 1995}{http://www.pbs.org:80/wgbh/nova/proof}} + +\begin{document} +\htmlhead[center]{section}{Math examples} +\begin{flushright} +\begin{makeimage} +\begin{eqnarray} + \phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty} + \exp \left( u \ln u + \lambda u \right ) du \hspace{1cm}\mbox{for } c \geq 0 \\ + \lambda & = & \frac{\epsilon -\bar{\epsilon} }{\xi} + - \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}} \\ + \gamma & = & 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)} \\ + \gamma' & = & 0.422784\dots = 1 - \gamma \\ + \epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss} +\end{eqnarray} +\end{makeimage} +\end{flushright} + +Since~\eqref{eqn:stress-sr} or~\eqref{gdef} should hold for arbitrary $\delta\bm{c}$% +-vectors, it is clear that $\Ker(A) = \Range(B)$ and that when $y=B(x)$ one has...\\ +...the \Pythagorians{} knew infinitely many solutions in integers to $a^2+b^2=c^2$. +That no non-trivial integer solutions exist for $a^n+b^n=c^n$ with integers $n>2$ has long +been suspected (\Fermat). Only during the current decade has this been proved (\Wiles). + +\begin{flushright} +\begin{eqnarray}\htmlimage{thumbnail=.4} +\label{eqn:stress-sr} + V \bm{\pi}^{sr} & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i + + \sum_i \sum_{j>i} \bm{R}_{ij} \bm{F}_{ij}\right> \\ \nonumber + & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i + + \sum_{i}\sum_{j>i}\sum_\alpha\sum_\beta \bm{r}_{i\alpha j\beta}\bm{f}_{i\alpha j\beta} + - \sum_i \sum_\alpha \bm{p}_{i\alpha} \bm{f}_{i\alpha} \right> +\end{eqnarray} +\end{flushright} + +\begin{flushright} +\begin{subequations}\htmlimage{thumbnail=.3} +\label{bgdefs} +\begin{align} B_{ij}^\alpha & = + \left(B_{ij}^\alpha\right)_0 + \left(B_{ij}^\alpha\right)_a \label{bdef} \\ + \left(B_{ij}^\alpha\right)_0 & = \frac{1}{2}\left(\frac{\d N_i^\alpha}{\d X_j} + + \frac{\d N_j^\alpha} {\d X_i} \right) \label{b0def} \\ + \left(B_{ij}^\alpha\right)_a & = H_{ij}^{\alpha \beta} a^\beta \label{budef} \\ + H_{ij}^{\alpha \beta} & = + \frac{1}{2}\left( \frac{\d N_k^\alpha}{\d X_i} \frac{\d N_k^\beta}{\d X_j} + + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right) \label{gdef} +\end{align} +\end{subequations} +\end{flushright} +\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3/tac2dim.eps b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/tac2dim.eps new file mode 100644 index 00000000000..b96e3e23e90 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch3/tac2dim.eps @@ -0,0 +1,201 @@ +%!CERNPS_include //ddtrg2/user/goossens/pawmanual/tutex21.ps +%%BoundingBox: 0 0 582 582 +/d {lineto} def /m {moveto} def /t {translate} def +/sw {stringwidth} def /r {rotate} def /rl {roll} def +/rd {rlineto} def /rm {rmoveto} def /gr {grestore} def +/lw {setlinewidth} def /sd {setdash} def +/s {stroke} def /rgb {setrgbcolor} def +/c {closepath} def /sf {scalefont setfont} def +/oshow {gsave [] 0 sd true charpath stroke gr} def +/cs {gsave dup sw pop 2 div neg 5 -1 rl 5 -1 rl t 3 -1 rl r 0 m show gr} def +/rs 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1078 d s +showpage grestore diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/Makefile b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/Makefile deleted file mode 100644 index 896b004a5aa..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/Makefile +++ /dev/null @@ -1,62 +0,0 @@ -# Makefile for Example 3 -L2H = $(L2HNEW)/latex2html -link 4 -L2HTOP = $(L2HNEW)/latex2html -split 0 -LTX = latex -EX = ex3 -HTML = .html -TX = .tex -TEXES = $(EX)*$(TX) -TOP = ex30 -BIB = $(EX)bib -TEXTOP = $(TOP)$(TX) -INT = internals.pl -BIBREF = '\#BIBLIO' -# Directories containing the segments -EX30 = ../$(TOP)/$(TOP) -EX31 = ../$(EX)1/$(EX)1 -EX32 = ../$(EX)2/$(EX)2 -EX3b = ../$(TOP)/$(TOP)$(HTML) -# Titles for navigation to the segments -EX30t = Exemple_d\'un_document_segmenté -EX31t = Une_figure_EPS -EX32t = Exemple_d\'un_tableau -EX3bt = Références - -COMMON = -info 0 -split 1 -link 4 -no_auto_link -biblio $(EX3b) -external_file $(TOP) \ - -up_url $(EX30)$(HTML) -up_title $(EX30t) -index $(EX3b) -index_in_navigation -update: $(TOP).ind - make $(TOP)/$(INT) $(EX)2/$(INT) $(EX)1/$(INT); make $(TOP)/$(INT) -fresh: - rm $(EX)*/$(INT) $(TOP).aux; make $(TOP).ind; - make $(TOP)$(HTML) $(EX)2$(HTML) $(EX)1$(HTML); make $(TOP)$(HTML) -$(TOP)$(HTML) : - $(L2HTOP) -down_url $(EX31)$(HTML) -down_title $(EX31t) -biblio $(BIBREF) $(TOP) -$(TOP)/$(INT) : $(TEXTOP) $(BIB)$(TX) $(EX)1/$(INT) $(EX)2/$(INT) - make $(TOP)$(HTML) -$(EX)1$(HTML) : - $(L2H) $(COMMON) -t $(EX31t) -prev_url $(EX30)$(HTML) -prev_title $(EX30t) \ - -down_url $(EX32)$(HTML) -down_title $(EX32t) $(EX)1 -$(EX)1/$(INT) : $(EX)1$(TX) - make $(EX)1$(HTML) -$(EX)2$(HTML) : - $(L2H) $(COMMON) -t $(EX32t) -prev_url $(EX31)$(HTML) -prev_title $(EX31t) \ - -down_url $(EX3b)$(BIBREF) -down_title $(EX3bt) $(EX)2 -$(EX)2/$(INT) : $(EX)2$(TX) - make $(EX)2$(HTML) - -# handle LaTeX/dvips/makeindex etc. -$(TOP).aux: $(TEXES) - make dvi -$(TOP).dvi: - make dvi -dvi: - $(LTX) $(TEXTOP); $(LTX) $(TEXTOP); make $(TOP).ind -$(TOP).ind: $(TOP).aux - makeindex $(TOP).idx; $(LTX) $(TEXTOP); touch $(TOP).ind -ps: - make $(TOP).ps -$(TOP).ps: $(TOP).dvi - dvips $(TOP).dvi -o -clean: - rm *.ps *.dvi *.log *.ilg - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/Makefile.ex2 b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/Makefile.ex2 deleted file mode 100644 index c84db2a0f15..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/Makefile.ex2 +++ /dev/null @@ -1,10 +0,0 @@ -# Makefile for Example 2 -LTX = latex -L2H2 = latex2html -init_file myinit.pl -info "External_links_test" - -ex2 : ex21.aux ex22.aux - $(L2H2) ex2bib ex21 ex22 ex20 -ex21.aux : - $(LTX) ex21.tex -ex22.aux : - $(LTX) ex22.tex diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/Makefile.ex3 b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/Makefile.ex3 deleted file mode 100644 index 896b004a5aa..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/Makefile.ex3 +++ /dev/null @@ -1,62 +0,0 @@ -# Makefile for Example 3 -L2H = $(L2HNEW)/latex2html -link 4 -L2HTOP = $(L2HNEW)/latex2html -split 0 -LTX = latex -EX = ex3 -HTML = .html -TX = .tex -TEXES = $(EX)*$(TX) -TOP = ex30 -BIB = $(EX)bib -TEXTOP = $(TOP)$(TX) -INT = internals.pl -BIBREF = '\#BIBLIO' -# Directories containing the segments -EX30 = ../$(TOP)/$(TOP) -EX31 = ../$(EX)1/$(EX)1 -EX32 = ../$(EX)2/$(EX)2 -EX3b = ../$(TOP)/$(TOP)$(HTML) -# Titles for navigation to the segments -EX30t = Exemple_d\'un_document_segmenté -EX31t = Une_figure_EPS -EX32t = Exemple_d\'un_tableau -EX3bt = Références - -COMMON = -info 0 -split 1 -link 4 -no_auto_link -biblio $(EX3b) -external_file $(TOP) \ - -up_url $(EX30)$(HTML) -up_title $(EX30t) -index $(EX3b) -index_in_navigation -update: $(TOP).ind - make $(TOP)/$(INT) $(EX)2/$(INT) $(EX)1/$(INT); make $(TOP)/$(INT) -fresh: - rm $(EX)*/$(INT) $(TOP).aux; make $(TOP).ind; - make $(TOP)$(HTML) $(EX)2$(HTML) $(EX)1$(HTML); make $(TOP)$(HTML) -$(TOP)$(HTML) : - $(L2HTOP) -down_url $(EX31)$(HTML) -down_title $(EX31t) -biblio $(BIBREF) $(TOP) -$(TOP)/$(INT) : $(TEXTOP) $(BIB)$(TX) $(EX)1/$(INT) $(EX)2/$(INT) - make $(TOP)$(HTML) -$(EX)1$(HTML) : - $(L2H) $(COMMON) -t $(EX31t) -prev_url $(EX30)$(HTML) -prev_title $(EX30t) \ - -down_url $(EX32)$(HTML) -down_title $(EX32t) $(EX)1 -$(EX)1/$(INT) : $(EX)1$(TX) - make $(EX)1$(HTML) -$(EX)2$(HTML) : - $(L2H) $(COMMON) -t $(EX32t) -prev_url $(EX31)$(HTML) -prev_title $(EX31t) \ - -down_url $(EX3b)$(BIBREF) -down_title $(EX3bt) $(EX)2 -$(EX)2/$(INT) : $(EX)2$(TX) - make $(EX)2$(HTML) - -# handle LaTeX/dvips/makeindex etc. -$(TOP).aux: $(TEXES) - make dvi -$(TOP).dvi: - make dvi -dvi: - $(LTX) $(TEXTOP); $(LTX) $(TEXTOP); make $(TOP).ind -$(TOP).ind: $(TOP).aux - makeindex $(TOP).idx; $(LTX) $(TEXTOP); touch $(TOP).ind -ps: - make $(TOP).ps -$(TOP).ps: $(TOP).dvi - dvips $(TOP).dvi -o -clean: - rm *.ps *.dvi *.log *.ilg - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/README.ch3 b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/README.ch3 deleted file mode 100644 index 67eb2b6615a..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/README.ch3 +++ /dev/null @@ -1,37 +0,0 @@ -Source files for examples in Chapter 3 of the LaTeX Web Companion - -File for Section 3.2.1 - -l2hexa.tex Latex source -colorcir.eps EPS file used by several examples -tac2dim.eps " " - -Files for Section 3.3 - -sampleAMS.tex Latex sources -sampleMath.tex " -sampleAMS.css CSS style file for use with sampleAMS - see Section 3.3.4 - (copy into the sampleAMS directory) - -sampleMathImages.tex Special source files for Section 3.3.5 -sampleMathThumb.tex - -Files for Section 3.5.6 - -Makefile.ex2 Makefile for running the example - (rename to Makefile to run) -ex20.tex Latex sources -ex21.tex " -ex22.tex " -ex2bib.tex " -myinit.pl LaTeX2html customization file - -Files for Section 3.5.7.3 - -Makefile.ex3 Makefile for running the example - (rename to Makefile to run) -ex30.tex Latex sources -ex31.tex " -ex32.tex " -ex3bib.tex " diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/colorcir.eps b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/colorcir.eps deleted file mode 100644 index 149d0c170fb..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/colorcir.eps +++ /dev/null @@ -1,109 +0,0 @@ -%! -%%BoundingBox: 19 164 581 636 -0.0 setlinewidth - -/hsvcircle { -gsave - /h 0.0 def - 0 4 360 { - pop - gsave - 0.5 0.0 translate - - newpath - 0.0 0.0 moveto - 0.1 0.0 lineto - 0.1 0.02 lineto - 0.0 0.02 lineto - closepath - h 1.0 1.0 sethsbcolor - fill - - %newpath - %0.0 0.0 moveto - %0.1 0.0 lineto - %0.1 0.02 lineto - %0.0 0.02 lineto - %closepath - %0.0 setgray - %stroke - - grestore - /h h 4 360 div add def - 4 rotate - } for -grestore -} def - -/graycircle { -gsave - /h -1.0 def - 0 4 360 { - pop - gsave - 0.5 0.0 translate - - newpath - 0.0 0.0 moveto - 0.1 0.0 lineto - 0.1 0.02 lineto - 0.0 0.02 lineto - closepath - - h abs setgray - fill - - %newpath - %0.0 0.0 moveto - %0.1 0.0 lineto - %0.1 0.02 lineto - %0.0 0.02 lineto - %closepath - %0.0 setgray - %stroke - grestore - - /h h 8 360 div add def - 4 rotate - } for -grestore -} def - -0.0 setlinewidth -0.0 setgray -300 400 translate -500 500 scale - -30 rotate -1.0 0.7 scale --30 rotate - -hsvcircle -0.8 0.8 scale -graycircle -0.8 0.8 scale -hsvcircle -0.8 0.8 scale -graycircle -0.8 0.8 scale -hsvcircle -0.8 0.8 scale -graycircle -0.8 0.8 scale -hsvcircle -0.8 0.8 scale -graycircle -0.8 0.8 scale -hsvcircle -0.8 0.8 scale -graycircle -0.8 0.8 scale -hsvcircle -0.8 0.8 scale -graycircle -0.8 0.8 scale -hsvcircle -0.8 0.8 scale -graycircle - -showpage diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex20.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex20.tex deleted file mode 100644 index 6ff0504b594..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex20.tex +++ /dev/null @@ -1,25 +0,0 @@ -\documentclass{article} -\usepackage{html} -%begin{latexonly} -\usepackage[T1]{fontenc} -%end{latexonly} -\usepackage[dvips]{graphicx} -\usepackage{francais} -\begin{document} -\begin{center}\Large - Exemple d'un document composé\\ -\end{center} - -\htmladdnormallink{Les Images}{../ex21/ex21.html} - -\externallabels{../ex21}{../ex21/labels.pl} -Référence à une figure externe~\externalref{Fpsfig}. - -\htmladdnormallink{Les tableaux}{../ex22/ex22.html} - -\externallabels{../ex22}{../ex22/labels.pl} -Référence à un tableau externe~\externalref{tab-exa}. - -\htmladdnormallink{La bibliographie}% - {../ex2bib/ex2bib.html} -\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex21.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex21.tex deleted file mode 100644 index 9b6bc130524..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex21.tex +++ /dev/null @@ -1,27 +0,0 @@ -\documentclass{article} -\usepackage{html} -%begin{latexonly} -\usepackage[T1]{fontenc} -%end{latexonly} -\usepackage[dvips]{graphicx} -\usepackage{francais} -\makeindex -\begin{document} -\section{Une figure EPS} -\label{sec-figure} -Cette section montre comment inclure une figure -\externallabels{../ex2bib}{../ex2bib/labels.pl}% -PostScript\externalref{bibPS} dans un document \LaTeX. -La \hyperref{figure}{figure }{}{Fpsfig} -est insérée dans le texte à l'aide de la commande -\verb!\includegraphics{colorcir}!. -\begin{figure} -\htmlimage{thumbnail=0.4} -\centering - \begin{tabular}{c@{\qquad}c} - \includegraphics[width=3cm]{colorcir} & - \includegraphics[width=3cm]{tac2dim} - \end{tabular} - \caption{Deux images EPS}\label{Fpsfig} -\end{figure} -\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex22.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex22.tex deleted file mode 100644 index ff97376b120..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex22.tex +++ /dev/null @@ -1,29 +0,0 @@ -\documentclass{article} -\usepackage{html} -%begin{latexonly} -\usepackage[T1]{fontenc} -%end{latexonly} -\usepackage[dvips]{graphicx} -\usepackage{francais} -\newcommand{\Lcs}[1]{\texttt{\symbol{'134}#1}} -\begin{document} -\section{Exemple d'un tableau} -\label{sec-tableau} -Le \hyperref{tableau}{tableau }{}{tab-exa} montre -l'utilisation de l'environnement \texttt{table}. -\begin{table} -\centering - \begin{tabular}{cccccc} - \Lcs{primo} & \primo & \Lcs{secundo} & \secundo & - \Lcs{tertio} & \tertio \\ - \Lcs{quatro} & \quatro& 1\Lcs{ier} & 1\ier & - 1\Lcs{iere} & 1\iere \\ - \Lcs{fprimo)}&\fprimo)& \Lcs{No} 10 & \No 10 & - \Lcs{no} 15 & \no 15 \\ - \Lcs{og} a \Lcs{fg}&\og a \fg&3\Lcs{ieme}&3\ieme & - 10\Lcs{iemes}& 10\iemes - \end{tabular} -\caption{Quelques commandes de l'option - \texttt{french} de \texttt{babel}}\label{tab-exa} -\end{table} -\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex2bib.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex2bib.tex deleted file mode 100644 index f691e5acfc9..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex2bib.tex +++ /dev/null @@ -1,16 +0,0 @@ -\documentclass{article} -\usepackage{html} -%begin{latexonly} -\usepackage[T1]{fontenc} -%end{latexonly} -\usepackage[dvips]{graphicx} -\usepackage{francais} -\makeindex -\begin{document} -\begin{thebibliography}{99} -\bibitem{bib-PS}\label{bibPS} -Adobe Inc. -\emph{PostScript, manuel de référence (2ième édition)} -InterÉditions (France), 1992 -\end{thebibliography} -\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30.dvi b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30.dvi deleted file mode 100644 index b0a2ca47330..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30.dvi and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30.tex deleted file mode 100644 index 0b1b755235f..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30.tex +++ /dev/null @@ -1,43 +0,0 @@ -\documentclass{article} -\usepackage[dvips]{graphicx} -\usepackage{francais} -\usepackage{html} -\usepackage{makeidx} -%begin{latexonly} -\usepackage[T1]{fontenc} -%end{latexonly} - -\internal{../ex31/} -\internal[sections]{../ex31/} -%\internal[contents]{../ex31/} -\internal[figure]{../ex31/} -\internal[index]{../ex31/} - -\internal{../ex32/} -\internal[sections]{../ex32/} -%\internal[contents]{../ex32/} -\internal[table]{../ex32/} -\internal[index]{../ex32/} - -\makeindex -\title{Exemple d'un document segmenté} -\author{Ross Moore \& Michel Goossens} - -\begin{document} -\maketitle\htmlrule -\tableofchildlinks\htmlrule -%begin{latexonly} -\tableofcontents -%end{latexonly} -\listoffigures\listoftables\htmlrule - -\segment{ex31}{section}{Une figure EPS} -\endsegment[section] -\html{Référence à figure~\ref{Fpsfig}.} - -\segment{ex32}{section}{Exemple d'un tableau} -\endsegment[section] -\html{Référence à tableau~\ref{tab-exa}.} -\htmlrule \input{ex3bib} -\htmlrule \printindex \htmlrule -\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/contents.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/contents.pl deleted file mode 100644 index 314b2567f8f..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/contents.pl +++ /dev/null @@ -1,30 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate contents original text with physical files. - - -$key = q/0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$toc_section_info{$key} = '0%:%'."$dir".q|ex30.html%:%Exemple d'un document segmenté| unless ($toc_section_info{$key}); -$noresave{$key} = "$nosave"; - -$key = q/0 0 0 8 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$toc_section_info{$key} = '3%:%'."$dir".q|ex30.html%:%À propos de ce document...%:%| unless ($toc_section_info{$key}); -$noresave{$key} = "$nosave"; - -$key = q/0 0 0 1 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$toc_section_info{$key} = '3%:%'."$dir".q|ex30.html%:%Liste des figures| unless ($toc_section_info{$key}); -$noresave{$key} = "$nosave"; - -$key = q/0 0 0 2 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$toc_section_info{$key} = '3%:%'."$dir".q|ex30.html%:%Liste des tableaux| unless ($toc_section_info{$key}); -$noresave{$key} = "$nosave"; - -$key = q/0 0 0 6 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$toc_section_info{$key} = '3%:%'."$dir".q|ex30.html%:%Bibliographie| unless ($toc_section_info{$key}); -$noresave{$key} = "$nosave"; - -$key = q/0 0 0 7 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$toc_section_info{$key} = '3%:%'."$dir".q|ex30.html%:%Index| unless ($toc_section_info{$key}); -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/ex30.css b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/ex30.css deleted file mode 100644 index 1993b851311..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/ex30.css +++ /dev/null @@ -1,31 +0,0 @@ - -/* Century Schoolbook font is very similar to Computer Modern Math: cmmi */ -.MATH { font-family: "Century Schoolbook", serif; } -.MATH I { font-family: "Century Schoolbook", serif; font-shape: italic } -.BOLDMATH { font-family: "Century Schoolbook", serif; font-weight: bold } - -/* implement both fixed-size and relative sizes */ -SMALL.XTINY { font-size : xx-small } -SMALL.TINY { font-size : x-small } -SMALL.SCRIPTSIZE { font-size : smaller } -SMALL.FOOTNOTESIZE { font-size : small } -SMALL.SMALL { } -BIG.LARGE { } -BIG.XLARGE { font-size : large } -BIG.XXLARGE { font-size : x-large } -BIG.HUGE { font-size : larger } -BIG.XHUGE { font-size : xx-large } - -/* heading styles */ -H1 { } -H2 { } -H3 { } -H4 { } -H5 { } - -/* mathematics styles */ -DIV.displaymath { } /* math displays */ -TD.eqno { } /* equation-number cells */ - - -/* document-specific styles come next */ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/ex30.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/ex30.html deleted file mode 100644 index 5b7110ef179..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/ex30.html +++ /dev/null @@ -1,139 +0,0 @@ - - - - - -Exemple d'un document segmenté - - - - - - - - - - - - - - - - -next_group -up -previous -
- suivant: Une_figure_EPS -

- -

Exemple d'un document segmenté

-

Ross Moore & Michel Goossens


-
-
- - - - - -
-
-
- -

-Liste des figures -

  1. Deux images EPS

- -

-Liste des tableaux -

  1. Quelques commandes de l'option french - de babel

-
- -

-Référence à figure 1. - -

-Référence à tableau 1. -
-


-


-Bibliographie -

-

1 -
-Adobe Inc. PostScript, manuel de référence - (2ième édition) InterÉditions (France), 1992 -
-
-

- -

-Index -

-
figure -
Une figure EPS -
PostScript -
Une figure EPS -
références -
Bibliographie -
section -
-
figure -
Une figure EPS -
tableau -
Exemple d'un tableau -
-
tableau -
Exemple d'un tableau - -

-
-

-À propos de ce document... -

- Exemple d'un document segmenté

-This document was generated using the -LaTeX2HTML translator Version 99.1 release (March 30, 1999) -

-Copyright © 1993, 1994, 1995, 1996, -Nikos Drakos, -Computer Based Learning Unit, University of Leeds. -
Copyright © 1997, 1998, 1999, -Ross Moore, -Mathematics Department, Macquarie University, Sydney. -

-The command line arguments were:
- latex2html -split 0 -down_url ../ex31/ex31.html -down_title Une_figure_EPS -biblio #BIBLIO ex30 -

-The translation was initiated by Michel Goossens on 1999-03-30


-
-Michel Goossens -
1999-03-30 -
- - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/index.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/index.html deleted file mode 100644 index 5b7110ef179..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/index.html +++ /dev/null @@ -1,139 +0,0 @@ - - - - - -Exemple d'un document segmenté - - - - - - - - - - - - - - - - -next_group -up -previous -
- suivant: Une_figure_EPS -

- -

Exemple d'un document segmenté

-

Ross Moore & Michel Goossens


-
-
- - - - - -
-
-
- -

-Liste des figures -

  1. Deux images EPS

- -

-Liste des tableaux -

  1. Quelques commandes de l'option french - de babel

-
- -

-Référence à figure 1. - -

-Référence à tableau 1. -
-


-


-Bibliographie -

-

1 -
-Adobe Inc. PostScript, manuel de référence - (2ième édition) InterÉditions (France), 1992 -
-
-

- -

-Index -

-
figure -
Une figure EPS -
PostScript -
Une figure EPS -
références -
Bibliographie -
section -
-
figure -
Une figure EPS -
tableau -
Exemple d'un tableau -
-
tableau -
Exemple d'un tableau - -

-
-

-À propos de ce document... -

- Exemple d'un document segmenté

-This document was generated using the -LaTeX2HTML translator Version 99.1 release (March 30, 1999) -

-Copyright © 1993, 1994, 1995, 1996, -Nikos Drakos, -Computer Based Learning Unit, University of Leeds. -
Copyright © 1997, 1998, 1999, -Ross Moore, -Mathematics Department, Macquarie University, Sydney. -

-The command line arguments were:
- latex2html -split 0 -down_url ../ex31/ex31.html -down_title Une_figure_EPS -biblio #BIBLIO ex30 -

-The translation was initiated by Michel Goossens on 1999-03-30


-
-Michel Goossens -
1999-03-30 -
- - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/index.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/index.pl deleted file mode 100644 index 406d89c0350..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/index.pl +++ /dev/null @@ -1,23 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate index original text with physical files. - - -$key = q/références/; -$index{$key} .= q|Bibliographie - \| |; -$noresave{$key} = "$nosave"; - -# LaTeX2HTML 99.1 release (March 30, 1999) -# Printable index-keys from sub_index array. - - -# LaTeX2HTML 99.1 release (March 30, 1999) -# Printable index-keys from printable_key array. - - -$key = q/références/; -$printable_key{$key} = q|références| unless ($printable_key{$key}); -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/internals.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/internals.pl deleted file mode 100644 index 0074f6991b7..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/internals.pl +++ /dev/null @@ -1,10 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate internals original text with physical files. - - -$key = q/BIBLIO/; -$ref_files{$key} = "$dir".q|ex30.html|; -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/labels.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/labels.pl deleted file mode 100644 index 2d5f13bbd03..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/labels.pl +++ /dev/null @@ -1,21 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate labels original text with physical files. - - -$key = q/BIBLIO/; -$external_labels{$key} = "$URL/" . q|ex30.html|; -$noresave{$key} = "$nosave"; - -1; - - -# LaTeX2HTML 99.1 release (March 30, 1999) -# labels from external_latex_labels array. - - -$key = q/BIBLIO/; -$external_latex_labels{$key} = q|2|; -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/sections.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/sections.pl deleted file mode 100644 index d33b319b068..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex30/sections.pl +++ /dev/null @@ -1,36 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate sections original text with physical files. - - -$key = q/0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$section_info{$key} = '0%:%'."$dir".q|ex30.html%:%Exemple d'un document segmenté%:%| unless ($section_info{$key}); -$noresave{$key} = "$nosave"; -$done{"${dir}ex30.html"} = 1; - -$key = q/0 0 0 1 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$section_info{$key} = '3%:%'."$dir".q|ex30.html%:%<#137#>Liste des figures<#137#>%:%| unless ($section_info{$key}); -$noresave{$key} = "$nosave"; -$done{"${dir}ex30.html"} = 1; - -$key = q/0 0 0 2 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$section_info{$key} = '3%:%'."$dir".q|ex30.html%:%<#138#>Liste des tableaux<#138#>%:%| unless ($section_info{$key}); -$noresave{$key} = "$nosave"; -$done{"${dir}ex30.html"} = 1; - -$key = q/0 0 0 6 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$section_info{$key} = '3%:%'."$dir".q|ex30.html%:%<#139#>Bibliographie<#139#>%:%| unless ($section_info{$key}); -$noresave{$key} = "$nosave"; -$done{"${dir}ex30.html"} = 1; - -$key = q/0 0 0 7 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$section_info{$key} = '3%:%'."$dir".q|ex30.html%:%<#141#>Index<#141#>%:%| unless ($section_info{$key}); -$noresave{$key} = "$nosave"; -$done{"${dir}ex30.html"} = 1; - -$key = q/0 0 0 8 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$section_info{$key} = '3%:%'."$dir".q|ex30.html%:%À propos de ce document...%:%| unless ($section_info{$key}); -$noresave{$key} = "$nosave"; -$done{"${dir}ex30.html"} = 1; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31.ptr b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31.ptr deleted file mode 100644 index d7266d00c9a..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31.ptr +++ /dev/null @@ -1,9 +0,0 @@ -\setcounter {lpart}{0} -\setcounter {lsection}{4} -\setcounter {lsubsection}{0} -\setcounter {lsubsubsection}{0} -\setcounter {lparagraph}{0} -\setcounter {lsubparagraph}{0} -\setcounter {equation}{0} -\setcounter {footnote}{0} -\htmlhead {section}{Une figure EPS} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31.tex deleted file mode 100644 index 1f5c97339f3..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31.tex +++ /dev/null @@ -1,27 +0,0 @@ -\begin{htmlonly} -\documentclass{article} -\usepackage{makeidx,html} -\usepackage[T1]{fontenc} -\usepackage[dvips]{graphicx} -\usepackage{francais} -\input ex31.ptr -\end{htmlonly} -\startdocument -\index{section!figure} - -Cette section montre comment inclure une figure -PostScript\cite{bib-PS} dans un document \LaTeX. -La \hyperref{figure}{figure }{}{Fpsfig} -est insérée dans le texte à l'aide de la commande -\verb!\includegraphics{colorcir}!. -\index{figure} -\index{PostScript} -\begin{figure}[h] -\htmlimage{thumbnail=0.4} -\centering - \begin{tabular}{c@{\qquad}c} - \includegraphics[width=3cm]{colorcir} & - \includegraphics[width=3cm]{tac2dim} - \end{tabular} - \caption{Deux images EPS}\label{Fpsfig} -\end{figure} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/Timg1.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/Timg1.gif deleted file mode 100644 index 1326d4c62cd..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/Timg1.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/WARNINGS b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/WARNINGS deleted file mode 100644 index 4fa64c73914..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/WARNINGS +++ /dev/null @@ -1 +0,0 @@ -No implementation found for style `fontenc' diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/contents.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/contents.pl deleted file mode 100644 index 64825ef5ddb..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/contents.pl +++ /dev/null @@ -1,10 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate contents original text with physical files. - - -$key = q/0 0 0 4 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$toc_section_info{$key} = '3%:%'."$dir".q|ex31.html%:%Une figure EPS| unless ($toc_section_info{$key}); -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/ex31.css b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/ex31.css deleted file mode 100644 index 1993b851311..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/ex31.css +++ /dev/null @@ -1,31 +0,0 @@ - -/* Century Schoolbook font is very similar to Computer Modern Math: cmmi */ -.MATH { font-family: "Century Schoolbook", serif; } -.MATH I { font-family: "Century Schoolbook", serif; font-shape: italic } -.BOLDMATH { font-family: "Century Schoolbook", serif; font-weight: bold } - -/* implement both fixed-size and relative sizes */ -SMALL.XTINY { font-size : xx-small } -SMALL.TINY { font-size : x-small } -SMALL.SCRIPTSIZE { font-size : smaller } -SMALL.FOOTNOTESIZE { font-size : small } -SMALL.SMALL { } -BIG.LARGE { } -BIG.XLARGE { font-size : large } -BIG.XXLARGE { font-size : x-large } -BIG.HUGE { font-size : larger } -BIG.XHUGE { font-size : xx-large } - -/* heading styles */ -H1 { } -H2 { } -H3 { } -H4 { } -H5 { } - -/* mathematics styles */ -DIV.displaymath { } /* math displays */ -TD.eqno { } /* equation-number cells */ - - -/* document-specific styles come next */ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/ex31.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/ex31.html deleted file mode 100644 index b9404537d86..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/ex31.html +++ /dev/null @@ -1,90 +0,0 @@ - - - - - -Une figure EPS - - - - - - - - - - - - - - - - -next - -up - -previous - -index -
- suivant: Exemple_d'un_tableau - monter: Exemple_d'un_document_segmenté - précédent: Exemple_d'un_document_segmenté -   Index -
-
- -

-

-Une figure EPS -

- -

-Cette section montre comment inclure une figure -PostScript[1] dans un document LATEX . -La figure -est insérée dans le texte à l'aide de la commande -\includegraphics{colorcir}. - - - -

-
- - - -
Figure 1: -Deux images EPS
\begin{figure}
-\centering \begin{tabular}{c@{\qquad}c}
-\includegraphics[width=3cm]{colorcir}&
-\includegraphics[width=3cm]{tac2dim} \end{tabular} \end{figure}
-

-

-
-Michel Goossens -
1999-03-30 -
- - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/figure.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/figure.pl deleted file mode 100644 index 9d53aec77d7..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/figure.pl +++ /dev/null @@ -1 +0,0 @@ -'
  • Deux images EPS' diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/images.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/images.pl deleted file mode 100644 index c73c4f191be..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/images.pl +++ /dev/null @@ -1,16 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate images original text with physical files. - - -$key = q/{figure}htmlimage{thumbnail=0.4}{centering{tabular{{c@{qquad}c}{includegraphics[]{colorcir}{&{includegraphics[width=3cm]{tac2dim}{tabular{{{{figure};FSF=1.6;AAT/; -$cached_env_img{$key} = q|\begin{figure}
-\centering \begin{tabular}{c@{\qquad}c}
-\includegraphics[width=3cm]{colorcir}&
-\includegraphics[width=3cm]{tac2dim} \end{tabular} \end{figure}|; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/images.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/images.tex deleted file mode 100644 index 3d534cab653..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/images.tex +++ /dev/null @@ -1,136 +0,0 @@ -\batchmode -\documentclass{article} - -\usepackage{makeidx,html} -\usepackage[T1]{fontenc} -\usepackage[dvips]{graphicx} -\usepackage{francais} -\setcounter {lpart}{0}\setcounter {lsection}{4}\setcounter {lsubsection}{0}\setcounter {lsubsubsection}{0}\setcounter {lparagraph}{0}\setcounter {lsubparagraph}{0}\setcounter {equation}{0}\setcounter {footnote}{0}\htmlhead {section}{Une figure EPS} -\usepackage[dvips]{color} -\pagecolor[gray]{.7} - - - -\makeatletter - -\makeatletter -\count@=\the\catcode`\_ \catcode`\_=8 -\newenvironment{tex2html_wrap}{}{} \catcode`\_=\count@ -\newcommand{\renewedcommand}[1]{\expandafter\renewcommand\csname #1\endcsname}% -\makeatother -\let\mathon=$ -\let\mathoff=$ -\ifx\AtBeginDocument\undefined \newcommand{\AtBeginDocument}[1]{}\fi -\newbox\sizebox -\setlength{\hoffset}{0pt}\setlength{\voffset}{0pt} -\addtolength{\textheight}{\footskip}\setlength{\footskip}{0pt} -\addtolength{\textheight}{\topmargin}\setlength{\topmargin}{0pt} -\addtolength{\textheight}{\headheight}\setlength{\headheight}{0pt} -\addtolength{\textheight}{\headsep}\setlength{\headsep}{0pt} -\setlength{\textwidth}{349pt} -\newwrite\lthtmlwrite -\makeatletter -\let\realnormalsize=\normalsize -\global\topskip=2sp -\def\preveqno{}\let\real@float=\@float \let\realend@float=\end@float -\def\@float{\let\@savefreelist\@freelist\real@float} -\def\end@float{\realend@float\global\let\@freelist\@savefreelist} -\let\real@dbflt=\@dbflt \let\end@dblfloat=\end@float -\let\@largefloatcheck=\relax -\let\if@boxedmulticols=\iftrue -\def\@dbflt{\let\@savefreelist\@freelist\real@dbflt} -\def\adjustnormalsize{\def\normalsize{\mathsurround=0pt \realnormalsize - \parindent=0pt\abovedisplayskip=0pt\belowdisplayskip=0pt}% - \def\phantompar{\csname par\endcsname}\normalsize}% -\def\lthtmltypeout#1{{\let\protect\string\immediate\write\lthtmlwrite{#1}}}% -\newcommand\lthtmlhboxmathA{\adjustnormalsize\setbox\sizebox=\hbox\bgroup\kern.05em }% -\newcommand\lthtmlhboxmathB{\adjustnormalsize\setbox\sizebox=\hbox to\hsize\bgroup\hfill }% -\newcommand\lthtmlvboxmathA{\adjustnormalsize\setbox\sizebox=\vbox\bgroup % - \let\ifinner=\iffalse }% -\newcommand\lthtmlboxmathZ{\@next\next\@currlist{}{\def\next{\voidb@x}}% - \expandafter\box\next\egroup}% -\newcommand\lthtmlmathtype[1]{\def\lthtmlmathenv{#1}}% -\newcommand\lthtmllogmath{\lthtmltypeout{l2hSize % -:\lthtmlmathenv:\the\ht\sizebox::\the\dp\sizebox::\the\wd\sizebox.\preveqno}}% -\newcommand\lthtmlfigureA[1]{\let\@savefreelist\@freelist - \lthtmlmathtype{#1}\lthtmlvboxmathA}% -\newcommand\lthtmlpictureA[1]{\let\@savefreelist\@freelist - \lthtmlmathtype{#1}\lthtmlhboxmathB}% -\newcommand\lthtmlpictureZ[1]{\hfill\lthtmlfigureZ}% -\newcommand\lthtmlfigureZ{\lthtmlboxmathZ\lthtmllogmath\copy\sizebox - \global\let\@freelist\@savefreelist}% -\newcommand\lthtmldisplayA[1]{\lthtmlmathtype{#1}\lthtmlvboxmathA}% -\newcommand\lthtmldisplayB[1]{\edef\preveqno{(\theequation)}% - \lthtmldisplayA{#1}\let\@eqnnum\relax}% -\newcommand\lthtmldisplayZ{\lthtmlboxmathZ\lthtmllogmath\lthtmlsetmath}% -\newcommand\lthtmlinlinemathA[1]{\lthtmlmathtype{#1}\lthtmlhboxmathA - \vrule height1.5ex width0pt }% -\newcommand\lthtmlinlineA[1]{\lthtmlmathtype{#1}\lthtmlhboxmathA}% -\newcommand\lthtmlinlineZ{\egroup\expandafter\ifdim\dp\sizebox>0pt % - \expandafter\centerinlinemath\fi\lthtmllogmath\lthtmlsetinline} -\newcommand\lthtmlinlinemathZ{\egroup\expandafter\ifdim\dp\sizebox>0pt % - \expandafter\centerinlinemath\fi\lthtmllogmath\lthtmlsetmath} -\newcommand\lthtmlindisplaymathZ{\egroup % - \centerinlinemath\lthtmllogmath\lthtmlsetmath} -\def\lthtmlsetinline{\hbox{\vrule width.1em\kern-.05em\vtop{\vbox{% - \kern.1em\copy\sizebox}\ifdim\dp\sizebox>0pt\kern.1em\else\kern.3pt\fi - \ifdim\hsize>\wd\sizebox \hrule depth1pt\fi}}} -\def\lthtmlsetmath{\hbox{\vrule width.1em\kern-.05em\vtop{\vbox{% - \kern.1em\kern0.8 pt\hbox{\hglue.17em\copy\sizebox\hglue0.8 pt}}\kern.3pt% - \ifdim\dp\sizebox>0pt\kern.1em\fi \kern0.8 pt% - \ifdim\hsize>\wd\sizebox \hrule depth1pt\fi}}} -\def\centerinlinemath{% - \dimen1=\ifdim\ht\sizebox<\dp\sizebox \dp\sizebox\else\ht\sizebox\fi - \advance\dimen1by.5pt \vrule width0pt height\dimen1 depth\dimen1 - \dp\sizebox=\dimen1\ht\sizebox=\dimen1\relax} - -\def\lthtmlcheckvsize{\ifdim\ht\sizebox<\vsize - \ifdim\wd\sizebox<\hsize\expandafter\hfill\fi \expandafter\vfill - \else\expandafter\vss\fi}% -\providecommand{\selectlanguage}[1]{}% -\makeatletter \tracingstats = 1 - - -\begin{document} -\pagestyle{empty}\thispagestyle{empty}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength hsize=\the\hsize}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength vsize=\the\vsize}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength hoffset=\the\hoffset}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength voffset=\the\voffset}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength topmargin=\the\topmargin}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength topskip=\the\topskip}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength headheight=\the\headheight}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength headsep=\the\headsep}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength parskip=\the\parskip}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength oddsidemargin=\the\oddsidemargin}\lthtmltypeout{}% -\makeatletter -\if@twoside\lthtmltypeout{latex2htmlLength evensidemargin=\the\evensidemargin}% -\else\lthtmltypeout{latex2htmlLength evensidemargin=\the\oddsidemargin}\fi% -\lthtmltypeout{}% -\makeatother -\setcounter{page}{1} -\onecolumn - -% !!! IMAGES START HERE !!! - -\setcounter{part}{0} -\setcounter{section}{4} -\setcounter{subsection}{0} -\setcounter{subsubsection}{0} -\setcounter{paragraph}{0} -\setcounter{subparagraph}{0} -\setcounter{equation}{0} -\setcounter{footnote}{0} -{\newpage\clearpage -\lthtmlfigureA{figure32}% -\begin{figure} -\htmlimage{thumbnail=0.4} -\centering \begin{tabular}{c@{\qquad}c} - \includegraphics[width=3cm]{colorcir}& - \includegraphics[width=3cm]{tac2dim} \end{tabular} - \end{figure}% -\lthtmlfigureZ -\lthtmlcheckvsize\clearpage} - - -\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/img1.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/img1.gif deleted file mode 100644 index 224cf5785c7..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/img1.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/index.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/index.pl deleted file mode 100644 index 800c5e8a9a1..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/index.pl +++ /dev/null @@ -1,49 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate index original text with physical files. - - -$key = q/sectionfigure/; -$index{$key} .= q|Une figure EPS - \| |; -$noresave{$key} = "$nosave"; - -$key = q/figure/; -$index{$key} .= q|Une figure EPS - \| |; -$noresave{$key} = "$nosave"; - -$key = q/postscript/; -$index{$key} .= q|Une figure EPS - \| |; -$noresave{$key} = "$nosave"; - -# LaTeX2HTML 99.1 release (March 30, 1999) -# Printable index-keys from sub_index array. - - -$key = q/section/; -$sub_index{$key} .= q|sectionfigure|; -$noresave{$key} = "$nosave"; - -# LaTeX2HTML 99.1 release (March 30, 1999) -# Printable index-keys from printable_key array. - - -$key = q/sectionfigure/; -$printable_key{$key} = q|figure| unless ($printable_key{$key}); -$noresave{$key} = "$nosave"; - -$key = q/figure/; -$printable_key{$key} = q|figure| unless ($printable_key{$key}); -$noresave{$key} = "$nosave"; - -$key = q/postscript/; -$printable_key{$key} = q|PostScript| unless ($printable_key{$key}); -$noresave{$key} = "$nosave"; - -$key = q/section/; -$printable_key{$key} = q|section| unless ($printable_key{$key}); -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/internals.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/internals.pl deleted file mode 100644 index e3a9dff2e90..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/internals.pl +++ /dev/null @@ -1,14 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate internals original text with physical files. - - -$key = q/cite_bib-PS/; -$ref_files{$key} = "$dir".q|../ex30/ex30.html|; -$noresave{$key} = "$nosave"; - -$key = q/Fpsfig/; -$ref_files{$key} = "$dir".q|ex31.html|; -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/labels.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/labels.pl deleted file mode 100644 index 2c0c67b85fe..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/labels.pl +++ /dev/null @@ -1,33 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate labels original text with physical files. - - -$key = q/cite_bib-PS/; -$external_labels{$key} = "$URL/" . q|../ex30/ex30.html|; -$noresave{$key} = "$nosave"; - -$key = q/Fpsfig/; -$external_labels{$key} = "$URL/" . q|ex31.html|; -$noresave{$key} = "$nosave"; - -1; - - -# LaTeX2HTML 99.1 release (March 30, 1999) -# labels from external_latex_labels array. - - -$key = q/BIBLIO/; -$external_latex_labels{$key} = q|2|; -$noresave{$key} = "$nosave"; - -$key = q/tab-exa/; -$external_latex_labels{$key} = q|1|; -$noresave{$key} = "$nosave"; - -$key = q/Fpsfig/; -$external_latex_labels{$key} = q|1|; -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/sections.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/sections.pl deleted file mode 100644 index 61916f95c0a..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex31/sections.pl +++ /dev/null @@ -1,11 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate sections original text with physical files. - - -$key = q/0 0 0 4 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$section_info{$key} = '3%:%'."$dir".q|ex31.html%:%Une figure EPS%:%| unless ($section_info{$key}); -$noresave{$key} = "$nosave"; -$done{"${dir}ex31.html"} = 1; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32.ptr b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32.ptr deleted file mode 100644 index fd7cd38344c..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32.ptr +++ /dev/null @@ -1,9 +0,0 @@ -\setcounter {lpart}{0} -\setcounter {lsection}{5} -\setcounter {lsubsection}{0} -\setcounter {lsubsubsection}{0} -\setcounter {lparagraph}{0} -\setcounter {lsubparagraph}{0} -\setcounter {equation}{0} -\setcounter {footnote}{0} -\htmlhead {section}{Exemple d'un tableau} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32.tex deleted file mode 100644 index 293d66f4650..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32.tex +++ /dev/null @@ -1,27 +0,0 @@ -\begin{htmlonly} -\usepackage{makeidx,html} -\usepackage{francais} -\input ex32.ptr -\end{htmlonly} -\newcommand{\Lcs}[1]{\texttt{\symbol{'134}#1}} -\startdocument -\index{section!tableau} - -Le \hyperref{tableau}{tableau }{}{tab-exa} -montre l'utilisation de l'environnement \texttt{table}. -\begin{table}[h] -\centering - \begin{tabular}{cccccc} - \Lcs{primo} & \primo & \Lcs{secundo} & \secundo - & \Lcs{tertio} & \tertio \\ - \Lcs{quatro} & \quatro& 1\Lcs{ier} & 1\ier - & 1\Lcs{iere} & 1\iere \\ - \Lcs{fprimo)}&\fprimo)& \Lcs{No} 10 & \No 10 - & \Lcs{no} 15 & \no 15 \\ - \Lcs{og} a \Lcs{fg}&\og a \fg&3\Lcs{ieme}&3\ieme - & 10\Lcs{iemes}& 10\iemes - \end{tabular} -\caption{Quelques commandes de l'option \texttt{french} - de \texttt{babel}}\label{tab-exa} -\index{tableau} -\end{table} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/contents.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/contents.pl deleted file mode 100644 index 38110d910b2..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/contents.pl +++ /dev/null @@ -1,10 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate contents original text with physical files. - - -$key = q/0 0 0 5 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$toc_section_info{$key} = '3%:%'."$dir".q|ex32.html%:%Exemple d'un tableau| unless ($toc_section_info{$key}); -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/ex32.css b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/ex32.css deleted file mode 100644 index 1993b851311..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/ex32.css +++ /dev/null @@ -1,31 +0,0 @@ - -/* Century Schoolbook font is very similar to Computer Modern Math: cmmi */ -.MATH { font-family: "Century Schoolbook", serif; } -.MATH I { font-family: "Century Schoolbook", serif; font-shape: italic } -.BOLDMATH { font-family: "Century Schoolbook", serif; font-weight: bold } - -/* implement both fixed-size and relative sizes */ -SMALL.XTINY { font-size : xx-small } -SMALL.TINY { font-size : x-small } -SMALL.SCRIPTSIZE { font-size : smaller } -SMALL.FOOTNOTESIZE { font-size : small } -SMALL.SMALL { } -BIG.LARGE { } -BIG.XLARGE { font-size : large } -BIG.XXLARGE { font-size : x-large } -BIG.HUGE { font-size : larger } -BIG.XHUGE { font-size : xx-large } - -/* heading styles */ -H1 { } -H2 { } -H3 { } -H4 { } -H5 { } - -/* mathematics styles */ -DIV.displaymath { } /* math displays */ -TD.eqno { } /* equation-number cells */ - - -/* document-specific styles come next */ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/ex32.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/ex32.html deleted file mode 100644 index 6b7c6815f82..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/ex32.html +++ /dev/null @@ -1,111 +0,0 @@ - - - - - -Exemple d'un tableau - - - - - - - - - - - - - - - - -next - -up - -previous - -index -
    - suivant: Références - monter: Exemple_d'un_document_segmenté - précédent: Une_figure_EPS -   Index -
    -
    - -

    -

    -Exemple d'un tableau -

    - - -

    -Le tableau -montre l'utilisation de l'environnement table. -

    -
    - - - -
    Tableau 1: -Quelques commandes de l'option french - de babel
    -
    - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
    \primo1o\secundo2o\tertio3o
    \quatro4o1\ier1er1\iere1re
    \fprimo)1o)\No 10No10\no 15no15
    \og a \fg«a »3\ieme3e10\iemes10es
    - -
    -

    -
    -

    -
    -Michel Goossens -
    1999-03-30 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/index.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/index.pl deleted file mode 100644 index 9b32933d9ff..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/index.pl +++ /dev/null @@ -1,40 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate index original text with physical files. - - -$key = q/sectiontableau/; -$index{$key} .= q|Exemple d'un tableau - \| |; -$noresave{$key} = "$nosave"; - -$key = q/tableau/; -$index{$key} .= q|Exemple d'un tableau - \| |; -$noresave{$key} = "$nosave"; - -# LaTeX2HTML 99.1 release (March 30, 1999) -# Printable index-keys from sub_index array. - - -$key = q/section/; -$sub_index{$key} .= q|sectiontableau|; -$noresave{$key} = "$nosave"; - -# LaTeX2HTML 99.1 release (March 30, 1999) -# Printable index-keys from printable_key array. - - -$key = q/sectiontableau/; -$printable_key{$key} = q|tableau| unless ($printable_key{$key}); -$noresave{$key} = "$nosave"; - -$key = q/section/; -$printable_key{$key} = q|section| unless ($printable_key{$key}); -$noresave{$key} = "$nosave"; - -$key = q/tableau/; -$printable_key{$key} = q|tableau| unless ($printable_key{$key}); -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/internals.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/internals.pl deleted file mode 100644 index 0c2e1c5a4ee..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/internals.pl +++ /dev/null @@ -1,10 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate internals original text with physical files. - - -$key = q/tab-exa/; -$ref_files{$key} = "$dir".q|ex32.html|; -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/labels.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/labels.pl deleted file mode 100644 index 33b8d26526d..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/labels.pl +++ /dev/null @@ -1,29 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate labels original text with physical files. - - -$key = q/tab-exa/; -$external_labels{$key} = "$URL/" . q|ex32.html|; -$noresave{$key} = "$nosave"; - -1; - - -# LaTeX2HTML 99.1 release (March 30, 1999) -# labels from external_latex_labels array. - - -$key = q/BIBLIO/; -$external_latex_labels{$key} = q|2|; -$noresave{$key} = "$nosave"; - -$key = q/tab-exa/; -$external_latex_labels{$key} = q|1|; -$noresave{$key} = "$nosave"; - -$key = q/Fpsfig/; -$external_latex_labels{$key} = q|1|; -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/sections.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/sections.pl deleted file mode 100644 index 300a790077a..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/sections.pl +++ /dev/null @@ -1,11 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate sections original text with physical files. - - -$key = q/0 0 0 5 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0/; -$section_info{$key} = '3%:%'."$dir".q|ex32.html%:%Exemple d'un tableau%:%| unless ($section_info{$key}); -$noresave{$key} = "$nosave"; -$done{"${dir}ex32.html"} = 1; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/table.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/table.pl deleted file mode 100644 index a9598937fb0..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex32/table.pl +++ /dev/null @@ -1,2 +0,0 @@ -'
  • Quelques commandes de l\'option french - de babel' diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex3bib.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex3bib.tex deleted file mode 100644 index 12e197babf2..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/ex3bib.tex +++ /dev/null @@ -1,6 +0,0 @@ -\begin{thebibliography}{99} -\label{BIBLIO}\index{références} -\bibitem{bib-PS} -Adobe Inc. \emph{PostScript, manuel de référence - (2ième édition)} InterÉditions (France), 1992 -\end{thebibliography} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa.dvi b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa.dvi deleted file mode 100644 index e2d87ea688c..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa.dvi and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa.tex deleted file mode 100644 index 817ffbe7f1d..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa.tex +++ /dev/null @@ -1,62 +0,0 @@ -\documentclass{article} -\usepackage{graphicx} -\usepackage{francais} -\usepackage{makeidx} -\newcommand{\Lcs}[1]{\texttt{\symbol{'134}#1}} -\makeindex -\title{Exemple d'un article en fran\c{c}ais} -\author{Michel Goossens} -\begin{document} -\maketitle -\tableofcontents -\listoffigures -\listoftables -\section{Une figure EPS} -\index{section} -Cette section montre comment inclure une figure PostScript\cite{bib-PS} -dans un document \LaTeX. La figure~\ref{Fpsfig} -est ins\'er\'ee dans le texte \`a l'aide de la commande - \verb!\includegraphics{colorcir.eps}!. -\index{figure} -\index{PostScript} -\begin{figure} - \begin{center} - \begin{tabular}{c@{\qquad}c} - \includegraphics[width=3cm]{colorcir} & - \includegraphics[width=3cm]{tac2dim} - \end{tabular} - \end{center} - \caption{Deux images EPS} - \label{Fpsfig} -\end{figure} - -\section{Exemple d'un tableau} - -Le tableau~\ref{tab:exa} \`a la page \pageref{tab:exa} -montre l'utilisation de l'environnement \texttt{table}. - -\begin{table} - \begin{center} - \begin{tabular}{cccccc} - \Lcs{primo} & \primo & \Lcs{secundo} & \secundo & \Lcs{tertio} & \tertio \\ - \Lcs{quatro} & \quatro& 1\Lcs{ier} & 1\ier & 1\Lcs{iere} & 1\iere \\ - \Lcs{fprimo)}&\fprimo)& \Lcs{No} 10 & \No 10 & \Lcs{no} 15 & \no 15 \\ - \Lcs{og} a \Lcs{fg}&\og a \fg&3\Lcs{ieme}&3\ieme & 10\Lcs{iemes}& 10\iemes - \end{tabular} - \end{center} - \caption{Quelques commandes de l'option \texttt{francais} de \texttt{babel}} - \label{tab:exa} - \index{tableau} -\end{table} - -\begin{thebibliography}{99} -\index{r\'ef\'erences} -\bibitem{bib-PS} -Adobe Inc. -\emph{PostScript, manuel de r\'ef\'erence (2\ieme \'edition)} -Inter\'Editions (France), 1992 -\end{thebibliography} -\printindex -\index{index} -\end{document} -% End of document. diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/images.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/images.pl deleted file mode 100644 index 5b93bd63d0a..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/images.pl +++ /dev/null @@ -1,18 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate images original text with physical files. - - -$key = q/includegraphics[width=3cm]{tac2dim};AAT/; -$cached_env_img{$key} = q|\includegraphics [width=3cm]{tac2dim}|; - -$key = q/includegraphics[width=3cm]{colorcir};AAT/; -$cached_env_img{$key} = q|\includegraphics [width=3cm]{colorcir}|; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/images.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/images.tex deleted file mode 100644 index e02d4a8d173..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/images.tex +++ /dev/null @@ -1,132 +0,0 @@ -\batchmode -\documentclass{article} - -\usepackage{graphicx} -\usepackage{francais} -\usepackage{makeidx}% -\providecommand{\Lcs}[1]{\texttt{\symbol{'134}#1}}\makeindex -\title{Exemple d'un article en fran\c{c}ais} -\author {Michel Goossens} -\usepackage[dvips]{color} -\pagecolor[gray]{.7} - - - -\makeatletter - -\makeatletter -\count@=\the\catcode`\_ \catcode`\_=8 -\newenvironment{tex2html_wrap}{}{} \catcode`\_=\count@ -\newcommand{\renewedcommand}[1]{\expandafter\renewcommand\csname #1\endcsname}% -\makeatother -\let\mathon=$ -\let\mathoff=$ -\ifx\AtBeginDocument\undefined \newcommand{\AtBeginDocument}[1]{}\fi -\newbox\sizebox -\setlength{\hoffset}{0pt}\setlength{\voffset}{0pt} -\addtolength{\textheight}{\footskip}\setlength{\footskip}{0pt} -\addtolength{\textheight}{\topmargin}\setlength{\topmargin}{0pt} -\addtolength{\textheight}{\headheight}\setlength{\headheight}{0pt} -\addtolength{\textheight}{\headsep}\setlength{\headsep}{0pt} -\setlength{\textwidth}{349pt} -\newwrite\lthtmlwrite -\makeatletter -\let\realnormalsize=\normalsize -\global\topskip=2sp -\def\preveqno{}\let\real@float=\@float \let\realend@float=\end@float -\def\@float{\let\@savefreelist\@freelist\real@float} -\def\end@float{\realend@float\global\let\@freelist\@savefreelist} -\let\real@dbflt=\@dbflt \let\end@dblfloat=\end@float -\let\@largefloatcheck=\relax -\let\if@boxedmulticols=\iftrue -\def\@dbflt{\let\@savefreelist\@freelist\real@dbflt} -\def\adjustnormalsize{\def\normalsize{\mathsurround=0pt \realnormalsize - 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-% !!! IMAGES START HERE !!! - -\stepcounter{section} -{\newpage\clearpage -\lthtmlpictureA{tex2html_wrap106}% -\includegraphics [width=3cm]{colorcir}% -\lthtmlpictureZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlpictureA{tex2html_wrap108}% -\includegraphics [width=3cm]{tac2dim}% -\lthtmlpictureZ -\lthtmlcheckvsize\clearpage} - -\stepcounter{section} - -\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/img1.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/img1.gif deleted file mode 100644 index 4f4addd2785..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/img1.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/img2.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/img2.gif deleted file mode 100644 index 7b9dcaf127d..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/img2.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/index.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/index.html deleted file mode 100644 index f03e4818bce..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/index.html +++ /dev/null @@ -1,84 +0,0 @@ - - - - - -Exemple d'un article en français - - - - - - - - - - - - - - - - - -next -up -previous - -contents - -index -
    - suivant: Table des matières -   Table des matières -   Index -
    -
    - -

    Exemple d'un article en français

    -

    Michel Goossens

    -

    - - - - - -

    -
    -Michel Goossens -
    1999-03-31 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/internals.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/internals.pl deleted file mode 100644 index b437e91cbec..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/internals.pl +++ /dev/null @@ -1,18 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate internals original text with physical files. - - -$key = q/cite_bib-PS/; -$ref_files{$key} = "$dir".q|node6.html|; -$noresave{$key} = "$nosave"; - -$key = q/Fpsfig/; -$ref_files{$key} = "$dir".q|node4.html|; -$noresave{$key} = "$nosave"; - -$key = q/tab:exa/; -$ref_files{$key} = "$dir".q|node5.html|; -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/l2hexa.css b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/l2hexa.css deleted file mode 100644 index 1993b851311..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/l2hexa.css +++ /dev/null @@ -1,31 +0,0 @@ - -/* Century Schoolbook font is very similar to Computer Modern Math: cmmi */ -.MATH { font-family: "Century Schoolbook", serif; } -.MATH I { font-family: "Century Schoolbook", serif; font-shape: italic } -.BOLDMATH { font-family: "Century Schoolbook", serif; font-weight: bold } - -/* implement both fixed-size and relative sizes */ -SMALL.XTINY { font-size : xx-small } -SMALL.TINY { font-size : x-small } -SMALL.SCRIPTSIZE { font-size : smaller } -SMALL.FOOTNOTESIZE { font-size : small } -SMALL.SMALL { } -BIG.LARGE { } -BIG.XLARGE { font-size : large } -BIG.XXLARGE { font-size : x-large } -BIG.HUGE { font-size : larger } -BIG.XHUGE { font-size : xx-large } - -/* heading styles */ -H1 { } -H2 { } -H3 { } -H4 { } -H5 { } - -/* mathematics styles */ -DIV.displaymath { } /* math displays */ -TD.eqno { } /* equation-number cells */ - - -/* document-specific styles come next */ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/l2hexa.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/l2hexa.html deleted file mode 100644 index f03e4818bce..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/l2hexa.html +++ /dev/null @@ -1,84 +0,0 @@ - - - - - -Exemple d'un article en français - - - - - - - - - - - - - - - - - -next -up -previous - -contents - -index -
    - suivant: Table des matières -   Table des matières -   Index -
    -
    - -

    Exemple d'un article en français

    -

    Michel Goossens

    -

    - - - - - -

    -
    -Michel Goossens -
    1999-03-31 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/labels.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/labels.pl deleted file mode 100644 index 7a800316923..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/labels.pl +++ /dev/null @@ -1,33 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate labels original text with physical files. - - -$key = q/cite_bib-PS/; -$external_labels{$key} = "$URL/" . q|node6.html|; -$noresave{$key} = "$nosave"; - -$key = q/Fpsfig/; -$external_labels{$key} = "$URL/" . q|node4.html|; -$noresave{$key} = "$nosave"; - -$key = q/tab:exa/; -$external_labels{$key} = "$URL/" . q|node5.html|; -$noresave{$key} = "$nosave"; - -1; - - -# LaTeX2HTML 99.1 release (March 30, 1999) -# labels from external_latex_labels array. - - -$key = q/Fpsfig/; -$external_latex_labels{$key} = q|1|; -$noresave{$key} = "$nosave"; - -$key = q/tab:exa/; -$external_latex_labels{$key} = q|1|; -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node1.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node1.html deleted file mode 100644 index 830a5ca9d57..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node1.html +++ /dev/null @@ -1,88 +0,0 @@ - - - - - -Table des matières - - - - - - - - - - - - - - - - - - - - -next - -up - -previous - -index -
    - suivant: Liste des figures - monter: Exemple d'un article en - précédent: Exemple d'un article en -   Index -
    -
    - -
    - -

    -Table des matières -

    - - - - -

    -
    -Michel Goossens -
    1999-03-31 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node2.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node2.html deleted file mode 100644 index 7bd56f893d5..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node2.html +++ /dev/null @@ -1,77 +0,0 @@ - - - - - -Liste des figures - - - - - - - - - - - - - - - - - - - - -next - -up - -previous - -contents - -index -
    - suivant: Liste des tableaux - monter: Exemple d'un article en - précédent: Table des matières -   Table des matières -   Index -
    -
    - -
    - -

    -Liste des figures -

      -
    1. Deux images EPS
    -

    -
    -Michel Goossens -
    1999-03-31 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node3.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node3.html deleted file mode 100644 index 41e0a771c78..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node3.html +++ /dev/null @@ -1,77 +0,0 @@ - - - - - -Liste des tableaux - - - - - - - - - - - - - - - - - - - - -next - -up - -previous - -contents - -index -
    - suivant: Une figure EPS - monter: Exemple d'un article en - précédent: Liste des figures -   Table des matières -   Index -
    -
    - -
    - -

    -Liste des tableaux -

      -
    1. Quelques commandes de l'option francais de babel
    -

    -
    -Michel Goossens -
    1999-03-31 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node4.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node4.html deleted file mode 100644 index b1ed0f3f45c..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node4.html +++ /dev/null @@ -1,115 +0,0 @@ - - - - - -Une figure EPS - - - - - - - - - - - - - - - - - - - - -next - -up - -previous - -contents - -index -
    - suivant: Exemple d'un tableau - monter: Exemple d'un article en - précédent: Liste des tableaux -   Table des matières -   Index -
    -
    - - -

    - -
    -Une figure EPS -

    -Cette section montre comment inclure une figure PostScript[1] -dans un document LATEX . La figure 1 -est insérée dans le texte à l'aide de la commande - \includegraphics{colorcir.eps}. - - - -

    -
    - - - -
    Figure 1: -Deux images EPS
    -
    - - - - -
    - -\includegraphics [width=3cm]{colorcir}         - -\includegraphics [width=3cm]{tac2dim}
    -
    -

    - -

    -


    -
    -Michel Goossens -
    1999-03-31 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node5.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node5.html deleted file mode 100644 index 4826c728c04..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node5.html +++ /dev/null @@ -1,128 +0,0 @@ - - - - - -Exemple d'un tableau - - - - - - - - - - - - - - - - - - - - -next - -up - -previous - -contents - -index -
    - suivant: Bibliographie - monter: Exemple d'un article en - précédent: Une figure EPS -   Table des matières -   Index -
    -
    - - -

    -Exemple d'un tableau -

    - -

    -Le tableau 1 à la page [*] -montre l'utilisation de l'environnement table. - -

    - -

    -
    - - - -
    Tableau 1: -Quelques commandes de l'option francais de babel
    -
    - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
    \primo1o\secundo2o\tertio3o
    \quatro4o1\ier1er1\iere1re
    \fprimo)1o)\No 10No10\no 15no15
    \og a \fg«a »3\ieme3e10\iemes10es
    -
    - - -
    -

    -
    - -

    -


    -
    -Michel Goossens -
    1999-03-31 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node6.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node6.html deleted file mode 100644 index 8a6828f88c9..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node6.html +++ /dev/null @@ -1,78 +0,0 @@ - - - - - -Bibliographie - - - - - - - - - - - - - - - - - - - - -next - -up - -previous - -contents - -index -
    - suivant: Index - monter: Exemple d'un article en - précédent: Exemple d'un tableau -   Table des matières -   Index -

    - - -


    -Bibliographie -

    -

    1 -
    -Adobe Inc. -PostScript, manuel de référence (2eédition) -InterÉditions (France), 1992 -


    -
    -Michel Goossens -
    1999-03-31 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node7.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node7.html deleted file mode 100644 index 7bdbe540ef0..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node7.html +++ /dev/null @@ -1,85 +0,0 @@ - - - - - -Index - - - - - - - - - - - - - - - - - - - - -next - -up - -previous - -contents -
    - suivant: À propos de ce - monter: Exemple d'un article en - précédent: Bibliographie -   Table des matières -
    -
    - -
    - -

    - -
    -Index -

    -
    figure -
    Une figure EPS -
    index -
    Index -
    PostScript -
    Une figure EPS -
    références -
    Bibliographie -
    section -
    Une figure EPS -
    tableau -
    Exemple d'un tableau - -
    -

    -
    -Michel Goossens -
    1999-03-31 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node8.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node8.html deleted file mode 100644 index b04bea52df8..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/l2hexa/node8.html +++ /dev/null @@ -1,84 +0,0 @@ - - - - - -À propos de ce document... - - - - - - - - - - - - - - - - - -next - -up - -previous - -contents - -index -
    - monter: Exemple d'un article en - précédent: Index -   Table des matières -   Index -
    -
    - - -

    -À propos de ce document... -

    - Exemple d'un article en français

    -This document was generated using the -LaTeX2HTML translator Version 99.1 release (March 30, 1999) -

    -Copyright © 1993, 1994, 1995, 1996, -Nikos Drakos, -Computer Based Learning Unit, University of Leeds. -
    -Copyright © 1997, 1998, 1999, -Ross Moore, -Mathematics Department, Macquarie University, Sydney. -

    -The command line arguments were:
    - latex2html l2hexa -

    -The translation was initiated by Michel Goossens on 1999-03-31 -


    -
    -Michel Goossens -
    1999-03-31 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/myinit.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/myinit.pl deleted file mode 100644 index b24da780bf5..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/myinit.pl +++ /dev/null @@ -1,8 +0,0 @@ -# File myinit.pl -$ADDRESS = "Michel Goossens
    " . - "Division IT
    " . - "Tél. 767.5028
    " . - "$address_data[1]
    "; -$MAX_SPLIT_DEPTH = 0; # do not split document -$NO_NAVIGATION = 1; # no navigation panel -1; # Mandatory last line diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS.css b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS.css deleted file mode 100644 index daee915b4dd..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS.css +++ /dev/null @@ -1,4 +0,0 @@ -H2 { border : 2pt solid brown ; color : maroon ; padding : 5pt } -TD.eqno {color : green ; fontweight : 700 } /* equation-number cells */ -TABLE.subequations { background-color : #E0E0E0 ; } -P { line-height : 18pt ; } diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS.dvi b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS.dvi deleted file mode 100644 index f960f94f533..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS.dvi and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS.tex deleted file mode 100644 index 7a0f0ea4629..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS.tex +++ /dev/null @@ -1,54 +0,0 @@ -\documentclass[a4paper,twoside]{article} -\usepackage{html} -\usepackage{amsmath} - -\renewcommand{\d}{\partial}\providecommand{\bm}[1]{\mathbf{#1}} -\providecommand{\Range}{\mathcal{R}}\providecommand{\Ker}{\mathcal{N}} -\providecommand{\Quat}{\vec{\mathbf{Q}}} - -\newcommand{\StAndrews}{\htmlurl{http://www-groups.dcs.st-and.ac.uk/~history}}% -\newcommand{\Pythagorians}{\htmladdnormallink - {Pythagorians}{\StAndrews/Mathematicians/Pythagoras.html}} -\newcommand{\Fermat}{\htmladdnormallink - {Fermat, c.1637}{\StAndrews/HistTopics/Fermat's_last_theorem.html}} -\newcommand{\Wiles}{\htmladdnormallink - {Wiles, 1995}{\htmlurl{http://www.pbs.org:80/wgbh/nova/proof}}} - -\begin{document} -\htmlhead[center]{section}{Math examples} -\begin{eqnarray} - \phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty} - \exp \left( u \ln u + \lambda u \right ) du \hspace{1cm}\mbox{for } c \geq 0 \\ - \lambda & = & \frac{\epsilon -\bar{\epsilon} }{\xi} - - \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}} \\ - \gamma & = & 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)} \\ - \gamma' & = & 0.422784\dots = 1 - \gamma \\ - \epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss} -\end{eqnarray} - -Since~\eqref{eqn:stress-sr} or~\eqref{gdef} should hold for arbitrary $\delta\bm{c}$% --vectors, it is clear that $\Ker(A) = \Range(B)$ and that when $y=B(x)$ one has...\\ -...the \Pythagorians{} knew infinitely many solutions in integers to $a^2+b^2=c^2$. -That no non-trivial integer solutions exist for $a^n+b^n=c^n$ with integers $n>2$ has long -been suspected (\Fermat). Only during the current decade has this been proved (\Wiles). - -\begin{eqnarray}\label{eqn:stress-sr} - V \bm{\pi}^{sr} & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i - + \sum_i \sum_{j>i} \bm{R}_{ij} \bm{F}_{ij}\right> \\ \nonumber - & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i - + \sum_{i}\sum_{j>i}\sum_\alpha\sum_\beta \bm{r}_{i\alpha j\beta}\bm{f}_{i\alpha j\beta} - - \sum_i \sum_\alpha \bm{p}_{i\alpha} \bm{f}_{i\alpha} \right> -\end{eqnarray} - -\begin{subequations}\label{bgdefs} -\begin{align} B_{ij}^\alpha & = - \left(B_{ij}^\alpha\right)_0 + \left(B_{ij}^\alpha\right)_a \label{bdef} \\ - \left(B_{ij}^\alpha\right)_0 & = \frac{1}{2}\left(\frac{\d N_i^\alpha}{\d X_j} - + \frac{\d N_j^\alpha} {\d X_i} \right) \label{b0def} \\ - \left(B_{ij}^\alpha\right)_a & = H_{ij}^{\alpha \beta} a^\beta \label{budef} \\ - H_{ij}^{\alpha \beta} & = - \frac{1}{2}\left( \frac{\d N_k^\alpha}{\d X_i} \frac{\d N_k^\beta}{\d X_j} - + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right) \label{gdef} -\end{align} -\end{subequations} -\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS/WARNINGS b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS/WARNINGS deleted file mode 100644 index 9d1d9f764ee..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS/WARNINGS +++ /dev/null @@ -1,2 +0,0 @@ - -redefining command \d diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS/images.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS/images.pl deleted file mode 100644 index 9a62f68699c..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS/images.pl +++ /dev/null @@ -1,139 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate images original text with physical files. - - -$key = q/displaystylefrac{epsilon-bar{epsilon}}{xi}-gamma'-beta^2-lnfrac{xi}{E_{{rm{max}};MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \frac{\epsilon -\bar{\epsilon} }{\xi}
-- \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}}$|; - -$key = q/a^2+b^2=c^2;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ a^2+b^2=c^2$|; - -$key = q/n>2;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ n>2$|; - -$key = q/{subequations}align{B_{ij}^alpha=left(B_{ij}^alpharight)_0+left(B_{ij}}{{d{X_i}frac{{d{N_k^alpha}{{d{X_j}right)align{{subequations};MSF=1.6;TAGS=R;AAT/; -$cached_env_img{$key} = q|\begin{subequations}\begin{align}B_{ij}^\alpha & = \left(B_{ij}^\alpha\right)_0 ...
-...\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right)\end{align}\end{subequations}|; - -$key = q/y=B(x);MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ y=B(x)$|; - -$key = q/displaystyle=;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle =$|; - -$key = q/mathcal{N}(A)=mathcal{R}(B);MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ \mathcal{N}(A) = \mathcal{R}(B)$|; - -$key = q/displaystylelambda;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \lambda$|; - -$key = q/displaystyle0.577215dotsmathrm{hspace{5mm}(Euler'sconstant)};MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)}$|; - -$key = q/displaystylegamma;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \gamma$|; - -$key = q/displaystylelefti}mathbf{R}_{ij}mathbf{F}_{ij}right>;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \left< \sum_i M_i \mathbf{V}_i \mathbf{V}_i
-+ \sum_i \sum_{j>i} \mathbf{R}_{ij} \mathbf{F}_{ij}\right>$|; - -$key = q/displaystylegamma';MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \gamma'$|; - -$key = q/a^n+b^n=c^n;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ a^n+b^n=c^n$|; - -$key = q/displaystyleepsilon,bar{epsilon};MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \epsilon , \bar{\epsilon}$|; - -$key = q/displaystylelefti}sum_alphasum_betalphajbeta}-sum_isum_alphamathbf{p}_{ialpha}mathbf{f}_{ialpha}right>;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \left< \sum_i M_i \mathbf{V}_i \mathbf{V}_i
-+ \sum_{i}\sum_{j>i}\...
-... j\beta}
-- \sum_i \sum_\alpha \mathbf{p}_{i\alpha} \mathbf{f}_{i\alpha} \right>$|; - -$key = q/displaystylecgeq0;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle c \geq 0$|; - -$key = q/deltamathbf{c};MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ \delta\mathbf{c}$|; - -$key = q/displaystyle0.422784dots=1-gamma;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle 0.422784\dots = 1 - \gamma$|; - -$key = q/displaystylefrac{1}{2pii}int^{c+iinfty}_{c-iinfty}expleft(ulnu+lambdauright)du;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty}
-\exp \left( u \ln u + \lambda u \right ) du$|; - -$key = q/displaystylephi(lambda);MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \phi(\lambda)$|; - -$key = q/displaystyleVmathbf{pi}^{sr};MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle V \mathbf{\pi}^{sr}$|; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS/images.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS/images.tex deleted file mode 100644 index 0d853551381..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleAMS/images.tex +++ /dev/null @@ -1,276 +0,0 @@ -\batchmode -\documentclass[a4paper,twoside]{article} - -\usepackage{html} -\usepackage{amsmath} - -% -\renewcommand{\d}{\partial}% -\providecommand{\bm}[1]{\mathbf{#1}}% -\providecommand{\Range}{\mathcal{R}}% -\providecommand{\Ker}{\mathcal{N}}% -\providecommand{\Quat}{\vec{\mathbf{Q}}} -% -\providecommand{\StAndrews}{\htmlurl{http://www-groups.dcs.st-and.ac.uk/~history}}%% -\providecommand{\Pythagorians}{\htmladdnormallink - 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    -
    - -

    -

    -Math examples -

    -
    -
    - - - - - - - - - - - - - - - - - - - - - - - - -
    $\displaystyle \phi(\lambda)$$\displaystyle =$$\displaystyle \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty}
-\exp \left( u \ln u + \lambda u \right ) du$   for $\displaystyle c \geq 0$ -(1)
    $\displaystyle \lambda$$\displaystyle =$$\displaystyle \frac{\epsilon -\bar{\epsilon} }{\xi}
-- \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}}$ -(2)
    $\displaystyle \gamma$$\displaystyle =$$\displaystyle 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)}$ -(3)
    $\displaystyle \gamma'$$\displaystyle =$$\displaystyle 0.422784\dots = 1 - \gamma$ -(4)
    $\displaystyle \epsilon , \bar{\epsilon}$$\displaystyle =$actual/average energy loss -(5)
    -

    - -

    -Since (6) or (7d) should hold for arbitrary - -$ \delta\mathbf{c}$-vectors, it is clear that - -$ \mathcal{N}(A) = \mathcal{R}(B)$ and that when $ y=B(x)$ one has... -
    -...the Pythagorians knew infinitely many solutions in integers to - -$ a^2+b^2=c^2$. -That no non-trivial integer solutions exist for - -$ a^n+b^n=c^n$ with integers $ n>2$ has long -been suspected (Fermat, c.1637). Only during the current decade has this been proved (Wiles, 1995). - -

    -
    -

    - - - - - - - - - - - -
    $\displaystyle V \mathbf{\pi}^{sr}$$\displaystyle =$$\displaystyle \left< \sum_i M_i \mathbf{V}_i \mathbf{V}_i
-+ \sum_i \sum_{j>i} \mathbf{R}_{ij} \mathbf{F}_{ij}\right>$ -(6)
     $\displaystyle =$$\displaystyle \left< \sum_i M_i \mathbf{V}_i \mathbf{V}_i
-+ \sum_{i}\sum_{j>i}\...
-... j\beta}
-- \sum_i \sum_\alpha \mathbf{p}_{i\alpha} \mathbf{f}_{i\alpha} \right>$
    -

    - -

    - -

    - - - - -
    \begin{subequations}\begin{align}B_{ij}^\alpha & = \left(B_{ij}^\alpha\right)_0 ...
-...\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right)\end{align}\end{subequations}
    -
    -

    - -Subsections - - - -
    - - -next -up -previous -
    - Next: About this document ... - -
    -Michel Goossens -
    1999-03-30 -
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    - Up: sampleAMS - Previous: sampleAMS -
    -
    - - -

    -About this document ... -

    -

    -This document was generated using the -LaTeX2HTML translator Version 99.1 release (March 30, 1999) -

    -Copyright © 1993, 1994, 1995, 1996, -Nikos Drakos, -Computer Based Learning Unit, University of Leeds. -
    -Copyright © 1997, 1998, 1999, -Ross Moore, -Mathematics Department, Macquarie University, Sydney. -

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    -The translation was initiated by Michel Goossens on 1999-03-30 -


    -
    -Michel Goossens -
    1999-03-30 -
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    - Next: About this document ... -
    -
    - -

    -

    -Math examples -

    -
    -
    - - - - - - - - - - - - - - - - - - - - - - - - -
    $\displaystyle \phi(\lambda)$$\displaystyle =$$\displaystyle \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty}
-\exp \left( u \ln u + \lambda u \right ) du$   for $\displaystyle c \geq 0$ -(1)
    $\displaystyle \lambda$$\displaystyle =$$\displaystyle \frac{\epsilon -\bar{\epsilon} }{\xi}
-- \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}}$ -(2)
    $\displaystyle \gamma$$\displaystyle =$$\displaystyle 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)}$ -(3)
    $\displaystyle \gamma'$$\displaystyle =$$\displaystyle 0.422784\dots = 1 - \gamma$ -(4)
    $\displaystyle \epsilon , \bar{\epsilon}$$\displaystyle =$actual/average energy loss -(5)
    -

    - -

    -Since (6) or (7d) should hold for arbitrary - -$ \delta\mathbf{c}$-vectors, it is clear that - -$ \mathcal{N}(A) = \mathcal{R}(B)$ and that when $ y=B(x)$ one has... -
    -...the Pythagorians knew infinitely many solutions in integers to - -$ a^2+b^2=c^2$. -That no non-trivial integer solutions exist for - -$ a^n+b^n=c^n$ with integers $ n>2$ has long -been suspected (Fermat, c.1637). Only during the current decade has this been proved (Wiles, 1995). - -

    -
    -

    - - - - - - - - - - - -
    $\displaystyle V \mathbf{\pi}^{sr}$$\displaystyle =$$\displaystyle \left< \sum_i M_i \mathbf{V}_i \mathbf{V}_i
-+ \sum_i \sum_{j>i} \mathbf{R}_{ij} \mathbf{F}_{ij}\right>$ -(6)
     $\displaystyle =$$\displaystyle \left< \sum_i M_i \mathbf{V}_i \mathbf{V}_i
-+ \sum_{i}\sum_{j>i}\...
-... j\beta}
-- \sum_i \sum_\alpha \mathbf{p}_{i\alpha} \mathbf{f}_{i\alpha} \right>$
    -

    - -

    - -

    - - - - -
    \begin{subequations}\begin{align}B_{ij}^\alpha & = \left(B_{ij}^\alpha\right)_0 ...
-...\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right)\end{align}\end{subequations}
    -
    -

    - -Subsections - - - -
    - - -next -up -previous -
    - Next: About this document ... - -
    -Michel Goossens -
    1999-03-30 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath.dvi b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath.dvi deleted file mode 100644 index 64f8631b113..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath.dvi and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath.tex deleted file mode 100644 index 26ab42edddc..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath.tex +++ /dev/null @@ -1,54 +0,0 @@ -\documentclass[a4paper,twoside]{article} -\usepackage{html} -%\usepackage{amsmath} - -\renewcommand{\d}{\partial}\providecommand{\bm}[1]{\mathbf{#1}} -\providecommand{\Range}{\mathcal{R}}\providecommand{\Ker}{\mathcal{N}} -\providecommand{\Quat}{\vec{\mathbf{Q}}} - -\newcommand{\StAndrews}{\htmlurl{http://www-groups.dcs.st-and.ac.uk/~history}}% -\newcommand{\Pythagorians}{\htmladdnormallink - {Pythagorians}{\StAndrews/Mathematicians/Pythagoras.html}} -\newcommand{\Fermat}{\htmladdnormallink - {Fermat, c.1637}{\StAndrews/HistTopics/Fermat's_last_theorem.html}} -\newcommand{\Wiles}{\htmladdnormallink - {Wiles, 1995}{\htmlurl{http://www.pbs.org:80/wgbh/nova/proof}}} - -\begin{document} -\htmlhead[center]{section}{Math examples} -\begin{eqnarray} - \phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty} - \exp \left( u \ln u + \lambda u \right ) du \hspace{1cm}\mbox{for } c \geq 0 \\ - \lambda & = & \frac{\epsilon -\bar{\epsilon} }{\xi} - - \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}}\label{xiEmax} \\ - \gamma & = & 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)} \\ - \gamma' & = & 0.422784\dots = 1 - \gamma \\ - \epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss} -\end{eqnarray} - -Since~\ref{xiEmax} and \ref{eqn:stress-sr} hold for arbitrary $\delta\bm{c}$-vectors, -it is clear that $\Ker(A) = \Range(B)$ and that when $y=B(x)$ one has...\\ -...the \Pythagorians{} knew infinitely many solutions in integers to $a^2+b^2=c^2$. -That no non-trivial integer solutions exist for $a^n+b^n=c^n$ with integers $n>2$ has long -been suspected (\Fermat). Only during the current decade has this been proved (\Wiles). - -\begin{eqnarray}\label{eqn:stress-sr} - V \bm{\pi}^{sr} & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i - + \sum_i \sum_{j>i} \bm{R}_{ij} \bm{F}_{ij}\right> \\ \nonumber - & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i - + \sum_{i}\sum_{j>i}\sum_\alpha\sum_\beta \bm{r}_{i\alpha j\beta}\bm{f}_{i\alpha j\beta} - - \sum_i \sum_\alpha \bm{p}_{i\alpha} \bm{f}_{i\alpha} \right> -\end{eqnarray} -\end{document} -\begin{subequations}\label{bgdefs} -\begin{align} B_{ij}^\alpha & = - \left(B_{ij}^\alpha\right)_0 + \left(B_{ij}^\alpha\right)_a \label{bdef} \\ - \left(B_{ij}^\alpha\right)_0 & = \frac{1}{2}\left(\frac{\d N_i^\alpha}{\d X_j} - + \frac{\d N_j^\alpha} {\d X_i} \right) \label{b0def} \\ - \left(B_{ij}^\alpha\right)_a & = H_{ij}^{\alpha \beta} a^\beta \label{budef} \\ - H_{ij}^{\alpha \beta} & = - \frac{1}{2}\left( \frac{\d N_k^\alpha}{\d X_i} \frac{\d N_k^\beta}{\d X_j} - + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right) \label{gdef} -\end{align} -\end{subequations} -\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/WARNINGS b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/WARNINGS deleted file mode 100644 index 9d1d9f764ee..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/WARNINGS +++ /dev/null @@ -1,2 +0,0 @@ - -redefining command \d diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/images.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/images.pl deleted file mode 100644 index a319f5c597b..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/images.pl +++ /dev/null @@ -1,132 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate images original text with physical files. - - -$key = q/displaystylefrac{epsilon-bar{epsilon}}{xi}-gamma'-beta^2-lnfrac{xi}{E_{{rm{max}};MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \frac{\epsilon -\bar{\epsilon} }{\xi}
-- \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}}$|; - -$key = q/a^2+b^2=c^2;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$a^2+b^2=c^2$|; - -$key = q/n>2;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$n>2$|; - -$key = q/y=B(x);MSF=1.6;AAT/; -$cached_env_img{$key} = q|$y=B(x)$|; - -$key = q/mathcal{N}(A)=mathcal{R}(B);MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\mathcal{N}(A) = \mathcal{R}(B)$|; - -$key = q/displaystylelambda;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \lambda$|; - -$key = q/displaystyle0.577215dotsmathrm{hspace{5mm}(Euler'sconstant)};MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)}$|; - -$key = q/displaystylegamma;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \gamma$|; - -$key = q/displaystylefrac{1}{2pii}int^{c+iinfty}_{c-iinfty}expleft(ulnu+lambdauright)duhspace{1cm}mbox{for}cgeq0;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty}
-\exp \left( u \ln u + \lambda u \right ) du \hspace{1cm}\mbox{for } c \geq 0$|; - -$key = q/displaystylembox{actualslashaverageenergyloss};MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \mbox{actual/average energy loss}$|; - -$key = q/displaystylelefti}mathbf{R}_{ij}mathbf{F}_{ij}right>;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \left< \sum_i M_i \mathbf{V}_i \mathbf{V}_i
-+ \sum_i \sum_{j>i} \mathbf{R}_{ij} \mathbf{F}_{ij}\right>$|; - -$key = q/displaystylegamma';MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \gamma'$|; - -$key = q/a^n+b^n=c^n;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$a^n+b^n=c^n$|; - -$key = q/textstyle=;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\textstyle =$|; - -$key = q/displaystyleepsilon,bar{epsilon};MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \epsilon , \bar{\epsilon}$|; - -$key = q/displaystylelefti}sum_alphasum_betalphajbeta}-sum_isum_alphamathbf{p}_{ialpha}mathbf{f}_{ialpha}right>;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \left< \sum_i M_i \mathbf{V}_i \mathbf{V}_i
-+ \sum_{i}\sum_{j>i}\...
-... j\beta}
-- \sum_i \sum_\alpha \mathbf{p}_{i\alpha} \mathbf{f}_{i\alpha} \right>$|; - -$key = q/deltamathbf{c};MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\delta\mathbf{c}$|; - -$key = q/displaystyle0.422784dots=1-gamma;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle 0.422784\dots = 1 - \gamma$|; - -$key = q/displaystylephi(lambda);MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \phi(\lambda)$|; - -$key = q/displaystyleVmathbf{pi}^{sr};MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle V \mathbf{\pi}^{sr}$|; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/images.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/images.tex deleted file mode 100644 index 9b738e34b59..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/images.tex +++ /dev/null @@ -1,254 +0,0 @@ -\batchmode -\documentclass[a4paper,twoside]{article} - -\usepackage{html} - -% -\renewcommand{\d}{\partial}% -\providecommand{\bm}[1]{\mathbf{#1}}% -\providecommand{\Range}{\mathcal{R}}% -\providecommand{\Ker}{\mathcal{N}}% -\providecommand{\Quat}{\vec{\mathbf{Q}}} -% -\providecommand{\StAndrews}{\htmlurl{http://www-groups.dcs.st-and.ac.uk/~history}}%% -\providecommand{\Pythagorians}{\htmladdnormallink - 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-\lthtmlinlinemathA{tex2html_wrap_indisplay179}% -$\displaystyle \gamma$% -\lthtmlindisplaymathZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_indisplay181}% -$\displaystyle 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)}$% -\lthtmlindisplaymathZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_indisplay182}% -$\displaystyle \gamma'$% -\lthtmlindisplaymathZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_indisplay184}% -$\displaystyle 0.422784\dots = 1 - \gamma$% -\lthtmlindisplaymathZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_indisplay185}% -$\displaystyle \epsilon , \bar{\epsilon}$% -\lthtmlindisplaymathZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_indisplay187}% -$\displaystyle \mbox{actual/average energy loss}$% -\lthtmlindisplaymathZ -\lthtmlcheckvsize\clearpage} - 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    - Next: About this document ... -
    -
    - -

    -

    -Math examples -

    -
    -
    - - - - - - - - - - - - - - - - - - - - - - - - -
    $\displaystyle \phi(\lambda)$$\textstyle =$$\displaystyle \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty}
-\exp \left( u \ln u + \lambda u \right ) du \hspace{1cm}\mbox{for } c \geq 0$ -(1)
    $\displaystyle \lambda$$\textstyle =$$\displaystyle \frac{\epsilon -\bar{\epsilon} }{\xi}
-- \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}}$ -(2)
    $\displaystyle \gamma$$\textstyle =$$\displaystyle 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)}$ -(3)
    $\displaystyle \gamma'$$\textstyle =$$\displaystyle 0.422784\dots = 1 - \gamma$ -(4)
    $\displaystyle \epsilon , \bar{\epsilon}$$\textstyle =$$\displaystyle \mbox{actual/average energy loss}$ -(5)
    -

    - -

    -Since 2 and 6 hold for arbitrary - -$\delta\mathbf{c}$-vectors, -it is clear that - -$\mathcal{N}(A) = \mathcal{R}(B)$ and that when $y=B(x)$ one has... -
    -...the Pythagorians knew infinitely many solutions in integers to $a^2+b^2=c^2$. -That no non-trivial integer solutions exist for $a^n+b^n=c^n$ with integers $n>2$ has long -been suspected (Fermat, c.1637). Only during the current decade has this been proved (Wiles, 1995). - -

    -
    -

    - - - - - - - - - - - - -
    $\displaystyle V \mathbf{\pi}^{sr}$$\textstyle =$$\displaystyle \left< \sum_i M_i \mathbf{V}_i \mathbf{V}_i
-+ \sum_i \sum_{j>i} \mathbf{R}_{ij} \mathbf{F}_{ij}\right>$ -(6)
     $\textstyle =$$\displaystyle \left< \sum_i M_i \mathbf{V}_i \mathbf{V}_i
-+ \sum_{i}\sum_{j>i}\...
-... j\beta}
-- \sum_i \sum_\alpha \mathbf{p}_{i\alpha} \mathbf{f}_{i\alpha} \right>$
    -

    -

    - -Subsections - - - -

    -
    -Michel Goossens -
    1999-03-30 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/internals.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/internals.pl deleted file mode 100644 index 129a18c5241..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/internals.pl +++ /dev/null @@ -1,14 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate internals original text with physical files. - - -$key = q/xiEmax/; -$ref_files{$key} = "$dir".q|sampleMath.html|; -$noresave{$key} = "$nosave"; - -$key = q/eqn:stress-sr/; -$ref_files{$key} = "$dir".q|sampleMath.html|; -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/labels.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/labels.pl deleted file mode 100644 index 47f50cc587b..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/labels.pl +++ /dev/null @@ -1,29 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate labels original text with physical files. - - -$key = q/xiEmax/; -$external_labels{$key} = "$URL/" . q|sampleMath.html|; -$noresave{$key} = "$nosave"; - -$key = q/eqn:stress-sr/; -$external_labels{$key} = "$URL/" . q|sampleMath.html|; -$noresave{$key} = "$nosave"; - -1; - - -# LaTeX2HTML 99.1 release (March 30, 1999) -# labels from external_latex_labels array. - - -$key = q/xiEmax/; -$external_latex_labels{$key} = q|2|; -$noresave{$key} = "$nosave"; - -$key = q/eqn:stress-sr/; -$external_latex_labels{$key} = q|6|; -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/node1.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/node1.html deleted file mode 100644 index 35ab2f29258..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/node1.html +++ /dev/null @@ -1,72 +0,0 @@ - - - - - -About this document ... - - - - - - - - - - - - - - - - - -next - -up - -previous -
    - Up: sampleMath - Previous: sampleMath -
    -
    - - -

    -About this document ... -

    -

    -This document was generated using the -LaTeX2HTML translator Version 99.1 release (March 30, 1999) -

    -Copyright © 1993, 1994, 1995, 1996, -Nikos Drakos, -Computer Based Learning Unit, University of Leeds. -
    -Copyright © 1997, 1998, 1999, -Ross Moore, -Mathematics Department, Macquarie University, Sydney. -

    -The command line arguments were:
    - latex2html sampleMath -

    -The translation was initiated by Michel Goossens on 1999-03-30 -


    -
    -Michel Goossens -
    1999-03-30 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/sampleMath.css b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/sampleMath.css deleted file mode 100644 index 1993b851311..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/sampleMath.css +++ /dev/null @@ -1,31 +0,0 @@ - -/* Century Schoolbook font is very similar to Computer Modern Math: cmmi */ -.MATH { font-family: "Century Schoolbook", serif; } -.MATH I { font-family: "Century Schoolbook", serif; font-shape: italic } -.BOLDMATH { font-family: "Century Schoolbook", serif; font-weight: bold } - -/* implement both fixed-size and relative sizes */ -SMALL.XTINY { font-size : xx-small } -SMALL.TINY { font-size : x-small } -SMALL.SCRIPTSIZE { font-size : smaller } -SMALL.FOOTNOTESIZE { font-size : small } -SMALL.SMALL { } -BIG.LARGE { } -BIG.XLARGE { font-size : large } -BIG.XXLARGE { font-size : x-large } -BIG.HUGE { font-size : larger } -BIG.XHUGE { font-size : xx-large } - -/* heading styles */ -H1 { } -H2 { } -H3 { } -H4 { } -H5 { } - -/* mathematics styles */ -DIV.displaymath { } /* math displays */ -TD.eqno { } /* equation-number cells */ - - -/* document-specific styles come next */ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/sampleMath.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/sampleMath.html deleted file mode 100644 index 47104a5ce76..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMath/sampleMath.html +++ /dev/null @@ -1,235 +0,0 @@ - - - - - -sampleMath - - - - - - - - - - - - - - - - - - -next -up -previous -
    - Next: About this document ... -
    -
    - -

    -

    -Math examples -

    -
    -
    - - - - - - - - - - - - - - - - - - - - - - - - -
    $\displaystyle \phi(\lambda)$$\textstyle =$$\displaystyle \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty}
-\exp \left( u \ln u + \lambda u \right ) du \hspace{1cm}\mbox{for } c \geq 0$ -(1)
    $\displaystyle \lambda$$\textstyle =$$\displaystyle \frac{\epsilon -\bar{\epsilon} }{\xi}
-- \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}}$ -(2)
    $\displaystyle \gamma$$\textstyle =$$\displaystyle 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)}$ -(3)
    $\displaystyle \gamma'$$\textstyle =$$\displaystyle 0.422784\dots = 1 - \gamma$ -(4)
    $\displaystyle \epsilon , \bar{\epsilon}$$\textstyle =$$\displaystyle \mbox{actual/average energy loss}$ -(5)
    -

    - -

    -Since 2 and 6 hold for arbitrary - -$\delta\mathbf{c}$-vectors, -it is clear that - -$\mathcal{N}(A) = \mathcal{R}(B)$ and that when $y=B(x)$ one has... -
    -...the Pythagorians knew infinitely many solutions in integers to $a^2+b^2=c^2$. -That no non-trivial integer solutions exist for $a^n+b^n=c^n$ with integers $n>2$ has long -been suspected (Fermat, c.1637). Only during the current decade has this been proved (Wiles, 1995). - -

    -
    -

    - - - - - - - - - - - - -
    $\displaystyle V \mathbf{\pi}^{sr}$$\textstyle =$$\displaystyle \left< \sum_i M_i \mathbf{V}_i \mathbf{V}_i
-+ \sum_i \sum_{j>i} \mathbf{R}_{ij} \mathbf{F}_{ij}\right>$ -(6)
     $\textstyle =$$\displaystyle \left< \sum_i M_i \mathbf{V}_i \mathbf{V}_i
-+ \sum_{i}\sum_{j>i}\...
-... j\beta}
-- \sum_i \sum_\alpha \mathbf{p}_{i\alpha} \mathbf{f}_{i\alpha} \right>$
    -

    -

    - -Subsections - - - -

    -
    -Michel Goossens -
    1999-03-30 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages.dvi b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages.dvi deleted file mode 100644 index 0af1abe023b..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages.dvi and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages.tex deleted file mode 100644 index cca8e754e57..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages.tex +++ /dev/null @@ -1,64 +0,0 @@ -\documentclass[a4paper,twoside]{article} -\usepackage{html} -\usepackage{amsmath} - -\renewcommand{\d}{\partial}\providecommand{\bm}[1]{\mathbf{#1}} -\providecommand{\Range}{\mathcal{R}}\providecommand{\Ker}{\mathcal{N}} -\providecommand{\Quat}{\vec{\mathbf{Q}}} - -\newcommand{\StAndrews}{\url{http://www-groups.dcs.st-and.ac.uk/~history}}% -\newcommand{\Pythagorians}{\htmladdnormallink - {Pythagorians}{\StAndrews/Mathematicians/Pythagoras.html}} -\newcommand{\Fermat}{\htmladdnormallink - {Fermat, c.1637}{\StAndrews/HistTopics/Fermat's_last_theorem.html}} -\newcommand{\Wiles}{\htmladdnormallink - {Wiles, 1995}{http://www.pbs.org:80/wgbh/nova/proof}} - -\begin{document} -\htmlhead[center]{section}{Math examples} -\begin{flushright} -\begin{makeimage} -\begin{eqnarray} - \phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty} - \exp \left( u \ln u + \lambda u \right ) du \hspace{1cm}\mbox{for } c \geq 0 \\ - \lambda & = & \frac{\epsilon -\bar{\epsilon} }{\xi} - - \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}} \\ - \gamma & = & 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)} \\ - \gamma' & = & 0.422784\dots = 1 - \gamma \\ - \epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss} -\end{eqnarray} -\end{makeimage} -\end{flushright} - -Since~\eqref{eqn:stress-sr} or~\eqref{gdef} should hold for arbitrary $\delta\bm{c}$% --vectors, it is clear that $\Ker(A) = \Range(B)$ and that when $y=B(x)$ one has...\\ -...the \Pythagorians{} knew infinitely many solutions in integers to $a^2+b^2=c^2$. -That no non-trivial integer solutions exist for $a^n+b^n=c^n$ with integers $n>2$ has long -been suspected (\Fermat). Only during the current decade has this been proved (\Wiles). - -\begin{flushright} -\begin{eqnarray}\htmlimage{} -\label{eqn:stress-sr} - V \bm{\pi}^{sr} & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i - + \sum_i \sum_{j>i} \bm{R}_{ij} \bm{F}_{ij}\right> \\ \nonumber - & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i - + \sum_{i}\sum_{j>i}\sum_\alpha\sum_\beta \bm{r}_{i\alpha j\beta}\bm{f}_{i\alpha j\beta} - - \sum_i \sum_\alpha \bm{p}_{i\alpha} \bm{f}_{i\alpha} \right> -\end{eqnarray} -\end{flushright} - -\begin{flushright} -\begin{subequations}\htmlimage{} -\label{bgdefs} -\begin{align} B_{ij}^\alpha & = - \left(B_{ij}^\alpha\right)_0 + \left(B_{ij}^\alpha\right)_a \label{bdef} \\ - \left(B_{ij}^\alpha\right)_0 & = \frac{1}{2}\left(\frac{\d N_i^\alpha}{\d X_j} - + \frac{\d N_j^\alpha} {\d X_i} \right) \label{b0def} \\ - \left(B_{ij}^\alpha\right)_a & = H_{ij}^{\alpha \beta} a^\beta \label{budef} \\ - H_{ij}^{\alpha \beta} & = - \frac{1}{2}\left( \frac{\d N_k^\alpha}{\d X_i} \frac{\d N_k^\beta}{\d X_j} - + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right) \label{gdef} -\end{align} -\end{subequations} -\end{flushright} -\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/WARNINGS b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/WARNINGS deleted file mode 100644 index 4ec77a7a5b1..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/WARNINGS +++ /dev/null @@ -1,4 +0,0 @@ - -redefining command \d - -sampleMathImages.tex is newer than sampleMathImages.aux: Please rerun latex. diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/images.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/images.pl deleted file mode 100644 index 1d06c6a2144..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/images.pl +++ /dev/null @@ -1,66 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate images original text with physical files. - - -$key = q/{makeimage}eqnarray{phi(lambda)&=&frac{1}{2pii}int^{c+iinfty}_{c-iinfty}expleft(ar{epsilon}&=&mbox{actualslashaverageenergyloss}eqnarray{{makeimage};MSF=1.6;AAT/; -$cached_env_img{$key} = q|\begin{eqnarray}
-\phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\in...
-...\epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss}
-\end{eqnarray}|; - -$key = q/a^2+b^2=c^2;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ a^2+b^2=c^2$|; - -$key = q/n>2;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ n>2$|; - -$key = q/{eqnarray}htmlimage{}Vmathbf{pi}^{sr}&=&left{eqnarray};MSF=1.6;TAGS=R;AAT/; -$cached_env_img{$key} = q|\begin{eqnarray}V \mathbf{\pi}^{sr} & = & \left< \sum_i M_i \mathbf{V}_i \mathbf...
-...m_i \sum_\alpha \mathbf{p}_{i\alpha} \mathbf{f}_{i\alpha} \right>
-\end{eqnarray}|; - -$key = q/y=B(x);MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ y=B(x)$|; - -$key = q/a^n+b^n=c^n;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ a^n+b^n=c^n$|; - -$key = q/displaystylehtmlimage{}align{B_{ij}^alpha=left(B_{ij}^alpharight)_0+leX_j}+frac{{d{N_k^beta}{{d{X_i}frac{{d{N_k^alpha}{{d{X_j}right)align{;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \begin{align}B_{ij}^\alpha & = \left(B_{ij}^\alpha\right)_0 + \le...
-...} + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right)\end{align}$|; - -$key = q/mathcal{N}(A)=mathcal{R}(B);MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ \mathcal{N}(A) = \mathcal{R}(B)$|; - -$key = q/deltamathbf{c};MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ \delta\mathbf{c}$|; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/images.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/images.tex deleted file mode 100644 index f874044e50b..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/images.tex +++ /dev/null @@ -1,213 +0,0 @@ -\batchmode -\documentclass[a4paper,twoside]{article} - -\usepackage{html} -\usepackage{amsmath} - -% -\renewcommand{\d}{\partial}% -\providecommand{\bm}[1]{\mathbf{#1}}% -\providecommand{\Range}{\mathcal{R}}% -\providecommand{\Ker}{\mathcal{N}}% -\providecommand{\Quat}{\vec{\mathbf{Q}}} -% -\providecommand{\StAndrews}{\url{http://www-groups.dcs.st-and.ac.uk/~history}}%% -\providecommand{\Pythagorians}{\htmladdnormallink - {Pythagorians}{\url{http://www-groups.dcs.st-and.ac.uk/~history}/Mathematicians/Pythagoras.html}}% -\providecommand{\Fermat}{\htmladdnormallink - {Fermat, c.1637}{\url{http://www-groups.dcs.st-and.ac.uk/~history}/HistTopics/Fermat's_last_theorem.html}}% -\providecommand{\Wiles}{\htmladdnormallink - {Wiles, 1995}{http://www.pbs.org:80/wgbh/nova/proof}} - -\usepackage[dvips]{color} -\pagecolor[gray]{.7} - - - -\makeatletter - -\makeatletter -\count@=\the\catcode`\_ \catcode`\_=8 -\newenvironment{tex2html_wrap}{}{} \catcode`\_=\count@ -\newcommand{\renewedcommand}[1]{\expandafter\renewcommand\csname #1\endcsname}% -\makeatother -\let\mathon=$ -\let\mathoff=$ -\ifx\AtBeginDocument\undefined \newcommand{\AtBeginDocument}[1]{}\fi -\newbox\sizebox -\setlength{\hoffset}{0pt}\setlength{\voffset}{0pt} -\addtolength{\textheight}{\footskip}\setlength{\footskip}{0pt} -\addtolength{\textheight}{\topmargin}\setlength{\topmargin}{0pt} -\addtolength{\textheight}{\headheight}\setlength{\headheight}{0pt} -\addtolength{\textheight}{\headsep}\setlength{\headsep}{0pt} -\setlength{\textwidth}{349pt} -\newwrite\lthtmlwrite -\makeatletter -\let\realnormalsize=\normalsize -\global\topskip=2sp -\def\preveqno{}\let\real@float=\@float \let\realend@float=\end@float -\def\@float{\let\@savefreelist\@freelist\real@float} -\def\end@float{\realend@float\global\let\@freelist\@savefreelist} -\let\real@dbflt=\@dbflt \let\end@dblfloat=\end@float -\let\@largefloatcheck=\relax -\let\if@boxedmulticols=\iftrue -\def\@dbflt{\let\@savefreelist\@freelist\real@dbflt} -\def\adjustnormalsize{\def\normalsize{\mathsurround=0pt \realnormalsize - \parindent=0pt\abovedisplayskip=0pt\belowdisplayskip=0pt}% - \def\phantompar{\csname par\endcsname}\normalsize}% -\def\lthtmltypeout#1{{\let\protect\string\immediate\write\lthtmlwrite{#1}}}% -\newcommand\lthtmlhboxmathA{\adjustnormalsize\setbox\sizebox=\hbox\bgroup\kern.05em }% -\newcommand\lthtmlhboxmathB{\adjustnormalsize\setbox\sizebox=\hbox to\hsize\bgroup\hfill }% -\newcommand\lthtmlvboxmathA{\adjustnormalsize\setbox\sizebox=\vbox\bgroup % - \let\ifinner=\iffalse }% -\newcommand\lthtmlboxmathZ{\@next\next\@currlist{}{\def\next{\voidb@x}}% - \expandafter\box\next\egroup}% -\newcommand\lthtmlmathtype[1]{\def\lthtmlmathenv{#1}}% -\newcommand\lthtmllogmath{\lthtmltypeout{l2hSize % -:\lthtmlmathenv:\the\ht\sizebox::\the\dp\sizebox::\the\wd\sizebox.\preveqno}}% -\newcommand\lthtmlfigureA[1]{\let\@savefreelist\@freelist - \lthtmlmathtype{#1}\lthtmlvboxmathA}% -\newcommand\lthtmlpictureA[1]{\let\@savefreelist\@freelist - \lthtmlmathtype{#1}\lthtmlhboxmathB}% -\newcommand\lthtmlpictureZ[1]{\hfill\lthtmlfigureZ}% -\newcommand\lthtmlfigureZ{\lthtmlboxmathZ\lthtmllogmath\copy\sizebox - \global\let\@freelist\@savefreelist}% -\newcommand\lthtmldisplayA[1]{\lthtmlmathtype{#1}\lthtmlvboxmathA}% -\newcommand\lthtmldisplayB[1]{\edef\preveqno{(\theequation)}% - \lthtmldisplayA{#1}\let\@eqnnum\relax}% -\newcommand\lthtmldisplayZ{\lthtmlboxmathZ\lthtmllogmath\lthtmlsetmath}% -\newcommand\lthtmlinlinemathA[1]{\lthtmlmathtype{#1}\lthtmlhboxmathA - \vrule height1.5ex width0pt }% -\newcommand\lthtmlinlineA[1]{\lthtmlmathtype{#1}\lthtmlhboxmathA}% -\newcommand\lthtmlinlineZ{\egroup\expandafter\ifdim\dp\sizebox>0pt % - \expandafter\centerinlinemath\fi\lthtmllogmath\lthtmlsetinline} -\newcommand\lthtmlinlinemathZ{\egroup\expandafter\ifdim\dp\sizebox>0pt % - \expandafter\centerinlinemath\fi\lthtmllogmath\lthtmlsetmath} -\newcommand\lthtmlindisplaymathZ{\egroup % - \centerinlinemath\lthtmllogmath\lthtmlsetmath} -\def\lthtmlsetinline{\hbox{\vrule width.1em\kern-.05em\vtop{\vbox{% - \kern.1em\copy\sizebox}\ifdim\dp\sizebox>0pt\kern.1em\else\kern.3pt\fi - \ifdim\hsize>\wd\sizebox \hrule depth1pt\fi}}} -\def\lthtmlsetmath{\hbox{\vrule width.1em\kern-.05em\vtop{\vbox{% - \kern.1em\kern0.8 pt\hbox{\hglue.17em\copy\sizebox\hglue0.8 pt}}\kern.3pt% - \ifdim\dp\sizebox>0pt\kern.1em\fi \kern0.8 pt% - \ifdim\hsize>\wd\sizebox \hrule depth1pt\fi}}} -\def\centerinlinemath{% - \dimen1=\ifdim\ht\sizebox<\dp\sizebox \dp\sizebox\else\ht\sizebox\fi - \advance\dimen1by.5pt \vrule width0pt height\dimen1 depth\dimen1 - \dp\sizebox=\dimen1\ht\sizebox=\dimen1\relax} - -\def\lthtmlcheckvsize{\ifdim\ht\sizebox<\vsize - \ifdim\wd\sizebox<\hsize\expandafter\hfill\fi \expandafter\vfill - \else\expandafter\vss\fi}% -\providecommand{\selectlanguage}[1]{}% -\makeatletter \tracingstats = 1 -\providecommand{\Mu}{\textrm{M}} -\providecommand{\Nu}{\textrm{N}} -\providecommand{\Chi}{\textrm{X}} -\providecommand{\Zeta}{\textrm{Z}} -\providecommand{\Alpha}{\textrm{A}} -\providecommand{\Omicron}{\textrm{O}} -\providecommand{\omicron}{\textrm{o}} -\providecommand{\Rho}{\textrm{R}} -\providecommand{\Tau}{\textrm{T}} -\providecommand{\Epsilon}{\textrm{E}} -\providecommand{\Eta}{\textrm{H}} -\providecommand{\Beta}{\textrm{B}} -\providecommand{\Iota}{\textrm{J}} -\providecommand{\Kappa}{\textrm{K}} - - -\begin{document} -\pagestyle{empty}\thispagestyle{empty}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength hsize=\the\hsize}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength vsize=\the\vsize}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength hoffset=\the\hoffset}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength voffset=\the\voffset}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength topmargin=\the\topmargin}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength topskip=\the\topskip}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength headheight=\the\headheight}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength headsep=\the\headsep}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength parskip=\the\parskip}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength oddsidemargin=\the\oddsidemargin}\lthtmltypeout{}% -\makeatletter -\if@twoside\lthtmltypeout{latex2htmlLength evensidemargin=\the\evensidemargin}% -\else\lthtmltypeout{latex2htmlLength evensidemargin=\the\oddsidemargin}\fi% -\lthtmltypeout{}% -\makeatother -\setcounter{page}{1} -\onecolumn - -% !!! IMAGES START HERE !!! - -{\newpage\clearpage -\lthtmldisplayA{makeimage29}% -\begin{eqnarray} - \phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty} - \exp \left( u \ln u + \lambda u \right ) du \hspace{1cm}\mbox{for } c \geq 0 \\ - \lambda & = & \frac{\epsilon -\bar{\epsilon} }{\xi} - - \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}} \\ - \gamma & = & 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)} \\ - \gamma' & = & 0.422784\dots = 1 - \gamma \\ - \epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss} -\end{eqnarray} -% -\lthtmldisplayZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_inline255}% -$ \delta\mathbf{c}$% -\lthtmlinlinemathZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_inline257}% -$ \mathcal{N}(A) = \mathcal{R}(B)$% -\lthtmlinlinemathZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_inline259}% -$ y=B(x)$% -\lthtmlinlinemathZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_inline261}% -$ a^2+b^2=c^2$% -\lthtmlinlinemathZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_inline263}% -$ a^n+b^n=c^n$% -\lthtmlinlinemathZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_inline265}% -$ n>2$% -\lthtmlinlinemathZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmldisplayA{eqnarray52}% -\begin{eqnarray}\htmlimage{} - V \mathbf{\pi}^{sr} & = & \left< \sum_i M_i \mathbf{V}_i \mathbf{V}_i - + \sum_i \sum_{j>i} \mathbf{R}_{ij} \mathbf{F}_{ij}\right> \\\nonumber - & = & \left< \sum_i M_i \mathbf{V}_i \mathbf{V}_i - + \sum_{i}\sum_{j>i}\sum_\alpha\sum_\beta \mathbf{r}_{i\alpha j\beta}\mathbf{f}_{i\alpha j\beta} - - \sum_i \sum_\alpha \mathbf{p}_{i\alpha} \mathbf{f}_{i\alpha} \right> -\end{eqnarray}% -\lthtmldisplayZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_indisplay268}% -$\displaystyle \htmlimage{}\begin{align} B_{ij}^\alpha & = \left(B_{ij}^\alpha\right)_0 + \left(B_{ij}^\alpha\right)_a\\ \left(B_{ij}^\alpha\right)_0 & = \frac{1}{2}\left(\frac{\d N_i^\alpha}{\d X_j} + \frac{\d N_j^\alpha} {\d X_i} \right)\\ \left(B_{ij}^\alpha\right)_a & = H_{ij}^{\alpha \beta} a^\beta\\ H_{ij}^{\alpha \beta} & = \frac{1}{2}\left( \frac{\d N_k^\alpha}{\d X_i} \frac{\d N_k^\beta}{\d X_j} + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right)\end{align}$% -\lthtmlindisplaymathZ -\lthtmlcheckvsize\clearpage} - - -\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img1.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img1.gif deleted file mode 100644 index 8e6129a71ca..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img1.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img2.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img2.gif deleted file mode 100644 index f0b3d7892e0..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img2.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img3.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img3.gif deleted file mode 100644 index cbddfb5e467..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img3.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img4.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img4.gif deleted file mode 100644 index 7de6ffffe7c..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img4.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img5.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img5.gif deleted file mode 100644 index a23285e2c3e..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img5.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img6.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img6.gif deleted file mode 100644 index 7b38866db53..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img6.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img7.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img7.gif deleted file mode 100644 index 9f0fe8adafe..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img7.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img8.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img8.gif deleted file mode 100644 index d2fde624eb0..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img8.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img9.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img9.gif deleted file mode 100644 index 502a74b58a4..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/img9.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/index.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/index.html deleted file mode 100644 index 5e482e67124..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/index.html +++ /dev/null @@ -1,169 +0,0 @@ - - - - - -sampleMathImages - - - - - - - - - - - - - - - - - - -next -up -previous -
    - Next: About this document ... -
    -
    - -

    -

    -Math examples -

    -
    -\begin{eqnarray}
-\phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\in...
-...\epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss}
-\end{eqnarray} -
    - -
    - -

    -Since (6) or (7d) should hold for arbitrary - -$ \delta\mathbf{c}$-vectors, it is clear that - -$ \mathcal{N}(A) = \mathcal{R}(B)$ and that when $ y=B(x)$ one has... -
    -...the Pythagorians knew infinitely many solutions in integers to - -$ a^2+b^2=c^2$. -That no non-trivial integer solutions exist for - -$ a^n+b^n=c^n$ with integers $ n>2$ has long -been suspected (Fermat, c.1637). Only during the current decade has this been proved (Wiles, 1995). - -

    -

    -
    -
    -
    -

    - -\begin{eqnarray}V \mathbf{\pi}^{sr} & = & \left< \sum_i M_i \mathbf{V}_i \mathbf...
-...m_i \sum_\alpha \mathbf{p}_{i\alpha} \mathbf{f}_{i\alpha} \right>
-\end{eqnarray} -
    -

    -

    -
    -
    - -

    -

    -
    - - - - -
    $\displaystyle \begin{align}B_{ij}^\alpha & = \left(B_{ij}^\alpha\right)_0 + \le...
-...} + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right)\end{align}$
    -
    -
    -

    - -Subsections - - - -

    -
    -Michel Goossens -
    1999-03-30 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/internals.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/internals.pl deleted file mode 100644 index 19324793ac1..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/internals.pl +++ /dev/null @@ -1,30 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate internals original text with physical files. - - -$key = q/bdef/; -$ref_files{$key} = "$dir".q|sampleMathImages.html|; -$noresave{$key} = "$nosave"; - -$key = q/b0def/; -$ref_files{$key} = "$dir".q|sampleMathImages.html|; -$noresave{$key} = "$nosave"; - -$key = q/bgdefs/; -$ref_files{$key} = "$dir".q|sampleMathImages.html|; -$noresave{$key} = "$nosave"; - -$key = q/eqn:stress-sr/; -$ref_files{$key} = "$dir".q|sampleMathImages.html|; -$noresave{$key} = "$nosave"; - -$key = q/budef/; -$ref_files{$key} = "$dir".q|sampleMathImages.html|; -$noresave{$key} = "$nosave"; - -$key = q/gdef/; -$ref_files{$key} = "$dir".q|sampleMathImages.html|; -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/labels.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/labels.pl deleted file mode 100644 index fee23dac250..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/labels.pl +++ /dev/null @@ -1,61 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate labels original text with physical files. - - -$key = q/bdef/; -$external_labels{$key} = "$URL/" . q|sampleMathImages.html|; -$noresave{$key} = "$nosave"; - -$key = q/b0def/; -$external_labels{$key} = "$URL/" . q|sampleMathImages.html|; -$noresave{$key} = "$nosave"; - -$key = q/bgdefs/; -$external_labels{$key} = "$URL/" . q|sampleMathImages.html|; -$noresave{$key} = "$nosave"; - -$key = q/eqn:stress-sr/; -$external_labels{$key} = "$URL/" . q|sampleMathImages.html|; -$noresave{$key} = "$nosave"; - -$key = q/budef/; -$external_labels{$key} = "$URL/" . q|sampleMathImages.html|; -$noresave{$key} = "$nosave"; - -$key = q/gdef/; -$external_labels{$key} = "$URL/" . q|sampleMathImages.html|; -$noresave{$key} = "$nosave"; - -1; - - -# LaTeX2HTML 99.1 release (March 30, 1999) -# labels from external_latex_labels array. - - -$key = q/bdef/; -$external_latex_labels{$key} = q|7a|; -$noresave{$key} = "$nosave"; - -$key = q/b0def/; -$external_latex_labels{$key} = q|7b|; -$noresave{$key} = "$nosave"; - -$key = q/bgdefs/; -$external_latex_labels{$key} = q|7|; -$noresave{$key} = "$nosave"; - -$key = q/eqn:stress-sr/; -$external_latex_labels{$key} = q|6|; -$noresave{$key} = "$nosave"; - -$key = q/budef/; -$external_latex_labels{$key} = q|7c|; -$noresave{$key} = "$nosave"; - -$key = q/gdef/; -$external_latex_labels{$key} = q|7d|; -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/node1.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/node1.html deleted file mode 100644 index 44cd641eb3a..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/node1.html +++ /dev/null @@ -1,73 +0,0 @@ - - - - - -About this document ... - - - - - - - - - - - - - - - - - -next - -up - -previous -
    - Up: sampleMathImages - Previous: sampleMathImages -
    -
    - - -

    -About this document ... -

    -

    -This document was generated using the -LaTeX2HTML translator Version 99.1 release (March 30, 1999) -

    -Copyright © 1993, 1994, 1995, 1996, -Nikos Drakos, -Computer Based Learning Unit, University of Leeds. -
    -Copyright © 1997, 1998, 1999, -Ross Moore, -Mathematics Department, Macquarie University, Sydney. -

    -The command line arguments were:
    - latex2html sampleMathImages.tex -

    -The translation was initiated by Michel Goossens on 1999-03-30 -


    -
    -Michel Goossens -
    1999-03-30 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/sampleMathImages.css b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/sampleMathImages.css deleted file mode 100644 index 1993b851311..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/sampleMathImages.css +++ /dev/null @@ -1,31 +0,0 @@ - -/* Century Schoolbook font is very similar to Computer Modern Math: cmmi */ -.MATH { font-family: "Century Schoolbook", serif; } -.MATH I { font-family: "Century Schoolbook", serif; font-shape: italic } -.BOLDMATH { font-family: "Century Schoolbook", serif; font-weight: bold } - -/* implement both fixed-size and relative sizes */ -SMALL.XTINY { font-size : xx-small } -SMALL.TINY { font-size : x-small } -SMALL.SCRIPTSIZE { font-size : smaller } -SMALL.FOOTNOTESIZE { font-size : small } -SMALL.SMALL { } -BIG.LARGE { } -BIG.XLARGE { font-size : large } -BIG.XXLARGE { font-size : x-large } -BIG.HUGE { font-size : larger } -BIG.XHUGE { font-size : xx-large } - -/* heading styles */ -H1 { } -H2 { } -H3 { } -H4 { } -H5 { } - -/* mathematics styles */ -DIV.displaymath { } /* math displays */ -TD.eqno { } /* equation-number cells */ - - -/* document-specific styles come next */ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/sampleMathImages.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/sampleMathImages.html deleted file mode 100644 index 5e482e67124..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathImages/sampleMathImages.html +++ /dev/null @@ -1,169 +0,0 @@ - - - - - -sampleMathImages - - - - - - - - - - - - - - - - - - -next -up -previous -
    - Next: About this document ... -
    -
    - -

    -

    -Math examples -

    -
    -\begin{eqnarray}
-\phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\in...
-...\epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss}
-\end{eqnarray} -
    - -
    - -

    -Since (6) or (7d) should hold for arbitrary - -$ \delta\mathbf{c}$-vectors, it is clear that - -$ \mathcal{N}(A) = \mathcal{R}(B)$ and that when $ y=B(x)$ one has... -
    -...the Pythagorians knew infinitely many solutions in integers to - -$ a^2+b^2=c^2$. -That no non-trivial integer solutions exist for - -$ a^n+b^n=c^n$ with integers $ n>2$ has long -been suspected (Fermat, c.1637). Only during the current decade has this been proved (Wiles, 1995). - -

    -

    -
    -
    -
    -

    - -\begin{eqnarray}V \mathbf{\pi}^{sr} & = & \left< \sum_i M_i \mathbf{V}_i \mathbf...
-...m_i \sum_\alpha \mathbf{p}_{i\alpha} \mathbf{f}_{i\alpha} \right>
-\end{eqnarray} -
    -

    -

    -
    -
    - -

    -

    -
    - - - - -
    $\displaystyle \begin{align}B_{ij}^\alpha & = \left(B_{ij}^\alpha\right)_0 + \le...
-...} + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right)\end{align}$
    -
    -
    -

    - -Subsections - - - -

    -
    -Michel Goossens -
    1999-03-30 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb.dvi b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb.dvi deleted file mode 100644 index 4c1f556d437..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb.dvi and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb.tex deleted file mode 100644 index b6c61782721..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb.tex +++ /dev/null @@ -1,64 +0,0 @@ -\documentclass[a4paper,twoside]{article} -\usepackage{html} -\usepackage{amsmath} - -\renewcommand{\d}{\partial}\providecommand{\bm}[1]{\mathbf{#1}} -\providecommand{\Range}{\mathcal{R}}\providecommand{\Ker}{\mathcal{N}} -\providecommand{\Quat}{\vec{\mathbf{Q}}} - -\newcommand{\StAndrews}{\url{http://www-groups.dcs.st-and.ac.uk/~history}}% -\newcommand{\Pythagorians}{\htmladdnormallink - {Pythagorians}{\StAndrews/Mathematicians/Pythagoras.html}} -\newcommand{\Fermat}{\htmladdnormallink - {Fermat, c.1637}{\StAndrews/HistTopics/Fermat's_last_theorem.html}} -\newcommand{\Wiles}{\htmladdnormallink - {Wiles, 1995}{http://www.pbs.org:80/wgbh/nova/proof}} - -\begin{document} -\htmlhead[center]{section}{Math examples} -\begin{flushright} -\begin{makeimage} -\begin{eqnarray} - \phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty} - \exp \left( u \ln u + \lambda u \right ) du \hspace{1cm}\mbox{for } c \geq 0 \\ - \lambda & = & \frac{\epsilon -\bar{\epsilon} }{\xi} - - \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}} \\ - \gamma & = & 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)} \\ - \gamma' & = & 0.422784\dots = 1 - \gamma \\ - \epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss} -\end{eqnarray} -\end{makeimage} -\end{flushright} - -Since~\eqref{eqn:stress-sr} or~\eqref{gdef} should hold for arbitrary $\delta\bm{c}$% --vectors, it is clear that $\Ker(A) = \Range(B)$ and that when $y=B(x)$ one has...\\ -...the \Pythagorians{} knew infinitely many solutions in integers to $a^2+b^2=c^2$. -That no non-trivial integer solutions exist for $a^n+b^n=c^n$ with integers $n>2$ has long -been suspected (\Fermat). Only during the current decade has this been proved (\Wiles). - -\begin{flushright} -\begin{eqnarray}\htmlimage{thumbnail=.4} -\label{eqn:stress-sr} - V \bm{\pi}^{sr} & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i - + \sum_i \sum_{j>i} \bm{R}_{ij} \bm{F}_{ij}\right> \\ \nonumber - & = & \left< \sum_i M_i \bm{V}_i \bm{V}_i - + \sum_{i}\sum_{j>i}\sum_\alpha\sum_\beta \bm{r}_{i\alpha j\beta}\bm{f}_{i\alpha j\beta} - - \sum_i \sum_\alpha \bm{p}_{i\alpha} \bm{f}_{i\alpha} \right> -\end{eqnarray} -\end{flushright} - -\begin{flushright} -\begin{subequations}\htmlimage{thumbnail=.3} -\label{bgdefs} -\begin{align} B_{ij}^\alpha & = - \left(B_{ij}^\alpha\right)_0 + \left(B_{ij}^\alpha\right)_a \label{bdef} \\ - \left(B_{ij}^\alpha\right)_0 & = \frac{1}{2}\left(\frac{\d N_i^\alpha}{\d X_j} - + \frac{\d N_j^\alpha} {\d X_i} \right) \label{b0def} \\ - \left(B_{ij}^\alpha\right)_a & = H_{ij}^{\alpha \beta} a^\beta \label{budef} \\ - H_{ij}^{\alpha \beta} & = - \frac{1}{2}\left( \frac{\d N_k^\alpha}{\d X_i} \frac{\d N_k^\beta}{\d X_j} - + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right) \label{gdef} -\end{align} -\end{subequations} -\end{flushright} -\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/Timg8.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/Timg8.gif deleted file mode 100644 index 16c30f3cfe7..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/Timg8.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/Timg9.gif b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/Timg9.gif deleted file mode 100644 index c5e4abd0d6a..00000000000 Binary files a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/Timg9.gif and /dev/null differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/WARNINGS b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/WARNINGS deleted file mode 100644 index 9d1d9f764ee..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/WARNINGS +++ /dev/null @@ -1,2 +0,0 @@ - -redefining command \d diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/images.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/images.pl deleted file mode 100644 index ac47e21f1fb..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/images.pl +++ /dev/null @@ -1,68 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate images original text with physical files. - - -$key = q/{makeimage}eqnarray{phi(lambda)&=&frac{1}{2pii}int^{c+iinfty}_{c-iinfty}expleft(ar{epsilon}&=&mbox{actualslashaverageenergyloss}eqnarray{{makeimage};MSF=1.6;AAT/; -$cached_env_img{$key} = q|\begin{eqnarray}
-\phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\in...
-...\epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss}
-\end{eqnarray}|; - -$key = q/a^2+b^2=c^2;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ a^2+b^2=c^2$|; - -$key = q/n>2;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ n>2$|; - -$key = q/y=B(x);MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ y=B(x)$|; - -$key = q/a^n+b^n=c^n;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ a^n+b^n=c^n$|; - -$key = q/displaystylehtmlimage{thumbnail=.3}align{B_{ij}^alpha=left(B_{ij}^alphX_j}+frac{{d{N_k^beta}{{d{X_i}frac{{d{N_k^alpha}{{d{X_j}right)align{;MSF=1.6;AAT/; -$cached_env_img{$key} = q|$\displaystyle \begin{align}B_{ij}^\alpha & = \left(B_{ij}^\alpha\right)_0 + \le...
-...} + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right)\end{align}$|; - -$key = q/mathcal{N}(A)=mathcal{R}(B);MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ \mathcal{N}(A) = \mathcal{R}(B)$|; - -$key = q/{eqnarray}htmlimage{thumbnail=.4}Vmathbf{pi}^{sr}&=&left{eqnarray};MSF=1.6;TAGS=R;AAT/; -$cached_env_img{$key} = q|\begin{eqnarray}V \mathbf{\pi}^{sr} & = & \left< \sum_i M_i \mathbf{V}_i \mathbf...
-...m_i \sum_\alpha \mathbf{p}_{i\alpha} \mathbf{f}_{i\alpha} \right>
-\end{eqnarray}|; - -$key = q/deltamathbf{c};MSF=1.6;AAT/; -$cached_env_img{$key} = q|$ \delta\mathbf{c}$|; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/images.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/images.tex deleted file mode 100644 index 80070005079..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/images.tex +++ /dev/null @@ -1,213 +0,0 @@ -\batchmode -\documentclass[a4paper,twoside]{article} - -\usepackage{html} -\usepackage{amsmath} - -% -\renewcommand{\d}{\partial}% -\providecommand{\bm}[1]{\mathbf{#1}}% -\providecommand{\Range}{\mathcal{R}}% -\providecommand{\Ker}{\mathcal{N}}% -\providecommand{\Quat}{\vec{\mathbf{Q}}} -% -\providecommand{\StAndrews}{\url{http://www-groups.dcs.st-and.ac.uk/~history}}%% -\providecommand{\Pythagorians}{\htmladdnormallink - {Pythagorians}{\url{http://www-groups.dcs.st-and.ac.uk/~history}/Mathematicians/Pythagoras.html}}% -\providecommand{\Fermat}{\htmladdnormallink - {Fermat, c.1637}{\url{http://www-groups.dcs.st-and.ac.uk/~history}/HistTopics/Fermat's_last_theorem.html}}% -\providecommand{\Wiles}{\htmladdnormallink - {Wiles, 1995}{http://www.pbs.org:80/wgbh/nova/proof}} - -\usepackage[dvips]{color} -\pagecolor[gray]{.7} - - - -\makeatletter - -\makeatletter -\count@=\the\catcode`\_ \catcode`\_=8 -\newenvironment{tex2html_wrap}{}{} \catcode`\_=\count@ -\newcommand{\renewedcommand}[1]{\expandafter\renewcommand\csname #1\endcsname}% -\makeatother -\let\mathon=$ -\let\mathoff=$ -\ifx\AtBeginDocument\undefined \newcommand{\AtBeginDocument}[1]{}\fi -\newbox\sizebox -\setlength{\hoffset}{0pt}\setlength{\voffset}{0pt} -\addtolength{\textheight}{\footskip}\setlength{\footskip}{0pt} -\addtolength{\textheight}{\topmargin}\setlength{\topmargin}{0pt} -\addtolength{\textheight}{\headheight}\setlength{\headheight}{0pt} -\addtolength{\textheight}{\headsep}\setlength{\headsep}{0pt} -\setlength{\textwidth}{349pt} -\newwrite\lthtmlwrite -\makeatletter -\let\realnormalsize=\normalsize -\global\topskip=2sp -\def\preveqno{}\let\real@float=\@float \let\realend@float=\end@float -\def\@float{\let\@savefreelist\@freelist\real@float} -\def\end@float{\realend@float\global\let\@freelist\@savefreelist} -\let\real@dbflt=\@dbflt \let\end@dblfloat=\end@float -\let\@largefloatcheck=\relax -\let\if@boxedmulticols=\iftrue -\def\@dbflt{\let\@savefreelist\@freelist\real@dbflt} -\def\adjustnormalsize{\def\normalsize{\mathsurround=0pt \realnormalsize - 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- -\begin{document} -\pagestyle{empty}\thispagestyle{empty}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength hsize=\the\hsize}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength vsize=\the\vsize}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength hoffset=\the\hoffset}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength voffset=\the\voffset}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength topmargin=\the\topmargin}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength topskip=\the\topskip}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength headheight=\the\headheight}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength headsep=\the\headsep}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength parskip=\the\parskip}\lthtmltypeout{}% -\lthtmltypeout{latex2htmlLength oddsidemargin=\the\oddsidemargin}\lthtmltypeout{}% -\makeatletter -\if@twoside\lthtmltypeout{latex2htmlLength evensidemargin=\the\evensidemargin}% -\else\lthtmltypeout{latex2htmlLength evensidemargin=\the\oddsidemargin}\fi% -\lthtmltypeout{}% -\makeatother -\setcounter{page}{1} -\onecolumn - -% !!! IMAGES START HERE !!! - -{\newpage\clearpage -\lthtmldisplayA{makeimage29}% -\begin{eqnarray} - \phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty} - \exp \left( u \ln u + \lambda u \right ) du \hspace{1cm}\mbox{for } c \geq 0 \\ - \lambda & = & \frac{\epsilon -\bar{\epsilon} }{\xi} - - \gamma' - \beta^2 - \ln \frac{\xi} {E_{\rm max}} \\ - \gamma & = & 0.577215\dots \mathrm{\hspace{5mm}(Euler's\ constant)} \\ - \gamma' & = & 0.422784\dots = 1 - \gamma \\ - \epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss} -\end{eqnarray} -% -\lthtmldisplayZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_inline255}% -$ \delta\mathbf{c}$% -\lthtmlinlinemathZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_inline257}% -$ \mathcal{N}(A) = \mathcal{R}(B)$% -\lthtmlinlinemathZ -\lthtmlcheckvsize\clearpage} - -{\newpage\clearpage -\lthtmlinlinemathA{tex2html_wrap_inline259}% -$ y=B(x)$% -\lthtmlinlinemathZ -\lthtmlcheckvsize\clearpage} - 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- - - - -sampleMathThumb - - - - - - - - - - - - - - - - - - -next -up -previous -
    - Next: About this document ... -
    -
    - -

    -

    -Math examples -

    -
    -\begin{eqnarray}
-\phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\in...
-...\epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss}
-\end{eqnarray} -
    - -
    - -

    -Since (6) or (7d) should hold for arbitrary - -$ \delta\mathbf{c}$-vectors, it is clear that - -$ \mathcal{N}(A) = \mathcal{R}(B)$ and that when $ y=B(x)$ one has... -
    -...the Pythagorians knew infinitely many solutions in integers to - -$ a^2+b^2=c^2$. -That no non-trivial integer solutions exist for - -$ a^n+b^n=c^n$ with integers $ n>2$ has long -been suspected (Fermat, c.1637). Only during the current decade has this been proved (Wiles, 1995). - -

    -

    -
    -
    -
    -

    - -\begin{eqnarray}V \mathbf{\pi}^{sr} & = & \left< \sum_i M_i \mathbf{V}_i \mathbf...
-...m_i \sum_\alpha \mathbf{p}_{i\alpha} \mathbf{f}_{i\alpha} \right>
-\end{eqnarray} -
    -

    -

    -
    -
    - -

    -

    -
    - - - - -
    $\displaystyle \begin{align}B_{ij}^\alpha & = \left(B_{ij}^\alpha\right)_0 + \le...
-...} + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right)\end{align}$
    -
    -
    -

    - -Subsections - - - -

    -
    -Michel Goossens -
    1999-03-30 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/internals.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/internals.pl deleted file mode 100644 index 736c0485786..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/internals.pl +++ /dev/null @@ -1,30 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate internals original text with physical files. - - -$key = q/bdef/; -$ref_files{$key} = "$dir".q|sampleMathThumb.html|; -$noresave{$key} = "$nosave"; - -$key = q/b0def/; -$ref_files{$key} = "$dir".q|sampleMathThumb.html|; -$noresave{$key} = "$nosave"; - -$key = q/bgdefs/; -$ref_files{$key} = "$dir".q|sampleMathThumb.html|; -$noresave{$key} = "$nosave"; - -$key = q/eqn:stress-sr/; -$ref_files{$key} = "$dir".q|sampleMathThumb.html|; -$noresave{$key} = "$nosave"; - -$key = q/budef/; -$ref_files{$key} = "$dir".q|sampleMathThumb.html|; -$noresave{$key} = "$nosave"; - -$key = q/gdef/; -$ref_files{$key} = "$dir".q|sampleMathThumb.html|; -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/labels.pl b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/labels.pl deleted file mode 100644 index 3f2fa8c9444..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/labels.pl +++ /dev/null @@ -1,61 +0,0 @@ -# LaTeX2HTML 99.1 release (March 30, 1999) -# Associate labels original text with physical files. - - -$key = q/bdef/; -$external_labels{$key} = "$URL/" . q|sampleMathThumb.html|; -$noresave{$key} = "$nosave"; - -$key = q/b0def/; -$external_labels{$key} = "$URL/" . q|sampleMathThumb.html|; -$noresave{$key} = "$nosave"; - -$key = q/bgdefs/; -$external_labels{$key} = "$URL/" . q|sampleMathThumb.html|; -$noresave{$key} = "$nosave"; - -$key = q/eqn:stress-sr/; -$external_labels{$key} = "$URL/" . q|sampleMathThumb.html|; -$noresave{$key} = "$nosave"; - -$key = q/budef/; -$external_labels{$key} = "$URL/" . q|sampleMathThumb.html|; -$noresave{$key} = "$nosave"; - -$key = q/gdef/; -$external_labels{$key} = "$URL/" . q|sampleMathThumb.html|; -$noresave{$key} = "$nosave"; - -1; - - -# LaTeX2HTML 99.1 release (March 30, 1999) -# labels from external_latex_labels array. - - -$key = q/bdef/; -$external_latex_labels{$key} = q|7a|; -$noresave{$key} = "$nosave"; - -$key = q/b0def/; -$external_latex_labels{$key} = q|7b|; -$noresave{$key} = "$nosave"; - -$key = q/bgdefs/; -$external_latex_labels{$key} = q|7|; -$noresave{$key} = "$nosave"; - -$key = q/eqn:stress-sr/; -$external_latex_labels{$key} = q|6|; -$noresave{$key} = "$nosave"; - -$key = q/budef/; -$external_latex_labels{$key} = q|7c|; -$noresave{$key} = "$nosave"; - -$key = q/gdef/; -$external_latex_labels{$key} = q|7d|; -$noresave{$key} = "$nosave"; - -1; - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/node1.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/node1.html deleted file mode 100644 index fa3daa64290..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/node1.html +++ /dev/null @@ -1,73 +0,0 @@ - - - - - -About this document ... - - - - - - - - - - - - - - - - - -next - -up - -previous -
    - Up: sampleMathThumb - Previous: sampleMathThumb -
    -
    - - -

    -About this document ... -

    -

    -This document was generated using the -LaTeX2HTML translator Version 99.1 release (March 30, 1999) -

    -Copyright © 1993, 1994, 1995, 1996, -Nikos Drakos, -Computer Based Learning Unit, University of Leeds. -
    -Copyright © 1997, 1998, 1999, -Ross Moore, -Mathematics Department, Macquarie University, Sydney. -

    -The command line arguments were:
    - latex2html sampleMathThumb.tex -

    -The translation was initiated by Michel Goossens on 1999-03-30 -


    -
    -Michel Goossens -
    1999-03-30 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/sampleMathThumb.css b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/sampleMathThumb.css deleted file mode 100644 index 1993b851311..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/sampleMathThumb.css +++ /dev/null @@ -1,31 +0,0 @@ - -/* Century Schoolbook font is very similar to Computer Modern Math: cmmi */ -.MATH { font-family: "Century Schoolbook", serif; } -.MATH I { font-family: "Century Schoolbook", serif; font-shape: italic } -.BOLDMATH { font-family: "Century Schoolbook", serif; font-weight: bold } - -/* implement both fixed-size and relative sizes */ -SMALL.XTINY { font-size : xx-small } -SMALL.TINY { font-size : x-small } -SMALL.SCRIPTSIZE { font-size : smaller } -SMALL.FOOTNOTESIZE { font-size : small } -SMALL.SMALL { } -BIG.LARGE { } -BIG.XLARGE { font-size : large } -BIG.XXLARGE { font-size : x-large } -BIG.HUGE { font-size : larger } -BIG.XHUGE { font-size : xx-large } - -/* heading styles */ -H1 { } -H2 { } -H3 { } -H4 { } -H5 { } - -/* mathematics styles */ -DIV.displaymath { } /* math displays */ -TD.eqno { } /* equation-number cells */ - - -/* document-specific styles come next */ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/sampleMathThumb.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/sampleMathThumb.html deleted file mode 100644 index b8c1d4fd048..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/sampleMathThumb/sampleMathThumb.html +++ /dev/null @@ -1,171 +0,0 @@ - - - - - -sampleMathThumb - - - - - - - - - - - - - - - - - - -next -up -previous -
    - Next: About this document ... -
    -
    - -

    -

    -Math examples -

    -
    -\begin{eqnarray}
-\phi(\lambda) & = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\in...
-...\epsilon , \bar{\epsilon} & = & \mbox{actual/average energy loss}
-\end{eqnarray} -
    - -
    - -

    -Since (6) or (7d) should hold for arbitrary - -$ \delta\mathbf{c}$-vectors, it is clear that - -$ \mathcal{N}(A) = \mathcal{R}(B)$ and that when $ y=B(x)$ one has... -
    -...the Pythagorians knew infinitely many solutions in integers to - -$ a^2+b^2=c^2$. -That no non-trivial integer solutions exist for - -$ a^n+b^n=c^n$ with integers $ n>2$ has long -been suspected (Fermat, c.1637). Only during the current decade has this been proved (Wiles, 1995). - -

    -

    -
    -
    -
    -

    - -\begin{eqnarray}V \mathbf{\pi}^{sr} & = & \left< \sum_i M_i \mathbf{V}_i \mathbf...
-...m_i \sum_\alpha \mathbf{p}_{i\alpha} \mathbf{f}_{i\alpha} \right>
-\end{eqnarray} -
    -

    -

    -
    -
    - -

    -

    -
    - - - - -
    $\displaystyle \begin{align}B_{ij}^\alpha & = \left(B_{ij}^\alpha\right)_0 + \le...
-...} + \frac{\d N_k^\beta}{\d X_i} \frac{\d N_k^\alpha}{\d X_j} \right)\end{align}$
    -
    -
    -

    - -Subsections - - - -

    -
    -Michel Goossens -
    1999-03-30 -
    - - diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/tac2dim.eps b/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/tac2dim.eps deleted file mode 100644 index b96e3e23e90..00000000000 --- a/Master/texmf-dist/doc/latex/latex-web-companion/ch3bis/tac2dim.eps +++ /dev/null @@ -1,201 +0,0 @@ -%!CERNPS_include //ddtrg2/user/goossens/pawmanual/tutex21.ps -%%BoundingBox: 0 0 582 582 -/d {lineto} def /m {moveto} def /t {translate} def -/sw {stringwidth} def /r {rotate} def /rl {roll} def -/rd {rlineto} def /rm {rmoveto} def /gr {grestore} def -/lw {setlinewidth} def /sd {setdash} def -/s {stroke} def /rgb {setrgbcolor} def -/c {closepath} def /sf {scalefont setfont} def -/oshow {gsave [] 0 sd true charpath stroke gr} def -/cs {gsave dup sw pop 2 div neg 5 -1 rl 5 -1 rl t 3 -1 rl r 0 m show gr} def -/rs {gsave dup sw pop neg 5 -1 rl 5 -1 rl t 3 -1 rl r 0 m show gr} def -/ocs {gsave dup sw pop 2 div neg 5 -1 rl 5 -1 rl t 3 -1 rl r 0 m oshow gr} def -/ors {gsave dup 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+\newlabel{eq:flnsum}{{\rEfLiNK{1-6005r5}{5}}{\rEfLiNK{1-6005r5}{14}}} +\newlabel{eq:phys332-5}{{\rEfLiNK{1-7001r13}{13}}{\rEfLiNK{1-7001r13}{17}}} +\newlabel{eq:phys332-1}{{\rEfLiNK{1-7004r16}{16}}{\rEfLiNK{1-7004r16}{17}}} +\newlabel{eq:phys332-2}{{\rEfLiNK{1-7004r17}{17}}{\rEfLiNK{1-7004r17}{17}}} +\newlabel{eq:phys332-3}{{\rEfLiNK{1-7005r18}{18}}{\rEfLiNK{1-7005r18}{18}}} +\newlabel{eq:phys332-4}{{\rEfLiNK{1-7005r19}{19}}{\rEfLiNK{1-7005r19}{18}}} +\newlabel{eq:phys332-6}{{\rEfLiNK{1-7008r22}{22}}{\rEfLiNK{1-7008r22}{18}}} +\newlabel{eq:phys332-7}{{\rEfLiNK{1-7008r23}{23}}{\rEfLiNK{1-7008r23}{18}}} +\newlabel{eq:phys332-8}{{\rEfLiNK{1-7008r24}{24}}{\rEfLiNK{1-7008r24}{19}}} +\bibcite{bib-LAND}{1} +\bibcite{bib-SCH1}{2} +\bibcite{bib-SELT}{3} +\bibcite{bib-TALM}{4} +\bibcite{bib-VAVI}{5} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.css b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.css new file mode 100644 index 00000000000..333d950a156 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bold;} +/* end css.sty */ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.dvi b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.dvi new file mode 100644 index 00000000000..49e057e59c8 Binary files /dev/null and b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.dvi differ diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.html b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.html new file mode 100644 index 00000000000..7461e32259f --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.html @@ -0,0 +1,1510 @@ + + + + +Simulation of Energy Loss Straggling
    +

    Simulation of Energy Loss Straggling

    +
    Maria Physicist
    +
    +
    March 31, 1999
    +
    +

    1 Introduction

    +

    Due to the statistical nature of ionisation energy loss, large fluctuations can occur in +the amount of energy deposited by a particle traversing an absorber element. +Continuous processes such as multiple scattering and energy loss play a +relevant role in the longitudinal and lateral development of electromagnetic and +hadronic showers, and in the case of sampling calorimeters the measured +resolution can be significantly affected by such fluctuations in their active +layers. The description of ionisation fluctuations is characterised by the +significance parameter k, which is proportional to the ratio of mean energy loss to +the maximum allowed energy transfer in a single collision with an atomic +electron +

    +     q
+k = E----
+     max
    Emax +is the maximum transferable energy in a single collision with an atomic +electron. +
    +               2m b2g2
+Emax = ----------e----------2-,
+       1 +2gme/mx  + (me/mx)
    where +g = E/mx , E is energy and mx the mass of the incident particle, b2 = 1 - 1/g2 and +me is the electron mass. q comes from the Rutherford scattering cross section and is +defined as:
    +
    q = 2pz2e4NAvZrdx + meb2c2A = 153.4 z2 +b2 Z +Ardx keV,
    +
    where +
    + + + + + +
    z
    charge of the incident particle
    NAv
    Avogadro's number
    Z
    atomic number of the material
    A
    atomic weight of the material
    r
    density
    dx
    thickness of the material
    +
    +

    k measures the contribution of the collisions with energy transfer close to Emax. +For a given absorber, k tends towards large values if dx is large and/or if b is +small. Likewise, k tends towards zero if dx is small and/or if b approaches +1. +

    The value of k distinguishes two regimes which occur in the description of +ionisation fluctuations : +

      +
    1. A large number of collisions involving the loss of all or most of the incident + particle energy during the traversal of an absorber. +

      As the total energy transfer is composed of a multitude of small energy + losses, we can apply the central limit theorem and describe the fluctuations + by a Gaussian distribution. This case is applicable to non-relativistic + particles and is described by the inequality k > 10 (i.e. when the mean + energy loss in the absorber is greater than the maximum energy transfer + in a single collision). +

    2. +
    3. Particles traversing thin counters and incident electrons under any + conditions. +

      The relevant inequalities and distributions are 0.01 < k < 10, Vavilov + distribution, and k < 0.01, Landau distribution.

    +

    +

    An additional regime is defined by the contribution of the collisions with low +energy transfer which can be estimated with the relation q/I0, where I0 is the mean +ionisation potential of the atom. Landau theory assumes that the number of these +collisions is high, and consequently, it has a restriction q/I0 » 1. In GEANT (see URL +http://wwwinfo.cern.ch/asdoc/geant/geantall.html), the limit of Landau +theory has been set at q/I0 = 50. Below this limit special models taking into account +the atomic structure of the material are used. This is important in thin layers and +gaseous materials. Figure 1 shows the behaviour of q/I0 as a function of the layer +thickness for an electron of 100 keV and 1 GeV of kinetic energy in Argon, Silicon +and Uranium. + +


    +PIC +
    Figure 1The variable q/I0 can be used to measure the validity range of the +Landau theory. It depends on the type and energy of the particle, Z , A and the +ionisation potential of the material and the layer thickness.
    +

    +

    In the following sections, the different theories and models for the energy loss +fluctuation are described. First, the Landau theory and its limitations are discussed, +and then, the Vavilov and Gaussian straggling functions and the methods in the thin +layers and gaseous materials are presented. +

    2 Landau theory

    +

    For a particle of mass mx traversing a thickness of material dx, the Landau +probability distribution may be written in terms of the universal Landau function +f(c) as[1]:

    +
    f(e, dx)=1 + q f(c)
    +
    where
    + + + + + +
    f(c)= 1_ +2pi  integral + c - i oo c + i oo exp (u ln u+ cu) du      c > 0
    c =e - e + q - g' - b2 - ln q ___ +Emax
    g' =0.422784 . . . = 1 - g
    g =0.577215 . . . (Euler's constant)
    e =average energy loss
    e =actual energy loss
    +
    +

    2.1 Restrictions

    +

    The Landau formalism makes two restrictive assumptions : +

      +
    1. The typical energy loss is small compared to the maximum energy loss in + a single collision. This restriction is removed in the Vavilov theory (see + section 3). +
    2. +
    3. The typical energy loss in the absorber should be large compared to the + binding energy of the most tightly bound electron. For gaseous detectors, + typical energy losses are a few keV which is comparable to the binding + energies of the inner electrons. In such cases a more sophisticated approach + which accounts for atomic energy levels[4] is necessary to accurately + simulate data distributions. In GEANT, a parameterised model by L. Urbán + is used (see section 5).
    +

    +

    In addition, the average value of the Landau distribution is infinite. Summing the +Landau fluctuation obtained to the average energy from the dE/dx tables, we +obtain a value which is larger than the one coming from the table. The +probability to sample a large value is small, so it takes a large number of steps +(extractions) for the average fluctuation to be significantly larger than zero. This +introduces a dependence of the energy loss on the step size which can affect +calculations. +

    A solution to this has been to introduce a limit on the value of the variable +sampled by the Landau distribution in order to keep the average fluctuation to 0. +The value obtained from the GLANDO routine is: +

    +ddE/dx = e- e = q(c -g'+ b2 + ln--q-)
+                               Emax
    In +order for this to have average 0, we must impose that: +
    +c = -g'- b2 -ln -q---
+                Emax
    +

    This is realised introducing a cmax(c) such that if only values of c < cmax are +accepted, the average value of the distribution is c. +

    A parametric fit to the universal Landau distribution has been performed, with +following result: +

    +cmax = 0.60715+ 1.1934c + (0.67794+ 0.052382c)exp(0.94753 +0.74442c)
    +only values smaller than cmax are accepted, otherwise the distribution is +resampled. +

    3 Vavilov theory

    +

    Vavilov[5] derived a more accurate straggling distribution by introducing the +kinematic limit on the maximum transferable energy in a single collision, rather than +using Emax =  oo . Now we can write[2]:

    +
    f(e,ds)=1 + q fv(       )
+ cv,k,b2
    +
    where
    + + +
    fv(cv,k,b2)= 1_ +2pi  integral + c - i oo c + i oo f(s) ecsds      c > 0
    f(s) =exp [      2  ]
+ k(1+ b g)   exp [y(s)] ,
    y(s) =s ln k + (s + b2k)[ln(s/k)+ E1(s/k)] - ke-s/k,
    +
    and
    + +
    E1(z)= integral + z oo t-1e-tdt   (the exponential integral)
    cv =k[             ]
+ e--e - g'- b2
+   q
    +
    +

    The Vavilov parameters are simply related to the Landau parameter by +cL = cv/k - ln k. It can be shown that as k --> 0, the distribution of the variable cL +approaches that of Landau. For k < 0.01 the two distributions are already practically +identical. Contrary to what many textbooks report, the Vavilov distribution does not +approximate the Landau distribution for small k, but rather the distribution of cL +defined above tends to the distribution of the true c from the Landau density +function. Thus the routine GVAVIV samples the variable cL rather than cv. For +k > 10 the Vavilov distribution tends to a Gaussian distribution (see next +section). +

    4 Gaussian Theory

    +

    Various conflicting forms have been proposed for Gaussian straggling functions, but +most of these appear to have little theoretical or experimental basis. However, it has +been shown[3] that for k > 10 the Vavilov distribution can be replaced by a Gaussian +of the form :

    +
    f(e, ds)  ~~ 1 __________ +q V~ ------------
+  2pk (1- b2/2) exp [(e- e)2     k     ]
+ --------2-----2---
+    2   q (1- b /2)
    +
    thus implying
    + +
    mean=e
    s2 =q2 + k (1 - b2/2) = qE +max(1 - b2/2)
    +
    +

    5 Urbán model

    +

    The method for computing restricted energy losses with d-ray production +above given threshold energy in GEANT is a Monte Carlo method that can +be used for thin layers. It is fast and it can be used for any thickness of +a medium. Approaching the limit of the validity of Landau's theory, the +loss distribution approaches smoothly the Landau form as shown in Figure +2. + +


    +PIC +
    Figure 2Energy loss distribution for a 3 GeV electron in Argon as given by +standard GEANT. The width of the layers is given in centimeters.
    +

    +

    It is assumed that the atoms have only two energy levels with binding energy E1 +and E2. The particle--atom interaction will then be an excitation with energy loss E1 +or E2, or an ionisation with an energy loss distributed according to a function +g(E) ~ 1/E2:
    +
    +       (Emax +-I)I-1
+g(E) =    Emax   E2
    (1)
    +

    The macroscopic cross-section for excitations (i = 1, 2) is
    +
    +     f ln(2mb2g2/E  )- b2
+i = C-i-------2-2-i----2 (1- r)
+     Ei ln(2mb  g/I) - b
    (2)
    +and the macroscopic cross-section for ionisation is
    +
    +3 = C-------Emax---------r
+     I(Emax + I)ln(EmaIx+I)
    (3)
    +Emax is the GEANT cut for d-production, or the maximum energy transfer minus mean +ionisation energy, if it is smaller than this cut-off value. The following notation is +used: +

    + + +
    r, C
    parameters of the model
    Ei
    atomic energy levels
    I
    mean ionisation energy
    fi
    oscillator strengths
    +
    +

    The model has the parameters fi , Ei , C and r (0 < r < 1). The oscillator +strengths fi and the atomic level energies Ei should satisfy the constraints +

    + +
    f1 + f2 =1(4)
    f1 ln E1 + f2 ln E2=ln I(5)
    +
    The parameter C can be defined with the help of the mean energy loss dE/dx in the +following way: The numbers of collisions (ni , i = 1,2 for the excitation and 3 for the +ionisation) follow the Poisson distribution with a mean number <ni>. In a step x +the mean number of collisions is
    +
    +<n> =    x
+  i    i
    (6)
    +The mean energy loss dE/dx in a step is the sum of the excitation and ionisation +contributions
    +
    +        [                                 ]
+dE                        integral  Emax+I
+dx- x =   1E1 +  2E2 +  3        E g(E) dE   x
+                          I
    (7)
    +From this, using the equations (2), (3), (4) and (5), one can define the parameter C +
    +
    +C = dE-
+    dx
    (8)
    +

    The following values have been chosen in GEANT for the other parameters: +

    +    {
+       0    ifZ < 2
+f2 =   2/Z  ifZ > 2   ==>  f1 = 1- f2
+                              (    )f11
+E2 = 10Z2eV           ==>  E1 =   EIf2
+r = 0.4                           2
    With +these values the atomic level E2 corresponds approximately the K-shell energy of the +atoms and Zf2 the number of K-shell electrons. r is the only variable which can be +tuned freely. It determines the relative contribution of ionisation and excitation to +the energy loss. +

    The energy loss is computed with the assumption that the step length (or the +relative energy loss) is small, and---in consequence---the cross-section can be +considered constant along the path length. The energy loss due to the excitation is +
    +
    +Ee = n1E1 +n2E2
    (9)
    +where n1 and n2 are sampled from Poisson distribution as discussed above. The loss +due to the ionisation can be generated from the distribution g(E) by the inverse +transformation method:

    + + +
    u = F(E) = integral + IEg(x)dx
    E = F-1(u)= I_____ +1 - u Emax__ +Emax+I (10)
    (11)
    +
    where u is a uniform random number between F(I) = 0 and F(Emax + I) = 1. The +contribution from the ionisations will be
    +
    +     n sum 3 -----I------
+Ei =    1 -uj -Emax--
+     j=1      Emax+I
    (12)
    +where n3 is the number of ionisation (sampled from Poisson distribution). The +energy loss in a step will then be E = Ee + Ei. +

    5.1 Fast simulation for n3 > 16

    +

    If the number of ionisation n3 is bigger than 16, a faster sampling method can be +used. The possible energy loss interval is divided in two parts: one in which the +number of collisions is large and the sampling can be done from a Gaussian +distribution and the other in which the energy loss is sampled for each collision. Let +us call the former interval [I, aI] the interval A, and the latter [aI, Emax] the interval +B. a lies between 1 and Emax/I. A collision with a loss in the interval A happens +with the probability
    +
    +       integral  aI
+P(a) =    g(E)dE = (Emax-+-I)(a---1)
+       I                Emaxa
    (13)
    +The mean energy loss and the standard deviation for this type of collision are +
    +
    +          --1--  integral  aI          Ia-lna-
+<  E(a)> = P (a) I E g(E) dE =  a- 1
    (14)
    +and
    +
    +              integral  aI              (        2  )
+s2(a) =--1--    E2 g(E) dE = I2a  1 - -aln-a2
+       P (a) I                      (a- 1)
    (15)
    +If the collision number is high , we assume that the number of the type A collisions +can be calculated from a Gaussian distribution with the following mean value and +standard deviation:

    + +
    <nA>=n3P(a) (16)
    sA2 =n3P(a)(1 - P(a))(17)
    +
    It is further assumed that the energy loss in these collisions has a Gaussian +distribution with
    + +
    <EA>=nA<E(a)>(18)
    sE, A2=nAs2(a)(19)
    +
    The energy loss of these collision can then be sampled from the Gaussian +distribution. +

    The collisions where the energy loss is in the interval B are sampled directly from +
    +
    +      n3- sum  nA      aI
+EB  =      1--u-Emax+I-aI
+       i=1       i Emax+I
    (20)
    +The total energy loss is the sum of these two types of collisions:
    +
    +E =   EA +   EB
    (21)
    +

    The approximation of equations ((16), (17), (18) and (19) can be used under the +following conditions:

    + + +
    <nA> - c sA >0(22)
    <nA> + c sA <n3(23)
    <EA> - c sE,A>0(24)
    +
    where c > 4. From the equations (13), (16) and (18) and from the conditions (22) +and (23) the following limits can be derived:
    +
    +      (n3 + c2)(Emax + I)              (n3 + c2)(Emax +I)
+amin =---------------2- < a  < amax = -2---------------
+       n3(Emax + I)+ c I               c(Emax + I)+ n3I
    (25)
    +This conditions gives a lower limit to number of the ionisations n3 for which the fast +sampling can be done:
    +
    +n3  > c2
    (26)
    +As in the conditions (22), (23) and (24) the value of c is as minimum 4, one gets +n3 > 16. In order to speed the simulation, the maximum value is used for +a. +

    The number of collisions with energy loss in the interval B (the number of +interactions which has to be simulated directly) increases slowly with the total +number of collisions n3. The maximum number of these collisions can be estimated +as
    +
    +nB,max = n3 -nA,min  ~~  n3(<nA> - sA)
    (27)
    +From the previous expressions for <nA> and sA one can derive the condition +
    +
    +              -2n3c2-
+nB <  nB,max = n3 + c2
    (28)
    +The following values are obtained with c = 4: +

    + + + +
    n3
    nB,max
    n3
    nB,max





    16
    16
    200
    29.63
    20
    17.78
    500
    31.01
    50
    24.24
    1000
    31.50
    100
    27.59
     oo
    32.00
    +
    +

    5.2 Special sampling for lower part of the spectrum

    +

    If the step length is very small (< 5 mm in gases, < 2-3 mm in solids) the model gives +0 energy loss for some events. To avoid this, the probability of 0 energy loss is +computed
    +
    +             -(<n >+<n >+<n >)
+P(  E = 0) = e  1   2   3
    (29)
    +If the probability is bigger than 0.01 a special sampling is done, taking into +account the fact that in these cases the projectile interacts only with the outer +electrons of the atom. An energy level E0 = 10 eV is chosen to correspond to +the outer electrons. The mean number of collisions can be calculated from +
    +
    +      1 dE
+<n> = -----  x
+      E0 dx
    (30)
    +The number of collisions n is sampled from Poisson distribution. In the case of the +thin layers, all the collisions are considered as ionisations and the energy loss is +computed as
    +
    +     n
+     sum  -----E0------
+E =    1 - EEmax+E-ui
+    i=1     max  0
    (31)
    +

    References

    +

    + [1]   L.Landau. On the Energy Loss of Fast Particles by Ionisation. Originally + published in J. Phys., 8:201, 1944. Reprinted in D.ter Haar, Editor, + L.D.Landau, Collected papers , page 417. Pergamon Press, Oxford, 1965. +

    + [2]   B.Schorr. Programs for the Landau and the Vavilov distributions and + the corresponding random numbers. Comp. Phys. Comm., 7:216, 1974. +

    + [3]   S.M.Seltzer and M.J.Berger. Energy loss straggling of protons and + mesons. In Studies in Penetration of Charged Particles in Matter , Nuclear + Science Series 39, Nat. Academy of Sciences, Washington DC, 1964. +

    + [4]   R.Talman. On the statistics of particle identification using ionization. + Nucl. Inst. Meth., 159:189, 1979. +

    + [5]   P.V.Vavilov. Ionisation losses of high energy heavy particles. Soviet + Physics JETP , 5:749, 1957.

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pages, 73912 bytes). diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.otc b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.otc new file mode 100644 index 00000000000..43614e1f94f --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.otc @@ -0,0 +1,13 @@ +\expandafter\ifx\csname doTocEntry\endcsname\relax \expandafter\endinput\fi +\doTocEntry\tocsection{1}{\csname a:TocEntry\endcsname{1}{QQ1-1-1}{QQ2-1-1}{Introduction}}{2}\relax +\doTocEntry\toclof{1}{\Link{1-10061}{}\ignorespaces The variable $\xi /I_0$ can be used to measure the validity range of the Landau theory. It depends on the type and energy of the particle, $Z$, $A$ and the ionisation potential of the material and the layer thickness. \EndLink}{figure} +\doTocEntry\tocsection{2}{\csname a:TocEntry\endcsname{1}{QQ1-1-3}{QQ2-1-3}{Landau theory}}{7}\relax +\doTocEntry\tocsubsection{2.1}{\csname a:TocEntry\endcsname{1}{QQ1-1-4}{QQ2-1-4}{Restrictions}}{7}\relax +\doTocEntry\tocsection{3}{\csname a:TocEntry\endcsname{1}{QQ1-1-5}{QQ2-1-5}{Vavilov theory}}{9}\relax +\doTocEntry\tocsection{4}{\csname a:TocEntry\endcsname{1}{QQ1-1-6}{QQ2-1-6}{Gaussian Theory}}{10}\relax +\doTocEntry\tocsection{5}{\csname a:TocEntry\endcsname{1}{QQ1-1-7}{QQ2-1-7}{Urb\protect\' an model}}{10}\relax +\doTocEntry\toclof{2}{\Link{1-60012}{}\ignorespaces Energy loss distribution for a 3 GeV electron in Argon as given by standard \protect\texttt {GEANT}. The width of the layers is given in centimeters.\EndLink}{figure} +\doTocEntry\tocsubsection{5.1}{\csname a:TocEntry\endcsname{1}{QQ1-1-9}{QQ2-1-9}{Fast simulation for $n_3 \geq 16$}}{16}\relax +\doTocEntry\tocsubsection{5.2}{\csname a:TocEntry\endcsname{1}{QQ1-1-10}{QQ2-1-10}{Special sampling for lower part of the spectrum}}{20}\relax +\doTocEntry\toclikesection{}{\csname a:TocEntry\endcsname{1}{QQ1-1-11}{QQ2-1-11}{References}}{21}\relax +\par diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.tex b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.tex new file mode 100644 index 00000000000..faa7158a0ca --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.tex @@ -0,0 +1,549 @@ +\documentclass{article} +\usepackage{graphicx} +\usepackage{url} +\title{Simulation of Energy Loss Straggling} +\author{Maria Physicist} +\newcommand{\Emax}{\ensuremath{E_{\mathrm{max}}}} +\newcommand{\GEANT}{\texttt{GEANT}} +\usepackage[T1]{fontenc} +\usepackage{em} +\usepackage{tex4ht} +\begin{document} +\maketitle + +\section{Introduction} + +Due to the statistical nature of ionisation energy loss, large +fluctuations can occur in the amount of energy deposited by a particle +traversing an absorber element. Continuous processes such as multiple +scattering and energy loss play a relevant role in the longitudinal +and lateral development of electromagnetic and hadronic +showers, and in the case of sampling calorimeters the +measured resolution can be significantly affected by such fluctuations +in their active layers. The description of ionisation fluctuations is +characterised by the significance parameter $\kappa$, which is +proportional to the ratio of mean energy loss to the maximum allowed +energy transfer in a single collision with an atomic electron +\[ +\kappa =\frac{\xi}{\Emax} +\] +\Emax{} +is the maximum transferable energy in a single collision with +an atomic electron. +\[ +\Emax =\frac{2 m_e \beta^2\gamma^2 } +{1 + 2\gamma m_e/m_x + \left ( m_e/m_x\right)^2}, +\] +where $\gamma = E/m_x$, $E$ is energy and +$m_x$ the mass of the incident particle, +$\beta^2 = 1 - 1/\gamma^2$ and $m_e$ is the electron mass. +$\xi$ comes from the Rutherford scattering cross section +and is defined as: +\begin{eqnarray*} \xi = \frac{2\pi z^2 e^4 N_{Av} Z \rho \delta x} + {m_e \beta^2 c^2 A} = 153.4 \frac{z^2} {\beta^2} \frac{Z}{A} + \rho \delta x \quad\mathrm{keV}, +\end{eqnarray*} +where + +\begin{tabular}{ll} +$z$ & charge of the incident particle \\ +$N_{Av}$ & Avogadro's number \\ +$Z$ & atomic number of the material \\ +$A$ & atomic weight of the material \\ +$\rho$ & density \\ +$ \delta x$ & thickness of the material \\ +\end{tabular} + +$\kappa$ measures the contribution of the collisions with energy +transfer close to \Emax. For a given absorber, $\kappa$ tends +towards large values if $\delta x$ is large and/or if $\beta$ is +small. Likewise, $\kappa$ tends towards zero if $\delta x $ is small +and/or if $\beta$ approaches 1. + +The value of $\kappa$ distinguishes two regimes which occur in the +description of ionisation fluctuations : + +\begin{enumerate} +\item A large number of collisions involving the loss of all or most + of the incident particle energy during the traversal of an absorber. + + As the total energy transfer is composed of a multitude of small + energy losses, we can apply the central limit theorem and describe + the fluctuations by a Gaussian distribution. This case is + applicable to non-relativistic particles and is described by the + inequality $\kappa > 10 $ (i.e. when the mean energy loss in the + absorber is greater than the maximum energy transfer in a single + collision). + +\item Particles traversing thin counters and incident electrons under + any conditions. + + The relevant inequalities and distributions are $ 0.01 < \kappa < 10 + $, Vavilov distribution, and $\kappa < 0.01 $, Landau distribution. +\end{enumerate} + +An additional regime is defined by the contribution of the collisions +with low energy transfer which can be estimated with the relation +$\xi/I_0$, where $I_0$ is the mean ionisation potential of the atom. +Landau theory assumes that the number of these collisions is high, and +consequently, it has a restriction $\xi/I_0 \gg 1$. In \GEANT{} +(see URL \url{http://wwwinfo.cern.ch/asdoc/geant/geantall.html}), the +limit of Landau theory has been set at $\xi/I_0 = 50$. Below this +limit special models taking into account the atomic structure of the +material are used. This is important in thin layers and gaseous +materials. Figure \ref{fg:phys332-1} shows the behaviour of $\xi/I_0$ +as a function of the layer thickness for an electron of 100 keV and 1 +GeV of kinetic energy in Argon, Silicon and Uranium. + +\begin{figure} + \centering + \includegraphics[width=.6\linewidth]{phys332-1} + \caption{The variable $\xi/I_0$ can be used to measure the + validity range of the Landau theory. It depends + on the type and energy of the particle, $Z$, $A$ + and the ionisation potential of the material and + the layer thickness. + } + \label{fg:phys332-1} +\end{figure} + +In the following sections, the different theories and models for the +energy loss fluctuation are described. First, the Landau theory and +its limitations are discussed, and then, the Vavilov and Gaussian +straggling functions and the methods in the thin layers and gaseous +materials are presented. + +\section{Landau theory} +\label{sec:phys332-1} + +For a particle of mass $m_x$ traversing a thickness of material +$\delta x $, the Landau probability distribution may be written in +terms of the universal Landau function $\phi(\lambda)$ +as\cite{bib-LAND}: +\begin{eqnarray*} +f( \epsilon , \delta x ) & = &\frac{1}{\xi} \phi ( \lambda ) +\end{eqnarray*} +where +\begin{eqnarray*} +\phi(\lambda )& = & \frac{1} {2 \pi i}\int^{c+i\infty}_{c-i\infty} +\exp \left ( u \ln u + \lambda u \right ) du \hspace{2cm} c \geq 0 \\ +\lambda & = & \frac{\epsilon -\bar{\epsilon} }{\xi} + - \gamma' - \beta^2 - \ln \frac{\xi}{\Emax} \\ +\gamma' & = & 0.422784\dots = 1 - \gamma \\ +\gamma & = & 0.577215\dots \mbox{(Euler's constant)} \\ +\bar{\epsilon} & = & \mbox{average energy loss} \\ +\epsilon & = & \mbox{actual energy loss} +\end{eqnarray*} + +\subsection{Restrictions} + +The Landau formalism makes two restrictive assumptions : +\begin{enumerate} +\item The typical energy loss is small compared to the maximum energy + loss in a single collision. This restriction is removed in the + Vavilov theory (see section \ref{vavref}). +\item The typical energy loss in the absorber should be large compared + to the binding energy of the most tightly bound electron. For + gaseous detectors, typical energy losses are a few keV which is + comparable to the binding energies of the inner electrons. In such + cases a more sophisticated approach which accounts for atomic energy + levels\cite{bib-TALM} is necessary to accurately simulate data + distributions. In \GEANT, a parameterised model by L. Urb\'{a}n is + used (see section \ref{urban}). +\end{enumerate} + +In addition, the average value of the Landau distribution is infinite. +Summing the Landau fluctuation obtained to the average energy from the +$dE/dx$ tables, we obtain a value which is larger than the one coming +from the table. The probability to sample a large value is small, so +it takes a large number of steps (extractions) for the average +fluctuation to be significantly larger than zero. This introduces a +dependence of the energy loss on the step size which can affect +calculations. + +A solution to this has been to introduce a limit on the value of the +variable sampled by the Landau distribution in order to keep the +average fluctuation to 0. The value obtained from the \texttt{GLANDO} +routine is: +\[ +\delta dE/dx = \epsilon - \bar{\epsilon} = \xi ( \lambda - \gamma' ++\beta^2 +\ln \frac{\xi}{\Emax}) +\] +In order for this to have average 0, we must impose that: +\[ +\bar{\lambda} = -\gamma' - \beta^2 -\ln \frac{\xi}{\Emax} +\] + +This is realised introducing a $\lambda_{\mathrm{max}}(\bar{\lambda})$ +such that if only values of $\lambda \leq \lambda_{\mathrm{max}}$ are +accepted, the average value of the distribution is $\bar{\lambda}$. + +A parametric fit to the universal Landau distribution has been +performed, with following result: +\[ +\lambda_{\mathrm{max}} = 0.60715 + + 1.1934\bar{\lambda}+(0.67794+0.052382\bar{\lambda}) + \exp(0.94753+0.74442\bar{\lambda}) +\] +only values smaller than $\lambda_{\mathrm{max}}$ are accepted, otherwise the +distribution is resampled. + + + +\newpage +\section{Vavilov theory} +\label{vavref} + +Vavilov\cite{bib-VAVI} derived a more accurate straggling distribution +by introducing the kinematic limit on the maximum transferable energy +in a single collision, rather than using $ \Emax = \infty $. +Now we can write\cite{bib-SCH1}: +\begin{eqnarray*} +f \left ( \epsilon, \delta s \right ) & = & \frac{1}{\xi} \phi_{v} +\left ( \lambda_{v}, \kappa, \beta^{2} \right ) +\end{eqnarray*} +where +\begin{eqnarray*} +\phi_{v} \left ( \lambda_{v}, \kappa, \beta^{2} \right ) & = & +\frac{1}{2 \pi i} \int^{c+i\infty}_{c-i\infty}\phi \left( s \right ) +e^{\lambda s} ds \hspace{2cm} c \geq 0 \\ +\phi \left ( s \right ) & = & +\exp \left [ \kappa ( 1 + \beta^{2}\gamma ) \right ] +~ \exp \left [ \psi \left ( s \right ) \right ], \\ +\psi \left ( s \right ) & = & s \ln \kappa + ( s + \beta^{2} \kappa ) +\left [ \ln (s/\kappa) + E_{1} (s/\kappa) \right ] - \kappa e^{-s/\kappa}, +\end{eqnarray*} +and +\begin{eqnarray*} +E_{1}(z) & = & \int^{\infty}_{z} t^{-1} e^{-t} dt +\mbox{\hspace{1cm} (the exponential integral)} \\ +\lambda_v & = & \kappa \left [ \frac{\epsilon - \bar{\epsilon}}{\xi} +- \gamma' - \beta^2 \right] +\end{eqnarray*} + +The Vavilov parameters are simply related to the Landau parameter by +$\lambda_L = \lambda_v/\kappa - \ln\kappa $. It can be shown that as +$\kappa \rightarrow 0$, the distribution of the variable $\lambda_L$ +approaches that of Landau. For $\kappa \leq 0.01$ the two +distributions are already practically identical. Contrary to what many +textbooks report, the Vavilov distribution \emph{does not} approximate +the Landau distribution for small $\kappa$, but rather the +distribution of $\lambda_L$ defined above tends to the distribution of +the true $\lambda$ from the Landau density function. Thus the routine +\texttt{GVAVIV} samples the variable $\lambda_L$ rather than +$\lambda_v$. For $\kappa \geq 10$ the Vavilov distribution tends to a +Gaussian distribution (see next section). + +\section{Gaussian Theory} + +Various conflicting forms have been proposed for Gaussian straggling +functions, but most of these appear to have little theoretical or +experimental basis. However, it has been shown\cite{bib-SELT} that +for $\kappa \geq 10 $ the Vavilov distribution can be replaced by a +Gaussian of the form : +\begin{eqnarray*} +f( \epsilon , \delta s) \approx \frac{1} +{\xi \sqrt{\frac{2 \pi}{\kappa} \left( 1 - \beta^2/2 \right)}} + \exp \left [ \frac{( \epsilon - \bar{\epsilon} )^2}{2} \frac{\kappa} + {\xi^2 (1- \beta^2/2)}\right ] +\end{eqnarray*} +thus implying +\begin{eqnarray*} +\mathrm{mean} & = & \bar{\epsilon} \\ +\sigma^2 & = & \frac{\xi^2}{\kappa} (1-\beta^2/2) = \xi + \Emax (1-\beta^2/2) +\end{eqnarray*} + +\section{Urb\'an model} +\label{urban} + +The method for computing restricted energy losses with $\delta$-ray +production above given threshold energy in \GEANT{} is a Monte +Carlo method that can be used for thin layers. It is fast and it can +be used for any thickness of a medium. Approaching the limit of the +validity of Landau's theory, the loss distribution approaches smoothly +the Landau form as shown in Figure \ref{fg:phys332-2}. +\begin{figure} + \centering + \includegraphics[width=.6\linewidth]{phys332-2} + \caption{Energy loss distribution for a 3 GeV electron in + Argon as given by standard \GEANT. The width of the layers is + given in centimeters.} + \label{fg:phys332-2} +\end{figure} + +It is assumed that the atoms have only two energy levels with binding +energy $E_1$ and $E_2$. The particle--atom interaction will then be +an excitation with energy loss $E_1$ or $E_2$, or an ionisation with +an energy loss distributed according to a function $g(E) \sim 1/E^2$: +\begin{equation} +g(E) = \frac{(\Emax + I)I}{\Emax} \frac{1}{E^2} +\end{equation} + +The macroscopic cross-section for excitations ($i=1,2$) is +\begin{equation} +\label{eq:sigex} +\Sigma_i = C \frac{f_i}{E_i} \frac{\ln (2 m \beta^2 \gamma^2/E_i) - \beta^2} + {\ln (2 m \beta^2 \gamma^2/ I) - \beta^2}(1-r) +\end{equation} +and the macroscopic cross-section for ionisation is +\begin{equation} +\label{eq:sigion} +\Sigma_3 = C \frac{\Emax}{I(\Emax+I) \ln(\frac{\Emax+I}{I})} + ~ r +\end{equation} +\Emax{} is the \GEANT{} cut for $\delta$-production, or the maximum +energy transfer minus mean ionisation energy, if it is smaller than +this cut-off value. The following notation is used: + +\begin{tabular}{ll} +$r, C$ & parameters of the model \\ +$E_i$ & atomic energy levels \\ +$I$ & mean ionisation energy \\ +${f_i}$ & oscillator strengths +\end{tabular} + +The model has the parameters $f_i$, $E_i$, $C$ and $r ~(0\leq r\leq +1)$. The oscillator strengths $f_i$ and the atomic level energies +$E_i$ should satisfy the constraints +\begin{eqnarray} +f_1 + f_2 & = & 1 \label{eq:fisum}\\ +f_1 \ln E_1 + f_2 \ln E_2 & = & \ln I \label{eq:flnsum} +\end{eqnarray} +The parameter $C$ can be defined with the help of the mean energy loss +$dE/dx$ in the following way: The numbers of collisions ($n_i$, i = +1,2 for the excitation and 3 for the ionisation) follow the Poisson +distribution with a mean number $ \langle n_i \rangle $. In a step +$\Delta x$ the mean number of collisions is +\begin{equation} +\langle n_i \rangle = \Sigma_i \Delta x +\end{equation} +The mean energy loss $dE/dx$ in a step is the sum of the excitation +and ionisation contributions +\begin{equation} +\frac{dE}{dx} \Delta x = \left[ \Sigma_1 E_1 + \Sigma_2 E_2 + + \Sigma_3 \int_{I}^{\Emax+I} E~g(E)~dE \right] + \Delta x +\end{equation} +From this, using the equations (\ref{eq:sigex}), (\ref{eq:sigion}), +(\ref{eq:fisum}) and (\ref{eq:flnsum}), one can define the parameter +$C$ +\begin{equation} +C = \frac{dE}{dx} +\end{equation} + +The following values have been chosen in \GEANT{} for the other +parameters: +\[ +\begin{array}{lcl} +f_2 = \left\{ \begin{array}{ll} + 0 & \mathrm{if}\, Z \leq 2 \\ + 2/Z & \mathrm{if}\, Z > 2 \\ + \end{array} \right. & \Rightarrow & f_1 = 1 - f_2 \\ +E_2 = 10 Z^2 \mathrm{eV} & \Rightarrow & E_1 = \left(\frac{I}{E_{2}^{f_2}} + \right)^{\frac{1}{f_1}} \\ +r = 0.4 & & \\ +\end{array} +\] +With these values the atomic level $E_2$ corresponds approximately +the K-shell energy of the atoms and $Zf_2$ the number of K-shell +electrons. $r$ is the only variable which can be tuned freely. It +determines the relative contribution of ionisation and +excitation to the energy loss. + +The energy loss is computed with the assumption that the step length +(or the relative energy loss) is small, and---in consequence---the +cross-section can be considered constant along the path length. The +energy loss due to the excitation is +\begin{equation} +\Delta E_e = n_1 E_1 + n_2 E_2 +\end{equation} +where $n_1$ and $n_2$ are sampled from Poisson distribution as +discussed above. The loss due to the ionisation can be generated from +the distribution $g(E)$ by the inverse transformation method: +\begin{eqnarray} +u = F(E) & = & \int_{I}^E g(x) dx \nonumber \\ +E = F^{-1}(u) & = & \frac{I}{1 - u \frac {\Emax}{\Emax+I}} \\ +\end{eqnarray} +where $u$ is a uniform random number between $F(I)=0$ and +$F(\Emax+I)=1$. The contribution from the ionisations will be +\begin{equation} +\Delta E_i = \sum_{j=1}^{n_3} \frac{I} + {1 - u_j \frac {\Emax}{\Emax + I}} +\end{equation} +where $n_3$ is the number of ionisation (sampled from Poisson +distribution). The energy loss in a step will then be $\Delta E = +\Delta E_e + \Delta E_i$. + +\subsection{Fast simulation for $n_3 \geq 16$} + +If the number of ionisation $n_3$ is bigger than 16, a faster sampling +method can be used. The possible energy loss interval is divided in +two parts: one in which the number of collisions is large and the +sampling can be done from a Gaussian distribution and the other in +which the energy loss is sampled for each collision. Let us call the +former interval $[I, \alpha I]$ the interval A, and the latter +$[\alpha I,\Emax]$ the interval B. $\alpha$ lies between 1 and +$\Emax/I$. A collision with a loss in the interval A happens with +the probability +\begin{equation} +\label{eq:phys332-5} +P(\alpha) = \int_I^{\alpha I} g(\!E\!) \, dE = + \frac {( \Emax + I) (\alpha - 1)}{\Emax \alpha} +\end{equation} +The mean energy loss and the standard deviation for this type +of collision are +\begin{equation} +\langle \Delta E(\alpha) \rangle = \frac{1}{P(\alpha)} + \int_I^{\alpha I} E \, g(\!E\!) \, dE = + \frac{I \alpha \ln \alpha}{\alpha - 1} +\end{equation} +and +\begin{equation} +\sigma^2(\alpha) = \frac{1}{P(\alpha)} + \int_I^{\alpha I} E^2 \, g(\!E\!) \, dE = + I^2 \alpha \left( 1 - \frac{\alpha \ln \! ^2 \alpha}{(\alpha - 1)^2} \right) +\end{equation} +If the collision number is high , we assume that the number of the +type A collisions can be calculated from a Gaussian distribution +with the following mean value and standard deviation: +\begin{eqnarray} +\label{eq:phys332-1} +\langle n_A \rangle & = & n_3 P(\alpha) \\ +\label{eq:phys332-2} +\sigma_A^2 & = & n_3 P(\alpha) ( 1 - P(\alpha)) +\end{eqnarray} +It is further assumed that the energy loss in these collisions +has a Gaussian distribution with +\begin{eqnarray} +\label{eq:phys332-3} +\langle \Delta E_A \rangle & = & n_A \langle \Delta E(\alpha) \rangle \\ +\label{eq:phys332-4} +\sigma_{E,A}^2 & = & n_A \sigma^2(\alpha) +\end{eqnarray} +The energy loss of these collision can then be sampled from the +Gaussian distribution. + +The collisions where the energy loss is in the interval B are sampled +directly from +\begin{equation} +\Delta E_B = \sum_{i=1}^{n_3 - n_A} \frac{\alpha I} + {1 - u_i \frac{\Emax + I - \alpha I}{\Emax + I}} +\end{equation} +The total energy loss is the sum of these two types of collisions: +\begin{equation} +\Delta E = \Delta E_A + \Delta E_B +\end{equation} + +The approximation of equations ((\ref{eq:phys332-1}), +(\ref{eq:phys332-2}), (\ref{eq:phys332-3}) and (\ref{eq:phys332-4}) +can be used under the following conditions: +\begin{eqnarray} +\label{eq:phys332-6} +\langle n_A \rangle - c \, \sigma_A & \geq & 0 \\ +\label{eq:phys332-7} +\langle n_A \rangle + c \, \sigma_A & \leq & n_3 \\ +\label{eq:phys332-8} +\langle \Delta E_A \rangle - c \, \sigma_{E,A} & \geq & 0 +\end{eqnarray} +where $c \geq 4$. From the equations (\ref{eq:phys332-5}), +(\ref{eq:phys332-1}) and (\ref{eq:phys332-3}) and from the conditions +(\ref{eq:phys332-6}) and (\ref{eq:phys332-7}) the following limits can +be derived: +\begin{equation} +\alpha_{\mathrm{min}} = \frac{(n_3 + c^2)(\Emax+I)} + {n_3 (\Emax + I) + c^2 I} \; \leq \alpha \; \leq +\alpha_{\mathrm{max}} = \frac{(n_3 + c^2)(\Emax+I)} + {c^2 (\Emax + I) + n_3 I} +\end{equation} +This conditions gives a lower limit to number of the ionisations $n_3$ +for which the fast sampling can be done: +\begin{equation} +n_3 \; \geq \; c^2 +\end{equation} +As in the conditions (\ref{eq:phys332-6}), (\ref{eq:phys332-7}) and +(\ref{eq:phys332-8}) the value of $c$ is as minimum 4, one gets $n_3 +\; \geq 16$. In order to speed the simulation, the maximum value is +used for $\alpha$. + +The number of collisions with energy loss in the interval B (the +number of interactions which has to be simulated directly) increases +slowly with the total number of collisions $n_3$. The maximum number +of these collisions can be estimated as +\begin{equation} +n_{B,max} = n_3 - n_{A,min} \approx n_3 (\langle n_A \rangle + - \sigma_A) +\end{equation} +From the previous expressions for $\langle n_A \rangle$ and $\sigma_A$ +one can derive the condition +\begin{equation} +n_B \; \leq \; n_{B,max} = \frac{2 n_3 c^2}{n_3+c^2} +\end{equation} +The following values are obtained with $c=4$: + +\begin{tabular}{llcrr} +$n_3$ & $n_{B,max}$ & & $n_3$ & $n_{B,max}$\\ \hline +16 & 16 & & 200 & 29.63\\ +20 & 17.78 & & 500 & 31.01 \\ +50 & 24.24 & & 1000 & 31.50 \\ +100 & 27.59 & & $\infty$ & 32.00 +\end{tabular} + +\subsection{Special sampling for lower part of the spectrum} + +If the step length is very small ($\leq 5$ mm in gases, $\leq$ 2-3 +$\mu$m in solids) the model gives 0 energy loss for some events. To +avoid this, the probability of 0 energy loss is computed +\begin{equation} +P( \Delta E=0) = e^{-( \langle n_1 \rangle + \langle n_2 \rangle + + \langle n_3 \rangle )} +\end{equation} +If the probability is bigger than 0.01 a special sampling is done, +taking into account the fact that in these cases the projectile +interacts only with the outer electrons of the atom. An energy level +$E_0 = 10$ eV is chosen to correspond to the outer electrons. The mean +number of collisions can be calculated from +\begin{equation} +\langle n \rangle = \frac{1}{E_0} \frac{dE}{dx} \Delta x +\end{equation} +The number of collisions $n$ is sampled from Poisson distribution. +In the case of the thin layers, all the collisions are considered as +ionisations and the energy loss is computed as +\begin{equation} +\Delta E = \sum_{i=1}^n \frac{E_0} + {1 - \frac {\Emax}{\Emax + E_0} u_i} +\end{equation} + +\begin{thebibliography}{10} +\bibitem{bib-LAND} +L.Landau. +\newblock On the Energy Loss of Fast Particles by Ionisation. +\newblock Originally published in \emph{J. Phys.}, 8:201, 1944. +\newblock Reprinted in D.ter Haar, Editor, \emph{L.D.Landau, Collected + papers}, page 417. Pergamon Press, Oxford, 1965. + +\bibitem{bib-SCH1} +B.Schorr. +\newblock Programs for the Landau and the Vavilov distributions and the + corresponding random numbers. +\newblock \emph{Comp. Phys. Comm.}, 7:216, 1974. + +\bibitem{bib-SELT} +S.M.Seltzer and M.J.Berger. +\newblock Energy loss straggling of protons and mesons. +\newblock In \emph{Studies in Penetration of Charged Particles in + Matter}, Nuclear Science Series~39, Nat. Academy of Sciences, + Washington DC, 1964. + +\bibitem{bib-TALM} +R.Talman. +\newblock On the statistics of particle identification using ionization. +\newblock \emph{Nucl. Inst. Meth.}, 159:189, 1979. + +\bibitem{bib-VAVI} +P.V.Vavilov. +\newblock Ionisation losses of high energy heavy particles. +\newblock \emph{Soviet Physics JETP}, 5:749, 1957. +\end{thebibliography} + +\end{document} diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.toc b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.toc new file mode 100644 index 00000000000..15064d9096e --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/latexexa.toc @@ -0,0 +1,12 @@ +\expandafter\ifx\csname doTocEntry\endcsname\relax \expandafter\endinput\fi +\doTocEntry\tocsection{1}{\csname a:TocEntry\endcsname{1}{QQ1-1-1}{QQ2-1-1}{Introduction}}{2}\relax +\doTocEntry\toclof{1}{\Link{1-10061}{}\ignorespaces The variable $\xi /I_0$ can be used to measure the validity range of the Landau theory. It depends on the type and energy of the particle, $Z$, $A$ and the ionisation potential of the material and the layer thickness. \EndLink}{figure} +\doTocEntry\tocsection{2}{\csname a:TocEntry\endcsname{1}{QQ1-1-3}{QQ2-1-3}{Landau theory}}{7}\relax +\doTocEntry\tocsubsection{2.1}{\csname a:TocEntry\endcsname{1}{QQ1-1-4}{QQ2-1-4}{Restrictions}}{7}\relax +\doTocEntry\tocsection{3}{\csname a:TocEntry\endcsname{1}{QQ1-1-5}{QQ2-1-5}{Vavilov theory}}{9}\relax +\doTocEntry\tocsection{4}{\csname a:TocEntry\endcsname{1}{QQ1-1-6}{QQ2-1-6}{Gaussian Theory}}{10}\relax +\doTocEntry\tocsection{5}{\csname a:TocEntry\endcsname{1}{QQ1-1-7}{QQ2-1-7}{Urb\protect\' an model}}{10}\relax +\doTocEntry\toclof{2}{\Link{1-60012}{}\ignorespaces Energy loss distribution for a 3 GeV electron in Argon as given by standard \protect\texttt {GEANT}. 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+ gsave 679 1852 + t 0 r 0 0 m + /Helvetica-Bold findfont 78 sf 0 0 m +(1 GeV) + show + gr + gsave 223 1907 + t 0 r 0 0 m + /Helvetica-Bold findfont 78 sf 0 0 m +(100 keV) + show + gr + /xs 0 def +(Step,\040) + /Helvetica-Bold 43 stwn +(\133) + /Special 43 stwn +(cm) + /Helvetica-Bold 43 stwn +(\135) + /Special 43 stwn + gsave 2041 104 + t 0 r xs neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(Step,\040) + show + currentpoint pop 0 t + /Special findfont 43 sf 0 0 m +(\133) + show + currentpoint pop 0 t + /Helvetica-Bold findfont 43 sf 0 0 m +(cm) + show + currentpoint pop 0 t + /Special findfont 43 sf 0 0 m +(\135) + show + gr + gsave 57 2009 + t 0 r 0 0 m + /Symbol findfont 43 sf 0 0 m +(x) + show + currentpoint pop 0 t + /Helvetica-Bold findfont 43 sf 0 0 m +(/I) + show + currentpoint pop 0 t + /Helvetica-Bold findfont 30 sf 0 -14 m +(0) + show + gr +gr gr showpage +end +%%EOF diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch4/phys332-2.eps b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/phys332-2.eps new file mode 100644 index 00000000000..e255ddadf55 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/phys332-2.eps @@ -0,0 +1,556 @@ +%!PS-Adobe-2.0 EPSF-2.0 +%%BoundingBox: 0 0 567 567 +%%Title: curves.eps +%%Creator: HIGZ Version 1.19/01 +%%CreationDate: 93/07/16 12.02 +%%EndComments +80 dict begin +/s {stroke} def /l {lineto} def /m {moveto} def /t { translate} def +/sw {stringwidth} def /r {rotate} def /rl {roll} def +/d {rlineto} def /rm {rmoveto} def /gr {grestore} def /f {eofill} def +/c {setrgbcolor} def /lw {setlinewidth} def /sd {setdash} def +/cl {closepath} def /sf {scalefont setfont} def +/box {m dup 0 exch d exch 0 d 0 exch neg d cl} def +/bl {box s} def /bf {box f} def +/mp {newpath /y exch def /x exch def} def +/side {[w .77 mul w .23 mul] .385 w mul sd w 0 l currentpoint t -144 r} def +/mr {mp x y w2 0 360 arc} def /m24 {mr s} def /m20 {mr f} def +/mb {mp x y w2 add m w2 neg 0 d 0 w neg d w 0 d 0 w d cl} def +/mt {mp x y w2 add m w2 neg w neg d w 0 d cl} def +/m21 {mb f} def /m25 {mb s} def /m22 {mt f} def /m26 {mt s} def +/m23 {mp x y w2 sub m w2 w d w neg 0 d cl f} def + /m27 {mp x y w2 add m w3 neg w2 neg d w3 w2 neg d w3 w2 d cl s} def + /m28 {mp x w2 sub y w2 sub w3 add m w3 0 d 0 w3 neg d w3 0 d 0 w3 d w3 0 d + 0 w3 d w3 neg 0 d 0 w3 d w3 neg 0 d 0 w3 neg d w3 neg 0 d cl s } def + /m29 {mp gsave x w2 sub y w2 add w3 sub m currentpoint t + 4 {side} repeat cl fill gr} def + /m30 {mp gsave x w2 sub y w2 add w3 sub m currentpoint t + 5 {side} repeat s gr} def /m31 {mp x y w2 sub m 0 w d x w2 sub y m w 0 d + x w2 sub y w2 add m w w neg d x w2 sub y w2 + sub m w w d s} def +/m2 {mp x y w2 sub m 0 w d x w2 sub y m w 0 d s} def +/m5 {mp x w2 sub y w2 sub m w w d x w2 sub y w2 add m w w neg d s} def +/reencdict 24 dict def /ReEncode {reencdict begin /nco&na exch def +/nfnam exch def /basefontname exch def /basefontdict basefontname findfont def +/newfont basefontdict maxlength dict def basefontdict {exch dup /FID ne +{dup /Encoding eq {exch dup length array copy newfont 3 1 roll put} {exch +newfont 3 1 roll put} ifelse} {pop pop} ifelse } forall newfont +/FontName nfnam put nco&na aload pop nco&na length 2 idiv {newfont +/Encoding get 3 1 roll put} repeat nfnam newfont definefont pop end } def +/accvec [ 176 /agrave 181 /Agrave 190 /acircumflex 192 /Acircumflex +201 /adieresis 204 /Adieresis 209 /ccedilla 210 /Ccedilla 211 /eacute +212 /Eacute 213 /egrave 214 /Egrave 215 /ecircumflex 216 /Ecircumflex +217 /edieresis 218 /Edieresis 219 /icircumflex 220 /Icircumflex +221 /idieresis 222 /Idieresis 223 /ntilde 224 /Ntilde 226 /ocircumflex +228 /Ocircumflex 229 /odieresis 230 /Odieresis 231 /ucircumflex 236 /Ucircumflex +237 /udieresis 238 /Udieresis 239 /aring 242 /Aring 243 /ydieresis +244 /Ydieresis 246 /aacute 247 /Aacute 252 /ugrave 253 /Ugrave] def +/Times-Roman /Times-Roman accvec ReEncode +/Times-Italic /Times-Italic accvec ReEncode +/Times-Bold /Times-Bold accvec ReEncode +/Times-BoldItalic /Times-BoldItalic accvec ReEncode +/Helvetica /Helvetica accvec ReEncode +/Helvetica-Oblique /Helvetica-Oblique accvec ReEncode +/Helvetica-Bold /Helvetica-Bold accvec ReEncode +/Helvetica-BoldOblique /Helvetica-BoldOblique accvec ReEncode +/Courier /Courier accvec ReEncode +/Courier-Oblique /Courier-Oblique accvec ReEncode +/Courier-Bold /Courier-Bold accvec ReEncode +/Courier-BoldOblique /Courier-BoldOblique accvec ReEncode +/oshow {gsave [] 0 sd true charpath stroke gr} def +/stwn { /fs exch def /fn exch def /text exch def fn findfont fs sf + text sw pop xs add /xs exch def} def +/stwb { /fs exch def /fn exch def /nbas exch def /textf exch def +textf length /tlen exch def nbas tlen gt {/nbas tlen def} if +fn findfont fs sf textf dup length nbas sub nbas getinterval sw +pop neg xs add /xs exch def} def +/accspe [ 65 /plusminus 66 /bar 67 /existential 68 /universal +69 /exclam 70 /numbersign 71 /greater 72 /question 73 /integral +74 /colon 75 /semicolon 76 /less 77 /bracketleft 78 /bracketright +79 /greaterequal 80 /braceleft 81 /braceright 82 /radical +83 /spade 84 /heart 85 /diamond 86 /club 87 /lessequal +88 /multiply 89 /percent 90 /infinity 48 /circlemultiply 49 /circleplus +50 /emptyset 51 /lozenge 52 /bullet 53 /arrowright 54 /arrowup +55 /arrowleft 56 /arrowdown 57 /arrowboth 48 /degree 44 /comma 43 /plus + 45 /angle 42 /angleleft 47 /divide 61 /notequal 40 /equivalence 41 /second + 97 /approxequal 98 /congruent 99 /perpendicular 100 /partialdiff 101 /florin + 102 /intersection 103 /union 104 /propersuperset 105 /reflexsuperset + 106 /notsubset 107 /propersubset 108 /reflexsubset 109 /element 110 /notelement + 111 /gradient 112 /logicaland 113 /logicalor 114 /arrowdblboth + 115 /arrowdblleft 116 /arrowdblup 117 /arrowdblright 118 /arrowdbldown + 119 /ampersand 120 /omega1 121 /similar 122 /aleph ] def +/Symbol /Special accspe ReEncode +gsave .25 .25 scale +%%EndProlog + gsave 0 0 t 0 setgray 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/Helvetica-Bold findfont 43 sf 0 0 m +(300) + show + gr + /xs 0 def +(400) + /Helvetica-Bold 43 stwn + gsave 181 957 + t 0 r xs neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(400) + show + gr + /xs 0 def +(500) + /Helvetica-Bold 43 stwn + gsave 181 1144 + t 0 r xs neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(500) + show + gr + /xs 0 def +(600) + /Helvetica-Bold 43 stwn + gsave 181 1331 + t 0 r xs neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(600) + show + gr + /xs 0 def +(700) + /Helvetica-Bold 43 stwn + gsave 181 1517 + t 0 r xs neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(700) + show + gr + /xs 0 def +(800) + /Helvetica-Bold 43 stwn + gsave 181 1704 + t 0 r xs neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(800) + show + gr + /xs 0 def +(900) + /Helvetica-Bold 43 stwn + gsave 181 1891 + t 0 r xs neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(900) + show + gr + 1 lw 227 227 m 2041 227 l s 4 lw 227 261 m 227 227 l s 263 244 m 263 227 l s + 299 244 m 299 227 l s 336 244 m 336 227 l s 372 244 m 372 227 l s 408 261 m 408 + 227 l s 445 244 m 445 227 l s 481 244 m 481 227 l s 517 244 m 517 227 l s 553 + 244 m 553 227 l s 590 261 m 590 227 l s 626 244 m 626 227 l s 662 244 m 662 227 + l s 699 244 m 699 227 l s 735 244 m 735 227 l s 771 261 m 771 227 l s 807 244 m + 807 227 l s 844 244 m 844 227 l s 880 244 m 880 227 l s 916 244 m 916 227 l s + 953 261 m 953 227 l s 989 244 m 989 227 l s 1025 244 m 1025 227 l s 1061 244 m + 1061 227 l s 1098 244 m 1098 227 l s 1134 261 m 1134 227 l s 1170 244 m 1170 + 227 l s 1207 244 m 1207 227 l s 1243 244 m 1243 227 l s 1279 244 m 1279 227 l s + 1315 261 m 1315 227 l s 1352 244 m 1352 227 l s 1388 244 m 1388 227 l s 1424 + 244 m 1424 227 l s 1461 244 m 1461 227 l s 1497 261 m 1497 227 l s 1533 244 m + 1533 227 l s 1569 244 m 1569 227 l s 1606 244 m 1606 227 l s 1642 244 m 1642 + 227 l s 1678 261 m 1678 227 l s 1715 244 m 1715 227 l s 1751 244 m 1751 227 l s + 1787 244 m 1787 227 l s 1823 244 m 1823 227 l s 1860 261 m 1860 227 l s 1896 + 244 m 1896 227 l s 1932 244 m 1932 227 l s 1969 244 m 1969 227 l s 2005 244 m + 2005 227 l s 2041 261 m 2041 227 l s + /xs 0 def +(0) + /Helvetica-Bold 43 stwn + gsave 227 172 + t 0 r xs 2 div neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(0) + show + gr + /xs 0 def +(0.01) + /Helvetica-Bold 43 stwn + gsave 408 172 + t 0 r xs 2 div neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(0.01) + show + gr + /xs 0 def +(0.02) + /Helvetica-Bold 43 stwn + gsave 590 172 + t 0 r xs 2 div neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(0.02) + show + gr + /xs 0 def +(0.03) + /Helvetica-Bold 43 stwn + gsave 771 172 + t 0 r xs 2 div neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(0.03) + show + gr + /xs 0 def +(0.04) + /Helvetica-Bold 43 stwn + gsave 953 172 + t 0 r xs 2 div neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(0.04) + show + gr + /xs 0 def +(0.05) + /Helvetica-Bold 43 stwn + gsave 1134 172 + t 0 r xs 2 div neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(0.05) + show + gr + /xs 0 def +(0.06) + /Helvetica-Bold 43 stwn + gsave 1315 172 + t 0 r xs 2 div neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(0.06) + show + gr + /xs 0 def +(0.07) + /Helvetica-Bold 43 stwn + gsave 1497 172 + t 0 r xs 2 div neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(0.07) + show + gr + /xs 0 def +(0.08) + /Helvetica-Bold 43 stwn + gsave 1678 172 + t 0 r xs 2 div neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(0.08) + show + gr + /xs 0 def +(0.09) + /Helvetica-Bold 43 stwn + gsave 1860 172 + t 0 r xs 2 div neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(0.09) + show + gr + /xs 0 def +(0.1) + /Helvetica-Bold 43 stwn + gsave 2041 172 + t 0 r xs 2 div neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(0.1) + show + gr + /xs 0 def +(x 10) + /Helvetica-Bold 43 stwn + gsave 2041 109 + t 0 r xs 2 div neg 0 t 0 0 m + /Helvetica-Bold findfont 43 sf 0 0 m +(x 10) + show + gr + /xs 0 def +(-4) + /Helvetica-Bold 35 stwn + gsave 2105 141 + t 0 r xs 2 div neg 0 t 0 0 m + /Helvetica-Bold findfont 35 sf 0 0 m +(-4) + show + gr + [12 12] 0 sd 227 227 m 227 227 l 249 227 l 272 227 l 295 227 l 318 227 l 340 + 227 l 363 227 l 386 227 l 408 227 l 431 227 l 454 227 l 476 227 l 499 227 l 522 + 227 l 544 227 l 544 229 l 567 229 l 567 232 l 590 232 l 590 270 l 612 270 l 612 + 352 l 635 352 l 635 546 l 658 546 l 658 901 l 680 901 l 680 1199 l 703 1199 l + 703 1490 l 726 1490 l 726 1628 l 748 1628 l 748 1533 l 771 1533 l 771 1404 l + 794 1404 l 794 1048 l 816 1048 l 816 738 l 839 738 l 839 572 l 862 572 l 862 + 417 l 885 417 l 885 331 l 907 331 l 907 272 l 930 272 l 930 244 l 953 244 l 953 + 231 l 975 231 l 998 231 l 998 227 l 1021 227 l 1043 227 l 1066 227 l 1089 227 l + 1111 227 l 1134 227 l 1157 227 l 1179 227 l 1202 227 l 1225 227 l 1247 227 l + 1270 227 l 1293 227 l 1315 227 l 1338 227 l 1361 227 l 1361 227 l 1383 227 l + 1406 227 l 1429 227 l 1452 227 l 1474 227 l 1497 227 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247 l 454 247 l 454 277 l 476 277 l 476 324 l 499 324 l 499 419 l 522 + 419 l 522 544 l 544 544 l 544 600 l 567 600 l 567 738 l 590 738 l 590 742 l 612 + 742 l 612 830 l 635 830 l 635 798 l 658 798 l 658 789 l 680 789 l 680 764 l 703 + 764 l 703 772 l 726 772 l 726 766 l 748 766 l 748 691 l 771 691 l 771 596 l 794 + 596 l 794 619 l 816 619 l 816 565 l 839 565 l 839 553 l 862 553 l 862 479 l 885 + 479 l 885 430 l 907 430 l 907 423 l 930 423 l 930 456 l 953 456 l 953 393 l 975 + 393 l 975 361 l 998 361 l 998 359 l 1021 359 l 1021 346 l 1043 346 l 1043 329 l + 1066 329 l 1066 307 l 1089 307 l 1089 285 l 1111 285 l 1111 294 l 1134 294 l + 1134 281 l 1157 281 l 1157 270 l 1179 270 l 1179 260 l 1202 260 l 1202 247 l + 1225 247 l 1247 247 l 1247 245 l 1270 245 l 1270 234 l 1293 234 l 1315 234 l + 1338 234 l 1361 234 l 1361 244 l 1383 244 l 1383 229 l 1406 229 l 1406 232 l + 1429 232 l 1429 229 l 1452 229 l 1452 231 l 1474 231 l 1474 227 l 1497 227 l + 1497 229 l 1520 229 l 1520 227 l 1542 227 l 1542 231 l 1565 231 l 1565 229 l + 1588 229 l 1610 229 l 1610 227 l 1633 227 l 1656 227 l 1678 227 l 1701 227 l + 1724 227 l 1746 227 l 1769 227 l 1792 227 l 1814 227 l 1837 227 l 1860 227 l + 1882 227 l 1905 227 l 1928 227 l 1928 227 l 1950 227 l 1973 227 l 1996 227 l + 2019 227 l 2041 227 l s [] 0 sd 227 227 m 227 231 l 249 231 l 249 234 l 272 234 + l 272 249 l 295 249 l 295 266 l 318 266 l 318 270 l 340 270 l 340 300 l 363 300 + l 363 384 l 386 384 l 386 460 l 408 460 l 408 499 l 431 499 l 431 570 l 454 570 + l 454 667 l 476 667 l 476 691 l 499 691 l 499 706 l 522 706 l 522 699 l 544 699 + l 544 706 l 567 706 l 567 660 l 590 660 l 590 671 l 612 671 l 612 585 l 635 585 + l 635 563 l 658 563 l 658 559 l 680 559 l 680 555 l 703 555 l 703 490 l 726 490 + l 726 434 l 748 434 l 748 454 l 771 454 l 771 423 l 794 423 l 794 395 l 816 395 + l 816 393 l 839 393 l 839 389 l 862 389 l 862 331 l 885 331 l 885 348 l 907 348 + l 907 328 l 930 328 l 930 331 l 953 331 l 953 315 l 975 315 l 975 326 l 998 326 + l 998 303 l 1021 303 l 1021 309 l 1043 309 l 1043 287 l 1066 287 l 1066 303 l + 1089 303 l 1089 313 l 1111 313 l 1111 292 l 1134 292 l 1134 279 l 1157 279 l + 1157 272 l 1179 272 l 1179 292 l 1202 292 l 1202 305 l 1225 305 l 1225 257 l + 1247 257 l 1247 268 l 1270 268 l 1270 273 l 1293 273 l 1293 268 l 1315 268 l + 1315 270 l 1338 270 l 1338 255 l 1361 255 l 1361 259 l 1383 259 l 1383 255 l + 1406 255 l 1406 266 l 1429 266 l 1429 249 l 1452 249 l 1452 251 l 1474 251 l + 1474 268 l 1497 268 l 1497 244 l 1520 244 l 1520 238 l 1542 238 l 1542 244 l + 1565 244 l 1588 244 l 1588 247 l 1610 247 l 1633 247 l 1633 242 l 1656 242 l + 1656 238 l 1678 238 l 1678 240 l 1701 240 l 1701 245 l 1724 245 l 1724 244 l + 1746 244 l 1746 234 l 1769 234 l 1792 234 l 1814 234 l 1837 234 l 1837 238 l + 1860 238 l 1860 236 l 1882 236 l 1882 238 l 1905 238 l 1905 232 l 1928 232 l + 1928 232 l 1950 232 l 1950 236 l 1973 236 l 1973 234 l 1996 234 l 2019 234 l + 2019 236 l 2041 236 l 2041 227 l s [12 12] 0 sd 227 227 m 227 326 l 249 326 l + 249 268 l 272 268 l 272 354 l 295 354 l 295 404 l 318 404 l 318 406 l 340 406 l + 340 473 l 363 473 l 363 516 l 386 516 l 386 542 l 408 542 l 408 652 l 431 652 l + 431 654 l 454 654 l 454 593 l 476 593 l 476 667 l 499 667 l 499 568 l 522 568 l + 522 637 l 544 637 l 544 682 l 567 682 l 567 587 l 590 587 l 590 598 l 612 598 l + 612 496 l 635 496 l 635 522 l 658 522 l 658 527 l 680 527 l 680 466 l 703 466 l + 703 464 l 726 464 l 726 440 l 748 440 l 748 436 l 771 436 l 771 371 l 794 371 l + 794 400 l 816 400 l 816 384 l 839 384 l 839 341 l 862 341 l 862 335 l 885 335 l + 885 301 l 907 301 l 907 324 l 930 324 l 930 313 l 953 313 l 953 316 l 975 316 l + 975 296 l 998 296 l 998 285 l 1021 285 l 1021 288 l 1043 288 l 1043 279 l 1066 + 279 l 1066 268 l 1089 268 l 1089 260 l 1111 260 l 1111 283 l 1134 283 l 1134 + 255 l 1157 255 l 1157 266 l 1179 266 l 1179 255 l 1202 255 l 1202 259 l 1225 + 259 l 1225 245 l 1247 245 l 1247 251 l 1270 251 l 1270 245 l 1293 245 l 1293 + 257 l 1315 257 l 1315 251 l 1338 251 l 1338 245 l 1361 245 l 1361 242 l 1383 + 242 l 1383 255 l 1406 255 l 1406 236 l 1429 236 l 1429 242 l 1452 242 l 1452 + 249 l 1474 249 l 1474 257 l 1497 257 l 1497 238 l 1520 238 l 1542 238 l 1542 + 240 l 1565 240 l 1588 240 l 1588 242 l 1610 242 l 1610 244 l 1633 244 l 1633 + 253 l 1656 253 l 1656 247 l 1678 247 l 1678 245 l 1701 245 l 1701 253 l 1724 + 253 l 1724 240 l 1746 240 l 1746 238 l 1769 238 l 1769 242 l 1792 242 l 1792 + 240 l 1814 240 l 1814 249 l 1837 249 l 1837 236 l 1860 236 l 1860 240 l 1882 + 240 l 1905 240 l 1905 242 l 1928 242 l 1928 240 l 1950 240 l 1950 231 l 1973 + 231 l 1973 240 l 1996 240 l 1996 247 l 2019 247 l 2019 244 l 2041 244 l 2041 + 227 l s +gr gr showpage +end +%%EOF diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch4/tex4ht.env b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/tex4ht.env new file mode 100644 index 00000000000..4787cd8341c --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/tex4ht.env @@ -0,0 +1,70 @@ +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +% tex4ht.env / .tex4ht % +% % +% Notes: % +% 1. empty lines are harmful % +% 2. place this file in your work % +% directory and/or root directory % +% and/or in directory `xxx' of your % +% choice. In the latest case, compile % +% tex4ht.c with `#define HTFDIR xxx' % +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +% Replace the directories `candy/...' % +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +tcandy/tex/texmf/fonts/tfm/! +tcandy/tex/texmf/fonts/vf/! +icandy/tex4ht.dir/ +icandy/tex4ht.dir/ht-fonts/iso88591/! +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +% aliases for .htf fonts % +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +acmbsy cmsy +acmbx cmr +acmitt cmtt +acmsl cmr +acmss cmti +acmtcsc cmtt +acmtex cmtt +acmu cmti +aptmb cmr +aptmr7 cmr +aptmri cmti +% To activate the following aliases, +% remove the leading space character + adcbx ectt + adccc ecsx + adcit ectt + adcr ectt + adcsi ecsx + adcsl ecsx + adcss ecsx + adctc ecsx + adcti ectt + aecbx ec + aecsl ec + aecsltt ec + aectt ec + apcrb7t pcrr7t + apcrro7t pcrr7t + aphvr7t ptmr7t + aptmb7t ptmr7t + aptmr8t ectt + aptmri8t ectt + aptmro7t ptmr7t + awncyi wncyr +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +% Default scripts, shifted rightward 1 pos +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +s--- needs --- %%1.idv[%%2] ==> /tmp/%%3 --- + b--- characters --- + g.gif +Gdvips -Pem -f %%1 -pp %%2 > tmp.ps +Gconvert -crop 0x0 -density 110x110 -transparency '#FFFFFF' tmp.ps %%3 +S* +% t4ht -d%%2 +Mmv %%1 %%2%%3 +Ccp %%1 %%2%%3 +% t4ht -d%%2 -m%%1 +Achmod %%1 %%2%%3 +Hgold/tex4ht.dir/ + diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch4/tex4ht.tmp b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/tex4ht.tmp new file mode 100644 index 00000000000..41b58e2cf47 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/tex4ht.tmp @@ -0,0 +1,2 @@ + +/* css.sty */ \ No newline at end of file diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch4/tmp.ps b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/tmp.ps new file mode 100644 index 00000000000..21e63e4bf00 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch4/tmp.ps @@ -0,0 +1,542 @@ +%!PS-Adobe-2.0 +%%Creator: dvips(k) 5.85 Copyright 1999 Radical Eye Software +%%Title: latexexa.idv +%%Pages: 1 +%%PageOrder: Ascend +%%BoundingBox: 0 0 596 842 +%%DocumentFonts: EMR10 EMMI7 +%%DocumentPaperSizes: a4 +%%EndComments +%DVIPSWebPage: (www.radicaleye.com) +%DVIPSCommandLine: dvips -Pem -f latexexa.idv -pp 66 +%DVIPSParameters: dpi=600, compressed +%DVIPSSource: TeX output 1999.03.31:0915 +%%BeginProcSet: texc.pro +%! +/TeXDict 300 dict def TeXDict begin/N{def}def/B{bind def}N/S{exch}N/X{S +N}B/A{dup}B/TR{translate}N/isls false N/vsize 11 72 mul N/hsize 8.5 72 +mul N/landplus90{false}def/@rigin{isls{[0 landplus90{1 -1}{-1 1}ifelse 0 +0 0]concat}if 72 Resolution div 72 VResolution div neg scale isls{ +landplus90{VResolution 72 div vsize mul 0 exch}{Resolution -72 div hsize +mul 0}ifelse TR}if Resolution VResolution vsize -72 div 1 add mul TR[ +matrix currentmatrix{A A round sub abs 0.00001 lt{round}if}forall round +exch round exch]setmatrix}N/@landscape{/isls true N}B/@manualfeed{ +statusdict/manualfeed true put}B/@copies{/#copies X}B/FMat[1 0 0 -1 0 0] +N/FBB[0 0 0 0]N/nn 0 N/IEn 0 N/ctr 0 N/df-tail{/nn 8 dict N nn begin +/FontType 3 N/FontMatrix fntrx N/FontBBox FBB N string/base X array +/BitMaps X/BuildChar{CharBuilder}N/Encoding IEn N end A{/foo setfont}2 +array copy cvx N load 0 nn put/ctr 0 N[}B/sf 0 N/df{/sf 1 N/fntrx FMat N +df-tail}B/dfs{div/sf X/fntrx[sf 0 0 sf neg 0 0]N df-tail}B/E{pop nn A +definefont setfont}B/Cw{Cd A length 5 sub get}B/Ch{Cd A length 4 sub get +}B/Cx{128 Cd A length 3 sub get sub}B/Cy{Cd A length 2 sub get 127 sub} +B/Cdx{Cd A length 1 sub get}B/Ci{Cd A type/stringtype ne{ctr get/ctr ctr +1 add N}if}B/id 0 N/rw 0 N/rc 0 N/gp 0 N/cp 0 N/G 0 N/CharBuilder{save 3 +1 roll S A/base get 2 index get S/BitMaps get S get/Cd X pop/ctr 0 N Cdx +0 Cx Cy Ch sub Cx Cw add Cy setcachedevice Cw Ch true[1 0 0 -1 -.1 Cx +sub Cy .1 sub]/id Ci N/rw Cw 7 add 8 idiv string N/rc 0 N/gp 0 N/cp 0 N{ +rc 0 ne{rc 1 sub/rc X rw}{G}ifelse}imagemask restore}B/G{{id gp get/gp +gp 1 add N A 18 mod S 18 idiv pl S get exec}loop}B/adv{cp add/cp X}B +/chg{rw cp id gp 4 index getinterval putinterval A gp add/gp X adv}B/nd{ +/cp 0 N rw exit}B/lsh{rw cp 2 copy get A 0 eq{pop 1}{A 255 eq{pop 254}{ +A A add 255 and S 1 and or}ifelse}ifelse put 1 adv}B/rsh{rw cp 2 copy +get A 0 eq{pop 128}{A 255 eq{pop 127}{A 2 idiv S 128 and or}ifelse} +ifelse put 1 adv}B/clr{rw cp 2 index string putinterval adv}B/set{rw cp +fillstr 0 4 index getinterval putinterval adv}B/fillstr 18 string 0 1 17 +{2 copy 255 put pop}for N/pl[{adv 1 chg}{adv 1 chg nd}{1 add chg}{1 add +chg nd}{adv lsh}{adv lsh nd}{adv rsh}{adv rsh nd}{1 add adv}{/rc X nd}{ +1 add set}{1 add clr}{adv 2 chg}{adv 2 chg nd}{pop nd}]A{bind pop} +forall N/D{/cc X A type/stringtype ne{]}if nn/base get cc ctr put nn +/BitMaps get S ctr S sf 1 ne{A A length 1 sub A 2 index S get sf div put +}if put/ctr ctr 1 add N}B/I{cc 1 add D}B/bop{userdict/bop-hook known{ +bop-hook}if/SI save N @rigin 0 0 moveto/V matrix currentmatrix A 1 get A +mul exch 0 get A mul add .99 lt{/QV}{/RV}ifelse load def pop pop}N/eop{ +SI restore userdict/eop-hook known{eop-hook}if showpage}N/@start{ +userdict/start-hook known{start-hook}if pop/VResolution X/Resolution X +1000 div/DVImag X/IEn 256 array N 2 string 0 1 255{IEn S A 360 add 36 4 +index cvrs cvn put}for pop 65781.76 div/vsize X 65781.76 div/hsize X}N +/p{show}N/RMat[1 0 0 -1 0 0]N/BDot 260 string N/Rx 0 N/Ry 0 N/V{}B/RV/v{ +/Ry X/Rx X V}B statusdict begin/product where{pop false[(Display)(NeXT) +(LaserWriter 16/600)]{A length product length le{A length product exch 0 +exch getinterval eq{pop true exit}if}{pop}ifelse}forall}{false}ifelse +end{{gsave TR -.1 .1 TR 1 1 scale Rx Ry false RMat{BDot}imagemask +grestore}}{{gsave TR -.1 .1 TR Rx Ry scale 1 1 false RMat{BDot} +imagemask grestore}}ifelse B/QV{gsave newpath transform round exch round +exch itransform moveto Rx 0 rlineto 0 Ry neg rlineto Rx neg 0 rlineto +fill grestore}B/a{moveto}B/delta 0 N/tail{A/delta X 0 rmoveto}B/M{S p +delta add tail}B/b{S p tail}B/c{-4 M}B/d{-3 M}B/e{-2 M}B/f{-1 M}B/g{0 M} +B/h{1 M}B/i{2 M}B/j{3 M}B/k{4 M}B/w{0 rmoveto}B/l{p -4 w}B/m{p -3 w}B/n{ +p -2 w}B/o{p -1 w}B/q{p 1 w}B/r{p 2 w}B/s{p 3 w}B/t{p 4 w}B/x{0 S +rmoveto}B/y{3 2 roll p a}B/bos{/SS save N}B/eos{SS restore}B end + +%%EndProcSet +%%BeginProcSet: tex256.enc +% @psencodingfile{ +% author = "Y&Y, Inc.", +% version = "1.1", +% date = "1 April 1996", +% filename = "tex256.enc", +% email = "tech-help@YandY.com", +% address = "45 Walden Street // Concord, MA 01742, USA", +% codetable = "ISO/ASCII", +% checksum = "xx", +% docstring = "Encoding for fonts in Adobe Type 1 format for use with TeX." +% } +% +% Character code assignments are those in Cork (T1) encoding +% +% SAMPLE USAGE (in `psfonts.map' file for DVIPS): +% +% lbr LucidaBright "T1Encoding ReEncodeFont" + + + + + + +]> + +The XML logo is shown in the image . +The image shows an alternative syntax for an empty element + + diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch6/invitation.dtd b/Master/texmf-dist/doc/latex/latex-web-companion/ch6/invitation.dtd new file mode 100644 index 00000000000..ad8df550474 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch6/invitation.dtd @@ -0,0 +1,14 @@ + + + + + + + + + + + + + + diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch6/invitation.xml b/Master/texmf-dist/doc/latex/latex-web-companion/ch6/invitation.xml new file mode 100644 index 00000000000..3209a96b3bd --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch6/invitation.xml @@ -0,0 +1,30 @@ + + + + + +Anna, Bernard, Didier, Johanna +Next Friday Evening at 8 pm +The Web Cafe +My first XML baby + + + + +I would like to invite you all to celebrate +the birth of Invitation, my +first XML document child. + + +Please do your best to come and join me next Friday +evening. And, do not forget to bring your friends. + + +I really look forward to see you soon! + + + + +Michel + + diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch6/wrong.xml b/Master/texmf-dist/doc/latex/latex-web-companion/ch6/wrong.xml new file mode 100644 index 00000000000..4f3827b7adc --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch6/wrong.xml @@ -0,0 +1,15 @@ + + + + +]> + +This part has wrong entity syntax <par>. +Emph text outside scope. +Here comes another error a second level +paragraph. +A wrongly nested construct. +Some more text outside valid scope +Reserved characters "&" "<" ">" ";" . + diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch6/xml.dcl b/Master/texmf-dist/doc/latex/latex-web-companion/ch6/xml.dcl new file mode 100644 index 00000000000..fed21030921 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch6/xml.dcl @@ -0,0 +1,179 @@ +" + PIC "?>" + SHORTREF NONE + + NAMES + SGMLREF + + QUANTITY NONE + + ENTITIES + "amp" 38 + "lt" 60 + "gt" 62 + "quot" 34 + "apos" 39 + + FEATURES + MINIMIZE + DATATAG NO + OMITTAG NO + RANK NO + SHORTTAG + STARTTAG + EMPTY NO + UNCLOSED NO + NETENABL IMMEDNET + ENDTAG + EMPTY NO + UNCLOSED NO + ATTRIB + DEFAULT YES + OMITNAME NO + VALUE NO + EMPTYNRM YES + IMPLYDEF + ATTLIST NO + DOCTYPE NO + ELEMENT NO + ENTITY NO + NOTATION NO + LINK + SIMPLE NO + IMPLICIT NO + EXPLICIT NO + OTHER + CONCUR NO + SUBDOC NO + FORMAL NO + URN NO + KEEPRSRE YES + VALIDITY TYPE + ENTITIES + REF ANY + INTEGRAL YES + APPINFO NONE + SEEALSO "ISO 8879:1986//NOTATION + Extensible Markup Language (XML) 1.0//EN" +> diff --git a/Master/texmf-dist/doc/latex/latex-web-companion/ch7/README.ch7 b/Master/texmf-dist/doc/latex/latex-web-companion/ch7/README.ch7 new file mode 100644 index 00000000000..29a69538029 --- /dev/null +++ b/Master/texmf-dist/doc/latex/latex-web-companion/ch7/README.ch7 @@ -0,0 +1,124 @@ +Examples in Chapter 7 of the LaTeX Graphics Companion + +Section 7.3 +=========== + +To run the examples in this section you have to install nsgmls +(as for chapter 6) and Megginson's SGMLSpm. You also have to +set the environment variable SGML_CATALOG_FILES as follows: + +Bourne shell + +SGML_CATALOG_FILES=catalog.xml +export SGML_CATALOG_FILES + +C shell + +setenv SGML_CATALOG_FILES catalog.xml + +Then you can type: + +nsgmls invitation.xml | perl sgmlspl.pl inv2lat.pl > invitation.tex + +Section 7.4 +=========== + +With similar settings for the environment variable SGML_CATALOG_FILES +we can generate HTML files using invitation.xml and invitation2.xml. + +We type the command (Section 7.4.4) + +nsgmls invitation.xml | perl sgmlspl.pl inv1html.pl > invcss.html + +and (Section 7.4.5) + +nsgmls invitation2.xml | perl sgmlspl.pl inv2html.pl > inv2css.html + +Together with the file invit.css, shown in Section 7.4.4, you will +obtain with a browser, which correctly understands how to include CSS +files, a view as the one shown in Figure 7.2 (some browsers might need +you to include the content of invit.css inside a