diff options
author | Karl Berry <karl@freefriends.org> | 2012-01-01 23:07:41 +0000 |
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committer | Karl Berry <karl@freefriends.org> | 2012-01-01 23:07:41 +0000 |
commit | 67397afcf6785310f9714a62248c632efdbadef9 (patch) | |
tree | d787caf42dc71337bb5bc88a5485d032ffc6235c /Master/texmf-dist/doc/generic/pst-solarsystem | |
parent | 23ab143d707b8fa83fb9c63646807bc43b9456af (diff) |
new pstricks package pst-solarsystem 0.12 (1jan12)
git-svn-id: svn://tug.org/texlive/trunk@24995 c570f23f-e606-0410-a88d-b1316a301751
Diffstat (limited to 'Master/texmf-dist/doc/generic/pst-solarsystem')
-rw-r--r-- | Master/texmf-dist/doc/generic/pst-solarsystem/Changes | 12 | ||||
-rw-r--r-- | Master/texmf-dist/doc/generic/pst-solarsystem/README | 12 | ||||
-rw-r--r-- | Master/texmf-dist/doc/generic/pst-solarsystem/pst-solarsystem-doc.bib | 166 | ||||
-rw-r--r-- | Master/texmf-dist/doc/generic/pst-solarsystem/pst-solarsystem-doc.pdf | bin | 0 -> 287125 bytes | |||
-rw-r--r-- | Master/texmf-dist/doc/generic/pst-solarsystem/pst-solarsystem-doc.tex | 94 |
5 files changed, 284 insertions, 0 deletions
diff --git a/Master/texmf-dist/doc/generic/pst-solarsystem/Changes b/Master/texmf-dist/doc/generic/pst-solarsystem/Changes new file mode 100644 index 00000000000..d649ad523a6 --- /dev/null +++ b/Master/texmf-dist/doc/generic/pst-solarsystem/Changes @@ -0,0 +1,12 @@ +..... pst-solarsystem.tex +0.12 2012-01-01 - first version + +..... pst-solarsystem.pro +0.10 2012-01-01 - first version + +..... pst-solarsystem.sty +0.10 2012-01-01 - first version + +..... pst-solarsystem-doc.tex + 2012-01-01 - first version + diff --git a/Master/texmf-dist/doc/generic/pst-solarsystem/README b/Master/texmf-dist/doc/generic/pst-solarsystem/README new file mode 100644 index 00000000000..f6e12cf47c9 --- /dev/null +++ b/Master/texmf-dist/doc/generic/pst-solarsystem/README @@ -0,0 +1,12 @@ +pst-mirror: objects on a spherical mirror + +Save the files pst-mirror.sty|tex|pro in a directory, which is part of your +local TeX tree. The pro file should go into $TEXMF/dvips/pstricks/ +Then do not forget to run texhash to update this tree. +For more information see the documentation of your LATEX distribution +on installing packages into your local TeX system or read the +TeX Frequently Asked Questions: +(http://www.tex.ac.uk/cgi-bin/texfaq2html?label=instpackages). + +PSTricks is PostScript Tricks, the documentation cannot be run +with pdftex, use the sequence latex->dvips->ps2pdf.
\ No newline at end of file diff --git a/Master/texmf-dist/doc/generic/pst-solarsystem/pst-solarsystem-doc.bib b/Master/texmf-dist/doc/generic/pst-solarsystem/pst-solarsystem-doc.bib new file mode 100644 index 00000000000..96838e3a2db --- /dev/null +++ b/Master/texmf-dist/doc/generic/pst-solarsystem/pst-solarsystem-doc.bib @@ -0,0 +1,166 @@ +@STRING{tugboat = {TUGboat} } +@STRING{beiprogramm = {{\TeX}-Beiprogramm} } +@STRING{bretter = {Bretter, die die Welt bedeuten} } +@STRING{dtk = {{D}ie {\TeX}nische {K}om{\"o}die} } +@STRING{editorial = {Editorial} } +@STRING{fremdebuehne = {Von fremden B{\"u}hnen} } +@STRING{fundus = {Aus dem Fundus} } +@STRING{hinterbuehne = {Hinter der B{\"u}hne} } +@STRING{leserbrief = {Leserbrief(e)} } +@STRING{magazin = {Magazin} } +@STRING{rezension = {Rezensionen} } +@STRING{schonimmer = {Was Sie schon immer {\"u}ber {\TeX} wissen wollten \dots} } +@STRING{theaterkasse = {Von der Theaterkasse} } +@STRING{theatertage = {{\TeX}-Theatertage} } + +@Article{ dtk02.2:jackson.voss:plot-funktionen, + author = {Laura E. Jackson and Herbert Vo{\ss}}, + title = {Die {P}lot-{F}unktionen von {\texttt{pst-plot}}}, + journal = dtk, + year = 2002, + volume = {2/02}, + altvolume = 2, + altnumber = 14, + month = jun, + pages = {27--34}, + annote = bretter, + keywords = {}, + abstract = { Im letzten Heft wurden die mathematischen Funktionen von + \PS~im Zusammenhang mit dem {\LaTeX}-Paket + \texttt{pst-plot} zum Zeichnen von Funktionen beschrieben + und durch Beispiele erl{\"a}utert. In diesem Teil werden + die bislang nur erw{\"a}hnten Plot-Funktionen f{\"u}r + externe Daten behandelt. } +} + +@Article{ dtk02.1:voss:mathematischen, + author = {Herbert Vo{\ss}}, + title = {Die mathematischen {F}unktionen von {P}ost{S}cript}, + journal = dtk, + year = 2002, + volume = {1/02}, + altvolume = 1, + altnumber = 14, + month = mar, + pages = {}, + annote = bretter, + keywords = {}, + abstract = { \PS, faktisch genauso alt wie {\TeX}, ist im + Verh{\"a}ltnis dazu allgemein noch weniger bekannt, wenn es + darum geht zu beurteilen, was es denn nun im eigentlichen + Sinne ist. Au{\ss}erdem wird h{\"a}ufig vergessen, dass + sich mit den \PS-Funktionen viele Dinge erledigen lassen, + bei denen sonst auf externe Programme zur{\"u}ckgegriffen + wird. Dies wird im Folgenden f{\"u}r die mathematischen + Funktionen im Zusammenhang mit dem Paket \texttt{pst-plot} + gezeigt. } +} + +@Book{tlgc2, + author = {Michel Goosens and Frank Mittelbach and Sebastian Rahtz and Denis Roegel and Herbert Vo{\ss}}, + title = {The {\LaTeX} {G}raphics {C}ompanion}, + publisher = {{Addison-Wesley Publishing Company}}, + edition = second, + year = {2007}, + address = {Reading, Mass.} +} + + +@Book{voss:chaos, + author = {Herbert Vo{\ss}}, + title = {Chaos und {F}raktale selbst programmieren: von {M}andelbrotmengen + {\"u}ber {F}arbmanipulationen zur perfekten Darstellung}, + publisher = {{Franzis Verlag}}, + year = {1994}, + address = {Poing} +} + +@Article{girou:01:, + author = {Denis Girou}, + title = {Pr\'esentation de {PST}ricks}, + journal = {Cahier {GUT}enberg}, + year = 1994, + volume = {16}, + month = apr, + pages = {21-70} +} + +@Article{girou:02:, + author = {{Timothy van} Zandt and Denis Girou}, + title = {Inside {PST}ricks}, + journal = TUGboat, + year = 1994, + volume = {15}, + month = sep, + pages = {239-246} +} + +@Book{PostScript, + Author = {Kollock, Nikolai G.}, + Title = {Post{S}cript richtig eingesetzt: vom {K}onzept zum + praktischen {E}insatz}, + Publisher = {IWT}, + Address = {Vaterstetten}, + year = 1989, +} + +@Manual{pstricks, + Title = {PSTricks - {\PS} macros for generic {\TeX}}, + Author = {{Timothy van} Zandt}, + Organization = {}, + Address = {\url{http://www.tug.org/application/PSTricks}}, + Note = {}, + year = 1993 +} + +@Manual{pst-plot, + Title = {\texttt{pst-plot}: Plotting two dimensional functions and data}, + Author = {{Timothy van} Zandt}, + Organization = {}, + Address = {\url{CTAN:graphics/pstricks/generic/pst-plot.tex}}, + Note = {}, + year = 1999 +} + +@Manual{multido, + Title = {\texttt{multido.tex} - a loop macro, that supports fixed-point addition}, + Author = {{Timothy van} Zandt}, + Organization = {}, + Address = {\url{CTAN:/graphics/pstricks/generic/multido.tex}}, + Note = {}, + year = 1997 +} + +@Book{PSTricks2, + author = {Herbert Vo\ss}, + title = {\texttt{PSTricks} -- {G}rafik f\"ur \TeX{} und \LaTeX}, + edition = {6.}, + publisher = {DANTE -- Lehmanns}, + year = {2010}, + address = {Heidelberg/Berlin} +} + +@Book{voss:math, + author = {Herbert Vo\ss}, + title = {Typesetting mathematics with \LaTeX}, + publisher = {UIT}, + year = {2010}, + address = {Cambridge} +} + +@Book{PSTricks2-UIT, + author = {Herbert Vo\ss}, + title = {PSTricks -- Graphics for \TeX\ and \LaTeX}, + publisher = {UIT}, + year = {2011}, + address = {Cambridge} +} + +@Manual{wolfram, + author = {Eric Weisstein}, + title = {Wolfram MathWorld}, + publisher = {{Wolfram}}, + year = {2007}, + address = {\url{http://mathworld.wolfram.com}} +} + diff --git a/Master/texmf-dist/doc/generic/pst-solarsystem/pst-solarsystem-doc.pdf b/Master/texmf-dist/doc/generic/pst-solarsystem/pst-solarsystem-doc.pdf Binary files differnew file mode 100644 index 00000000000..f7a69abd067 --- /dev/null +++ b/Master/texmf-dist/doc/generic/pst-solarsystem/pst-solarsystem-doc.pdf diff --git a/Master/texmf-dist/doc/generic/pst-solarsystem/pst-solarsystem-doc.tex b/Master/texmf-dist/doc/generic/pst-solarsystem/pst-solarsystem-doc.tex new file mode 100644 index 00000000000..5fb14555cb4 --- /dev/null +++ b/Master/texmf-dist/doc/generic/pst-solarsystem/pst-solarsystem-doc.tex @@ -0,0 +1,94 @@ +%% $Id: pst-solarsystem-doc.tex 620 2012-01-01 14:09:57Z herbert $ +\documentclass[11pt,english,BCOR10mm,DIV12,bibliography=totoc,parskip=false, + smallheadings, headexclude,footexclude,oneside]{pst-doc} +\usepackage[latin1]{inputenc} +\usepackage{pst-solarsystem} +\let\pstFV\fileversion +\usepackage{pstricks-add} +\renewcommand\bgImage{\resizebox{0.6\linewidth}{!}{\SolarSystem[Day=1,Month=1,Year=2012,Hour=12,viewpoint=1 -1 2]}} + +\lstset{language=PSTricks, + morekeywords={psGammaDist,psChiIIDist,psTDist,psFDist,psBetaDist,psPlotImpl},basicstyle=\footnotesize\ttfamily} +% +\begin{document} + +\title{\texttt{pst-solarsystem}} +\subtitle{Position of the visible planets, projected on the plane of the ecliptic; v.\pstFV} +\author{Manuel Luque \\Herbert Vo\ss} +\docauthor{} +\date{\today} +\maketitle + +\tableofcontents + +\vspace{2cm} +For the method of calculation, I was guided by: +\begin{itemize} +\item that given by \textit{Jean Meeus} astronomical calculations in the book for use by +published by the Amateur Astronomical Society of France. +\item and that of Guy Serane in \textit{Astronomy \& PC published} by Wiley \& Sons. +\end{itemize} + +As we can not represent all the planets in the real proportions, only Mercury, Venus, Earth and Mars are the proportions of the orbits and +their relative sizes observed. Saturn and Jupiter are in the right direction, but +obviously not at the right distance. + +The orbits are shown in solid lines for the portion above the ecliptic +and dashed for the portion located below. + +We can compare the view obtained with the following representation: + +\url{http://users.skynet.be/fa274406/rubriques/live/orbites/orbites.htm} + +The use of the command is very simple, just specify the date of observation +with the following parameters, for example: +\begin{verbatim} +\SolarSystem[Day=31,Month=06,Year=2001,Hour=23,Minute=59,Second=59] +\end{verbatim} +\xLkeyword{Day}\xLkeyword{Month}\xLkeyword{Year}\xLkeyword{Hour}\xLkeyword{Minute}\xLkeyword{Second} + +By default, if no parameter is specified, \Lcs{SolarSystem} gives the configuration +day 0 hours to compile. + +The \Lkeyword{values} is enabled by default. It displays the values of +longitude, latitude, and the distance in astronomical units. + +The accuracy of the calculations is about 0.1 to 0.3 degrees (comparing to ephemeris +the Bureau des Longitudes), which is more than enough for a performance +graph. + +\url{http://www.imcce.fr/fr/ephemerides/formulaire/form_ephepos.php} +\begin{center} +\SolarSystem + +\SolarSystem[Day=30,Month=06,Year=2001,Hour=23,Minute=59,Second=59,viewpoint=1 -1 2,values=false] +\end{center} + + +\begin{verbatim} +\SolarSystem[Day=30,Month=06,Year=2001, + Hour=23,Minute=59,Second=59, + viewpoint=1 -1 2,values=false] +\end{verbatim} + + +\clearpage +\section{List of all optional arguments for \texttt{pst-solarsystem}} + +\xkvview{family=pst-solarsystem,columns={key,type,default}} + + + + +\bgroup +\raggedright +\nocite{*} +\bibliographystyle{plain} +\bibliography{pst-solarsystem-doc} +\egroup + +\printindex + + + +\end{document} |