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-rw-r--r--Master/texmf-dist/doc/latex/mandi/mandi.pdfbin1274514 -> 1277991 bytes
-rw-r--r--Master/texmf-dist/source/latex/mandi/mandi.dtx105
-rw-r--r--Master/texmf-dist/tex/latex/mandi/mandi.sty9
3 files changed, 77 insertions, 37 deletions
diff --git a/Master/texmf-dist/doc/latex/mandi/mandi.pdf b/Master/texmf-dist/doc/latex/mandi/mandi.pdf
index 02030e5f658..7fd099d3fe3 100644
--- a/Master/texmf-dist/doc/latex/mandi/mandi.pdf
+++ b/Master/texmf-dist/doc/latex/mandi/mandi.pdf
Binary files differ
diff --git a/Master/texmf-dist/source/latex/mandi/mandi.dtx b/Master/texmf-dist/source/latex/mandi/mandi.dtx
index edc1e9747a3..b885828e801 100644
--- a/Master/texmf-dist/source/latex/mandi/mandi.dtx
+++ b/Master/texmf-dist/source/latex/mandi/mandi.dtx
@@ -32,7 +32,7 @@
%</internal>
%
%<*package>
-\ProvidesPackage{mandi}[2016/06/29 2.6.0 Macros for physics and astronomy]
+\ProvidesPackage{mandi}[2016/06/30 2.6.1 Macros for physics and astronomy]
\NeedsTeXFormat{LaTeX2e}[1999/12/01]
%</package>
%
@@ -125,7 +125,7 @@ while 1:
% package is indexed. There may be commands similar to indexed commands
% described in relevant parts of the documentation.}
%
-% \CheckSum{6353}
+% \CheckSum{6357}
%
% \CharacterTable
% {Upper-case \A\B\C\D\E\F\G\H\I\J\K\L\M\N\O\P\Q\R\S\T\U\V\W\X\Y\Z
@@ -281,6 +281,8 @@ while 1:
% \changes{v2.4.0}{2014/12/19}{Removed compatibility check for the \pkgname{physymb}
% package.}
% \changes{v2.6.0}{2016/05/20}{Documented \cs{mandiversion}.}
+% \changes{v2.6.1}{2016/06/30}{Fixed \cs{mandiversion} so it displays correctly
+% in math mode.}
%
%\iffalse
%<*example>
@@ -297,6 +299,7 @@ Gives the current package version number and build date.
%
% \changes{v2.6.0}{2016/05/16}{Extensive revisions to documentation.}
% \changes{v2.6.0}{2016/05/02}{Created a student guide.}
+% \changes{v2.6.1}{2016/06/30}{Fixed errors in Student Quick Guide documentation.}
% \newpage
% \section{Student Quick Guide}
% Use \refCom{vect} to put an arrow over a symbol to make it the symbol for a vector.
@@ -434,11 +437,11 @@ Gives the current package version number and build date.
%\fi
\begin{docCommand}{genericinteractionplaces}
{\marg{const}\marg{thing1}\marg{thing2}\marg{dist}\marg{direction}}
-Command for generic expression for an inverse square interaction. The required
-arguments are, from left to right, a constant of proportionality, a physical
-property of object 1, a physical property of object 2, the objects' mutual
-separation, and a vector direction. In practice, these should all be provided
-in numerical form.
+Command for generic expression for an inverse square interaction. The five
+required arguments are, from left to right, a constant of proportionality, a
+physical property of object 1, a physical property of object 2, the objects'
+mutual separation, and a vector direction. In practice, these should all be
+provided in numerical form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\genericinteractionplaces{}{}{}{}{}
@@ -452,13 +455,13 @@ in numerical form.
%\fi
\begin{docCommand}{genericfieldofparticleplaces}
{\marg{const}\marg{thing}\marg{dist}\marg{direction}}
-Command for generic expression for an inverse square field. The required
+Command for generic expression for an inverse square field. The four required
arguments are, from left to right, a constant of proportionality, a physical
property, relative distance to field point, and a vector direction. In practice,
these should all be provided in numerical form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
-\genericfieldofparticleplaces{}{}{}{}{}
+\genericfieldofparticleplaces{}{}{}{}
\end{dispExample*}
%\iffalse
%</example>
@@ -469,13 +472,13 @@ these should all be provided in numerical form.
%\fi
\begin{docCommand}{genericpotentialenergyplaces}
{\marg{const}\marg{thing1}\marg{thing2}\marg{dist}}
-Command for generic expression for an inverse square energy. The required
+Command for generic expression for an inverse square energy. The four required
arguments are, from left to right, a constant of proportionality, a physical
property of object 1, a physical property of object 2, and the objects' mutual
separation. In practice, these should all be provided in numerical form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
-\genericpotentialenergyplaces{}{}{}{}{}
+\genericpotentialenergyplaces{}{}{}{}
\end{dispExample*}
%\iffalse
%</example>
@@ -486,7 +489,10 @@ separation. In practice, these should all be provided in numerical form.
%\fi
\begin{docCommand}{gravitationalinteractionplaces}
{\marg{mass1}\marg{mass2}\marg{distance}\marg{direction}}
-Command for gravitational interaction.
+Command for gravitational interaction. The four required arguments are, from
+left to right, the first object's mass, the second object's mass, the objects'
+mutual separation, and a vector direction. In practice, these should all be
+provided in numerical form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\gravitationalinteractionplaces{}{}{}{}
@@ -500,7 +506,10 @@ Command for gravitational interaction.
%\fi
\begin{docCommand}{gfieldofparticleplaces}
{\marg{mass}\marg{distance}\marg{direction}}
-Command for gravitational field of a particle.
+Command for gravitational field of a particle. The three required arguments are,
+from left to right, the object's mass, the distance from the source to the field
+point, and a vector direction. In practice, these should all be provided in
+numerical form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\gfieldofparticleplaces{}{}{}
@@ -514,7 +523,10 @@ Command for gravitational field of a particle.
%\fi
\begin{docCommand}{gravitationalpotentialenergyplaces}
{\marg{mass1}\marg{mass2}\marg{distance}}
-Command for gravitational potential energy.
+Command for gravitational potential energy. The three required arguments are,
+from left to right, the first object's mass, the second object's mass, and
+the object's mutual distance. In practice, these should all be provided in
+numerical form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\gravitationalpotentialenergyplaces{}{}{}
@@ -528,7 +540,9 @@ Command for gravitational potential energy.
%\fi
\begin{docCommand}{springinteractionplaces}
{\marg{stiffness}\marg{stretch}\marg{direction}}
-Command for a spring interaction.
+Command for a spring interaction. The three required arguments are, from left
+to right, the spring stiffness, the spring's stretch, and a vector direction.
+In practice, these should all be provided in numerical form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\springinteractionplaces{}{}{}
@@ -542,7 +556,9 @@ Command for a spring interaction.
%\fi
\begin{docCommand}{springpotentialenergyplaces}
{\marg{stiffness}\marg{stretch}}
-Command for spring potential energy.
+Command for spring potential energy. The two required arguments are, from left
+to right, the spring stiffness and the spring stretch. In practice, these should
+be provided in numerical form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\springpotentialenergyplaces{}{}
@@ -556,10 +572,10 @@ Command for spring potential energy.
%\fi
\begin{docCommand}{genericelectricdipoleonaxisplaces}
{\marg{const}\marg{charge}\marg{separation}\marg{dist}\marg{direction}}
-Command for generic expression for dipole field on the dipole's axis. The required
-arguments are, from left to right, a constant of proportionality, a charge, a dipole
-separation, the distance to the field point, and a vector direction. In practice,
-these should all be provided in numerical form.
+Command for generic expression for dipole field on the dipole's axis. The five
+required arguments are, from left to right, a constant of proportionality, a charge,
+a dipole separation, the distance to the field point, and a vector direction. In
+practice, these should all be provided in numerical form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\genericelectricdipoleonaxisplaces{}{}{}{}{}
@@ -573,10 +589,10 @@ these should all be provided in numerical form.
%\fi
\begin{docCommand}{genericelectricdipoleplaces}
{\marg{const}\marg{charge}\marg{separation}\marg{dist}\marg{direction}}
-Command for generic expression for dipole field. The required arguments are, from
-left to right, a constant of proportionality, a charge, a dipole separation, the
-distance to the field point, and a vector direction. In practice, these should all
-be provided in numerical form.
+Command for generic expression for dipole field. The five required arguments are,
+from left to right, a constant of proportionality, a charge, a dipole separation,
+the distance to the field point, and a vector direction. In practice, these should
+all be provided in numerical form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\genericelectricdipoleplaces{}{}{}{}{}
@@ -590,7 +606,10 @@ be provided in numerical form.
%\fi
\begin{docCommand}{electricinteractionplaces}
{\marg{charge1}\marg{charge2}\marg{distance}\marg{direction}}
-Command for electric interaction.
+Command for electric interaction. The four required arguments are, from left to
+right, the first object's charge, the second object's charge, the objects' mutual
+separation, and a vector direction. In practice, these should all be provided in
+numerical form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\electricinteractionplaces{}{}{}{}
@@ -604,7 +623,10 @@ Command for electric interaction.
%\fi
\begin{docCommand}{Efieldofparticleplaces}
{\marg{charge}\marg{distance}\marg{direction}}
-Command for electric field of a particle.
+Command for electric field of a particle. The three required argument are, from
+left to right, the particle's charge, the distance form the source to the field
+point, and a vector direction. In practice, these should all be provided in
+numerical form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\Efieldofparticleplaces{}{}{}
@@ -618,7 +640,11 @@ Command for electric field of a particle.
%\fi
\begin{docCommand}{Bfieldofparticleplaces}
{\marg{charge}\marg{magvel}\marg{magr}\marg{vhat}\marg{rhat}}
-Command for magnetic field of a particle.
+Command for magnetic field of a particle. The five required arguments are, from
+left to right, the particle's charge, the particle's velocity, the distance from
+the source to the field point, the velocity's direction, and a direction vector
+from the source to the field point. In practice, these should all be provided in
+numerical form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\Bfieldofparticleplaces{}{}{}{}{}
@@ -632,7 +658,10 @@ Command for magnetic field of a particle.
%\fi
\begin{docCommand}{electricpotentialenergyplaces}
{\marg{charge1}\marg{charge2}\marg{distance}}
-Command for electric potential energy.
+Command for electric potential energy. The three required arguments are, from
+left to right, the first object's charge, the second object's charge, and the
+objects' mutual distance. In practice, these should all be provided in numerical
+form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\electricpotentialenergyplaces{}{}{}
@@ -646,9 +675,10 @@ Command for electric potential energy.
%\fi
\begin{docCommand}{electricdipoleonaxisplaces}
{\marg{charge}\marg{separation}\marg{dist}\marg{direction}}
-Command for dipole electric field on the dipole's axis. The required arguments are,
-from left to right, a charge, a dipole separation, the distance to the field point,
-and a vector direction. In practice, these should all be provided in numerical form.
+Command for dipole electric field on the dipole's axis. The four required arguments
+are, from left to right, a charge, a dipole separation, the distance to the field
+point, and a vector direction. In practice, these should all be provided in numerical
+form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\electricdipoleonaxisplaces{}{}{}{}
@@ -662,9 +692,9 @@ and a vector direction. In practice, these should all be provided in numerical f
%\fi
\begin{docCommand}{electricdipoleonbisectorplaces}
{\marg{charge}\marg{separation}\marg{dist}\marg{direction}}
-Command for dipole electric field. The required arguments are, from left to right,
-a charge, a dipole separation, the distance to the field point, and a vector
-direction. In practice, these should all be provided in numerical form.
+Command for dipole electric field. The four required arguments are, from left
+to right, a charge, a dipole separation, the distance to the field point, and
+a vector direction. In practice, these should all be provided in numerical form.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\electricdipoleonbisectorplaces{}{}{}{}
@@ -9351,7 +9381,12 @@ Command for QED symbol.
% \end{macrocode}
%
% \begin{macrocode}
-\newcommand*{\mandiversion}{2.6.0 dated 2016/06/29}
+\newcommand*{\mandiversion}{\ifmmode%
+ 2.6.1\mbox{ dated }2016/06/30%
+ \else%
+ 2.6.1 dated 2016/06/30%
+ \fi
+ }%
\typeout{mandi: You're using mandi version \mandiversion.}
% \end{macrocode}
%
diff --git a/Master/texmf-dist/tex/latex/mandi/mandi.sty b/Master/texmf-dist/tex/latex/mandi/mandi.sty
index d2e819cb89a..e0a8922ae84 100644
--- a/Master/texmf-dist/tex/latex/mandi/mandi.sty
+++ b/Master/texmf-dist/tex/latex/mandi/mandi.sty
@@ -28,7 +28,7 @@
%% vdemo.py.
%% ---------------------------------------------------------------------------
%%
-\ProvidesPackage{mandi}[2016/06/29 2.6.0 Macros for physics and astronomy]
+\ProvidesPackage{mandi}[2016/06/30 2.6.1 Macros for physics and astronomy]
\NeedsTeXFormat{LaTeX2e}[1999/12/01]
\RequirePackage{amsmath}
@@ -120,7 +120,12 @@
\DeclareOption{approxconsts}{\setboolean{@optapproxconsts}{true}}
\DeclareOption{useradians}{\setboolean{@optuseradians}{true}}
\ProcessOptions\relax
-\newcommand*{\mandiversion}{2.6.0 dated 2016/06/29}
+\newcommand*{\mandiversion}{\ifmmode%
+ 2.6.1\mbox{ dated }2016/06/30%
+ \else%
+ 2.6.1 dated 2016/06/30%
+ \fi
+ }%
\typeout{mandi: You're using mandi version \mandiversion.}
\@ifpackageloaded{amssymb}{%
\csundef{square}