mandi (1jul16)

git-svn-id: svn://tug.org/texlive/trunk@41598 c570f23f-e606-0410-a88d-b1316a301751

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
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}