[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 194)
knarf at cct.lsu.edu
knarf at cct.lsu.edu
Mon Nov 14 00:15:25 CST 2011
User: knarf
Date: 2011/11/14 12:15 AM
Modified:
/
ET.tex
Log:
left/right -> top/bottom
File Changes:
Directory: /
============
File [modified]: ET.tex
Delta lines: +2 -2
===================================================================
--- ET.tex 2011-11-14 06:14:52 UTC (rev 193)
+++ ET.tex 2011-11-14 06:15:25 UTC (rev 194)
@@ -2831,10 +2831,10 @@
\begin{figure}
\includegraphics[width=0.9\textwidth]{examples/cosmology/figs/kasner.pdf}
\includegraphics[width=0.9\textwidth]{examples/cosmology/figs/err.pdf}
- \caption{Left: the evolution of a vacuum spacetime of the type~\eref{eq:gowdyT3},
+ \caption{Top: the evolution of a vacuum spacetime of the type~\eref{eq:gowdyT3},
with $P=Q=\lambda=0$; the initial data are chosen as
$\gamma_{ij}=\delta_{ij}$ and $K_{ij}={\rm diag}(-2/3,-2/3,1/3)$.
- Right: the numerical error for a sequence of four time resolutions $dt=[0.0125,0.025,0.05,0.1]$;
+ Bottom: the numerical error for a sequence of four time resolutions $dt=[0.0125,0.025,0.05,0.1]$;
the errors are scaled according to the expectation for fourth-order convergence.
\label{fig:kasner}}
\end{figure}
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