[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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