[Commits] [svn:einsteintoolkit] www/about/gallery/ (Rev. 1483)

[rhaas at tapir.caltech.edu]

User: rhaas
Date: 2015/06/17 01:18 AM

Modified:
 /about/gallery/
  index.php

Log:
 Gallery: use headings to separate individual examples to make them more prominent

File Changes:

Directory: /about/gallery/
==========================

File [modified]: index.php
Delta lines: +5 -17
===================================================================
--- about/gallery/index.php	2015-06-02 13:14:27 UTC (rev 1482)
+++ about/gallery/index.php	2015-06-17 06:18:01 UTC (rev 1483)
@@ -12,19 +12,13 @@
 
 <h3>Using exclusively the Einstein Toolkit</h3>
 
-<ul>
 <!--
- <li>
-  Single black hole
- </li>
+ <h4> Single black hole</h4>
 -->
 <!--
- <li>
-  Binary black hole inspiral
- </li>
+ <h4> Binary black hole inspiral</h4>
 -->
- <li>
-  Single, stable neutron star
+ <h4> Single, stable neutron star</h4>
   <p>This simulation shows how to evolve a stable, single neutron star. It uses a TOV solution
      as initial data and follows the initial (numerical) perturbations, writing the maximum
      density to disk. What can be seen is that the oscillates for a few cycles (only very
@@ -41,14 +35,10 @@
    <tr><th>approx. runtime</th><td>2.5 SU</td></tr>
   </table>
   <a href="tov/rho_max.pdf"><img src="tov/rho_max.png" alt="Maximum density over time"></a>
- </li>
 <!--
- <li>
-  Single, collapsing neutron star
- </li>
+ <h4> Single, collapsing neutron star</h4>
 -->
- <li>
-  Binary, inspiraling neutron stars forming a hypermassive neutron star
+ <h4> Binary, inspiraling neutron stars forming a hypermassive neutron star</h4>
   <p>This simulation shows how to evolve a pair of neutron stars, reading in
      initial data provided by the <a href="http://www.lorene.obspm.fr/">LORENE</a> code. The video shows
      the rest mass density in an equatorial slice of the simulation. The
@@ -72,8 +62,6 @@
           width: 640, height: 480
       });
   </script>
- </li>
-</ul>
 
 <!--
 <h3>Using external but public code</h3>