meso-web

commit ab8f19c9982b07711c4a735beb7f8b62b7e377c3
parent 8c5dc7ce5ffc597b2ce3b3b7b929a2236f75e173
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Wed,  6 Jan 2021 14:31:20 +0100

Replace the foam IR rendering by the heatsink IR anim

Diffstat:
A
stardis/heatsink_anim.gif
 | 
2
++
A
stardis/heatsink_anim_thumb.gif
 | 
2
++
M
stardis/stardis.html.in
 | 
19
+++++++++++--------

3 files changed, 15 insertions(+), 8 deletions(-)
diff --git a/stardis/heatsink_anim.gif b/stardis/heatsink_anim.gif
@@ -0,0 +1 @@
+#$# git-wad c14089676f571e5673042b6c082398db39d7c2de2b4c394b13bcf92075a73ccd 3289467
+\ No newline at end of file
diff --git a/stardis/heatsink_anim_thumb.gif b/stardis/heatsink_anim_thumb.gif
@@ -0,0 +1 @@
+#$# git-wad b648deda857cbd45b7018f52e2d6954783791d0442152a50f011c0c3fce38ce5 405446
+\ No newline at end of file
diff --git a/stardis/stardis.html.in b/stardis/stardis.html.in
@@ -148,15 +148,18 @@ on the following hypothesis:</p>
 <p>The remaining of this section describes the main functionalities provided by
 Stardis-Solver upon the aforementonned hypothesis.</p>
 
-<div class="img" style="width: 18em">
-  <a href="IR_rendering.jpg"><img src="IR_rendering.jpg" alt="IR_rendering"></a>
+<div class="img" style="width: 18em;">
+  <a href="heatsink_anim.gif"><img src="heatsink_anim_thumb.gif" alt="heatsink"></a>
   <div class="caption">
-  Infrared image of a foam geometry. This rendering was performed by
-  Stardis-Solver without the knowledge of the temperature field. The radiative
-  paths that begin at the camera will propagate alternately in conductive,
-  convective and radiative path until reaching a boundary or a limit condition.
-  We point out that this computation is provided as an example of the <a
-  href="starter-pack.html">Stardis: Starter Pack</a>.
+  Unsteady infrared rendering of a chip and its heatsink during 15 seconds. One
+  image per second is simulated using Stardis. We point out that these
+  rendering was performed without any knowledge on the temperature field.
+  Thanks to Monte Carlo reformulation of heat transfers, the radiative paths
+  that begin at the camera will propagate alternately in conductive, convective
+  and radiative path until a boundary condition or a limit condition is
+  reached. Acknowledgment to <a
+  href=https://www.imt-mines-albi.fr/fr/eibner-simon>Simon Eibner</a> who
+  produced this animation.
   </div>
 </div>