commit b043173ce9b4522cebdfa2a53d18b6802afd5dba
parent 4c0f4bf388ac322a49950df8c55734b1374d450f
Author: Christophe Coustet <christophe.coustet@meso-star.com>
Date: Fri, 8 Jan 2021 10:13:38 +0100
Add information on the infrared rendering feature
Diffstat:
1 file changed, 12 insertions(+), 9 deletions(-)
diff --git a/stardis/stardis.html.in b/stardis/stardis.html.in
@@ -150,15 +150,11 @@ Stardis-Solver upon the aforementioned hypothesis.</p>
<div class="img" style="width: 18em;">
<a href="heatsink_anim.gif"><img src="heatsink_anim_thumb.gif" alt="heatsink"></a>
<div class="caption">
- Unsteady infrared rendering of a chip and its heatsink during 15 seconds. The
- temperature is expressed in Kelvin. 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/lea-penazzi>Léa Penazzi</a> and <a
- href=https://www.icam.fr/enseignant-chercheur/anne-castelan/>Anne
+ Infrared timelapse animation of a chip and its heatsink covering a 15-second
+ period of time. Computed using the stardis infrared rendering feature, one
+ image per simulated second. Acknowledgment to
+ <a href=https://www.imt-mines-albi.fr/fr/lea-penazzi>Léa Penazzi</a> and
+ <a href=https://www.icam.fr/enseignant-chercheur/anne-castelan/>Anne
Castelan</a> for the scene geometry (also available in <a
href=starter-pack.html>Stardis: Starter Pack</a>) actually used in an
upcoming research article, and to <a
@@ -201,6 +197,13 @@ simulation. This information, known as the Green function, can then be used in a
boundary and initial conditions (and also different internal power
sources/imposed flux).</p>
+<h3>Infrared rendering</h3>
+<p>Stardis can render a scene in infrared without prior knowledge of the
+temperature field. Thermal paths that start at the camera in radiative mode
+propagate through the model, possibly in conductive, convective or radiative
+mode until reaching a boundary condition (or a initial condition in a
+non-stationary case).</p>
+
<h3 id="temporal">Temporal dynamics analysis</h3>
<p>Stardis-Solver can output the end of each path sampled during a Monte-Carlo
