commit 6ea38e802e618d6bc8e2a1f0cd31e7260cfbef94
parent dc5ce6c1cb9759955984737fd6b1530f73c20a33
Author: christophe coustet <christophe.coustet@meso-star.com>
Date: Fri, 19 Feb 2021 17:38:56 +0100
Add a visual of temporal dynamics analysis to the stardis page
Diffstat:
4 files changed, 25 insertions(+), 7 deletions(-)
diff --git a/stardis/pulse.svg b/stardis/pulse.svg
@@ -0,0 +1 @@
+#$# git-wad 56342d54c28561591d5e5ca40aaa9232446c8f6c1f02f6b572c7d845c8a47ad2 137518
+\ No newline at end of file
diff --git a/stardis/sin.svg b/stardis/sin.svg
@@ -0,0 +1 @@
+#$# git-wad 50581b26e7ce230c34ea17abdca43944276974981da9d12b967279ae5c5a67d4 159020
+\ No newline at end of file
diff --git a/stardis/stardis.html.in b/stardis/stardis.html.in
@@ -154,9 +154,6 @@ on the following hypothesis:</p>
close enough to a known reference temperature.</li>
</ul>
-<p>The remaining of this section describes the main functionalities provided by
-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">
@@ -173,6 +170,9 @@ Stardis-Solver upon the aforementioned hypothesis.</p>
</div>
</div>
+<p>The remaining of this section describes the main functionalities provided by
+Stardis-Solver upon the aforementioned hypothesis.</p>
+
<h3>Probe computation</h3>
<p>Stardis-Solver computes the temperature at any given position (spatial and
@@ -198,14 +198,26 @@ path is the temperature of the boundary or initial condition that has been
reached; when internal power sources or imposed fluxes are taken into account,
additional contributions to the weight must be continuously evaluated by the
thermal conduction algorithm, but these contributions are proportional to the
-local dissipated power/imposed flux.</p>
+local dissipated power and imposed flux.</p>
+
+<div class="img" style="width: 18em;">
+ <a href="step.svg"><img src="step.svg" alt="step"></a>
+ <a href="sin.svg"><img src="sin.svg" alt="sin"></a>
+ <a href="pulse.svg"><img src="pulse.svg" alt="pulse"></a>
+ <div class="caption">
+ Temporal dynamics analysis of a solid cube which has temperatures imposed on
+ its left and right sides, and has adiabatic boundaries elsewhere. The
+ center temperature is the result of a simple postprocess of a <b>single
+ Monte-Carlo computation</b>.
+ </div>
+</div>
<p>In any case, the position and date at the end of each thermal path (and also
accumulation coefficients) can be stored during a first complete Monte-Carlo
simulation. This information, known as the Green function, can then be used in a
(very fast) post-processing step to compute all required results for different
boundary and initial conditions (and also different internal power
-sources/imposed flux).</p>
+sources and imposed flux).</p>
<h3>Infrared rendering</h3>
<p>Stardis can render a scene in infrared without prior knowledge of the
@@ -224,10 +236,10 @@ contributions.</p>
<h3 id="visu">Thermal path visualization</h3>
-<p>Stardis-Solver can store the complete history of a set of thermal paths for
+<p>Stardis-Solver can output the complete history of a set of thermal paths for
later visualization. In addition to positions and dates, physics data is stored
along thermal paths, such as the type of heat transfer phenomenon involved at
-each step, the accumulated power/flux, etc.</p>
+each step, the accumulated power and flux, etc.</p>
<h2 id="cli">Stardis CLI tools</h2>
diff --git a/stardis/step.svg b/stardis/step.svg
@@ -0,0 +1 @@
+#$# git-wad 99055e36829e4e838e8b548ed16d71fa49d3461480a834e25a16e3a284d5fed7 137284
+\ No newline at end of file
