meso-web

Sources of the |Méso|Star> website
git clone git://git.meso-star.fr/meso-web.git
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commit e40ba6ed44cc567c4d9cf9923d5153a2faaec319
parent 5b8031a1d91b5e6bd9685a4a246ff7be8c88a375
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Tue, 23 Feb 2021 12:17:23 +0100

Fix the layout of the stardis overview page

Diffstat:
Mstardis/stardis.html.in | 24++++++++++++------------
1 file changed, 12 insertions(+), 12 deletions(-)

diff --git a/stardis/stardis.html.in b/stardis/stardis.html.in @@ -173,6 +173,18 @@ on the following hypothesis:</p> <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="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> + <h3>Probe computation</h3> <p>Stardis-Solver computes the temperature at any given position (spatial and @@ -200,18 +212,6 @@ additional contributions to the weight must be continuously evaluated by the thermal conduction algorithm, but these contributions are proportional to the 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