meso-web

Sources of the |Méso|Star> website
git clone git://git.meso-star.fr/meso-web.git
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commit 6cbd1d854e0c2b2004ac16e5a277209324125598
parent f6fa38ee14eaa4ce4f719d7bfffec2994579db53
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Mon,  4 Dec 2017 11:50:59 +0100

Merge remote-tracking branch 'origin/master'

Diffstat:
Mstardis.html.in | 50++++++++++++++++++++++++--------------------------
1 file changed, 24 insertions(+), 26 deletions(-)

diff --git a/stardis.html.in b/stardis.html.in @@ -20,19 +20,21 @@ Propagators seamlessly agregate all the provided geometrical and physical information on the system in an unbiased and very-fast statistical model.</p> <p>Stardis' algorithms are based on state-of-the-art Monte-Carlo method applied -to radiative transfer physics (Delatorre [1]) combined with conduction's -statistical formulation (Kac [2] and Muller [3]). Thanks to recent advances in -computer graphics technology which has already been a game changer in the -cinema industry (FX and animated movies), this theoritical framework can now -be practically used on the most geometrically complex models.</p> +to radiative transfer physics (Delatorre [<a href="#1">1</a>]) combined with +conduction's statistical formulation (Kac [<a href="#2">2</a>] and Muller [<a +href="#3">3</a>]). Thanks to recent advances in computer graphics technology +which has already been a game changer in the cinema industry (FX and animated +movies), this theoritical framework can now be practically used on the most +geometrically complex models.</p> <p>Everytime the linear assumption is relevant, this theoritical framework -allows to encompass all the heat transfer mecanisms (conductive-convective- -radiative) in an <b>unified statistical model</b>. Such models can be solved by -a <b>Monte-Carlo approach</b> just by sampling <b>thermal paths</b>. This can -be seen as an extension of Monte-Carlo algorithms that solve radiative transfer -by sampling optical paths. A main property of this approach is that the -resulting algorithms does not rely on a volume mesh of the system.</p> +allows to encompass all the heat transfer mecanisms +(conductive-convective-radiative) in an <b>unified statistical model</b>. Such +models can be solved by a <b>Monte-Carlo approach</b> just by sampling +<b>thermal paths</b>. This can be seen as an extension of Monte-Carlo +algorithms that solve radiative transfer by sampling optical paths. A main +property of this approach is that the resulting algorithms does not rely on a +volume mesh of the system.</p> <h2>An example of propagator use</h2> @@ -124,21 +126,17 @@ you are always going to talk to someone that knows what they are doing.</p> <p>Our commercial offer is versatile:</p> <ul> <li>we provide software developers with a Stardis SDK,</li> - <li>we <a href=#syrthes>assist users</a> in integrating Stardis in their workflow,</li> - <li>we propose bot theoretical and technical trainings and support,</li> + <li>we <a href=#syrthes>assist users</a> in integrating Stardis in their + workflow,</li> + <li>we propose both theoretical and technical training and support,</li> <li>we develop <a href=#optisol>custom software</a> from / on top of - Stardis.</li> + Stardis,</li> + <li>we have a study service based on the method implemented in Stardis.</li> </ul> To get access to Stardis and for more informations on our offer, please <a href="mailto:contact@meso-star.com">contact us</a>. -<!--p>Depending on your status (industry or academic) and development constraints -(open or closed source, ...) Stardis can be made available under the adequate -license. Of course, both theoritical and software development training is -proposed on a regular basis as well as on demand to help you master all the -power of our innovative approach.</p--> - <h2>Examples of integration and development</h2> <h3 id="syrthes"> EDF R&D - SYRTHES </h3> @@ -192,15 +190,15 @@ and initial conditions, Star-Therm can compute the temperature at any position within the solid.</p> <h2>References</h2> -<p> +<div id=1> [1] Delatorre et al., <i>Monte Carlo advances and concentrated solar applications</i>, <b>Solar Energy</b>, 2014 -</p> -<p> +</div> +<div id=2> [2] Kac, <i>On Distributions of Certain Wiener Functionals</i>. <b>The Annals of Mathematical Statistics</b>, 1949. -</p> -<p> +</div> +<div id=3> [3] Muller, <i>Some continuous Monte-Carlo Methods for the Dirichlet Problem" </i>, <b>Transactions of the American Mathematical Society</b>, 1956. -</p> +</div>