meso-web

Sources of the |Méso|Star> website
git clone git://git.meso-star.fr/meso-web.git
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commit 18fda9a1448e29358203be5ddcbd10b3e2d780f7
parent 654c0b0f228df0e63a5ceb5614c174ec5d7a58ad
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Thu,  1 Oct 2020 11:29:58 +0200

Add a High-Tune "Related projecst" sub section

Diffstat:
Mhigh-tune/high-tune.html.in | 63++++++++++++++++++++++++++++++++++++++++++++++++++-------------
1 file changed, 50 insertions(+), 13 deletions(-)

diff --git a/high-tune/high-tune.html.in b/high-tune/high-tune.html.in @@ -88,7 +88,7 @@ run either directly or through a MPI process launcher like <code>mpirun</code>. </div> </div> -<h2>A straight interface</h2> +<h2 id="rel_projects">Related projects</h2> <div class="img" style="width: 20em"> <a href="CLEMENT.jpg"> @@ -106,6 +106,55 @@ run either directly or through a MPI process launcher like <code>mpirun</code>. </div> </div> +<p>High-Tune: RenDeRer is currently used, developped and extended in the +following research projects.</p> + +<ul> + <li>In project <a + href="https://www.umr-cnrm.fr/spip.php?article1204&lang=en">ModRadUrb</a> the + emphasis is put on taking into account the representation of <b>complex + geometries</b> (detailled city scenes) using <b>spectral properties of a + arbitrary number of materials</b>. The solver is going to be extended to + solve upward and downward <b>atmospheric fluxes</b> at any level in the + scene, both in the visible and the infrared spectral ranges.</li> + + <li>In project <a href="https://mcg-rad.ipsl.fr/en/">MCG-Rad</A> the + <code>htrdr</code> codebase is used to explore a whole new class of radiative + transfer algorithms: instead of relying on the full atmospheric radiative + properties data set (prerequisite for current algorithms), the so-called + <b>line sampling</b> algorithms will not require nor compute the absorption + coefficient of the atmosphere. Instead, it will sample energetic transitions + and use a Line-by-Line parameters database (such as <a + href="https://hitran.org/">HITRAN</a>) in order to perform a <b>rigorous + spectral integration</b>, both in the visible and the infrared spectral + ranges.</li> + + <li>In project <a + href="https://anr.fr/en/funded-projects-and-impact/funded-projects/project/funded/project/b2d9d3668f92a3b9fbbf7866072501ef-62de701ce7/?tx_anrprojects_funded%5Bcontroller%5D=Funded&cHash=d684bb545d6cd7afb9ec8b755c2d9df8">Astoria</a>, + <code>htrdr</code> will be used to produce both radiative transfer + computations in the infrared and images in the visible, in the presence of + <b>combustion chambers</b> where radiation scattering is performed by soot + aggregates. The main difficulty resides in the fact that the chamber is + <b>illuminated by a laser</b>: the classical solar radiative transfer + algorithm then fails to converge because of the collimated radiation source, + and a new algorithm has to be designed in order to ensure numerical + convergence.</li> +</ul> + +<h2>A straight interface</h2> + +<div class="img" style="width: 20em"> + <a href="CLEMENT_lw_9000_10000.jpg"> + <img src="CLEMENT_lw_9000_10000.jpg" alt="CLEMENT_lw"> + </a> + <div class="caption"> + Infrared rendering in [9000, 10000] nanometers of the 500<sup>3</sup> cloud + field of <a + href="https://rmets.onlinelibrary.wiley.com/doi/full/10.1002/qj.3614">Strauss + et al. (2019)</a>. The color map displays the brightness temperature in + Kelvin. </div> +</div> + <p><code>htrdr</code> is a <b>command-line tool</b> that performs computations on input data, writes the rendered image and nothing more. No assumption is made on how input data are created excepted that they have to follow the @@ -136,18 +185,6 @@ project: it provides CMake scripts that automate the download, the compilation and the installation of <code>htrdr</code> and its dependencies. This build procedure assumes the following prerequisites: -<div class="img" style="width: 20em"> - <a href="CLEMENT_lw_9000_10000.jpg"> - <img src="CLEMENT_lw_9000_10000.jpg" alt="CLEMENT_lw"> - </a> - <div class="caption"> - Infrared rendering in [9000, 10000] nanometers of the 500<sup>3</sup> cloud - field of <a - href="https://rmets.onlinelibrary.wiley.com/doi/full/10.1002/qj.3614">Strauss - et al. (2019)</a>. The color map displays the brightness temperature in - Kelvin. </div> -</div> - <ul> <li><a href=https://git-scm.com>git</a> source control as well its <a href=https://git-lfs.github.com>Large File System</a> extension.</li>