commit 20e639eead397f61cc5128abb9ddd99729d53a92
parent f7f0846dfdf7d8f8e4860db7e313df4818e36daf
Author: Vincent Forest <vincent.forest@meso-star.com>
Date: Wed, 8 Feb 2023 17:08:13 +0100
htrdr: add the planeto application to the overview
Diffstat:
1 file changed, 16 insertions(+), 12 deletions(-)
diff --git a/htrdr/htrdr.html.in b/htrdr/htrdr.html.in
@@ -1,12 +1,3 @@
-<script>
-// When the user clicks on <div>, open the popup
-function poptext(Id) {
- var popup = document.getElementById(Id);
- popup.classList.toggle("show");
-}
-</script>
-
-
<header>
<h1><code style="color: #000000">htrdr</code>
<span class=subtitle>
@@ -60,9 +51,9 @@ interest, in their most common formats, in each scientific community.
<ol>
<li>
- <p><a href="man/man1/htrdr-atmosphere.1.html">Atmospheric radiative
- transfer</a>: the clear-sky atmosphere is vertically stratified, cloud
- thermodynamic data is provided on a regular 3D rectangular grid, and surface
+ <p><a href="man/man1/htrdr-atmosphere.1.html">Plane-parallel atmospheric
+ radiative transfer</a>: a clear-sky atmosphere is vertically stratified,
+ cloud thermodynamic data is provided on a 3D rectangular grid, and surface
optical properties can be provided for an arbitrary number of materials.
Internal radiation and solar radiation are taken into account.</p>
</li>
@@ -73,6 +64,19 @@ interest, in their most common formats, in each scientific community.
The radiation source is only external: a monochromatic laser sheet
illuminates the inside of the combustion chamber for diagnostic purposes.</p>
</li>
+<li>
+ <p><a href="man/man1/htrdr-planeto.1.html">Planetology</a>: takes into
+ account the geometry of a "ground" of arbitrary shape, described by a
+ triangular mesh, with the possibility of using an arbitrary number of
+ materials. The radiative properties of a gas mixture must be provided on a
+ tetrahedral mesh, using the k-distribution spectral model. The radiative
+ properties of an arbitrary number of aerosol modes can also be provided on
+ their individual tetrahedral mesh. Calculations can be made for both internal
+ and external radiation sources. In the case of an external source, a sphere
+ of arbitrary size and position is used. This sphere can radiate as a Planck
+ source at a specified brightness temperature, or using a high-resolution
+ radiance spectrum.</p>
+</li>
</ol>
<p>Since any observable radiative transfer is expressed as an integral of the
