commit c01c1710be2b8b8965f7cf1e6ce06988c4c97537
parent 261149561b1be9f4034536bd2afe33a706e0912d
Author: Vincent Forest <vincent.forest@meso-star.com>
Date: Wed, 10 Jun 2020 21:23:21 +0200
Minor update the high tune overview
Diffstat:
1 file changed, 4 insertions(+), 5 deletions(-)
diff --git a/high-tune/high-tune.html.in b/high-tune/high-tune.html.in
@@ -32,9 +32,9 @@ algorithms in <b>inhomogeneous media</b>. It was then extended in the <a
href="https://www.umr-cnrm.fr/spip.php?article1204&lang=en">ModRadUrb</a>
project to handle longwave spectral integration and to add support of
<b>spectral reflectivities</b> to the geometries. <code>htrdr</code> is
-actually an <b>image renderer</b> in the <b>visible or infrared</b> part of the
-spectrum, for scenes composed of an atmospheric gas mixture, clouds and a
-ground. It uses volumetric spectral data that should be provided for the
+actually an <b>image renderer</b> in the <b>visible</b> or <b>infrared</b> part
+of the spectrum, for scenes composed of an atmospheric gas mixture, clouds and
+a ground. It uses volumetric spectral data that should be provided for the
pressure and temperature atmospheric vertical profile, the liquid water content
in suspension within the clouds that is a result of Large Eddy Simulation
computations, and the optical properties of water droplets that have been
@@ -61,8 +61,7 @@ spectrum in [380, 780] nanometers, for the three components of the <b>CIE 1931
XYZ colorimetric space</b> that are subsequently recombined in order to obtain
the final color for each pixel. As an alternative, one can explicitly define
the longwave or shortwave spectral range into which the wavelength are going to
-be continuously sampled according to the <b>Planck function</b> for a reference
-temperature.</p>
+be continuously sampled.</p>
<p>During the simulation, <code>htrdr</code> <b>dynamically loads/unloads</b>
cloud properties and thus it can handle clouds whose data do not feat in main
