htrdr

Solving radiative transfer in heterogeneous media
git clone git://git.meso-star.fr/htrdr.git
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commit ea91b71596eac58baadefc3a8dfeb2648e017ff4
parent 67609cd18c1bd3c08968e21e8b09f3250ea5e741
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Tue,  6 Jul 2021 16:35:14 +0200

Small update of the htrdr-atmosphere man page

Fix typos.

Diffstat:
Mdoc/htrdr-atmosphere.1.txt.in | 12++++++------
1 file changed, 6 insertions(+), 6 deletions(-)

diff --git a/doc/htrdr-atmosphere.1.txt.in b/doc/htrdr-atmosphere.1.txt.in @@ -75,12 +75,12 @@ domain is longwave or shortwave. In *htrdr-atmosphere* the spatial unit 1.0 corresponds to one meter and the temperatures are expressed in Kelvin. The estimated radiances are given in W/sr/m^2 excepted for monochromatic computations where the computed spectral -radiance is defined in W/sr/m^2/nm. The fluxes are saved in W/m^2. The results -are written to the output file if the *-o* option is defined and the standard -output otherwise. The output image is a list of raw ASCII data formatted with -respect to the *htrdr-image*(5) file format. Since *htrdr-atmosphere* relies -on the Monte-Carlo method, each estimation is given with its numerical -accuracy. +radiance is defined in W/sr/m^2/nm. The flux densities are saved in W/m^2. The +results are written to the output file if the *-o* option is defined and the +standard output otherwise. The output image is a list of raw ASCII data +formatted with respect to the *htrdr-image*(5) file format. Since +*htrdr-atmosphere* relies on the Monte-Carlo method, each estimation is given +with its numerical accuracy. During the simulation, *htrdr-atmosphere* dynamically loads/unloads cloud properties to handle clouds whose data that do not feat in main memory.