htrdr

Solving radiative transfer in heterogeneous media
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commit f4951426d14da412f4e2da64115d6042803c22a7
parent a3fc644b0cb496c115ad4cca2600871ff4dbe1ff
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Thu,  1 Dec 2022 14:09:31 +0100

htrdr-planeto: proofreading the man page

Diffstat:
Mdoc/htrdr-planeto.1.scd.in | 32++++++++++++++++++--------------
1 file changed, 18 insertions(+), 14 deletions(-)

diff --git a/doc/htrdr-planeto.1.scd.in b/doc/htrdr-planeto.1.scd.in @@ -37,7 +37,7 @@ TODO defined. Available aerosol parameters are: *mesh*=_path_ - Path to the *smsh*(5) file that stores the volumetric mesh of the aerosol. + Path to the *smsh*(5) file that stores the aerosol tetrahedral mesh. *name*=_string_ Name assigned to the aerosol. @@ -119,22 +119,22 @@ TODO defined in another file (see *prop* parameter). *mesh*=_path_ - Path to the *smsh*(5) file that stores the surface mesh of the ground. + Path to the *smsh*(5) file which stores the triangular mesh of the ground. *name*=_string_ Name assigned to the ground. *prop*=_path_ Path to the *rnsp*(5) file that stores ground surface properties. The - properties (BRDF index and temperature) are defined per surface mesh node - and, therefore, this file and the mesh file (see *mesh* parameter) must be + properties (BRDF index and temperature) are defined per triangle and, + therefore, this file and the mesh file (see *mesh* parameter) must be consistent with each other. *-g* <_gas-parameter_:...> Define the gas mixture. Available gas parameters are: *mesh*=_path_ - Path to the *smsh*(5) file that stores the volumetric mesh of the gas. + Path to the *smsh*(5) file that stores the gas tetrahedral mesh. *ck*=_path_ Path to the *sck*(5) file that stores the correlated K of the gas. The CKs @@ -187,7 +187,7 @@ TODO data is written to the standard output. *-S* <_source-parameter_:...> - Define the source. Available source parameters are: + Define the external source. Available source parameters are: *lat*=_real_ The latitude of the source, i.e. its angle between [-90, 90] degrees about @@ -218,21 +218,22 @@ TODO Perform continuous spectral sampling in the wavelength range [_wlen-min_, _wlen-max_] (wavelengths must be provided in nanometers) according to the Planck function for a reference temperature (see *Tref* parameter). If _wlen-min_ - and _wlen-max_ are equal, the calculation is monochromatic. *lw* means long - waves but is here a code word that actually means "calculation of radiance - using the internal source of radiation": in other words, radiation is - emitted by the medium and its limits (ground and space). + and _wlen-max_ are equal, the calculation is monochromatic. *lw* means + longwaves but is here a code word that actually means "calculation of + radiance using the internal source of radiation": in other words, radiation + is emitted by the medium and its limits (ground and space). *sw*=_wlen-min_,_wlen-max_ Perform continuous spectral sampling in the wavelength range [_wlen-min_, _wlen-max_] (wavelengths must be provided in nanometers) according to the - Planck function for a reference temperatura (see *Tref* parameter)e. If - _wlen-min_ and _wlen-max_ are equal, the calculation is monochromatic. In - this case, *sw* means that the radiation source is external to the medium. + Planck function for a reference temperatura (see *Tref* parameter). If + _wlen-min_ and _wlen-max_ are equal, the calculation is monochromatic. Here, + *sw* means shortwaves, i.e. the radiation source is external to the medium. *Tref*=_temperature_ The reference temperature in Kelvin of the Planck function used to - continuously sample the longwave/shortwave spectral range. + continuously sample the longwave/shortwave spectral range. This is a + required parameter for the *lw* and *sw* parameters. *-T* _optical-thickness_ Optical thickness used as a criterion to construct atmospheric acceleration @@ -253,6 +254,9 @@ TODO # SEE ALSO +. VTK file format - + <http://www.vtk.org/wp-content/uploads/2015/04/file-formats.pdf> + *mrumtl*(5), *rnpfi*(5), *rnsf*(5),