htrdr

Solving radiative transfer in heterogeneous media
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      1 .\" Copyright (C) 2018-2019, 2022-2025 Centre National de la Recherche Scientifique
      2 .\" Copyright (C) 2020-2022 Institut Mines Télécom Albi-Carmaux
      3 .\" Copyright (C) 2022-2025 Institut Pierre-Simon Laplace
      4 .\" Copyright (C) 2022-2025 Institut de Physique du Globe de Paris
      5 .\" Copyright (C) 2018-2025 |Méso|Star> (contact@meso-star.com)
      6 .\" Copyright (C) 2022-2025 Observatoire de Paris
      7 .\" Copyright (C) 2022-2025 Université de Reims Champagne-Ardenne
      8 .\" Copyright (C) 2022-2025 Université de Versaille Saint-Quentin
      9 .\" Copyright (C) 2018-2019, 2022-2025 Université Paul Sabatier
     10 .\"
     11 .\" This program is free software: you can redistribute it and/or modify
     12 .\" it under the terms of the GNU General Public License as published by
     13 .\" the Free Software Foundation, either version 3 of the License, or
     14 .\" (at your option) any later version.
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     16 .\" This program is distributed in the hope that it will be useful,
     17 .\" but WITHOUT ANY WARRANTY; without even the implied warranty of
     18 .\" MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
     19 .\" GNU General Public License for more details.
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     21 .\" You should have received a copy of the GNU General Public License
     22 .\" along with this program. If not, see <http://www.gnu.org/licenses/>.
     23 .Dd September 27, 2023
     24 .Dt HTRDR 1
     25 .Os
     26 .Sh NAME
     27 .Nm htrdr
     28 .Nd simulate radiative transfer
     29 .Sh SYNOPSIS
     30 .Nm
     31 .Op Fl vh
     32 .Op Ar mode Op Ar options ...
     33 .Sh DESCRIPTION
     34 .Nm
     35 simulates radiative transfer in scenes composed of heterogeneous
     36 semi-transparent materials and geometries with varying spectral
     37 reflectivities.
     38 .Pp
     39 The way the scenes are described and the Monte Carlo algorithms solved
     40 are controlled by the
     41 .Ar mode
     42 argument, which defines the computational context.
     43 A
     44 .Ar mode
     45 corresponds to a command line named
     46 .Li htrdr- Ns Ar mode
     47 with its set of options.
     48 See the corresponding manual page for a full description.
     49 .Pp
     50 The available modes are as follows:
     51 .Bl -tag -width Ds
     52 .It Cm atmosphere
     53 Calculate radiative transfer in a cloudy atmosphere
     54 .Pq see Xr htrdr-atmosphere 1 .
     55 .It Cm combustion
     56 Calculate radiative transfer in a combustion chamber
     57 .Pq see Xr htrdr-combustion 1 .
     58 .It Cm planeto
     59 Calculate radiative transfer in 3d planetary atmosphere
     60 .Pq see Xr htrdr-planeto 1 .
     61 .El
     62 .Pp
     63 The options are as follows:
     64 .Bl -tag -width Ds
     65 .It Fl h
     66 Display short help and exit.
     67 .It Fl v
     68 Display the version number and exit.
     69 .El
     70 .Sh EXIT STATUS
     71 .Ex -std
     72 .Sh SEE ALSO
     73 .Xr htrdr-atmosphere 1 ,
     74 .Xr htrdr-combustion 1 ,
     75 .Xr htrdr-planeto 1
     76 .\".Sh HISTORY
     77 .\".Nm
     78 .\"was initially developed for cloudy atmospheres in High-Tune
     79 .\".Li ANR-16-CE01-0010 .
     80 .\"It was then extended in
     81 .\".Li MODEVAL-URBA 2019 .
     82 .\"Support for combustion chambers was added in Astoria
     83 .\".Li ANR-18-CE05-0015 .
     84 .\"Planetology simulations were developed in RaD-net
     85 .\".Li ANR-21-CE49-0020 .