Source: mocassin Section: science Priority: optional Maintainer: Debian Astronomy Team Uploaders: Roger Wesson Build-Depends: debhelper-compat (= 13), gfortran, libmpich-dev Standards-Version: 4.5.1 Homepage: http://www.3d-mocassin.net Rules-Requires-Root: no Vcs-Git: https://salsa.debian.org/debian-astro-team/mocassin.git Vcs-Browser: https://salsa.debian.org/debian-astro-team/mocassin Package: mocassin Architecture: any Depends: ${misc:Depends}, ${shlibs:Depends}, mocassin-data Suggests: mocassin-benchmarks, mocassin-examples Description: MOnte CArlo SimulationS of Ionised Nebulae mocassin is a fully 3D or 2D photoionisation and dust radiative transfer code which employs a Monte Carlo approach to the transfer of radiation through media of arbitrary geometry and density distribution. It was originally developed for the modelling of photoionised regions like HII regions and planetary nebulae and has since expanded and been applied to a variety of astrophysical problems, including modelling clumpy dusty supernova envelopes, star forming galaxies, protoplanetary disks and inner shell fluorence emission in the photospheres of stars and disk atmospheres. The code can deal with arbitrary Cartesian grids of variable resolution, it has successfully been used to model complex density fields from SPH calculations and can deal with ionising radiation extending from Lyman edge to the X-ray. The dust and gas microphysics is fully coupled both in the radiation transfer and in the thermal balance. Package: mocassin-data Architecture: all Multi-Arch: foreign Depends: ${misc:Depends} Suggests: mocassin, mocassin-benchmarks, mocassin-examples Description: atomic and optical data for the photoionisation code MOCASSIN mocassin is a fully 3D or 2D photoionisation and dust radiative transfer code which employs a Monte Carlo approach to the transfer of radiation through media of arbitrary geometry and density distribution. This package contains the atomic and optical data necessary to run simulations. Package: mocassin-benchmarks Architecture: all Multi-Arch: foreign Depends: ${misc:Depends} Suggests: mocassin Description: benchmarks for the photoionisation code MOCASSIN mocassin is a fully 3D or 2D photoionisation and dust radiative transfer code which employs a Monte Carlo approach to the transfer of radiation through media of arbitrary geometry and density distribution. This package contains benchmark problems which can be run and compared with the outputs of other photoionisation codes. Package: mocassin-examples Architecture: all Multi-Arch: foreign Depends: ${misc:Depends} Suggests: mocassin Description: Examples for the photoionisation code MOCASSIN mocassin is a fully 3D or 2D photoionisation and dust radiative transfer code which employs a Monte Carlo approach to the transfer of radiation through media of arbitrary geometry and density distribution. This package contains example input for files for some of the complex simulations that MOCASSIN is capable of.