套件：mocassin（2.02.73.2-1）
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.
其他與 mocassin 有關的套件
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- dep: libc6 (>= 2.29)
- GNU C 函式庫：共用函式庫
同時作為一個虛擬套件由這些套件填實： libc6-udeb
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- dep: libgcc-s1 (>= 4.0)
- GCC 支援函式庫
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- dep: libgfortran5 (>= 10)
- Runtime library for GNU Fortran applications
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- dep: libmpich12 (>= 3.4.1)
- Shared libraries for MPICH
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- dep: mocassin-data
- atomic and optical data for the photoionisation code MOCASSIN
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- sug: mocassin-benchmarks
- benchmarks for the photoionisation code MOCASSIN
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- sug: mocassin-examples
- Examples for the photoionisation code MOCASSIN