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[ Source: mocassin  ]

Package: mocassin (2.02.73.2-1)

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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.

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Architecture Package Size Installed Size Files
amd64 355.1 kB2,562.0 kB [list of files]
arm64 324.8 kB2,222.0 kB [list of files]
armel 328.8 kB2,526.0 kB [list of files]
armhf 317.5 kB1,794.0 kB [list of files]
i386 306.8 kB2,866.0 kB [list of files]
mips64el 312.1 kB2,602.0 kB [list of files]
mipsel 323.7 kB2,582.0 kB [list of files]
ppc64el 337.9 kB2,866.0 kB [list of files]
s390x 342.8 kB2,610.0 kB [list of files]