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mocassin package

mocassin 2.02.73-2 source package in Ubuntu

Changelog

mocassin (2.02.73-2) unstable; urgency=low

  * updated standards-version
  * updated Format url in copyright
  * fixed wrong intent on variable (Closes: #952320)

 -- Roger Wesson <email address hidden>  Mon, 24 Feb 2020 14:41:24 +0000

Upload details

Uploaded by:
Debian Astronomy Maintainers
Uploaded to:
Sid
Original maintainer:
Debian Astronomy Maintainers
Architectures:
any all
Section:
misc
Urgency:
Low Urgency

See full publishing history Publishing

Series Pocket Published Component Section
Focal release universe misc

Downloads

File Size SHA-256 Checksum
mocassin_2.02.73-2.dsc 2.1 KiB 9f6bfe8835cf54968079053b6242449a80250fa7ca0db4e253cdcad5707c4cee
mocassin_2.02.73.orig.tar.gz 13.6 MiB 1b5fe306c89d2f0cc3631a946d2d575decfdaac53a2f5e5793bf05755031773b
mocassin_2.02.73-2.debian.tar.xz 3.7 KiB 8ea79c31d7b746beb7e2f3ab4e5a92ea8089125429b04d1abc60a89d64ede704

Available diffs

No changes file available.

Binary packages built by this source

mocassin: 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.

mocassin-benchmarks: 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.

mocassin-data: 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.

mocassin-dbgsym: debug symbols for mocassin
mocassin-examples: 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.