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 | 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
- diff from 2.02.73-1 to 2.02.73-2 (957 bytes)
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.