mocassin 2.02.72-2build1 source package in Ubuntu
Changelog
mocassin (2.02.72-2build1) artful; urgency=medium * No-change rebuild for libgfortran soname change. -- Matthias Klose <email address hidden> Fri, 04 Aug 2017 18:03:10 +0000
Upload details
- Uploaded by:
- Matthias Klose
- Uploaded to:
- Artful
- Original maintainer:
- Debian Astronomy Maintainers
- Architectures:
- any all
- Section:
- misc
- Urgency:
- Medium Urgency
See full publishing history Publishing
| Series | Published | Component | Section | |
|---|---|---|---|---|
| Bionic | release | universe | misc |
Downloads
| File | Size | SHA-256 Checksum |
|---|---|---|
| mocassin_2.02.72.orig.tar.gz | 13.6 MiB | 41c6d98be952e3726dfe409543f00feb21c1d13d0606428bf5e3f1dc4d33886c |
| mocassin_2.02.72-2build1.debian.tar.xz | 3.5 KiB | a59e2b66453cd117207dc7c4aeb2b7b42fa5b45cbb7b52912f0955db2ad75da7 |
| mocassin_2.02.72-2build1.dsc | 2.2 KiB | d03d70369da4f4e1d8648673a055d8d1e99739145df88fffd09dfd99cea996c5 |
Available diffs
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: No summary available for mocassin-data in ubuntu artful.
No description available for mocassin-data in ubuntu artful.
- mocassin-dbgsym: No summary available for mocassin-dbgsym in ubuntu artful.
No description available for mocassin-dbgsym in ubuntu artful.
- 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.
