Bug#827841: marked as done (ITP: mocassin -- Monte Carlo simulations of ionised nebulae)
Your message dated Mon, 22 Aug 2016 08:00:14 +0000
with message-id <E1bbk9W-0006yX-Uc@franck.debian.org>
and subject line Bug#827841: fixed in mocassin 2.02.71-1
has caused the Debian Bug report #827841,
regarding ITP: mocassin -- Monte Carlo simulations of ionised nebulae
to be marked as done.
This means that you claim that the problem has been dealt with.
If this is not the case it is now your responsibility to reopen the
Bug report if necessary, and/or fix the problem forthwith.
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827841: http://bugs.debian.org/cgi-bin/bugreport.cgi?bug=827841
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--- Begin Message ---
- To: Debian Bug Tracking System <submit@bugs.debian.org>
- Subject: ITP: mocassin -- Monte Carlo simulations of ionised nebulae
- From: Roger Wesson <rw@nebulousresearch.org>
- Date: Tue, 21 Jun 2016 16:52:14 +0100
- Message-id: <20160621155214.21518.57250.reportbug@laptop>
Package: wnpp
Severity: wishlist
Owner: Roger Wesson <rw@nebulousresearch.org>
* Package name : mocassin
Version : 2.02.70
Upstream Author : Barbara Ercolano
* URL : http://www.3d-mocassin.net
* License : GPL-2+
Programming Lang: fortran
Description : 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 is a widely used code, with papers describing it having nearly 200 citations in the astronomical literature. The source code is available from 3d-mocassin.net and is licensed under GPL-v2+. I propose to create a debian package which can be maintained within the Debian Astronomy Team.
--- End Message ---
--- Begin Message ---
Source: mocassin
Source-Version: 2.02.71-1
We believe that the bug you reported is fixed in the latest version of
mocassin, which is due to be installed in the Debian FTP archive.
A summary of the changes between this version and the previous one is
attached.
Thank you for reporting the bug, which will now be closed. If you
have further comments please address them to 827841@bugs.debian.org,
and the maintainer will reopen the bug report if appropriate.
Debian distribution maintenance software
pp.
Roger Wesson <rw@nebulousresearch.org> (supplier of updated mocassin package)
(This message was generated automatically at their request; if you
believe that there is a problem with it please contact the archive
administrators by mailing ftpmaster@ftp-master.debian.org)
-----BEGIN PGP SIGNED MESSAGE-----
Hash: SHA1
Format: 1.8
Date: Wed, 17 Aug 2016 20:23:02 +0100
Source: mocassin
Binary: mocassin mocassin-data mocassin-benchmarks mocassin-examples
Architecture: source all amd64
Version: 2.02.71-1
Distribution: unstable
Urgency: low
Maintainer: Debian Astronomy Team <debian-astro-maintainers@lists.alioth.debian.org>
Changed-By: Roger Wesson <rw@nebulousresearch.org>
Description:
mocassin - MOnte CArlo SimulationS of Ionised Nebulae
mocassin-benchmarks - benchmarks for the photoionisation code MOCASSIN
mocassin-data - atomic and optical data for the photoionisation code MOCASSIN
mocassin-examples - Examples for the photoionisation code MOCASSIN
Closes: 827841
Changes:
mocassin (2.02.71-1) unstable; urgency=low
.
* Initial release. (Closes: #827841)
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Files:
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