How to Install and Uninstall mocassin Package on Ubuntu 21.10 (Impish Indri)

Last updated: May 18,2024

1. Install "mocassin" package

This guide let you learn how to install mocassin on Ubuntu 21.10 (Impish Indri)


    
        
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                sudo apt update
            
                    
    
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                sudo apt install
            
                        
                mocassin
            
                    
    
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2. Uninstall "mocassin" package

This guide covers the steps necessary to uninstall mocassin on Ubuntu 21.10 (Impish Indri):


    
        
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                sudo apt remove
            
                        
                mocassin
            
                    
    
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                sudo apt autoclean && sudo apt autoremove
            
                    
    
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3. Information about the mocassin package on Ubuntu 21.10 (Impish Indri)

Package: mocassin
Architecture: amd64
Version: 2.02.73.2-1
Priority: optional
Section: universe/science
Origin: Ubuntu
Maintainer: Ubuntu Developers
Original-Maintainer: Debian Astronomy Team
Bugs: https://bugs.launchpad.net/ubuntu/+filebug
Installed-Size: 1406
Depends: libc6 (>= 2.29), libgcc-s1 (>= 4.0), libgfortran5 (>= 10), libmpich12 (>= 3.4.1-3build1), mocassin-data
Suggests: mocassin-benchmarks, mocassin-examples
Filename: pool/universe/m/mocassin/mocassin_2.02.73.2-1_amd64.deb
Size: 403732
MD5sum: 709d0da5bb323bbca0527238f2fe0009
SHA1: a3ce98a8f64bcb53537e12657d37783d2bd192f0
SHA256: a3e2f6a29ca8e93f43445351554a52e3075c34f8b99260b4c01b0d751c7c2ab0
SHA512: 736583b43a354fee3b1cbb2da33d7c61bd810c3fb53a27c28039dfa15da58609b17fc290d60e452320f9cb22e49dcbf0f0a4f1566975712276dd2bd9aca284d7
Homepage: http://www.3d-mocassin.net
Description-en: 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.
Description-md5: 8eff30b55e35a6cedaf01664028ad44e