How to Install and Uninstall mocassin Package on Kali Linux

Last updated: January 10,2025

1. Install "mocassin" package

This guide let you learn how to install mocassin on Kali Linux


    
        
            $
        

        
            
                sudo apt update
            
                    
    
    Copied


    
        
            $
        

        
            
                sudo apt install
            
                        
                mocassin
            
                    
    
    Copied

2. Uninstall "mocassin" package

This guide covers the steps necessary to uninstall mocassin on Kali Linux:


    
        
            $
        

        
            
                sudo apt remove
            
                        
                mocassin
            
                    
    
    Copied


    
        
            $
        

        
            
                sudo apt autoclean && sudo apt autoremove
            
                    
    
    Copied

3. Information about the mocassin package on Kali Linux

Package: mocassin
Version: 2.02.73.2-1
Installed-Size: 2562
Maintainer: Debian Astronomy Team
Architecture: amd64
Depends: libc6 (>= 2.29), libgcc-s1 (>= 4.0), libgfortran5 (>= 10), libmpich12 (>= 3.4.1-3), mocassin-data
Suggests: mocassin-benchmarks, mocassin-examples
Size: 363612
SHA256: c9f5d8762f1225ac2224f815cf4ae096ef19622283c9591d2f94e4c46c520a6d
SHA1: 8eb2be2ef0070cf6590bc085d067731efd8fd8cb
MD5sum: 8d1a5e43be81ab8f0c580b2307105f14
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.
Description-md5:
Homepage: http://www.3d-mocassin.net
Section: science
Priority: optional
Filename: pool/main/m/mocassin/mocassin_2.02.73.2-1_amd64.deb