How to Install and Uninstall cassbeam Package on Ubuntu 20.10 (Groovy Gorilla)

Last updated: December 23,2024

1. Install "cassbeam" package

Please follow the steps below to install cassbeam on Ubuntu 20.10 (Groovy Gorilla)


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

This tutorial shows how to uninstall cassbeam on Ubuntu 20.10 (Groovy Gorilla):


    
        
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                sudo apt remove
            
                        
                cassbeam
            
                    
    
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                sudo apt autoclean && sudo apt autoremove
            
                    
    
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3. Information about the cassbeam package on Ubuntu 20.10 (Groovy Gorilla)

Package: cassbeam
Architecture: amd64
Version: 1.1-2
Priority: optional
Section: universe/science
Origin: Ubuntu
Maintainer: Ubuntu Developers
Original-Maintainer: Debian Astro Team
Bugs: https://bugs.launchpad.net/ubuntu/+filebug
Installed-Size: 541
Depends: fftw2, libc6 (>= 2.29), libglib2.0-0 (>= 2.24.0)
Filename: pool/universe/c/cassbeam/cassbeam_1.1-2_amd64.deb
Size: 410132
MD5sum: 229a33664b307bd5b81fb348475bfc0e
SHA1: b78a0136012748198eb889489d2d78ef716da715
SHA256: 878a64d5c405c4eb434cb34f9cc6ee872f2696197a3b87752d9438c4fd046f06
SHA512: d510cf8fca1220156b7100f8c03f80484614096057833b0fe5a2687ae5debb8e2c1a983484b8b5f49ad6a7c3e7ea477b206bec2b480fe837d878e32a9bd45f83
Homepage: https://github.com/ratt-ru/cassbeam
Description-en: Cassegrain antenna modelling
Cassbeam is a Cassegrain antenna ray tracer. A Cassegrain antenna is
a double reflector system which works on the principle of cassegrain
optical telescope. A high gain cassegrain reflector antenna in
Ku-band has been successfully developed for command transmit
application for the missile programme. It can also be used for
monopulse radar, satellite communication.
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Based on an input text file, it computes several properties of the
antenna including gain, zenith system temperature, and the beam, in
full polarization. All calculations are done in the transmit sense
and use reciprocity to relate to the equivalent receiving system.
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Additionally, cassbeam allows deformations, or pathologies of the
optics to be modelled. Currently this is limited to rotations and
translations of the feed and secondary. In the future, large scale
deviations in the primary (such as a misplaced panel) will likely be
supported.
Description-md5: 8324519e6d631ade9e0430a434bbf7ca