How to Install and Uninstall cloudy.x86_64 Package on Fedora 35
Last updated: January 11,2025
1. Install "cloudy.x86_64" package
In this section, we are going to explain the necessary steps to install cloudy.x86_64 on Fedora 35
$
sudo dnf update
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$
sudo dnf install
cloudy.x86_64
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2. Uninstall "cloudy.x86_64" package
This tutorial shows how to uninstall cloudy.x86_64 on Fedora 35:
$
sudo dnf remove
cloudy.x86_64
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$
sudo dnf autoremove
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3. Information about the cloudy.x86_64 package on Fedora 35
Last metadata expiration check: 0:19:59 ago on Wed Sep 7 02:25:42 2022.
Available Packages
Name : cloudy
Version : 13.05
Release : 12.fc35
Architecture : x86_64
Size : 1.4 M
Source : cloudy-13.05-12.fc35.src.rpm
Repository : fedora
Summary : Spectral synthesis code to simulate conditions in interstellar matter
URL : http://www.nublado.org/
License : BSD
Description : Most of the quantitative information we have about the cosmos comes from
: spectroscopy. In many cases the light we analyze was produced by atoms in
: the first generations of stars and galaxies. The spectra are produced by
: dilute gas where such properties as the gas kinetic temperature, chemical
: state, level of ionization, and level populations, are determined by a
: host of microphysical processes rather than by a single temperature.
: Analytical solutions are seldom possible and computer solutions are
: needed to understand their physical properties. Numerical simulations make
: it possible to understand complex physical environments starting from
: first principles. Cloudy is designed to do exactly this.
Available Packages
Name : cloudy
Version : 13.05
Release : 12.fc35
Architecture : x86_64
Size : 1.4 M
Source : cloudy-13.05-12.fc35.src.rpm
Repository : fedora
Summary : Spectral synthesis code to simulate conditions in interstellar matter
URL : http://www.nublado.org/
License : BSD
Description : Most of the quantitative information we have about the cosmos comes from
: spectroscopy. In many cases the light we analyze was produced by atoms in
: the first generations of stars and galaxies. The spectra are produced by
: dilute gas where such properties as the gas kinetic temperature, chemical
: state, level of ionization, and level populations, are determined by a
: host of microphysical processes rather than by a single temperature.
: Analytical solutions are seldom possible and computer solutions are
: needed to understand their physical properties. Numerical simulations make
: it possible to understand complex physical environments starting from
: first principles. Cloudy is designed to do exactly this.