Parents (Total: 3)

The searched file hash is included in 3 parent files which include package known and seen by metalookup. A sample is included below:

Key	Value
MD5	4CC6420AEB128C81ADE15D3CD653C8B5
PackageArch	i586
PackageDescription	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.
PackageMaintainer	daviddavid <daviddavid>
PackageName	cloudy
PackageRelease	1.mga7
PackageVersion	13.05
SHA-1	AE84F41F75874787B5BFDF86B9F4F98052CAF5A5
SHA-256	F6EC2EF24E9C5F121601CA5FA0A6447E27F1748B6B10FD2AE4C6C5CDFC0A2AEF

Key	Value
MD5	5EA15AE3A14D558B0C03AA5B13765060
PackageArch	aarch64
PackageDescription	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.
PackageMaintainer	daviddavid <daviddavid>
PackageName	cloudy
PackageRelease	1.mga7
PackageVersion	13.05
SHA-1	214AD198E09E90DDFA72264357ED6005A4C62814
SHA-256	D1243D766088A84CA069CD949654D9F783C154B2FF5CBB3854B8784026F2741D

Key	Value
MD5	0E22008BB07F83764B856CE7EDA69E87
PackageArch	x86_64
PackageDescription	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.
PackageMaintainer	daviddavid <daviddavid>
PackageName	cloudy
PackageRelease	1.mga7
PackageVersion	13.05
SHA-1	6635B340ED81708A973641D2CD8DF0CE854994E3
SHA-256	F91307A098E1C4C9A8A285D6FC9497EFA96D53EE2B6CD19061173CF195EE03EE