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	166AA7849CA9ED8895E79549AA306A1D
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	ghibo <ghibo>
PackageName	cloudy
PackageRelease	4.mga9
PackageVersion	13.05
SHA-1	8DB4A8A0F4186E2B33B3B3EE557996AE1BDDBCE1
SHA-256	4FBF80314948F68175387BF40444679129CA1D86F8A400D47E478F93664427DC

Key	Value
MD5	BA4556FD40D5762EABA159D9844BF87F
PackageArch	armv7hl
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	ghibo <ghibo>
PackageName	cloudy
PackageRelease	4.mga9
PackageVersion	13.05
SHA-1	A8AB6642174D2182D6D8BB341D2661550BFBFA99
SHA-256	88B4C4B76D1465C02C9A9816E4BCB2C1A9533F8FB80038192FEF82996AC86F50

Key	Value
MD5	8BEEDE0C468BAF9B66465B04C1AFD638
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	ghibo <ghibo>
PackageName	cloudy
PackageRelease	4.mga9
PackageVersion	13.05
SHA-1	D547BD283B86F97ABE4D5A5B7CD7868BBC0723E3
SHA-256	C62CF8391FAA44E171CAF351D69F0ADC800C3034174FEA67859A181BBBA2113D