Result for 000B75257DAE88B2ABB4DCA6AA64A4FE90DB46BC

Query result

Key Value
FileName./usr/share/doc/cloudy/html/transition_8h__incl.md5
FileSize32
MD5D5AFC6F308D402F7D6902D52D040B47B
SHA-1000B75257DAE88B2ABB4DCA6AA64A4FE90DB46BC
SHA-256645FEB646AF48B300C0A0FA086A563F5F0C161141925BF8C30807E961C7568B7
SSDEEP3:mvJDCPGIxtG:mFCtG
TLSH
hashlookup:parent-total1
hashlookup:trust55

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Parents (Total: 1)

The searched file hash is included in 1 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
MD58AE9C750FED4245C6B29C3A9295DD0DF
PackageArcharmv7hl
PackageDescriptionMost 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.
PackageMaintainerdaviddavid <daviddavid>
PackageNamecloudy
PackageRelease1.mga7
PackageVersion13.05
SHA-1664A539F0878E6837670855DF037F842A3BA79C9
SHA-256A5905E0840579C6D9983B12D14FB8AB3E92C5FAD51C4C3C5D863D16CA7AB0C72