Result for 00167B4D4258ED15738C426668A972D18E2977E6

Query result

Key Value
FileName./usr/share/doc/cloudy/html/conv__itercheck_8cpp__incl.map
FileSize3017
MD5E6710BC37AFEF59478D68F61AB9DF6E4
SHA-100167B4D4258ED15738C426668A972D18E2977E6
SHA-25635D203B2CBF0F050DEF4554859405393A66C7951FEC4B30C80DFF304D591DF3C
SSDEEP48:MuquJmIlmehvAaUBApckbhAcSbMZMI6oHtX46QBuOXpehAuCffuuiXb:J7JHlmwvdcAaRMyIpI62uOZenouuq
TLSHT12251F84622A89F2FBD0A0AE493EC1C476561AF7673980C10A2C4FD378C87779F91A567
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