Key | Value |
---|---|
FileName | ./usr/share/coda/definitions/AURA_TES-20160919.codadef |
FileSize | 6932 |
MD5 | D40F66F751F72502349F1D970272D65A |
SHA-1 | 036D433913048B75A33E980D6D5177CEA301780A |
SHA-256 | 724BC727380DF133F50727F6F194D3B3C0DB1C8CEA7503A614FB7682A4F8FA97 |
SSDEEP | 192:RbDkOIQqQPd5brijSzpCCw39HqM8wpmBa9VmjLp8EMHMvlOy:RbDkjQJPd5brijUpnw39Hz8wYa90jLpT |
TLSH | T180E11079C630493ADD1ED3718819848174BFA74147A69ECF7C24B74989CEAC1AB37A0F |
hashlookup:parent-total | 1 |
hashlookup:trust | 55 |
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 |
---|---|
FileSize | 1465684 |
MD5 | A3DC45F24F2053469502A44EFB3822B0 |
PackageDescription | Data harmonization toolset for Earth Observation formats HARP is a toolset for ingesting, processing and inter-comparing satellite or model data against correlative data. The toolset is composed of a set of command line tools, a C library of analysis functions, and import/export interfaces for Python. The main goal of HARP is to assist in the inter-comparison of data sets. By appropriatelty chaining calls to the HARP command line tools one can preprocess satellite, model, and/or correlative data such that two datasets that need to be compared end up having the same temporal/spatial grid, same data format/structure, and same physical units. . This package provides the HARP binary utilities. |
PackageMaintainer | Debian Science Maintainers <debian-science-maintainers@lists.alioth.debian.org> |
PackageName | harp |
PackageSection | utils |
PackageVersion | 1.5+data-3 |
SHA-1 | 114B00463F1B49BA03818A10A0B073FD39B4BF27 |
SHA-256 | 76C029B529B48FBD33A3B4EFB99D08F7E801DCE28E78D90C0DB1FE7DF26BCB14 |