Key | Value |
---|---|
FileName | ./usr/share/coda/definitions/AURA_OMI-20161024.codadef |
FileSize | 6706 |
MD5 | 0CA5BF32A232D7C6A1C211AD85F79175 |
SHA-1 | 05DCBB2AC813A50C35AA60B94D11EBA8FE2B678A |
SHA-256 | 7CBF45B6B79D038FC9748004607F5F785BAAD3BB4B2119889F2EFA0E51F7076C |
SSDEEP | 192:Hma7Mk4aIWXizFoCehOgLBC8tZ+/j+cXZPbrQyHeao4XU8/sMd9t1+UkSbxdOsS:HmaIk43WyzyCehOgLBC8/+/j1XZPbrdg |
TLSH | T162D13269E934037DCA5FB430CC420ACC756381495A95678FB81CE68D7A6B1C65F35E8C |
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 | 1717800 |
MD5 | 1ECFDED1684467470FB2B63DD5C484CD |
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 | 1.12-1+b1 |
SHA-1 | 839C5BB6D681A044A62FB9360B117968ED971F1F |
SHA-256 | 698FAB59C99F7DF957005AA54A0CD789A302DEADCEBE8E4853F73800BA1561CB |