Key | Value |
---|---|
FileName | ./usr/share/coda/definitions/AURA_MLS-20160922.codadef |
FileSize | 7286 |
MD5 | 6BD3D7DA9A49D52ECC2EB3B6AF3CC6C7 |
SHA-1 | 0F22508D9A084F09873BE3A376526A2AC54ED2DD |
SHA-256 | EBCAB752C1F7DDED0D266E70A2ECD888F842D491696ABB58FC89BD6C35298586 |
SSDEEP | 192:V120g568sUNPJqKUevtauTpSg+AyotMW9YujHx4FF3m67TZyeLxms8W10Hkdd1jg:V12H56LUNIKdvtBTpSg+AyotMKYu14Fc |
TLSH | T12CE15575DB34896BC92F603280036BAABB96830117707D0E7D5073C67A679C5EFA432E |
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 | 1718624 |
MD5 | 168DF5250FEAA4F8C9B2E67F35E92757 |
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 | D9CAE73D431C39B5305814813871E60A70597B9B |
SHA-256 | E68D5EC309DDCB91501B17EAB5F67D7B10098E800632572F7E74E6E8B5368BF7 |