Key | Value |
---|---|
FileName | ./usr/share/coda/definitions/AURA_TES-20160919.codadef |
FileSize | 6932 |
MD5 | 838503858F0C1C867297C6F1B8BA62D9 |
SHA-1 | 2B0AEBC486FDCB99DF7F2B4876E70E9E0BA586DD |
SHA-256 | 09DC55629659599C4145274BB2CE041E379B9B3C230B44D088AF502A20DD84BF |
SSDEEP | 192:/bDkOIQqy7V1L9tSYBlgEQMejNjTgsVaBOR5rS39wQF+IOgR+Q:/bDkjQD7V1L9sQl7QLjNjsscORg39wQx |
TLSH | T1E8E131B9CB34AA1FC94F5270C08656C0A6DBB24203D56E4A7F04A2057EDB8C29F7761F |
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 | 1720928 |
MD5 | F2B88EA874CB522BCA291309860551E9 |
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 | 1.13-1+b1 |
SHA-1 | 1D609110F580B75411B4C68F1FF40CDA7A835422 |
SHA-256 | E65ECBBC0AA5E7992DCC23256D9E426CF66CA8086D4ECEFBB53276BC887719D9 |