Key | Value |
---|---|
FileName | ./usr/share/coda/definitions/AURA_OMI-20161024.codadef |
FileSize | 6706 |
MD5 | 5795599913500FC40B3199E583081F33 |
SHA-1 | 4E0BEC814A5ED504F4F5E1708A8DF6394AACEC37 |
SHA-256 | C4DDD40886757B9DFEB1F2CC0F6EB421DF1C024B4EA66DD8B90C92D137213BE8 |
SSDEEP | 192:ENa7LkpalWXh7FLCdpOBTICHt0t/jVcWEscCQ3GtArJJr+8uLD88cVtzY42ITXS:ENaXkp6WR7FCdpOBTICHat/jaWEscCUc |
TLSH | T146D153A5DD34012DDA5FF4308C031A88F663C2095BC477AFB858A68D7A7B1C55F35A9C |
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 | 1718412 |
MD5 | 9FA1948D0C06DA966F5E4BFD0D2EC9A0 |
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 | E00BC526D7661A0EF8729CD6A47F96958695F1F1 |
SHA-256 | 0B525DFD89DEC6C6A14F54705FC35C046AA7C9616A7294F3C60832969126571B |