Result for 1D553DC312D140DD6ABE3D44A138A839567830FE

Query result

Key Value
FileName./usr/bin/download_atm_correction_luts
FileSize1888
MD524C2389A5F2D7A1E8F27E979B7C4DCD2
SHA-11D553DC312D140DD6ABE3D44A138A839567830FE
SHA-256A96073C14FCFF9ED5ED3F4D6BBBD76C85FA17DAF882383F93CA7006767A0A060
SSDEEP24:Ye0L2nSCUgiyUVOkHxHqTbV3nqv4nNnlc/Zn3p1regdXHtCqWIegsZ:GySzjyUjH0Qd3DpXo
TLSHT1A54197182882E1704CC031B8281E6B8EF23756032B64F490359C6B7D7F07D79C5E79D9
hashlookup:parent-total3
hashlookup:trust65

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Parents (Total: 3)

The searched file hash is included in 3 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize12108
MD5BD7B4A3E991A085618567D882A514BCB
PackageDescriptionReading and manipulaing satellite sensor spectral responses - scripts Reading and manipulaing satellite sensor spectral responses and the solar spectrum, to perform various corrections to VIS and NIR band data. . Given a passive sensor on a meteorological satellite PySpectral provides the relative spectral response (rsr) function(s) and offer some basic operations like convolution with the solar spectrum to derive the in band solar flux, for instance. . The focus is on imaging sensors like AVHRR, VIIRS, MODIS, ABI, AHI, OLCI and SEVIRI. But more sensors are included and if others are needed they can be easily added. With PySpectral it is possible to derive the reflective and emissive parts of the signal observed in any NIR band around 3-4 microns where both passive terrestrial emission and solar backscatter mix the information received by the satellite. Furthermore PySpectral allows correcting true color imagery for the background (climatological) atmospheric signal due to Rayleigh scattering of molecules, absorption by atmospheric gases and aerosols, and Mie scattering of aerosols. . This package provides utilities and executable scripts.
PackageMaintainerDebian GIS Project <pkg-grass-devel@lists.alioth.debian.org>
PackageNamepyspectral-bin
PackageSectionutils
PackageVersion0.10.5+ds-1
SHA-1DCB4C93EB3E502E3E55C675F4113A757EEED247F
SHA-256866CE8AC9677A5A2ED47B4F5CC3C4363948A6F6EC1831B36F163FADAD16AEA59
Key Value
FileSize11980
MD5A3BEB38284BEEECBBDACAFA766A0DF34
PackageDescriptionReading and manipulaing satellite sensor spectral responses - scripts Reading and manipulaing satellite sensor spectral responses and the solar spectrum, to perform various corrections to VIS and NIR band data. . Given a passive sensor on a meteorological satellite PySpectral provides the relative spectral response (rsr) function(s) and offer some basic operations like convolution with the solar spectrum to derive the in band solar flux, for instance. . The focus is on imaging sensors like AVHRR, VIIRS, MODIS, ABI, AHI, OLCI and SEVIRI. But more sensors are included and if others are needed they can be easily added. With PySpectral it is possible to derive the reflective and emissive parts of the signal observed in any NIR band around 3-4 microns where both passive terrestrial emission and solar backscatter mix the information received by the satellite. Furthermore PySpectral allows correcting true color imagery for the background (climatological) atmospheric signal due to Rayleigh scattering of molecules, absorption by atmospheric gases and aerosols, and Mie scattering of aerosols. . This package provides utilities and executable scripts.
PackageMaintainerDebian GIS Project <pkg-grass-devel@lists.alioth.debian.org>
PackageNamepyspectral-bin
PackageSectionutils
PackageVersion0.10.4+ds-1
SHA-13EC59C51C3BF7087DCD9AA26077CB4F395AFA853
SHA-25626E94429E2D1CA216876E51413D2A58DCAF8751E63752EFBB9BDF0964225124E
Key Value
FileSize8412
MD5DD640845C0AB6CF5205A7AE28A8B9BD1
PackageDescriptionReading and manipulaing satellite sensor spectral responses - scripts Reading and manipulaing satellite sensor spectral responses and the solar spectrum, to perform various corrections to VIS and NIR band data. . Given a passive sensor on a meteorological satellite PySpectral provides the relative spectral response (rsr) function(s) and offer some basic operations like convolution with the solar spectrum to derive the in band solar flux, for instance. . The focus is on imaging sensors like AVHRR, VIIRS, MODIS, ABI, AHI, OLCI and SEVIRI. But more sensors are included and if others are needed they can be easily added. With PySpectral it is possible to derive the reflective and emissive parts of the signal observed in any NIR band around 3-4 microns where both passive terrestrial emission and solar backscatter mix the information received by the satellite. Furthermore PySpectral allows correcting true color imagery for the background (climatological) atmospheric signal due to Rayleigh scattering of molecules, absorption by atmospheric gases and aerosols, and Mie scattering of aerosols. . This package provides utilities and executable scripts.
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamepyspectral-bin
PackageSectionutils
PackageVersion0.10.4+ds-1
SHA-192E8234F0399814F4FD2B828E65862A97F180EC4
SHA-25632D69AAD075AE2643A81F9B74976B3C08427D26D44D8DF93F3F3A85BB3DF6337