Key | Value |
---|---|
FileName | ./usr/share/doc/python-pint-doc/html/_static/documentation_options.js |
FileSize | 355 |
MD5 | 3CEED40D4FABEB01CE471E073B0021C3 |
SHA-1 | 4740C100D56CD6FC1AE5B11EBAF85CC5B01BC889 |
SHA-256 | 9AA59531D03648710C16DCBD4AB04EE4A23B21000C8F876D670CC4E3AC3A41A7 |
SSDEEP | 6:qOppJXzibDRd7HyLmx5wB0FFukfBxd0aQWsIIdQnp/Ub/+aJ4VC:1yDRRZxbukf6II+np/U7/J4VC |
TLSH | T126E026F6383059AE28E22EB4B91E85813820C8231C6E3192300D10022FACF4D0138BAA |
hashlookup:parent-total | 15 |
hashlookup:trust | 100 |
The searched file hash is included in 15 parent files which include package known and seen by metalookup. A sample is included below:
Key | Value |
---|---|
FileSize | 3518344 |
MD5 | 10545D09B6213B79B20C52D18C9599C5 |
PackageDescription | Reading and manipulaing satellite sensor spectral responses - documentation 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 includes the PySpectral documentation in HTML format. |
PackageMaintainer | Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com> |
PackageName | python3-pyspectral-doc |
PackageSection | doc |
PackageVersion | 0.10.4+ds-1 |
SHA-1 | 07222F1B0CEE9136A262049976820DF1A3BE2849 |
SHA-256 | D39B7806271FDF5CDD47145887A8D4DD4B2D0952BFF2DF9302E1E9DA0DE6C076 |
Key | Value |
---|---|
FileSize | 35704 |
MD5 | 9B485A8B2AC0C1C91C8DA730A27612FB |
PackageDescription | Django model mixins and utilities — Documentation Django is a high-level web application framework that loosely follows the model-view-controller design pattern. . The ‘django-model-utils’ library provides some mixins and utilities for Django: . * QueryManager: one-line definition of Managers returning a custom QuerySet. * InheritanceCastModel: more efficient use of model inheritance * TimeStampedModel: self-updating ‘created’ and ‘modified’ fields. . This package installs the documentation for the library. |
PackageMaintainer | Debian Python Team <team+python@tracker.debian.org> |
PackageName | python-django-model-utils-doc |
PackageSection | doc |
PackageVersion | 4.1.1-2 |
SHA-1 | F0BB9FDFC1CCA5FBDF73BBAFEE9FE48B2D3F10BE |
SHA-256 | 9C4B22EB80E5B0844C8D79BC8EC7638C9F03E5D0CF8527686A8A87CAEB77B30A |
Key | Value |
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FileSize | 48096 |
MD5 | 3AB5B483084DE1C63DD8575F49CC63F4 |
PackageDescription | Django model mixins and utilities — Documentation Django is a high-level web application framework that loosely follows the model-view-controller design pattern. . The ‘django-model-utils’ library provides some mixins and utilities for Django: . * QueryManager: one-line definition of Managers returning a custom QuerySet. * InheritanceCastModel: more efficient use of model inheritance * TimeStampedModel: self-updating ‘created’ and ‘modified’ fields. . This package installs the documentation for the library. |
PackageMaintainer | Debian Python Team <team+python@tracker.debian.org> |
PackageName | python-django-model-utils-doc |
PackageSection | doc |
PackageVersion | 4.2.0-1 |
SHA-1 | 4BB80E53BEB9A842BA43D7EF1465C7D993A1922B |
SHA-256 | 15D24B5E4900183013BB8B75450B58FB0C49F1ED6B0041A0C1C59DE82C593BCD |
Key | Value |
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FileSize | 296460 |
MD5 | 89DC96FEA45AB7D612A5156B8DD282A9 |
PackageDescription | define, operate and manipulate physical quantities - doc Pint is Python module/package to define, operate and manipulate physical quantities: the product of a numerical value and a unit of measurement. It allows arithmetic operations between them and conversions from and to different units. . It is distributed with a comprehensive list of physical units, prefixes and constants. Due to its modular design, you can extend (or even rewrite!) the complete list without changing the source code. . This package contains the documentation. |
PackageMaintainer | Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com> |
PackageName | python-pint-doc |
PackageSection | doc |
PackageVersion | 0.16.1-1 |
SHA-1 | 42AB2891E5D6BD967FE36F8F99F71436CC2A3C8A |
SHA-256 | AC6B55E0B9EAABF60207683ECE7C5930DC80234AFEF0418AFC88B94D190D97B6 |
Key | Value |
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FileSize | 3521136 |
MD5 | 779F513AEE1A6FAD331996873D03F904 |
PackageDescription | Reading and manipulaing satellite sensor spectral responses - documentation 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 includes the PySpectral documentation in HTML format. |
PackageMaintainer | Debian GIS Project <pkg-grass-devel@lists.alioth.debian.org> |
PackageName | python3-pyspectral-doc |
PackageSection | doc |
PackageVersion | 0.10.4+ds-1 |
SHA-1 | 9779069BBC3C0BC805942D5DA50CF855A798D74E |
SHA-256 | 0D8252E3D38F47B77DBBA3C9064FA2A4B1C569DB670946EBF01B4A26F1F701D8 |
Key | Value |
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FileSize | 25932 |
MD5 | 4C7495AFC2511470A397B7EDD84B4E3B |
PackageDescription | Dithered image combination for Python (API documentation) The drizzle library is a Python package for combining dithered images into a single image. This library is derived from code used in drizzlepac. Like drizzlepac, most of the code is implemented in the C language. The biggest change from drizzlepac is that this code passes an array that maps the input to output image into the C code, while the drizzlepac code computes the mapping by using a Python callback. Switching to using an array allowed the code to be greatly simplified. . This package contains the API documentation. |
PackageMaintainer | Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com> |
PackageName | python-drizzle-doc |
PackageSection | doc |
PackageVersion | 1.13.1-2build4 |
SHA-1 | CFAC731929954DF6AEB58754C670A545775C5E5C |
SHA-256 | 0A476708437CA9C9191D7F4842D0E38A71590ADB523EA2E17BF08918FC50DC9E |
Key | Value |
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MD5 | FA7B2273A06B282CD3033C61443CBDCF |
PackageArch | noarch |
PackageDescription | Documentation for positional |
PackageMaintainer | Fedora Project |
PackageName | python-positional-doc |
PackageRelease | 18.fc34 |
PackageVersion | 1.1.1 |
SHA-1 | 3E7A7921D41B84AF10F6A17E336D66B90649008C |
SHA-256 | ED22342B80E258D0CB2CAAD759130F962923DF7864D34BDBD1B35EE973EEC70D |
Key | Value |
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FileSize | 55108 |
MD5 | C9ED7B6E23DE27873F9D3262FF84304F |
PackageDescription | Django LDAP authentication backend (documentation) Django authentication backend that authenticates against an LDAP service. Configuration can be as simple as a single distinguished name template, but there are many rich configuration options for working with users, groups, and permissions. . This package contains the documentation. |
PackageMaintainer | Debian Python Team <team+python@tracker.debian.org> |
PackageName | python-django-auth-ldap-doc |
PackageSection | doc |
PackageVersion | 3.0.0-1 |
SHA-1 | 12F23D3D84628F81A3B5E909A7BD73C812BCE20A |
SHA-256 | D29FA83D0F7EA00E93714089B9C771FE0C54A7F408D348C680729D0459EE345B |
Key | Value |
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MD5 | A3D2BE607F79D58F398FABE5FC22E96D |
PackageArch | noarch |
PackageDescription | HTML documentation for catkin_tools |
PackageMaintainer | Fedora Project |
PackageName | python-catkin_tools-doc |
PackageRelease | 3.fc34 |
PackageVersion | 0.6.1 |
SHA-1 | 4F15F909568314813319682439407BCECA16DE03 |
SHA-256 | 5152EF6475F5A27FF4272FC798384336E9867C71C47BA304BC806B0EE9BE19D3 |
Key | Value |
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FileSize | 307744 |
MD5 | B0A9FC4C50888D81E81E3EF489D4B5D7 |
PackageDescription | define, operate and manipulate physical quantities - doc Pint is Python module/package to define, operate and manipulate physical quantities: the product of a numerical value and a unit of measurement. It allows arithmetic operations between them and conversions from and to different units. . It is distributed with a comprehensive list of physical units, prefixes and constants. Due to its modular design, you can extend (or even rewrite!) the complete list without changing the source code. . This package contains the documentation. |
PackageMaintainer | Debian Python Team <team+python@tracker.debian.org> |
PackageName | python-pint-doc |
PackageSection | doc |
PackageVersion | 0.16.1-1 |
SHA-1 | AD1EED342E5E608B9274C8E6981C4B755C62CB40 |
SHA-256 | C0BA079C6EBE19BB34C5E3C2996073A1E0629D3C33ADC944B4973CB26FBD5199 |
Key | Value |
---|---|
MD5 | FF1F8B20F7E2E040043F68A12DD73BFD |
PackageArch | noarch |
PackageDescription | Documentation for positional |
PackageMaintainer | Fedora Project |
PackageName | python-positional-doc |
PackageRelease | 17.fc33 |
PackageVersion | 1.1.1 |
SHA-1 | BAA1AAEBA479233A476A6EA9C24416072C5D72D3 |
SHA-256 | 1D553FC98149CE82D7D72AC6A865B960E11C6AF1EC4BB80124681E14E8634B36 |
Key | Value |
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FileSize | 3521244 |
MD5 | A3D4439D87CC75C9040BEEC0191FCF61 |
PackageDescription | Reading and manipulaing satellite sensor spectral responses - documentation 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 includes the PySpectral documentation in HTML format. |
PackageMaintainer | Debian GIS Project <pkg-grass-devel@lists.alioth.debian.org> |
PackageName | python3-pyspectral-doc |
PackageSection | doc |
PackageVersion | 0.10.5+ds-1 |
SHA-1 | 413637B5202A91F2DBD7117960177AAE49F347E9 |
SHA-256 | 221D5CEE8D843E5B75C71785A421245B3BAB69B888A75C1B476CC83DFD765A9B |
Key | Value |
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MD5 | B13C1A046CC7637C83E2DBC0793280BC |
PackageArch | x86_64 |
PackageDescription | The javabridge Python package makes it easy to start a Java virtual machine (JVM) from Python and interact with it. Python code can interact with the JVM using a low-level API or a more convenient high-level API. |
PackageMaintainer | Fedora Project |
PackageName | python3-javabridge |
PackageRelease | 2.fc34 |
PackageVersion | 1.0.19 |
SHA-1 | DA3E865644A98C8317E4A34BDB8A49BDD2D57F94 |
SHA-256 | B08D7BD49F44712142AFA6F0C306E30284D383658EE23F366ACAC44776AC5133 |
Key | Value |
---|---|
MD5 | EBEBE2D2C2ADACC2160A7A6BE3CF829E |
PackageArch | noarch |
PackageDescription | HTML documentation for catkin_tools |
PackageMaintainer | Fedora Project |
PackageName | python-catkin_tools-doc |
PackageRelease | 2.fc33 |
PackageVersion | 0.6.1 |
SHA-1 | F45DC75D70069881609CAC506E0AAFEDCD2EE941 |
SHA-256 | 499A4F38BF4DB968216CCF75FB820B5FCE8E47508F6F6DAA2A0C5E6171C0F1A3 |
Key | Value |
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MD5 | EA917FEF5868BA75A2DC9C5D12AC56D5 |
PackageArch | x86_64 |
PackageDescription | The javabridge Python package makes it easy to start a Java virtual machine (JVM) from Python and interact with it. Python code can interact with the JVM using a low-level API or a more convenient high-level API. |
PackageMaintainer | Fedora Project |
PackageName | python3-javabridge |
PackageRelease | 1.fc33 |
PackageVersion | 1.0.19 |
SHA-1 | 0AF4E6C6B1EA52A6EF8EDCFD4FA08B06C5EF492E |
SHA-256 | 5D0FFA89D74B52E0F3BFEE61799B51E5D0FE016BDC65611C1778CA996B1D70CD |