Result for 0039A81B6CFBECBC360F124E14C5575FDCD3F110

Query result

Key Value
FileName./usr/share/doc/code-saturne/doxygen/src/doxygen.png
FileSize3829
MD56AAA93DDD24276B68CF27CCD7A0E1DB8
RDS:package_id182052
SHA-10039A81B6CFBECBC360F124E14C5575FDCD3F110
SHA-256AAB3C5BF4C58971288AE7B1F66B61FDA73F0E646D4A6CE6C4932F51615727B80
SSDEEP96:Rxt2RVadP3iSUA3I7gwaYltGjsuOnywtpDtmb3Wx0GR:Rxtf3mAjYltMaywTDCmx0GR
TLSHT1E7814CF1976550BC822E093A80892FB416AA4FDE5440AE4BF310F57CBAE22DB9525603
insert-timestamp1679427100.993856
sourceRDS.db
hashlookup:parent-total16
hashlookup:trust100

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Parents (Total: 16)

The searched file hash is included in 16 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize43958454
MD58E8FAF09CEB82B30D916112E5559EF61
PackageDescriptionGeneral purpose Computational Fluid Dynamics (CFD) software - Documentation The basic capabilities of Code_Saturne enable the handling of either incompressible or expandable flows with or without heat transfer and turbulence. Dedicated modules are available for specific physics such as radiative heat transfer, combustion (gas, coal, heavy fuel oil, ...), magneto-hydrodynamics, compressible flows, two-phase flows (Euler-Lagrange approach with two-way coupling), extensions to specific applications (e.g. Mercure_Saturne for atmospheric environment). . It runs in parallel with MPI on distributed memory machines. Developed since 1997 at EDF R&D, it is based on a co-located Finite Volume approach that accepts meshes with any type of cell (tetrahedral, hexahedral, prismatic, pyramidal, polyhedral...) and any type of grid structure (unstructured, block structured, hybrid, conforming or with hanging nodes, ...). . This package contains the documentation.
PackageMaintainerDebian Science Team <debian-science-maintainers@lists.alioth.debian.org>
PackageNamecode-saturne-doc
PackageSectiondoc
PackageVersion3.3.2-4
SHA-139C22774C38422FE85572A8EE03AC7E8AD0A046F
SHA-2567E5B415B999ECE80A6A3E583A0E4B582D462ACE5CB2847E16595EC38772DC2CA
Key Value
FileSize57553980
MD5E5958B7180D5B7C79005DBED0BFD6A04
PackageDescriptionGeneral purpose Computational Fluid Dynamics (CFD) software - Documentation The basic capabilities of Code_Saturne enable the handling of either incompressible or expandable flows with or without heat transfer and turbulence. Dedicated modules are available for specific physics such as radiative heat transfer, combustion (gas, coal, heavy fuel oil, ...), magneto-hydrodynamics, compressible flows, two-phase flows (Euler-Lagrange approach with two-way coupling), extensions to specific applications (e.g. Mercure_Saturne for atmospheric environment). . It runs in parallel with MPI on distributed memory machines. Developed since 1997 at EDF R&D, it is based on a co-located Finite Volume approach that accepts meshes with any type of cell (tetrahedral, hexahedral, prismatic, pyramidal, polyhedral...) and any type of grid structure (unstructured, block structured, hybrid, conforming or with hanging nodes, ...). . This package contains the documentation.
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecode-saturne-doc
PackageSectiondoc
PackageVersion4.2.1+repack-1
SHA-13E60A9C6435AE02946B8D38459E823F0F9494089
SHA-25659EB0B5717301F98FF8976DE3D8E8483567CD5728C9873596E3965D18E7091D6
Key Value
FileSize133396948
MD5DA456FD6DA5C3BBE3DA5F02591AA76E6
PackageDescriptionGeneral purpose Computational Fluid Dynamics (CFD) software - Documentation The basic capabilities of Code_Saturne enable the handling of either incompressible or expandable flows with or without heat transfer and turbulence. Dedicated modules are available for specific physics such as radiative heat transfer, combustion (gas, coal, heavy fuel oil, ...), magneto-hydrodynamics, compressible flows, two-phase flows (Euler-Lagrange approach with two-way coupling), extensions to specific applications (e.g. Mercure_Saturne for atmospheric environment). . It runs in parallel with MPI on distributed memory machines. Developed since 1997 at EDF R&D, it is based on a co-located Finite Volume approach that accepts meshes with any type of cell (tetrahedral, hexahedral, prismatic, pyramidal, polyhedral...) and any type of grid structure (unstructured, block structured, hybrid, conforming or with hanging nodes, ...). . This package contains the documentation.
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecode-saturne-doc
PackageSectiondoc
PackageVersion5.3.2+repack-1
SHA-140F95D52B1B9CD64FBE20A7C1EC88D81F73AA974
SHA-256F6AF975650DA9949C8DB996E0DE9C097582EB9D88C0E98D1A8659C4B4058F9D0
Key Value
FileSize145048308
MD522AF9AD7A0574DFA2D3BBC0D2DE58E03
PackageDescriptionGeneral purpose Computational Fluid Dynamics (CFD) software - Documentation The basic capabilities of Code_Saturne enable the handling of either incompressible or expandable flows with or without heat transfer and turbulence. Dedicated modules are available for specific physics such as radiative heat transfer, combustion (gas, coal, heavy fuel oil, ...), magneto-hydrodynamics, compressible flows, two-phase flows (Euler-Lagrange approach with two-way coupling), extensions to specific applications (e.g. Mercure_Saturne for atmospheric environment). . It runs in parallel with MPI on distributed memory machines. Developed since 1997 at EDF R&D, it is based on a co-located Finite Volume approach that accepts meshes with any type of cell (tetrahedral, hexahedral, prismatic, pyramidal, polyhedral...) and any type of grid structure (unstructured, block structured, hybrid, conforming or with hanging nodes, ...). . This package contains the documentation.
PackageMaintainerDebian Science Team <debian-science-maintainers@lists.alioth.debian.org>
PackageNamecode-saturne-doc
PackageSectiondoc
PackageVersion6.0.2-2
SHA-16D0A25DA653E5FA1C84C34FCB38E835A72E61566
SHA-2565225B18C04C8A95E593DB52DB7AF60805FE874F3B27866BB97A9BD11BD1FAD12
Key Value
FileSize79412400
MD5359D28CA1656E5AB3479685933D0EE51
PackageDescriptionGeneral purpose Computational Fluid Dynamics (CFD) software - Documentation The basic capabilities of Code_Saturne enable the handling of either incompressible or expandable flows with or without heat transfer and turbulence. Dedicated modules are available for specific physics such as radiative heat transfer, combustion (gas, coal, heavy fuel oil, ...), magneto-hydrodynamics, compressible flows, two-phase flows (Euler-Lagrange approach with two-way coupling), extensions to specific applications (e.g. Mercure_Saturne for atmospheric environment). . It runs in parallel with MPI on distributed memory machines. Developed since 1997 at EDF R&D, it is based on a co-located Finite Volume approach that accepts meshes with any type of cell (tetrahedral, hexahedral, prismatic, pyramidal, polyhedral...) and any type of grid structure (unstructured, block structured, hybrid, conforming or with hanging nodes, ...). . This package contains the documentation.
PackageMaintainerDebian Science Team <debian-science-maintainers@lists.alioth.debian.org>
PackageNamecode-saturne-doc
PackageSectiondoc
PackageVersion4.3.3+repack-1
SHA-1792E9B44A5E3F8DBF234D52C01F5FECAF6414EFE
SHA-256E5CA04C31F8589D71C63DA90602D24EE9F4981C43AD32F6E775CBF445CB778EA
Key Value
FileSize57717734
MD52B42487FAB3F3B551A6DDD342B53239A
PackageDescriptionGeneral purpose Computational Fluid Dynamics (CFD) software - Documentation The basic capabilities of Code_Saturne enable the handling of either incompressible or expandable flows with or without heat transfer and turbulence. Dedicated modules are available for specific physics such as radiative heat transfer, combustion (gas, coal, heavy fuel oil, ...), magneto-hydrodynamics, compressible flows, two-phase flows (Euler-Lagrange approach with two-way coupling), extensions to specific applications (e.g. Mercure_Saturne for atmospheric environment). . It runs in parallel with MPI on distributed memory machines. Developed since 1997 at EDF R&D, it is based on a co-located Finite Volume approach that accepts meshes with any type of cell (tetrahedral, hexahedral, prismatic, pyramidal, polyhedral...) and any type of grid structure (unstructured, block structured, hybrid, conforming or with hanging nodes, ...). . This package contains the documentation.
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecode-saturne-doc
PackageSectiondoc
PackageVersion4.2.0+repack-1build1
SHA-17E875D7C5903ABBEFE1A755829C4BE52D035FE0D
SHA-25601134C42E1AE678958D46D9E70A5CDEF746665DA4D94053A1E069D830F07D68E
Key Value
FileSize145041280
MD56125899C2B8960D88646FFADC46C2300
PackageDescriptionGeneral purpose Computational Fluid Dynamics (CFD) software - Documentation The basic capabilities of Code_Saturne enable the handling of either incompressible or expandable flows with or without heat transfer and turbulence. Dedicated modules are available for specific physics such as radiative heat transfer, combustion (gas, coal, heavy fuel oil, ...), magneto-hydrodynamics, compressible flows, two-phase flows (Euler-Lagrange approach with two-way coupling), extensions to specific applications (e.g. Mercure_Saturne for atmospheric environment). . It runs in parallel with MPI on distributed memory machines. Developed since 1997 at EDF R&D, it is based on a co-located Finite Volume approach that accepts meshes with any type of cell (tetrahedral, hexahedral, prismatic, pyramidal, polyhedral...) and any type of grid structure (unstructured, block structured, hybrid, conforming or with hanging nodes, ...). . This package contains the documentation.
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecode-saturne-doc
PackageSectiondoc
PackageVersion6.0.2-1
SHA-17EF517F337746D1570219A428C502B0B34DA603D
SHA-25692E6ABBF48CDA0F3EFB065C595DBC2534A848F86483AE1D50A0A7AD6ED9C89E3
Key Value
FileName13267
FileSize79031300
MD522F2146BA762891995FFF2FBD67638D5
PackageDescriptionGeneral purpose Computational Fluid Dynamics (CFD) software - Documentation The basic capabilities of Code_Saturne enable the handling of either incompressible or expandable flows with or without heat transfer and turbulence. Dedicated modules are available for specific physics such as radiative heat transfer, combustion (gas, coal, heavy fuel oil, ...), magneto-hydrodynamics, compressible flows, two-phase flows (Euler-Lagrange approach with two-way coupling), extensions to specific applications (e.g. Mercure_Saturne for atmospheric environment). . It runs in parallel with MPI on distributed memory machines. Developed since 1997 at EDF R&D, it is based on a co-located Finite Volume approach that accepts meshes with any type of cell (tetrahedral, hexahedral, prismatic, pyramidal, polyhedral...) and any type of grid structure (unstructured, block structured, hybrid, conforming or with hanging nodes, ...). . This package contains the documentation.
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecode-saturne-doc
PackageSectiondoc
PackageVersion4.3.3+repack-1
RDS:package_id182052
SHA-1861CEC504DB341D29AD253DB4A5682932C1A3174
SHA-256E835EC0D3C8B49063D15A7324055000EC4AFEDEC2AA34B2D34EB102DD94E97A4
insert-timestamp1679408379.7972708
sourceRDS.db
Key Value
FileSize44142056
MD5A034C5E27928EA1B87401679C0924C43
PackageDescriptionGeneral purpose Computational Fluid Dynamics (CFD) software - Documentation The basic capabilities of Code_Saturne enable the handling of either incompressible or expandable flows with or without heat transfer and turbulence. Dedicated modules are available for specific physics such as radiative heat transfer, combustion (gas, coal, heavy fuel oil, ...), magneto-hydrodynamics, compressible flows, two-phase flows (Euler-Lagrange approach with two-way coupling), extensions to specific applications (e.g. Mercure_Saturne for atmospheric environment). . It runs in parallel with MPI on distributed memory machines. Developed since 1997 at EDF R&D, it is based on a co-located Finite Volume approach that accepts meshes with any type of cell (tetrahedral, hexahedral, prismatic, pyramidal, polyhedral...) and any type of grid structure (unstructured, block structured, hybrid, conforming or with hanging nodes, ...). . This package contains the documentation.
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecode-saturne-doc
PackageSectiondoc
PackageVersion3.3.2-4
SHA-189DADC610A897BA08A29BE20D8E8F978A7F05C24
SHA-2564CECBBC4769F5318E1334726DC12AF3AF7A31FF5547133BAE871B6D7A4BCDA7B
Key Value
FileSize144596196
MD57FD936AAD5B27828369BC717C6459EA7
PackageDescriptionGeneral purpose Computational Fluid Dynamics (CFD) software - Documentation The basic capabilities of Code_Saturne enable the handling of either incompressible or expandable flows with or without heat transfer and turbulence. Dedicated modules are available for specific physics such as radiative heat transfer, combustion (gas, coal, heavy fuel oil, ...), magneto-hydrodynamics, compressible flows, two-phase flows (Euler-Lagrange approach with two-way coupling), extensions to specific applications (e.g. Mercure_Saturne for atmospheric environment). . It runs in parallel with MPI on distributed memory machines. Developed since 1997 at EDF R&D, it is based on a co-located Finite Volume approach that accepts meshes with any type of cell (tetrahedral, hexahedral, prismatic, pyramidal, polyhedral...) and any type of grid structure (unstructured, block structured, hybrid, conforming or with hanging nodes, ...). . This package contains the documentation.
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecode-saturne-doc
PackageSectiondoc
PackageVersion6.0.2-2build1
SHA-1917646970BF7D456A230410B213EB75E53C18E79
SHA-2567691F51E4E48286FC91D7BEB9A56BEE4EB9F1A99C7BBC2BEA746BCC45F04AB38