Result for 001D45E42ABDE3D9457D21AD595EE920B1389465

Query result

Key Value
FileName./usr/share/doc/code-saturne/doxygen/src/search/enumvalues_11.js
FileSize757
MD5BB5FA8E9C44853155C6DDE0CAE863EED
RDS:package_id182052
SHA-1001D45E42ABDE3D9457D21AD595EE920B1389465
SHA-25665733BB3A3E3AA65C971600443CBE6DDC49618463BF2B93A4D0E0D4EFB53558D
SSDEEP12:NQL5YQ95PDjzfYQ95PVw5qUYQ95P5Yn5FYQ95PrQ3n6akrw5w0YQ95PFA:NQpHVaC5p0XS05q
TLSHT17801D61103644C0B57A8FEE4AA86CFAE76C70C624DC69A6487D10AB622C7331FD3C277
insert-timestamp1679427095.029887
sourceRDS.db
hashlookup:parent-total5
hashlookup:trust75

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Parents (Total: 5)

The searched file hash is included in 5 parent files which include package known and seen by metalookup. A sample is included below:

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
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
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
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
FileSize80199426
MD5D3A3DBF8C21FF18AD925978E5D80CF42
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-1build1
SHA-1CA8E45F69BE498CF9C51A4C9CA328BB0FDAF159E
SHA-256A6B0A2A2B6B2D7F82BDB98A55B29AE887A6D5CD8A5BB5E73BC2F3853DB877F40