Result for 00619BC28E047160C09ED7EC6581E99F99052E46

Query result

Key Value
FileName./usr/share/doc/code-saturne/doxygen/src/form_421.png
FileSize361
MD52F0B627267E712AE35747D8724773026
RDS:package_id182052
SHA-100619BC28E047160C09ED7EC6581E99F99052E46
SHA-256B21513157A8784AC4B28DA429E97C2CE0E945AD02443D4A7BF4CE1DE5FC6939E
SSDEEP6:6v/lhPs2/A0M+9Y8+KuxrqPUAzQzSVjVB2RPTnkj4pIoEJs/KVnjvuUycYp:6v/7zAvELgqN4SVjX2lTXpIoEK/KFjVy
TLSHT124E07DD27110DC6FF2A37BB3C699383379610108C6B572C9C85EB412A11779AB3A2797
insert-timestamp1679427104.8722987
sourceRDS.db
hashlookup:parent-total4
hashlookup:trust70

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Parents (Total: 4)

The searched file hash is included in 4 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
FileSize124587540
MD522296F6A999528B7CD21D66CA6E997C6
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
PackageVersion5.2.0+repack-1build2
SHA-1E08CBBFC15DB415313E4C5B5894C779D29F83F37
SHA-2568AAFA6095F1CA94D5C0A6BBF252FAF06D81408A24E58F0138C0DF4A510841525
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