code-saturne 3.2.1-1 source package in Ubuntu
Changelog
code-saturne (3.2.1-1) unstable; urgency=low * New upstream release * Cherry-pick a patch from upstream to fix the install fix-the-make-install.diff * Use dh-autoreconf to rebuild the autotools files -- Sylvestre Ledru <email address hidden> Tue, 10 Dec 2013 09:51:14 +0100
Upload details
- Uploaded by:
- Debian Science Team
- Uploaded to:
- Sid
- Original maintainer:
- Debian Science Team
- Architectures:
- any all
- Section:
- science
- Urgency:
- Low Urgency
See full publishing history Publishing
Series | Published | Component | Section |
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Downloads
File | Size | SHA-256 Checksum |
---|---|---|
code-saturne_3.2.1-1.dsc | 2.6 KiB | 1f225962d45bc60f50b934bcce1e2f8da93c5ad76feff6de7e4bf157ed9d111d |
code-saturne_3.2.1.orig.tar.gz | 37.8 MiB | 383f7c18a06ae47fbe4eae47a8b45b6180cb04e70614309b34a750f0e4b158aa |
code-saturne_3.2.1-1.debian.tar.gz | 6.7 KiB | b902071083e0284f2546de19903dcfb25c1d6c4901beba1149b400017e177ab6 |
Available diffs
- diff from 3.1.0-1 to 3.2.1-1 (20.6 MiB)
No changes file available.
Binary packages built by this source
- code-saturne: General purpose Computational Fluid Dynamics (CFD) software
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, ...).
- code-saturne-bin: General purpose Computational Fluid Dynamics (CFD) software - binaries
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 binary files.
- code-saturne-data: General purpose Computational Fluid Dynamics (CFD) software - data
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 data.
- code-saturne-doc: General 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.
- code-saturne-include: General purpose Computational Fluid Dynamics (CFD) software - includes
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 include files.