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

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Uploaded by:
Debian Science Team
Uploaded to:
Sid
Original maintainer:
Debian Science Team
Architectures:
any all
Section:
science
Urgency:
Low Urgency

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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

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.