code-saturne 2.1.0-4 source package in Ubuntu

Changelog

code-saturne (2.1.0-4) unstable; urgency=low

  * Fix a as-needed issue. Thanks to Ilya Barygin for the patch
    (Closes: #651672)
 -- Bhavani Shankar <email address hidden>   Sun, 11 Dec 2011 19:26:58 +0100

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

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code-saturne_2.1.0-4.debian.tar.gz 5.1 KiB 724f8b591987637c200fd6cb1ddbc245158a8568259e224a046a5cfff516227f
code-saturne_2.1.0-4.dsc 2.2 KiB 537c3e8b0ca4c581836240c145b6db3b7b9c35485b1dcbc09778e2b5952fed43

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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.