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BATSRUS (Version 1)

Abstract
BATSRUS is a new 3-D magnetohydrodynamics (MHD) code that has been developed for massively parallel computers using adaptive mesh refinement (AMR) and a new 8-wave Riemann solver. The code was implemented on a CRAY T3D massively parallel computer with 512 processors. In the first application, which modeled the expansion of the solar wind from the solar surface, the code achieved 13 gigaFLOPS.
DateOfInformation
Wed Jul 15 08:19:10 1998
Domain
Scientific and Engineering Applications
Keyword
Heliospheric Physics, parallel programming/partitioning, solution-adaptive grids and methods
Language
Fortran 90
Name
BATSRUS (Version 1)
TargetEnvironment
CRAY T3D
Webpage
http://hpcc.engin.umich.edu/HPCC/codes/index.html
ContactIs
Tamas I. Gombosi
Files
BATSRUS (Code Version 1)

Meta Data URL from which this entry was created:
http://sdcd.gsfc.nasa.gov/rib/repositories/ESS/objects/Asset/batsrusv1.html
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