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Global MHD simulations of Saturn's magnetosphere at the time of Cassini approach

✍ Scribed by Hansen, K. C.

Book ID
119666179
Publisher
American Geophysical Union
Year
2005
Tongue
English
Weight
215 KB
Volume
32
Category
Article
ISSN
1944-8007

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This paper presents a dynamic domain decomposition (D 3 ) technique for implementing the parallelization of the piecewise parabolic method (PPM) for solving the ideal magnetohydrodynamics (MHD) equations. The key point of D 3 is distributing the work dynamically among processes during the execution