Statistics – Computation
Scientific paper
Aug 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989p%26ss...37..987f&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 37, Aug. 1989, p. 987-999.
Statistics
Computation
6
Computational Astrophysics, Coronal Holes, Plasma-Electromagnetic Interaction, Solar Magnetic Field, Solar Wind, Electric Current, Lines Of Force, Magnetic Field Configurations, Self Consistent Fields, Two Fluid Models
Scientific paper
A new model for the solar wind expansion out of diverging magnetic field configurations is proposed. By use of natural curvilinear coordinates the equations of a quasi-two-fluid model are solved along the field lines of such configurations. This allows a detailed analysis of the plasma parameters within a coronal hole and the calculation of the electric currents caused by the expanding plasma. It is then possible to iterate the plasma/magnetic-field interaction and obtain information about the degree of self-consistency of the computed solution in each iteration step. A method to determine the exact self-consistent solution is outlined.
Fahr Hans Jörg
Fichtner Horst
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