Physics
Scientific paper
Apr 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pcnf.rept..107w&link_type=abstract
In National Inst. for Fusion Science, Proceedings of the Second International Toki Conference on Plasma Physics and Controlled N
Physics
Computerized Simulation, Helical Flow, Magnetic Fields, Magnetohydrodynamics, Plasmas (Physics), Solar Wind, Mach Number, Magnetic Field Configurations, Plasma Control, Plasma Pinch, Solar Rotation, Stellar Rotation
Scientific paper
Structure of the solar/stellar wind plasma and the helical magnetic field are studies by means of MHD simulation in an axisymmetrical system. It is shown that, when the stellar rotation is much faster than the solar rotation, the magnetic pressure force works and the interplanetary current is pinched along the rotation axis and the equatorial plane.
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