A time-dependent solution of transonic, trans-Alfvenic MHD flow in the solar meridian

Details A time-dependent solution of transonic, trans-Alfvenic MHD flow in the solar meridian A time-dependent solution of transonic, trans-Alfvenic MHD flow in the solar meridian

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993scsmp..36...83z&link_type=abstract

Science in China, Series A - Mathematics, Physics, Astronomy and Technological Sciences (ISSN 1001-6511), vol. 36, no. 1, p. 83-

Statistics

Computation

2

Magnetohydrodynamic Flow, Solar Wind, Time Dependence, Transonic Flow, Computational Fluid Dynamics, Current Sheets, Heliosphere, Magnetic Field Configurations, Solar Corona

Scientific paper

A time-dependent method and a practical differentiating scheme are proposed for obtaining the transonic, trans-Alfvenic solution for the background solar wind with the formation of a heliospheric current sheet. The projected-characteristic boundary conditions in spherical coordinates is successfully used at the inner and outer boundaries. A closed magnetic field is shown to be drawn outside by the expanding solar wind to gradually change into the quasi-helmet type. The simulation results also indicate possible distributions of the dynamic and magnetic parameters over the solar meridian.

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