Calculation of steady MHD flows in the solar corona

Details Calculation of steady MHD flows in the solar corona Calculation of steady MHD flows in the solar corona

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25...17p&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, Jan.-Feb. 1985, p. 17-22. In Russian.

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5

Magnetohydrodynamic Flow, Solar Corona, Steady Flow, Flow Equations, High Reynolds Number, Inviscid Flow, Isothermal Processes

Scientific paper

A method is proposed for solving single-fluid MHD equations in order to study steady plasma flows in the solar corona. The method is characterized by the fact that it can be used to solve three-dimensional problems without assuming any sort of spatial symmetry of the flow. A numerical solution is obtained for an isothermal inviscid plasma in the case of large magnetic Reynolds numbers.

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