Magnetohydrodynamic models of coronal transients in the meridional plane. IV - Effect of the solar wind

Details Magnetohydrodynamic models of coronal transients in the meridional plane. IV - Effect of the solar wind Magnetohydrodynamic models of coronal transients in the meridional plane. IV - Effect of the solar wind

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...243..641w&link_type=abstract

Astrophysical Journal, Part 1, vol. 243, Jan. 15, 1981, p. 641-643.

Astronomy and Astrophysics

Astrophysics

10

Magnetohydrodynamics, Solar Corona, Solar Wind, Beta Factor, Boundary Value Problems, Thermodynamic Properties

Scientific paper

A two-dimensional, time-dependent magnetohydrodynamic model in the meridional plane with and without an ambient solar wind in an ambient radial magnetic field has been used to investigate mass motions associated with coronal transients. It is shown that the solar wind does not significantly affect the general dynamic characteristics of the mass motion. The ambient solar wind, however, increases the velocity of the mass motion and produces a moderate change in the thermodynamic properties of the coronal plasma.

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