Two-dimensional MHD equilibria in the solar corona

Details Two-dimensional MHD equilibria in the solar corona Two-dimensional MHD equilibria in the solar corona

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991chjss..11...81w&link_type=abstract

(Chinese Journal of Space Science, vol. 11, no. 2, 1991, p. 81-90) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 15,

Astronomy and Astrophysics

Astrophysics

Magnetohydrodynamic Flow, Plasma Equilibrium, Solar Corona, Solar Wind, Analytic Functions, Flow Velocity, Plasma Density

Scientific paper

A combined analytical and numerical method is used to treat the question
of two-dimensional MHD equilibrium in an inviscid compressible,
perfectly conducting plasma with an embedded magnetic field in the
spherically symmetric gravitational field of the sun. Two solutions are
obtained.

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