A theorem on the steady magnetohydrodynamic flows in the solar corona.

Details A theorem on the steady magnetohydrodynamic flows in the solar corona. A theorem on the steady magnetohydrodynamic flows in the solar corona.

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995acaps..15..387s&link_type=abstract

Acta Astrophys. Sin., Vol. 15, No. 4, p. 387 - 389

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Solar Corona: Magnetohydrodynamics

Scientific paper

A theorem and an important relation on the steady magnetohydrodynamic
flows flowing along the magnetic field lines in the solar corona or
other astrophysical circumstances are reported. They are derived by use
of the ratio of the macroscopic kinetic energy density to the magnetic
energy density.

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