A necessary condition for the energy loss function of the steady MHD flows in the solar corona.

Details A necessary condition for the energy loss function of the steady MHD flows in the solar corona. A necessary condition for the energy loss function of the steady MHD flows in the solar corona.

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995arbei..27...58s&link_type=abstract

Astrophysics Reports, Publications of the Beijing Astronomical Observatory, No. 27, p. 58 - 60

Astronomy and Astrophysics

Astrophysics

Solar Corona: Magnetohydrodynamics

Scientific paper

A newly derived necessary condition for the energy loss function of the
steady magnetohydrodynamic flows flowing along the magnetic field lines
is reported; therefore a constraint on the models of this kind of flow
in the solar corona is presented. A new method for solving this kind of
problem is outlined.

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