Magnetohydrodynamics of Astrophysical Winds

Details Magnetohydrodynamics of Astrophysical Winds Magnetohydrodynamics of Astrophysical Winds

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke2227h&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 2227. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Theoretical Concepts And Tools, Theoretical Concepts

Scientific paper

Stellar mass loss became an issue when Parker (1958) first introduced the concept of the solar wind. Such a thermal wind results from coronal heating processes indirectly associated with the existence of a convection zone, also responsible, with rotation, for the star's dynamo action (see articles on SOLAR WIND: THEORY, CORONAL HEATING MECHANISMS, SOLAR INTERIOR: CONVECTION ZONE and MAGNETOHYDROD...

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