Magnetic flux lifting from the relaxation zone to the photospheric level

Details Magnetic flux lifting from the relaxation zone to the photospheric level Magnetic flux lifting from the relaxation zone to the photospheric level

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70..134r&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 70, no. 1, p. 134-140.

Astronomy and Astrophysics

Astronomy

2

Magnetic Flux, Molecular Relaxation, Photosphere, Solar Convection (Astronomy), Solar Oscillations, Solar Magnetic Field, Solar Temperature

Scientific paper

The evolution of the oscillations of magnetic flux tubes in the relaxation zone and the lifting of magnetic flux from the relaxation zone to the photospheric level are investigated on the basis of a numerical solution of a nonlinear system of MHD equations. Rough estimates are made to determine the energy capacity of the relaxation zone in the solar dynamo. The heat transfer process is shown to be a major factor destroying the oscillation structure of magnetic fields in the relaxation zone.

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