Excitation of non-axially symmetric modes of the sun's mean magnetic field

Details Excitation of non-axially symmetric modes of the sun's mean magnetic field Excitation of non-axially symmetric modes of the sun's mean magnetic field

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..115....5r&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 115, no. 1, 1988, p. 5-15.

Physics

14

Dynamo Theory, Helioseismology, Kinematic Equations, Solar Magnetic Field, Angular Velocity, Asymptotic Methods, Modes, Wentzel-Kramer-Brillouin Method

Scientific paper

The kinematic dynamo equations for the mean magnetic field are solved with an asymptotic method of the WKB type. The excitation conditions and main characteristics of the non-axially symmetric modes for a given distribution of the sources are obtained. Utilization of the helioseismologic data on the Sun's internal rotation permits an explanation, within the framework of dynamo theory, of the excitation of the main non-axially symmetric modes revealed in the Sun's magnetic field sector structure.

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