Solar and stellar magnetic fields and atmospheric structures - Theory

Details Solar and stellar magnetic fields and atmospheric structures - Theory Solar and stellar magnetic fields and atmospheric structures - Theory

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..121..271p&link_type=abstract

(IAU, Colloquium on Solar and Stellar Flares, 104th, Stanford, CA, Aug. 15-19, 1988) Solar Physics (ISSN 0038-0938), vol. 121, n

Physics

40

Magnetoactivity, Solar Magnetic Field, Stellar Atmospheres, Stellar Magnetic Fields, Convective Flow, Current Sheets, Photosphere, Solar Prominences, Sunspots

Scientific paper

Theoretical understanding of the role of magnetic fields in the formation of solar atmospheric structure is reviewed. The origin of the solar magnetic field, the dynamical behavior of the azimuthal field in the convective zone, the fibril state of the field in the photosphere, the formation of sunspots and prominences, and the spontaneous formation of current sheets in the bipolar field above the solar surface are addressed. The relation of the latter to coronal heating and flare formation is considered.

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