Relation between the toroidal field in the solar convective layer and the BI-polar field of sunspots

Details Relation between the toroidal field in the solar convective layer and the BI-polar field of sunspots Relation between the toroidal field in the solar convective layer and the BI-polar field of sunspots

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982cha%26a...6..298z&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 6, Issue 4, p. 298-304.

Astronomy and Astrophysics

Astrophysics

Scientific paper

In the solar convective layer, there is a strong toroidal field and a vertical gradient in the turbulent magnetic diffusivity. As a fluid blob rises through magnetic buoyancy, a steep gradient in the turbulent magnetic diffusivity across the surface of the blob is generated. This will perturb the toroidal field, resulting in the formation of a magnetic ring around the blob. An attempt is made to account for the concentration of the bipolar sunspot field in terms of this ring.

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