Asymmetric Emerging Flux Loops and the Rotation of Sunspot Groups

Details Asymmetric Emerging Flux Loops and the Rotation of Sunspot Groups Asymmetric Emerging Flux Loops and the Rotation of Sunspot Groups

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cokon.100..287b&link_type=abstract

Communications of the Konkoly Observatory, No. 100 (Vol. XII, 2), p. 287-292 (1997)

Physics

Scientific paper

From the analysis of the rotation rate of the middle point between the
main spots of a given number (49) of sunspot groups taken from the
Greenwich Photoheliographic Results for the years 1964-1976 that cover
the solar cycle no. 20, it is proved that the magnetic flux loops
emerging from bipolar sunspot groups are asymmetric.

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