Study of possible subsurface influences on the emerging active regions

Details Study of possible subsurface influences on the emerging active regions Study of possible subsurface influences on the emerging active regions

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..139..247b&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 139, no. 2, June 1992, p. 247-254.

Physics

4

Angular Velocity, Coriolis Effect, Solar Activity, Solar Rotation, Sunspots, Azimuth, Magnetic Flux, Solar Magnetic Field

Scientific paper

A study is conducted of 1977's large-scale distribution of emerging sunspot-group orientations. It is noted that the tilts of axes of these new active regions is not unidirectional; in two-thirds of the cases examined the preceding part declines to the equator, while in the remaining cases the tilts are the opposite. If the theoretically predicted nonaxisymmetric global convection system is present, it is possible that the magnetic features are turned clockwise at the places of rising and expanding material, and counterclockwise in the sinking/contracting material in the Northern Hemisphere and in the opposite direction in the south, due to the Coriolis force.

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