On the latitude drift of sunspot groups and solar rotation

Details On the latitude drift of sunspot groups and solar rotation On the latitude drift of sunspot groups and solar rotation

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...79..161t&link_type=abstract

Solar Physics, vol. 79, July 1982, p. 161-172.

Physics

25

Drift, Latitude, Solar Rotation, Sunspots, Angular Velocity, Maxima, Minima, Solar Physics

Scientific paper

Sunspot group N-S drift is studied by means of the positions of recurrent groups for the years 1874-1976, confirming the existence of meridional motions and the dissimilarities between drift curve shapes around sunspot maxima and minima. Angular velocity differences are also noted near the times of sunspot maxima and minima. Tabularly presented data include the numbers of synodic rotations of sunspot groups, the medians of the latitudinal motions of sunspot groups, in latitudinal zones 2 deg wide, the distribution of latitude increase between transits in degrees per synodic rotation, and the synodic angular velocity in degrees per day.

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