Physics
Scientific paper
Dec 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...64..247g&link_type=abstract
Solar Physics, vol. 64, Dec. 1979, p. 247-254.
Physics
32
Solar Rotation, Sunspot Cycle, Diurnal Variations, Latitude, Solar Atmosphere, Solar Magnetic Field
Scientific paper
The paper presents an analysis of Greenwich sunspot data for cycle No. 18 which shows: (1) higher rotation rates for the southern sunspot belt than for the northern belt, (2) lower rotation rates and a tendency to a more rigid rotation for greater sunspot groups, (3) lower rotation rates and a tendency to a more rigid rotation for older sunspot groups, (4) no dependence of rotation rates on the lifetime of sunspot groups, (5) a tendency to a more rigid rotation at the activity minimum. It is noted that results Nos. 2, 3, and 5 could be interpreted in terms of the evolution and interplay of the active regions, as the regions age. Finally, if it is assumed that the sunspot group life-time is a function of their depth in the solar atmosphere, result No. 4 shows that the rotation rates do not depend on the depth.
Godoli Giovanni
Mazzucconi Fabrizio
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