Solar rotation rate from stable sunspot tracings

Details Solar rotation rate from stable sunspot tracings Solar rotation rate from stable sunspot tracings

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.153..345o&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 153, no. 2, March 1989, p. 345-349.

Astronomy and Astrophysics

Astrophysics

Angular Velocity, Solar Rotation, Sunspots, Least Squares Method, Long Term Effects, Northern Hemisphere, Position (Location), Southern Hemisphere

Scientific paper

Positions of sunspots between 1966 and 1976 as observed at Kandilli Observatory were used to determine the differential rotation of the sun. A total of 202 sunspot groups which were E, F, G, H, and J-types were chosen, and a least-squares solution was calculated with their daily rotations. A gradient difference was found between the two hemispheres of the sun.

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