On the solar rotation elements as determined from sunspot observations

Details On the solar rotation elements as determined from sunspot observations On the solar rotation elements as determined from sunspot observations

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....93..241s&link_type=abstract

Astronomy and Astrophysics, vol. 93, no. 1-2, Jan. 1981, p. 241-244.

Astronomy and Astrophysics

Astrophysics

8

Solar Rotation, Sunspots, Data Reduction, Deviation

Scientific paper

The solar rotation elements Omega and i have been determined from sunspot observations in the years 1940 to 1968 given in the 'Greenwich Photoheliographic results'. The result based on 2134 groups with at least 8 observations is: Omega (1980) 75.8 plus or minus 0.27 deg, i 7.15 plus or minus 0.034 deg. The results, though not significantly different from Carrington's rotation elements, are characterized by a smaller i and a larger Omega, in agreement with other authors

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