Velocity structures from sunspot statistics in cycles 10 to 22. I. Rotational velocity

Details Velocity structures from sunspot statistics in cycles 10 to 22. I. Rotational velocity Velocity structures from sunspot statistics in cycles 10 to 22. I. Rotational velocity

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...332..748p&link_type=abstract

Astronomy and Astrophysics, v.332, p.748-754 (1998)

Astronomy and Astrophysics

Astrophysics

33

Sun: Activity, Sun: Photosphere, Sun: Rotation, Sunspots

Scientific paper

Data from the whole era of modern sunspot observations (1853-1996) from four different sources is considered. We find that rotation is continuously changing, not only in the course of a cycle but also in a longer time period. We also find strong fluctuations in the equatorial rotation in the course of a sunspot cycle which can be connected with the observed north/south asymmetry of rotation. The importance of age dependence on rotation is emphasized, both for non-recurrent and recurrent sunspots as the slowing down of rotation along with the age is confirmed.

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