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The Rotation Rates of Solar Magnetic Fields During

โœ Scribed by Z. Chu; J. Zhang; Q. X. Nie; T. Li


Publisher
Springer
Year
2010
Tongue
English
Weight
747 KB
Volume
264
Category
Article
ISSN
0038-0938

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A study is made of the rotation of large-scale magnetic fields using the synoptic maps from the Kitt Peak National Observatory for the time interval 1976-1985. The auto-correlation method and the mass-centers method of magnetic structures was applied to infer mean differential rotation profiles and

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We have measured solar surface rotation from sunspot drawings made in A.D. 1642-1644 and find probable differences from present-day rates. The 17th century sunspots rotated faster near the equator by 3 or 4%, and the differential rotation between 0 and :t:20 ~ latitude was enhanced by about a factor