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The Maunder Minimum and the Solar Dynamo

✍ Scribed by D. Sokoloff

Publisher: Springer
Year: 2004
Tongue: English
Weight: 99 KB
Volume: 224
Category: Article
ISSN: 0038-0938
DOI: 10.1007/s11207-005-4176-6

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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

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