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Differential Rotation and Dynamics of the Solar Interior

✍ Scribed by Thompson, M. J.; Toomre, J.; Anderson, E. R.; Antia, H. M.; Berthomieu, G.; Burtonclay, D.; Chitre, S. M.; Christensen-Dalsgaard, J.; Corbard, T.; DeRosa, M.; Genovese, C. R.; Gough, D. O.; Haber, D. A.; Harvey, J. W.; Hill, F.; Howe, R.; Korzennik, S. G.; Kosovichev, A. G.; Leibacher, J. W.; Pijpers, F. P.; Provost, J.; Rhodes, E. J.; Schou, J.; Sekii, T.; Stark, P. B.; Wilson, P. R.

Book ID
121156255
Publisher
American Association for the Advancement of Science
Year
1996
Tongue
English
Weight
856 KB
Volume
272
Category
Article
ISSN
0036-8075

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Areas of sunspots and their positions taken from the Greenwich Photoheliographic Results (1874-1976) and typical intensities of the umbrae and penumbrae are used to calculate daily values of the solar flux at a wavelength of about 500 nm. Using overlapping time series of 512 days each solar rotation