Abstract
The rotation law of the Sun is often described by the Faye formula:
where φ is a heliographic latitude and a and b are constants. For a long time researchers have been studying the problem in what way the constants a and b change in time and in dependence on a phase of 11-year cycles.
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© 1976 IAU
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Chistyakov, V.F. (1976). Fast Variations of the Solar Rotation. In: Bumba, V., Kleczek, J. (eds) Basic Mechanisms of Solar Activity. International Astronomical Union / Union Astronomique Internationale, vol 71. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-1481-6_9
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DOI: https://doi.org/10.1007/978-94-010-1481-6_9
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-0681-2
Online ISBN: 978-94-010-1481-6
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