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Fast Variations of the Solar Rotation

Published online by Cambridge University Press:  14 August 2015

V. F. Chistyakov*
Affiliation:
Service of Sun, Ussurijsk, U.S.S.R.

Extract

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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.

Information

Type
Part 1: Basic Observed Parameters of the Solar Cycle
Copyright
Copyright © Reidel 1976