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Fast Variations of the Solar Rotation
Published online by Cambridge University Press: 14 August 2015
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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.
- Type
- Part 1: Basic Observed Parameters of the Solar Cycle
- Information
- Symposium - International Astronomical Union , Volume 71: Basic Mechanisms of Solar Activity , 1976 , pp. 107 - 111
- Copyright
- Copyright © Reidel 1976
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