Hostname: page-component-745bb68f8f-l4dxg Total loading time: 0 Render date: 2025-01-09T09:52:10.808Z Has data issue: false hasContentIssue false
  • English
  • Français

Fast Variations of the Solar Rotation

Published online by Cambridge University Press:  14 August 2015

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

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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