Solar Physics

, Volume 196, Issue 2, pp 421–426

On the Differences Between Odd and Even Solar Cycles

  • Bernard R. Durney
Article

DOI: 10.1023/A:1005285315323

Cite this article as:
Durney, B.R. Solar Physics (2000) 196: 421. doi:10.1023/A:1005285315323

Abstract

It is proposed that the observed differences between odd and even solar cycles are a consequence of the nonlinear interactions that provide the stabilizing mechanism for the cycle's amplitude. If, for example, the magnetic field is larger than average for a given cycle (say odd), the nonlinear feedback mechanism can generate a magnetic field that is smaller than average for the next cycle (even), and then one that is larger than average for the following cycle (odd), etc. As a consequence the odd cycles have larger amplitudes than even cycles. A very simply model having a nonlinear interaction that reproduces this behavior is discussed.

Copyright information

© Kluwer Academic Publishers 2000

Authors and Affiliations

  • Bernard R. Durney

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