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Interpretation of the “Third Harmonic” of the Solar Magnetic Cycle
Published online by Cambridge University Press: 19 July 2016
Abstract
The peak at ˜ 3/22 y−1 seen for all odd-degree axisymmetric modes in the SHF analysis of ‘nominal magnetic field’ seems to be an artifact of some non-linearity between the field magnitude and the sunspot occurence probability.
- Type
- IV. Photospheric Flows and Magnetic Fields
- Information
- Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 119 - 123
- Copyright
- Copyright © Kluwer 1990