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Interpretation of the “Third Harmonic” of the Solar Magnetic Cycle

Published online by Cambridge University Press:  19 July 2016

M.H. Gokhale  and
J. Javaraiah
M.H. Gokhale
Affiliation:
Indian Institute of Astrophysics Bangalore 560 034 India
J. Javaraiah
Affiliation:
Indian Institute of Astrophysics Bangalore 560 034 India

Abstract

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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 

References

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