Global resonances in the evolution of solar magnetic fields

Details Global resonances in the evolution of solar magnetic fields Global resonances in the evolution of solar magnetic fields

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986natur.319..285s&link_type=abstract

Nature (ISSN 0028-0836), vol. 319, Jan. 23, 1986, p. 285-290.

Other

75

Resonance, Solar Magnetic Field, Power Spectra, Solar Activity, Spherical Harmonics

Scientific paper

Decomposition of the pattern of solar magnetic fields in spherical harmonics for a data set of 25 years and power spectrum analysis of the harmonic coefficients reveals a strikingly resonant modal structure. The resonances for the modes of odd and even parity are decoupled from each other, indicating an underlying selection rule. This new 'emission line' spectrum of solar magnetic fields does not seem to be explicable within the framework of current concepts such as dynamo theory, but should contain potentially powerful diagnostic information on the interior magnetic structure of the sun and on the origins of solar activity.

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