The internal magnetic field of the sun and peculiarities of the solar activity cycles

Details The internal magnetic field of the sun and peculiarities of the solar activity cycles The internal magnetic field of the sun and peculiarities of the solar activity cycles

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...95..381p&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 95, Feb. 1985, p. 381-390.

Physics

5

Solar Activity, Solar Cycles, Solar Interior, Solar Magnetic Field, Solar Rotation, Astronomical Models, Fourier Series

Scientific paper

Leighton's model (1969) of a solar cycle with a hypothetical quasi-stationary internal magnetic field of the sun taken into account, is used to explain the long-term variations of solar activity, including prolonged periods of abnormally low and/or high activity. The model is modified in such a way as to agree with the experimental data. It is shown that there exists a close relation between the values of the radial component of the solar magnetic field and the values of the toroidal magnetic field intensity in the course of an 11-yr cycle, thus making it possible to predict the value of the toroidal field intensity (and, hence, the level of solar activity) 2-3 years ahead.

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