Oscillating dynamo in the presence of a fossil magnetic field - The solar cycle

Details Oscillating dynamo in the presence of a fossil magnetic field - The solar cycle Oscillating dynamo in the presence of a fossil magnetic field - The solar cycle

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...254l..19l&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 254, Mar. 1, 1982, p. L19-L22.

Astronomy and Astrophysics

Astrophysics

33

Dynamo Theory, Solar Cycles, Solar Magnetic Field, Convection, Magnetohydrodynamics, Solar Rotation, Stellar Models

Scientific paper

Hydromagnetic dynamo generation of oscillating magnetic fields in the presence of an external, ambient magnetic field introduces a marked polarity asymmetry between the two halves of the magnetic cycle. The principle of oscillating dynamo interaction with external fields is developed, and a tentative application to the sun is described. In the sun a dipole moment associated with the stable fluid beneath the convection zone would produce an asymmetrical solar cycle.

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