Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...253..277c&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 253, no. 1, Jan. 1992, p. 277-285. Research supported by ISRO.
Astronomy and Astrophysics
Astrophysics
65
Dynamo Theory, Magnetohydrodynamics, Solar Activity, Solar Cycles, Solar Magnetic Field, Irregularities, Mathematical Models, Nonlinear Feedback, Plasma Slabs, Stochastic Processes
Scientific paper
The solar dynamo equations are presently solved in a slab with a single mode, taking the alpha-coefficient to be constant in space, but fluctuating stochastically in time with given amplitude and correlation time. Choudhuri's (1990) contention that the solar dynamo is of the alpha-squared(omega) type is reinforced by the solar behavior's qualitative agreement with such a dynamo's level of irregularities, which increase with rising amplitude or correlation time of stochastic fluctuations.
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