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EGU GENERAL ASSEMBLY Oesterreich, Wien, April 2012 Theory, Simulations and Observations of Magnetic Dynamos Long-term dynamics of solar cycle, geomagnetic reversals and fluctuations of dynamo governing parameters Dmitry Sokoloff Moscow, Russia In collaboration with D.Moss, I.Usoskin, V.Pipin, G.Sobko, V.Tutubalin
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Magnetostrophic timescale
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Gassendi La Hire Dalton
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BP BT BT BP Parker Dynamo Ω Differential rotation α Mirror asymmetry
Fluctuations of governing parameters. Alpha is weak and fluctuations are stronger (up to 20%) Novelty: long-term fluctuations Suggested by Hoyng in 90th
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α-effect τ < v rot v > α = 3 E = αB
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Normal cycle
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Beginning of the Maunder minimum
Gassendi Scheiner Picard Hevelius No spots Asymmetric cycle
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Asymmetric dynamo wave
End of the Maunder Minimum Picard La Hire No dynamo wave Asymmetric dynamo wave Normal cycle
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Solar Cycle in XVIII cent.
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Grand Minima
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Geodynamo
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Basic Regimes of Parker Dynamo
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Field Reversals
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Simulated and observed timescales
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