Other
Scientific paper
Nov 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nawg.1996..247o&link_type=abstract
Nachr. Akad. Wiss. Göttingen II, Jahrg. 1996, Nr. 4, p. 247 - 253
Other
Solar Activity: Dynamo Theory, Solar Convective Zone: Solar Activity Cycles
Scientific paper
The authors study the effect of stochastic fluctuations in α using a simple axisymmetric mean field dynamo model. There are two main features: Firstly, the excitation of higher eigenmodes of the dynamo equation, providing a possible explanation of asymmetries between the two hemispheres and, close to the equator, the formation of small regions of the "wrong" polarity. Secondly, a correlation between fluctuations in phase and amplitude of the dipole field. Phase and amplitude are not locked onto one another, i.e. the dynamo has no "memory". The authors use the phase-amplitude correlation to compare the model with sunspot data, where a similar correlation is observed. This provides a rough estimate of the required strength of the α-fluctuations. It is found that α, defined as an azimuthal average, has fluctuations of the order δα/α0 ≍ 3 at mid latitudes.
Hoyng Peter
Ossendrijver J. H. A.
Schmitt Denis
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