The solar dynamo and the complex Lorenz equations

Details The solar dynamo and the complex Lorenz equations The solar dynamo and the complex Lorenz equations

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220...91j&link_type=abstract

In ESA The Hydromagnetics of the Sun p 91-95 (SEE N85-25091 14-92)

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3

Dynamo Theory, Lorentz Transformations, Solar Rotation, Stellar Models, Main Sequence Stars, Shear Flow, Stellar Magnetic Fields, Stochastic Processes, Time Series Analysis

Scientific paper

Nonlinear mechanisms in the dynamos associated with the Sun and other lower main sequence stars are discussed using truncated model dynamo equations. The predicted relationships between rotation rate, field strength and cycle frequency are examined. The time series derived from these model equations is compared with time series from stochastic models. The model time-variations in shear are too large to be plausible if they occur over the whole convection zone; it may be, however, that dynamo action is principally confined to a layer at the base of the convection zone, in which case the model is more plausible.

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