Effect of meridional flow on Parker's interface dynamo

Details Effect of meridional flow on Parker's interface dynamo Effect of meridional flow on Parker's interface dynamo

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003padeu..13...37k&link_type=abstract

In: Contributions to NATO Advanced Research Workshop Turbulence, Waves, and Instabilities in the Solar Plasma; Hungary, 16-20 Se

Astronomy and Astrophysics

Astronomy

Scientific paper

Parker's interface dynamo is generalized to the case of a transversal
(i.e. meridional) flow of constant speed, limited to the high
diffusivity volume. It is found that the Parker-Yoshimura sign law is
much more difficult to violate in this case than for a homogeneous
velocity field.

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