Exploring Turbulent Effects in Babcock-Leighton Solar Dynamo Models

Details Exploring Turbulent Effects in Babcock-Leighton Solar Dynamo Models Exploring Turbulent Effects in Babcock-Leighton Solar Dynamo Models

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..416..453g&link_type=abstract

Solar-Stellar Dynamos as Revealed by Helio- and Asteroseismology: GONG 2008/SOHO 21 ASP Conference Series, Vol. 416, proceedings

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Scientific paper

The effects of turbulent pumping and η-quenching on Babcock-Leighton dynamo models are explored separately. Turbulent pumping seems to be important for solving several reported problems in these dynamo models related to the magnetic flux transport and to the parity of the solutions. On the other hand, the suppression of the magnetic diffusivity η, could help in the formation of long-lived, small and intense structures of toroidal magnetic field.

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