Cross helicity in stellar magnetoconvection

Details Cross helicity in stellar magnetoconvection Cross helicity in stellar magnetoconvection

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..274..143k&link_type=abstract

Advances in Plasma Astrophysics, Proceedings of the International Astronomical Union, IAU Symposium, Volume 274, p. 143-145

Astronomy and Astrophysics

Astrophysics

Convection, Sun: Activity, Stars: Activity

Scientific paper

Magnetic diffusion is a key ingredient in mean-field dynamo models but neither observations nor theory are able to produce reliable values. Numerical simulations provide an alternative way to determine the turbulent electromotive force. Cross helicity allows us to determine the turbulent magnetic diffusion coefficient in simulations of stellar magnetoconvection.

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