Competing kinematic dynamo mechanisms in rotating convection with shear

Details Competing kinematic dynamo mechanisms in rotating convection with shear Competing kinematic dynamo mechanisms in rotating convection with shear

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..271..239p&link_type=abstract

Astrophysical Dynamics: From Stars to Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 271,

Astronomy and Astrophysics

Astrophysics

1

Convection, Instabilities, Magnetic Fields, Mhd, Sun: Activity, Sun: Magnetic Fields, Sun: Rotation

Scientific paper

Following earlier work by Hughes & Proctor (2009) on the role of velocity shear in convectively driven dynamos, we present preliminary results on the nature of dynamo action due to modified flows derived by filtration from the full convective flow. The results suggest that filtering the flow fields has surprisingly little effect on the dynamo growth rates.

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