New results on the mechanism of magnetic flux pumping by three-dimensional convection

Details New results on the mechanism of magnetic flux pumping by three-dimensional convection New results on the mechanism of magnetic flux pumping by three-dimensional convection

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.201p..57a&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 201, Dec. 1982, p. 57P-61P.

Astronomy and Astrophysics

Astronomy

17

Convection, Magnetic Pumping, Solar Magnetic Field, Stellar Magnetic Fields, Dynamo Theory, High Reynolds Number, Magnetic Flux

Scientific paper

New calculations indicate that the Drobyshevsky and Yuferev (1974) mechanism for the pumping of magnetic flux at the base of a stellar convection zone is radically altered in the case of high magnetic Reynolds number. As a result, the process is not likely to be operating in the sun in the form originally described, although the present, revised mechanism may be more effective in maintaining magnetic fields at the bottom of the convecting layer.

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