Dynamo action in a thin slab

Details Dynamo action in a thin slab Dynamo action in a thin slab

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...228..909b&link_type=abstract

Astrophysical Journal, Part 1, vol. 228, Mar. 15, 1979, p. 909-918.

Physics

Astronomical Models, Dynamo Theory, Gas Flow, Plasma Slabs, Solar Atmosphere, Boundary Value Problems, Electric Fields, Electric Potential, Electrical Resistance, Field Aligned Currents, Hall Effect, Interplanetary Magnetic Fields, Magnetic Field Configurations, Solar Activity, Solar Corona, Solar Magnetic Field, Solar Physics, Steady State

Scientific paper

We consider the dynamo action produced by convection of a partially ionized, electrically conducting gas in a magnetic field. The model consists of two thin, Cartesian unipolar inductors connected in series by the magnetic field. For the case of a uniform magnetic field we compute the total current system generated by an arbitrary gas flow; for the case of a nonuniform field, we compute only the field-aligned coupling current. Application is made to the solar atmosphere.

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