Turbulent transport of magnetic fields. IV - Damping of the mean field (B) in alpha-squared dynamos with alpha proportional to COS Theta

Details Turbulent transport of magnetic fields. IV - Damping of the mean field (B) in alpha-squared dynamos with alpha proportional to COS Theta Turbulent transport of magnetic fields. IV - Damping of the mean field (B) in alpha-squared dynamos with alpha proportional to COS Theta

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...213..429v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 213, no. 1-2, April 1989, p. 429, 430. Research supported by ASTRON and SRON.

Statistics

Computation

2

Dynamo Theory, Geomagnetism, Solar Magnetic Field, Turbulence Effects, Computational Astrophysics, Stochastic Processes

Scientific paper

It is proven that the dynamo equation for the mean field (B) of the
spherical alpha-squared dynamo with alpha proportional to cos Theta and
constant beta have only exponentially damped solutions, if the mean
energy density (B-squared) is nonzero and finite. The origin and
interpretation of this phenomenon is reviewed.

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