The magnetic field in mirror-invariant turbulence

Details The magnetic field in mirror-invariant turbulence The magnetic field in mirror-invariant turbulence

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pazh....7..701r&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 7, Nov. 1981, p. 701-704.) Soviet Astronomy Letters, vol. 7, Nov.-Dec. 1981, p. 388-390

Astronomy and Astrophysics

Astrophysics

1

Conducting Fluids, Dynamo Theory, Magnetic Flux, Magnetohydrodynamic Turbulence, Stellar Magnetic Fields, Turbulent Flow, Astronomical Models, Astrophysics, Homogeneous Turbulence, Isotropic Turbulence, Planetary Magnetic Fields

Scientific paper

Exponential magnetic field growth in a mirror-symmetric (in the mean)
turbulent conducting fluid is shown to be possible. The back action of
the field on the turbulent motion is neglected. The excitation criterion
and spectrum are obtained for small wave numbers.

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