On the parametric resonance in a thin disk galactic dynamo

Details On the parametric resonance in a thin disk galactic dynamo On the parametric resonance in a thin disk galactic dynamo

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992an....313..349k&link_type=abstract

Astronomische Nachrichten (ISSN 0004-6337), vol. 313, no. 6, p. 349-352.

Astronomy and Astrophysics

Astronomy

1

Dynamo Theory, Galactic Structure, Interstellar Magnetic Fields, Orbital Resonances (Celestial Mechanics), Astronomical Models, Magnetohydrodynamic Turbulence

Scientific paper

The absence of a parametric resonance due to the generation of a
large-scale bisymmetric magnetic field in the frame of the simplest thin
disk galactic dynamo model is shown. The resonance can be generated only
by taking more complicated phenomena into account.

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