Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.262..970n&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 262, no. 4, p. 970-992.
Astronomy and Astrophysics
Astronomy
2
Dynamo Theory, Galactic Structure, Interstellar Magnetic Fields, Magnetic Field Configurations, Eigenvalues, Plasma Dynamics, Velocity Distribution
Scientific paper
Axisymmetric MHD simulations for galactic (thin disk) alpha-squared-omega-dynamos with independent alpha-functions are performed in order to elucidate the mechanisms of the nonlinear back-reaction of large-scale dynamics to the induction equation. The amplitudes of the magnetic field and the velocity field, after exponentional growth with time, attain steady values with nonnegligible oscillations. Estimates for the steady amplitudes are given, and they are in rough agreement with the simulation results. The steady amplitude of the velocity field is proportional to the linear growth rate multiplied by the disk thickness. The steady amplitudes take various values according to the parameters of the system. Consequently, if strict equality between the magnetic energy density and the kinetic energy density of small-scale chaotic motions holds for all galactic disks, small-scale nonlinear limiting must be operating.
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