Stationary intensity of the fluctuating magnetic field in a nonlinear turbulent dynamo

Details Stationary intensity of the fluctuating magnetic field in a nonlinear turbulent dynamo Stationary intensity of the fluctuating magnetic field in a nonlinear turbulent dynamo

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70..381p&link_type=abstract

Astronomicheskij Zhurnal (ISSN 0004-6299), vol. 70, no. 2, p. 381-391.

Astronomy and Astrophysics

Astronomy

Celestial Bodies, Dynamo Theory, Magnetic Field Configurations, Magnetic Flux, Magnetohydrodynamic Turbulence, Mean Square Values, Astronomical Models, Nonlinear Equations, Transfer Functions

Scientific paper

The relationship between the stationary intensity of a magnetic field in
a cluster and an estimate of equidistribution is discussed. It is shown
that the nonlinear turbulent dynamo theory yields an rms of the magnetic
field in galactic clusters of about 1 microgauss and maximum values of
up to several microgauss.

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