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A&A 416, 411-422 (2004)
DOI: 10.1051/0004-6361:20031713
Galactic magnetic field generation by the electric current of cosmic rays
A. Z. Dolginov1 and I. N. Toptygin21 125, B-2, Hillcrest Vil.E., Schenectady, NY, 12309, USA
2 St. Petersburg State Polytechnical University 195251, St. Petersburg, Russia
(Received 4 March 2003 / Accepted 20 November 2003)
Abstract
In this paper we propose a new mechanism for the
generation of a large-scale galactic magnetic field by the
electric current created by cosmic rays. A model with the sources
of relativistic particles, distributed homogenously and continuously in the galactic disk
is used, and intensities of the sources correspond to the observed
intensities. The anisotropic diffusion of cosmic rays in the
galaxy is considered and it is shown that the created magnetic
field depends strongly on the symmetry of the diffusion tensor as
well as on the relationship between the tensor's components. The
helicity of turbulence (
-effect) is not considered. Only
the small-scale "seed" fields ejected from stars and generated by
cosmic rays are necessary to start the global magnetic field
generation. The diffusion of the field because of turbulent
motions and the differential rotation of the galactic disk are
taken into account. The diffusion coefficient values estimated
from the observed parameters of the galactic medium are used in
the calculations. The obtained magnetic field is approximately a
few micro-gauss which is of the same order of magnitude as the
observed galactic field. Therefore, it is concluded that the
relativistic particles are significant and, possibly, essential
for the process of the large-scale galactic magnetic field
generation. More precise determinations of the diffusion
coefficients for the field and the particles are needed to reach
the final conclusion about the field's value. The future
development of the theory should also include dynamo action, the
nonlinear effects, and the self-consistent approach to the
problem.
Key words: ISM: cosmic rays -- diffusion -- Galaxy: kinematics and dynamics -- ISM: magnetic field
Offprint request: A. Z. Dolginov, adolgi1@yahoo.com
© ESO 2004
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