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Parker Instability and the Galactic Dynamo

Published online by Cambridge University Press:  19 July 2016

M. Hanasz  and
H. Lesch
M. Hanasz
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, W-5300 Bonn, FRG
H. Lesch
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, W-5300 Bonn, FRG

Extract

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We imagine the interstellar medium as a system of molecular clouds and isolated magnetic flux tubes. We assume that: the flux tubes appear as a result of disruption of molecular clouds containing magnetic field, their length is comparable to the mean intercloud distance of about 100 pc and diameter comparable to the diameter of the clouds ∼ 10 pc.

Type
9. Magnetohydrodynamic Phenomena in the Interstellar Medium Related to Dynamo Processes
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993 , pp. 403 - 404
Copyright
Copyright © Kluwer 1993 

References

Ferriere, K.: 1993, This proceeding Google Scholar
Hanasz, M., Lesch, H.: Submited to Astron. Astrophys. Google Scholar
Parker, E.N.: 1967b, Ap. J. 149, 535 Google Scholar
Parker, E.N. 1979, Cosmical Magnetic Fields , Clarendon Press, Oxford.Google Scholar
Schüssler, M.: 1977, Astron. Astrophys. 56, 439 Google Scholar
Spruit, H.C.: 1981, Astron. Astrophys. 98, 155 Google Scholar