Random Magnetic Fields in Galactic Wind Flow

Details Random Magnetic Fields in Galactic Wind Flow Random Magnetic Fields in Galactic Wind Flow

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....5.1827z&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

The transport of random magnetic fields by a galactic wind driven by cosmic rays is considered. Magnetic field disturbances are advected by the gas flow from the upper part of the galactic disk to the halo. The magnetic field inhomogeneities become very elongated due to the flow acceleration. Applications for cosmic ray transport in the galactic wind are considered.

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