The regular magnetic field component in the galactic halo

Details The regular magnetic field component in the galactic halo The regular magnetic field component in the galactic halo

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..141m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Mar. 1980, p. 141-145.) Soviet Astronomy Letters, vol. 6, Mar.-Apr. 1980, p. 78-80.

Astronomy and Astrophysics

Astronomy

Galactic Radiation, Halos, Magnetic Fields, Milky Way Galaxy, Energetic Particles, Polarization Characteristics, Synchrotron Radiation

Scientific paper

A discussion is given of the prospects for detecting the regular magnetic field component of the galactic halo by measuring the characteristic arrival directions of ultrahigh-energy particles and the polarization of synchrotron radiation. An azimuthal halo field of constant sign, for example, would induce a north-south galactic asymmetry in the particle arrival. Particles of energy greater than 10 to the 19th eV coming from the galactic center would be deflected by the halo field, the amount of deflection depending on the particle energy.

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