Magnetic fields in our Galaxy: How much do we know?

Abstract

The large scale magnetic fields of our Galaxy have been mostly revealed by rotation measures ($RM$s) of pulsars and extragalactic radio sources. In the disk of our Galaxy, the average field strength over a few kpc scale is about 1.8 $\mu$G, while the total field, including the random fields on smaller scales, has a strength of about 5 $\mu$G. The local regular field, if it is part of the large scale field of a bisymmetric form, has a pitch angle of about $-8\degr$. There are at least three, and perhaps five, field reversals from the Norma arm to the outer skirt of our Galaxy.

4 pages. To appear in proceedings of IAU Collo.182, a special issue Astrophysics & Space Science

References in corpus (1)

• Pulsar rotation measures and the magnetic structure of our Galaxy

Cited by in corpus (15)

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