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Gyrosynchrotron Emission from Anisotropic Electron Distributions

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© 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation G. D. Fleishman and V. F. Melnikov 2003 ApJ 587 823 DOI 10.1086/368252

This article is corrected by 2003 ApJ 593 598

0004-637X/587/2/823

Abstract

We present numerical calculations of the intensity, degree of polarization, and spectral index of gyrosynchrotron emission produced by fast electrons with anisotropic pitch-angle distributions. The anisotropy is found to affect the emission substantially. The emission intensity can change up to a few orders of magnitude at the optically thin region compared with the isotropic case. The local value of spectral index changes considerably with the anisotropy. X-mode polarization increases for loss cone distributions and decreases for beamlike distributions. Moreover, the sense of polarization can correspond to the ordinary wave mode at the optically thin region for a certain range of view angles for beamlike distributions. We discuss possible applications and observability of the effects obtained.

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10.1086/368252