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 Isotropie 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.
Original language | English (US) |
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Pages (from-to) | 823-835 |
Number of pages | 13 |
Journal | Astrophysical Journal |
Volume | 587 |
Issue number | 2 I |
DOIs | |
State | Published - Apr 20 2003 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
Keywords
- Acceleration of particles
- Radiation mechanisms: nonthermal
- Sun: flares