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Synchrotron Radiation in Directions Close to Magnetic-Field Lines

Published online by Cambridge University Press:  25 May 2016

K. C. Westfold
K. C. Westfold*
Affiliation:
Monash University, Australia

Abstract

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(Astrophys. Space Sci.). It is characteristic of the radiation from a particle of mass m bearing a charge e moving with ultrarelativistic velocity βc in a magnetic field of induction B0 that the bulk of the emission is confined to a small cone of directions within O(ξ) of the direction of motion τ which makes a constant angle α with B0, and that for any direction n at an angle θ with B0 such emission is observed as harmonics of the fundamental frequency fB0ξ/a, where fB0 is the nonrelativistic cyclotron frequency and

Type
Part II The Flash Phase of Solar Flares
Information
Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 295 - 297
Copyright
Copyright © Reidel 1974