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Synchrotron Radiation Spectra
Published online by Cambridge University Press: 25 April 2016
Extract
In this paper we give an account of the corrections that must be made to the formula for the emissivity ηf due to a power-law energy distribution of ultrarelativistic charged particles in a uniform magnetic field B0 in directions well away from the field lines when the effects of upper and lower cut-off values E2 and E1 in the energy distribution are not negligible.
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- Contributions
- Information
- Publications of the Astronomical Society of Australia , Volume 2 , Issue 3 , October 1972 , pp. 142 - 144
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- Copyright © Astronomical Society of Australia 1972
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