Paper
14 July 2000 New method for ultrahigh-frequency cyclotron maser at low magnetic field
John A. Davies, Chiping Chen
Author Affiliations +
Abstract
A new method of electron cyclotron emission is reported in which electrons emit stimulated radiation at frequencies that are greater than the usual Doppler-shifted electron cyclotron frequency by orders of magnitude. In particular, stability properties are analyzed of a relativistic electron beam gyrating in a uniform magnetic field with a strong spatiotemporal correlation in electron gyrophases. Both field amplitude equations and dispersion relations have been obtained for small-amplitude electromagnetic and electrostatic waves on a spatiotemporally gyrating relativistic electron beam. Detailed properties of such a system are studied numerically. It is shown that, if the phase velocity of the gyration pattern is close to the axial velocity, then stimulated radiation emission occurs at a frequency that is must greater than the Doppler-shifted electron frequency in both relativistic and mildly relativistic regimes. Numerical examples are presented for cyclotron maser interactions at 35 GHz and 94 GHz for electron beam voltages ranging from 100 kV to 500 kV confined by an axial magnetic field less than 6 kG.15
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
John A. Davies and Chiping Chen "New method for ultrahigh-frequency cyclotron maser at low magnetic field", Proc. SPIE 4031, Intense Microwave Pulses VII, (14 July 2000); https://doi.org/10.1117/12.391811
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KEYWORDS
Phase velocity

Magnetism

Electron beams

Dispersion

Doppler effect

Electromagnetic radiation

Electromagnetism

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