Picture of a black hole

Strathclyde Open Access research that creates ripples...

The Strathprints institutional repository is a digital archive of University of Strathclyde's Open Access research outputs. Strathprints provides access to thousands of research papers by University of Strathclyde researchers, including by Strathclyde physicists involved in observing gravitational waves and black hole mergers as part of the Laser Interferometer Gravitational-Wave Observatory (LIGO) - but also other internationally significant research from the Department of Physics. Discover why Strathclyde's physics research is making ripples...

Strathprints also exposes world leading research from the Faculties of Science, Engineering, Humanities & Social Sciences, and from the Strathclyde Business School.

Discover more...

Pulse propagation effects in a cyclotron resonance maser amplifier

Aitken, P and McNeil, B W J and Robb, G R M and Phelps, A D R (1999) Pulse propagation effects in a cyclotron resonance maser amplifier. Physical Review E: Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics, 59 (1). pp. 1152-1166. ISSN 1063-651X

Full text not available in this repository. (Request a copy from the Strathclyde author)

Abstract

An analysis is presented of a cyclotron resonance maser amplifier operating with electron pulses. The electrons are resonant at two frequencies of the same waveguide mode. We consider both a single resonant frequency interaction and also a coupled two resonant frequency interaction. It is shown that, in general, the interaction with both resonant frequencies must be taken into account. The analysis includes propagation effects due to the difference between the axial velocity of the electrons and the group velocities of the radiation fields. Both linear and numerical solutions to the equations are given, and superradiant emission is demonstrated where the radiated power scales as the square of the electron pulse current. Two methods of low-frequency suppression are presented allowing the high-frequency emission to dominate. These results may have important consequences for the generation of short pulses of high-frequency, high-power microwave radiation. [S1063-651X(99)01001-6].