Numerical investigation of auroral cyclotron maser processes.

David C Speirs (Lead Author), Kevin Ronald, Sandra L McConville , Karen Gillespie, Alan D R Phelps , Adrian W Cross , Robert Bingham, Craig W Robertson, Colin G Whyte , Wenlong He, Irena Vorgul, Robert A Carins , Barry J Kellett

Research output: Contribution to journalArticlepeer-review

Abstract

When a mainly rectilinear electron beam is subject to significant magnetic compression, conservation of magnetic moment results in the formation of a horseshoe shaped velocity distribution. It has been shown that such a distribution is unstable to cyclotron emission and may be responsible for the generation of auroral kilometric radiation—an intense rf emission sourced at high altitudes in the terrestrial auroral magnetosphere. Particle-in-cell code simulations have been
undertaken to investigate the dynamics of the cyclotron emission process in the absence of cavity boundaries with particular consideration of the spatial growth rate, spectral output and rf conversion efficiency. Computations reveal that a well-defined cyclotron emission process occurs albeit with a low spatial growth rate compared with waveguide bounded simulations. The rf output is near
perpendicular to the electron beam with a slight backward-wave character reflected in the spectral output with a well defined peak at 2.68 GHz, just below the relativistic electron cyclotron frequency.
The corresponding rf conversion efficiency of 1.1% is comparable to waveguide bounded simulations and consistent with the predictions of kinetic theory that suggest efficient, spectrally well defined emission can be obtained from an electron horseshoe distribution in the absence of radiation boundaries.
Original languageEnglish
JournalPhysics of Plasmas
Volume17
Issue number6
Publication statusPublished - 2010
Externally publishedYes

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