Instabilities in non-thermal plasmas
Lead Research Organisation:
University of St Andrews
Department Name: Mathematics and Statistics
Abstract
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Organisations
People |
ORCID iD |
Robert Cairns (Principal Investigator) |
Publications
BINGHAM R
(2010)
Lower-hybrid waves generated by anomalous Doppler resonance in auroral plasmas
in Journal of Plasma Physics
Bingham R
(2013)
Laboratory astrophysics: Investigation of planetary and astrophysical maser emission
in Space Science Reviews
Cairns R
(2010)
Calculation of a wave field from ray tracing
in Nuclear Fusion
Cairns R
(2011)
Cyclotron maser radiation from inhomogeneous plasmas
in Physics of Plasmas
Humphrey K
(2013)
Effect of collisions on amplification of laser beams by Brillouin scattering in plasmas
in Physics of Plasmas
King M
(2014)
Progress towards numerical and experimental simulations of fusion relevant beam instabilities
in Journal of Physics: Conference Series
McConville S
(2014)
Scaled Experiment to Investigate Auroral Kilometric Radiation Mechanisms in the Presence of Background Electrons
in Journal of Physics: Conference Series
Ronald K
(2011)
Auroral magnetospheric cyclotron emission processes: numerical and experimental simulations
in Plasma Physics and Controlled Fusion
Speirs D
(2010)
Numerical investigation of auroral cyclotron maser processes
in Physics of Plasmas
Speirs D
(2014)
Numerical simulation of unconstrained cyclotron resonant maser emission
in Journal of Physics: Conference Series
Speirs D
(2010)
Publisher's Note: "Numerical investigation of auroral cyclotron maser processes" [Phys. Plasmas 17, 056501 (2010)]
in Physics of Plasmas
Vorgul I
(2011)
Cyclotron maser emission: Stars, planets, and laboratory
in Physics of Plasmas
Description | The project has looked at a variety of plasma instabilities driven by electron beams, providing theoretical support to experimental work carried out at the University of Strathclyde. Following on from earlier work on a cyclotron maser instability relevant to auroral kilometric radiation (AKR) we have investigated the effect of a background plasma on the original instability and possible competition with the two-stream instability. More detailed work on the instability has provided explanations for some of the details of AKR. We have also carried out some work on the anomalous Doppler instability, looking at the possibility of generating it using the Strathclyde apparatus. |