A New Cyclotron Radiation Mechanism in Astrophysics, Space and the Laboratory
POSTER
Abstract
From the study of the radio and X-ray emission from stars, we discovered a new radiation emission mechanism produced by energetic electrons entering a region of increasing magnetic field. This cyclotron maser process was found to be extremely efficient at converting electron energy into radio frequency emission. When a beam of electrons enters a region of increasing magnetic field strength, conservation of magnetic moment leads to the electron beam forming a crescent or horse-shoe shaped distribution in velocity space. Such a distribution is unstable and leads to the generation of cyclotron maser type radiation.
Authors
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Barry Kellett
Rutherford Appleton Laboratory
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Robert Bingham
Rutherford Appleton Laboratory, Rutherford Appleton Laboratory, UK, Rutherford Appleton Laboratory, Chilton, Didcot, United Kingdom
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Kevin Ronald
University of Strathclyde
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David C. Speirs
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Alan D.R. Phelps
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Adrian Cross
University of Strathclyde
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Irene Vorgul
St Andrews
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R.A. Cairns
University of St. Andrews, St Andrews, St. Andrews University
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C.G. Whyte
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Craig Robertson
University of Strathclyde
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J. Tonge
University of California