A new cyclotron maser radiation mechanism in space plasmas

Bingham, R and Cairns, R A (2002) A new cyclotron maser radiation mechanism in space plasmas. Physica Scripta, T98. pp. 160-162. ISSN 0031-8949 (https://doi.org/10.1238/Physica.Topical.098a00160)

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Abstract

In this paper, we discuss a new cyclotron maser type instability driven by a crescent or horseshaped electron distribution function. Such distribution functions are easily created by an electron beam moving into a stronger magnetic field region, where conservation of the first adiabatic invariant causes an increase in their pitch angle. This produces a broad region on the distribution function where ∂fe/∂v⊥ > 0. Planetary dipole magnetic fields are examples of where these types of distributions can be found. We examine the stability of these electron horseshoe distribution functions for right-hand extraordinary mode (R–X mode) radiation close to the electron cyclotron frequency propagating perpendicular to the magnetic field using both non-relativistic and relativistic beams.

ORCID iDs

Bingham, R ORCID logoORCID: https://orcid.org/0000-0002-9843-7635 and Cairns, R A;
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