Cyclotron maser radiation from astrophysical shocks

R. Bingham, B.J. Kellett, R.A. Cairns, J. Tonge, J.T. Mendonça

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Abstract

One of the most popular coherent radio emission mechanisms is electron cyclotron maser instability. In this article we demonstrate that electron cyclotron maser emission is directly associated with particular types of charged particle acceleration such as turbulence and shocks commonly inferred in astrophysical plasmas.
Original languageEnglish
Pages (from-to)279-284
Number of pages5
JournalAstrophysical Journal
Volume595
Issue number1
DOIs
Publication statusPublished - 20 Sep 2003

Keywords

  • masers
  • radiation mechanisms
  • nonthermal
  • plasmas

Cite this

Bingham, R., Kellett, B. J., Cairns, R. A., Tonge, J., & Mendonça, J. T. (2003). Cyclotron maser radiation from astrophysical shocks. Astrophysical Journal, 595(1), 279-284. https://doi.org/10.1086/376724