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Coherent Emission Mechanisms in Astrophysical Plasmas

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arxiv 1707.02009 v1 pith:Y25H3T6Z submitted 2017-07-07 physics.plasm-ph astro-ph.HE

D. B. Melrose This is my paper · ORCID
classification physics.plasm-phastro-ph.HE
keywords emissioncoherentradioastronomicalastrophysicalcyclotronecmeelectron
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Three known examples of coherent emission in radio astronomical sources are reviewed: plasma emission, electron cyclotron maser emission (ECME) and pulsar radio emission.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona

    astro-ph.SR 2026-05 unverdicted novelty 7.0 of 10

    Imaging spectroscopy identifies repeating solar radio burst pairs whose delayed components are interpreted as turbulent echoes of harmonic emission in anisotropic coronal plasma.

  2. Electromagnetic radiation by turbulent, magnetized and randomly inhomogeneous solar radio sources generated by electron beams

    astro-ph.SR 2025-06 conditional novelty 7.0 of 10

    Most fundamental radio emission from beam-generated turbulence in Type III sources is trapped Z-mode; the small escaping fraction is mainly O-mode, with X-mode only in weakly magnetized sources.

  3. Discovery of a radio-flaring M dwarf in a commensal transient search of the LADUMA field

    astro-ph.SR 2026-07 accept novelty 6.0 of 10

    MeerKAT LADUMA monitoring reveals a radio-flaring M3.5 dwarf, LP 888-63, with 13 detections in 41 epochs at 816 MHz.

  4. Unified kinetic theory of induced scattering: Compton, Brillouin, and Raman processes in magnetized electron and positron pair plasma

    astro-ph.HE 2025-10 conditional novelty 6.0 of 10

    In strongly magnetized pair plasma, induced Compton and Brillouin scattering dominate in ordinary/neutral modes, while stimulated Raman scattering is enabled in a charged mode with growth rate (t_R)^-1 = a_e (omega0/o...

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