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Electron cyclotron maser instability by evolving fast electron beams in the flare loops

The electron cyclotron maser instability (ECMI) stands as a pivotal coherent radio emission mechanism widely implicated in various astrophysical phenomena. In the context of solar activity, ECMI is primarily instigated by energetic electrons generated during solar eruptions, notably flares. These el...

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Hoofdauteurs: J. F. Tang, D. J. Wu, L. Chen, C. M. Tan, J. B. Wang
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: Frontiers Media S.A. 2024-05-01
Reeks:Frontiers in Astronomy and Space Sciences
Onderwerpen:
electron cyclotron maser instability
energetic electrons
radio radiation
evolution
flare loop
Online toegang:https://www.frontiersin.org/articles/10.3389/fspas.2024.1404145/full
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