Non-thermal electron velocity distribution functions due to 3D kinetic magnetic reconnection for solar coronal plasma conditions

Magnetic reconnection can convert magnetic energy into kinetic energy of non-thermal electron beams. Those accelerated electrons can, in turn, cause radio emission in astrophysical plasma environments, such as solar flares via micro-instabilities. The properties of the electron velocity distribution...

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Veröffentlicht in:	Physics of plasmas 2022-02, Vol.29 (2)
Hauptverfasser:	Yao, Xin, Muñoz, Patricio A., Büchner, Jörg
Format:	Artikel
Sprache:	eng
Schlagworte:	Algorithms Diffusion Distribution functions Electron beams Electron velocity distribution Field strength Free energy Kinetic energy Machine learning Magnetic fields Particle in cell technique Plasma physics Radio emission Solar corona Solar flares Velocity
Online-Zugang:	Volltext
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