Kappa-Distributed Electrons in Solar Outflows: Beam-Plasma Instabilities and Radio Emissions

Electrostatic (ES) wave instabilities are assumed to be at the origin of radio emissions from interplanetary shocks, and solar coronal sources are most likely induced by electron beams, more energetic but less dense than electron strahls in the solar wind. In this paper, we present the results of a...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	Solar physics 2023-05, Vol.298 (5), p.72, Article 72
Hauptverfasser:	Lazar, M., López, R. A., Poedts, S., Shaaban, S. M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Astrophysics Astrophysics and Astroparticles Atmospheric Sciences Electron beams Electron plasma Electrons Emissions Energy levels Heliosphere Higher harmonics Instability Langmuir waves Magnetohydrodynamic stability Mathematical models Numerical simulations Physics Physics and Astronomy Plasma Plasma frequencies Plasma instabilities Radio emission Radio sources (astronomy) Solar corona Solar physics Solar wind Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Spectral analysis Spectrum analysis Stability Stability analysis Wave energy
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!