The Multi-Species Farley-Buneman Instability in the Solar Chromosphere

Empirical models of the solar chromosphere show intense electron heating immediately above its temperature minimum. Mechanisms such as resistive dissipation and shock waves appear insufficient to account for the persistence and uniformity of this heating as inferred from both UV lines and continuum...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	arXiv.org 2014-03
Hauptverfasser:	Madsen, Chad A, Dimant, Yakov S, Oppenheim, Meers M, Fontenla, Juan M
Format:	Artikel
Sprache:	eng
Schlagworte:	Chromosphere Computational fluid dynamics Earth ionosphere Electric fields Electron drift velocity Electrons Empirical analysis Energy dissipation Heating Mathematical models Photosphere Physics - Solar and Stellar Astrophysics Shock waves Stability Thermal energy Turbulent flow
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!