Flow Shears at the Poleward Boundary of Omega Bands Observed During Conjunctions of Swarm and THEMIS ASI

Omega bands are curved aurora forms that evolve from a quiet arc located along the poleward edge of a diffuse auroral band within the midnight to morningside auroral oval. They usually propagate eastward. Because omega bands are a significant contributor to an active magnetotail, knowledge about the...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	Geophysical research letters 2018-02, Vol.45 (3), p.1218-1227
Hauptverfasser:	Liu, Jiang, Lyons, L. R., Archer, W. E., Gallardo‐Lacourt, B., Nishimura, Y., Zou, Ying, Gabrielse, C., Weygand, J. M.
Format:	Artikel
Sprache:	eng
Schlagworte:	aurora Auroral oval Auroral streamers Auroras Convection Dynamics Earth Earth magnetosphere flow shear Fluid flow Instability Interactions ionospheric flow Kelvin‐Helmholz instability Magnetohydrodynamic stability Magnetosphere Magnetospheric dynamics Magnetotails Omega omega band Plasma Plasma instabilities Saturn Shear Shear flow Spacecraft Streamers substorm
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!