Super Dual Auroral Radar Network observations of near‐noon plasma convection at small interplanetary magnetic field B z and B y

Routine Super Dual Auroral Radar Network ionospheric plasma convection maps are used to study the structure of the near‐noon convection established at small interplanetary magnetic field (IMF) B z and B y . During such intervals, the influence upon convection of the quasi‐viscous processes at the ma...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Journal of Geophysical Research: Space Physics 1998-03, Vol.103 (A3), p.4041-4050
Hauptverfasser:	Kustov, A. V., Lyatsky, W. B., Sofko, G. J.
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!