Old tail lobes effect on the solar-wind – Magnetosphere energy transport for the 27 August 2001 substorm

The magnetic flux of tail lobes Ψ is divided in two parts of comparable values Ψ1 and Ψ02, with the first that appears during substorm and the second, observed before substorm start. The first was named “new magnetic flux”, the second – “old magnetic flux”. The first, Ψ1, is known to play a definiti...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Advances in space research 2014-12, Vol.54 (12), p.2540-2548
Hauptverfasser:	Mishin, V.V., Mishin, V.M., Pu, Z., Lunyushkin, S.B., Sapronova, L.A., Sukhbaatar, U., Baishev, D.G.
Format:	Artikel
Sprache:	eng
Schlagworte:	Energy consumption Energy flux Energy use Lobes Magnetic flux Magnetospheres Magnetospheric convection Mathematical analysis Polar cap Polycarbonates Solar wind Tail lobes Transport
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!