Quantitative magnetotail characteristics of different magnetospheric states

Quantitative relationships allowing one to compute the lobe magnetic field, flaring angle and tail radius, and to evaluate magnetic flux based on solar wind/IMF parameters and spacecraft position are obtained for the middle magnetotail, <i>X</i>=(–15,–35)<i>R<sub>E</sub>...

Full description

Bibliographic Details
Main Authors: M. A. Shukhtina, N. P. Dmitrieva, V. A. Sergeev
Format: Article
Language:English
Published: Copernicus Publications 2004-03-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/22/1019/2004/angeo-22-1019-2004.pdf