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>...
Main Authors: | , , |
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Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2004-03-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/22/1019/2004/angeo-22-1019-2004.pdf |