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Magnetotail response during a strong substorm as observed by GEOTAIL in the distant tail

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Fig. 1. Magnetic ®eld and plasma beta variations observed along several di€erent trajectories relative to an idealised plasmoid (from Slavin et al
Table 1 presents an overview of the channel character- character-istics.
Fig. 2. The time plot of the magnetic ®eld and energetic particle conditions for October 10, 1993 between 0030 UT and 0130 UT are presented
Fig. 4. a The AE indices for October 9 and 10, 1993; b di€erential electron ¯uxes as measured at geostationary orbit by LANL  1990-095 spacecraft, from ®ve channels with energy ranges 50±75 keV, 75±105 keV, 105±150 keV, 150±225 keV, 225±315 keV, plotted re
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