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We selected the maximum Kp value, for example on the day of anomaly, for each anomaly case in Table 4.
In general, the correlation trend was consistent for each anomaly case, where R for E1 was larger than that for E2 and E3.
However, the overall trend for each anomaly case showed that lower-energy electrons (>30 keV, channel E1) had a good correlation with Kp and Dst values, as shown in Fig. 3.
Here we present a contractile morning glory disc anomaly case with a video recording of the contractions.
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Weak linkage was also found in GEO anomaly cases studied by Gubby and Evans (2002).
The rates of CP for the same four anomaly cases are shown in Table 2.
The LEO satellite anomaly cases used in this paper are listed in Table 4.
For example, we obtained only five anomaly cases for equatorial satellites, whereas the remaining cases involved polar satellites.
Variation of electron fluxes and Kp and Dst indices within selected intervals for other anomaly cases given in Table 4.
The former study used only a small number of LEO anomaly cases, whereas the latter study applied Kosmos data on anomalies attributed to high-energy particles.
This was also found in some anomaly cases studied by Farthing et al. (1982), Lam and Hruska (1991), and Iucci et al. (2006 ). 2.
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