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The same as Figure 11, for occurrence frequencies of large events, defined as exceeding the 95-perecentile of that parameter. Hence the top row shows the occurrence frequency of the 3-hourly means of the power input to the magnetosphere exceeding their 95-percentile, f[Pα > q(0.95)], the middle row shows the corresponding occurrence frequency for the am index, f[am > q(0.95)]; and the bottom row shows the corresponding occurrence frequency for [BS]GSEQ, f[BS,GSEQ > q(0.95)].
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