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Fig. 6


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Cumulative probability distributions (c.d.f.s) of the power input to the magnetosphere, Pα, as a ratio of its mean value Po = <Pα>all for the full interval of near-continuous interplanetary data (1995–2017, inclusive). The Pα/Po data are divided into 288 bins: 36 equal-sized bins in fraction of year F and the same eight 3-h Universal Time (UT) bins over which the range am index is evaluated. For each FUT bin the c.d.f. of Pα/Po as a ratio of the mean value for that bin <Pα/Po>F,UT was plotted and colored according to the value of that ratio. The black line is for all Pα/Po data, the orange line for the FUT bin giving the largest <Pα/Po>F,UT and the green line for the FUT bin giving the smallest <Pα/Po>F,UT.

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