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Distribution of response lags for the 288 F–UT bins studied for the response of the am index to the power input to the magnetosphere Pα/Po for 1995–2017, inclusive. (Top) The red line shows the distribution of the lags giving peak correlation dtp between Pα/Po and am for all the data. (Bottom) The same analysis but the am data have been further subdivided into the 8 other quantile ranges used in Figure 8. The distributions are taken in 1-min ranges and then smoothed with a 10-min running mean.
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