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Fig. 7

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Parts a, b, e, f, i and j are plots of probability distribution functions of (Pα/Po) as a function of F and beneath each (parts c, d, g, h, k and l) is the corresponding plot of the normalized am amplification factor, [am/Pα]n = (am/〈amall)/(Pα/Po), as a function of F and in the same (Pα/Po) bins as the p.d.f.s. The left hand panels are for IMF [BY]GSEQ < 0, the right hand panels are for IMF [BY]GSEQ > 0. The plots are in 3 groups of 4: parts a-d are for the lower tercile of the simultaneous (allowing for the propagation lag) solar wind dynamic pressure, pSW < q(0.33); parts e-h are for the middle tercile of the simultaneous solar wind dynamic pressure, q(0.33 ≤ pSW < q(0.67); parts i-l are for the upper tercile of the simultaneous solar wind dynamic pressure, pSW ≥ q(0.67), where q(x) is the xth quantile of the overall distribution of pSW values.

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