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Fig. A1


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Distributions of IMF parameters for the full 22-year Hale cycle between 1996 and 2018: (a) the IMF BY component, [BY]GSEQ, the IMF clock angle in GSEQ, θGSEQ = tan−1([BY]GSEQ/[BZ]GSEQ). In (a) the bins of [BY]GSEQ are 0.2nT wide and the vertical red dash line marks [BY]GSEQ = 0; in (b) the bins of θGSEQ are 2° wide and the vertical dashed red line marks θGSEQ = 0.

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