Fig. 6.
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(a–d) 0.08–0.12 Hz band-pass filtered gyrophase distributions of (a) 11.4 keV, (b) 8.2 keV, (c) 5.8 keV, and (d) 4.3 keV proton residual fluxes in the solar wind frame between 13:47:50–13:48:50 UT, derived from STEP measurements. The plus signs give the gyrophase of Bw. (e) 0.08–0.12 Hz band-pass filtered magnetic field B⊥, 1 and B⊥, 2 components in the mean (30 s) field-aligned coordinates.
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