Fig. 3.
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(a) Magnetic-field magnitude |B|. (b) Magnetic-field components in RTN coordinates. (c) PA distribution of Jp for 276.7 keV protons in the solar-wind frame. (d) Total differential flux of protons with PA smaller than 90°. (e) Total differential flux of protons with PA greater than 90°. (f) First-order flux anisotropy for 276.7 keV protons in the solar-wind frame. The vertical dashed gray lines indicate the times of the current-sheet boundaries and the shock.
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