Fig. 4.

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Plasma properties around the short excursion of the magnetic field from the sunward (BR < 0) to the antisunward. From top to bottom: magnetic field, protons bulk velocity, protons density with the magnetic field magnitude, and proton velocity distribution functions (VDF) in the plane containing vectors V and B. The horizontal axis VX in the VDF panels is an axis in the {V, B} plane maximally parallel to the spacecraft X axis. The vertical axis VP is perpendicular to VX in the plane. The horizontal bars in the panel of proton’s number density show the time intervals of antiparallel strahl electrons in green and the intervals of the positive Vαp (VHe + + > VH+) in red. The gray part of the strahl bar shows the bi-directional PAD. The blue bar shows the negative Vαp (VHe++ ≤ VH+).
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