Fig. 6.
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Four selected time intervals during PICAM observation time windows. For each observation, panels (a) report the ion energy spectrograms by PICAM and the inverse of the IMF radial component, −BR, panels (b) the cosine of the scalar product between the PICAM boresight and the spacecraft velocity, CVSC, (c) the radial component (blue) and magnitude (black) of the magnetic field, (d) the magnetic compressibility, CB, and (e) the normalised deflection parameter, z.
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