Fig. A.2.
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In situ observation of the ICME resulting from the 2013 April 11 solar event. Shown from top to bottom are magnetic field magnitude B, field inclination angle θ, azimuthal angle ϕ (0 deg pointing to the Sun), and three components (Vx, Vy, Vz) of the solar wind velocity in the GSE coordinate system. The closest approach d = 0.60, and the goodness of fit χn = 0.18.
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