Fig. A.2.
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Magnetic field fluctuations in the solar wind. (A) Zoom into Fig. 1C, showing the time profile of the radial magnetic field in the fast wind streams over a 1 hour interval. (B) Fluctuations in the corresponding magnetic field vector normalized to its magnitude. (C) and (D) are the same as panels (A) and (B) but plotted for the case of the Alfvénic slow wind streams (Fig. 3C).
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