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Fig. 1.

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Overview of time series of relevant solar wind parameters observed by Solar Orbiter at a heliocentric distance ranging between 0.4 and 0.32 AU. From top to bottom: solar wind bulk speed, Vsw, in km/s; heliocentric distance, R, in AU; v − b correlation coefficient computed at 30 min scale using a running window, CVB; radial component of the magnetic field, BR, in nT (black) and magnetic field magnitude, B, in nT (blue); number density, np, in cm−3; proton temperature, Tp, in K; angle the magnetic field forms with the velocity field, ΘBV, in degree. The boxes identify the intervals investigated in this study corresponding to portions of Alfvénic slow wind (AS1, AS2, AS3) and fast wind (F).

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