Fig. 4

Solar wind properties per solar wind type based on the Xu & Burovsky scheme (coronal hole wind (blue) and slow solar wind (green)), averaged over the respective CRs. In each panel, the median of all 4h bins of the respective solar wind type is shown, as well as the true variability of the 4h-resolution observations as indicated by the 15.9th and 84.1th percentiles. Row-wise from top left to bottom right: proton solar wind speed vp, proton temperature Tp, proton density np, magnetic field strength B, O charge state ratio nO7 +/nO6 +, C charge state ratio nC6 +/nC5 +, collisional age ac, and average Fe charge state .
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