Fig. 14
Time series of minimal temperature profiles with adaptive bin size for the first recurring coronal hole wind stream in CR 2045 and in the same format as in Fig. 13. Top left: O and C ion pairs, top right: Mg ion pairs, bottom left: Si ion pairs, and bottom right: Fe ion pairs. All panels refer to a κ-function with κ = 10 as the electron velocity distribution function.
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