Investigating the nature of the link between magnetic field orientation and proton temperature in the solar wind

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Fig. 4.

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Wind at 1 AU. Frequency counts normalized to the total number of cases of the correlation coefficient between θ_BR and T_∥ (upper panel) and between θ_BR and T_⊥ (lower panel) for fast wind (black circles) and slow wind (empty circles). The time intervals used to compute the histograms are indicated in the text.

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