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Fig. 2.
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Distribution of data points for the alpha temperature anisotropy in the Tα⊥/Tα∥ − Tp⊥/Tp∥ plane for (a) the slow solar wind with vsw < 500 km s−1, where the dashed line represents the strong correlation Tα⊥/Tα∥ = Tp⊥/Tp∥, and (b) the fast solar wind with vsw > 500 km s−1.
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