On Alfvénic turbulence of solar wind streams observed by Solar Orbiter during March 2022 perihelion and their source regions

Open Access

Fig. 12.

Scatter plots of the normal components of velocity of alpha particles, $V_{N}^{α}$ $V^{\alpha}_{\mathrm{N}}$ , and magnetic field, V_AN, in Alfvén units. The Pearson correlation coefficient, CC, along with the slope of the fit, γ, represented by the solid red line, is shown in each panel. The blue dashed lines corresponds to $V_{N}^{α} = V_{AN}$ $V^{\alpha}_{\mathrm{N}} = V_{\mathrm{AN}}$ .

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