First 3-D analysis of self-correlation level contours at 10^10 cm in solar wind shows near-isotropic (spherical) magnetic and velocity correlations in slow wind, with weak perpendicular elongation in fast wind.
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3-D feature of self-correlation level contours at $10^{10}\ \mathrm{cm}$ scale in solar wind turbulence
First 3-D analysis of self-correlation level contours at 10^10 cm in solar wind shows near-isotropic (spherical) magnetic and velocity correlations in slow wind, with weak perpendicular elongation in fast wind.