In the young solar wind below 0.3 au, slab fluctuations dominate over 2D fluctuations, with the 2D fraction only 26% in coronal-hole wind and 45% in streamer wind.
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Inertial-range Turbulence Anisotropy of the Young Solar Wind from Different Source Regions
In the young solar wind below 0.3 au, slab fluctuations dominate over 2D fluctuations, with the 2D fraction only 26% in coronal-hole wind and 45% in streamer wind.