Figure 4 from Distribution of Magnetic Discontinuities in the Solar Wind and in Magnetohydrodynamic Turbulence

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Distribution of Magnetic Discontinuities in the Solar Wind and in Magnetohydrodynamic Turbulence

Authors: Vladimir Zhdankin, Stanislav Boldyrev, and Joanne Mason

Zhdankin, Boldyrev, & Mason 2012 The Astrophysical Journal Letters 760 L22.

Provider: AAS Journals

Caption: Figure 4.

Comparison of the pdf for rotations measured in the solar wind (in blue) and the pdf derived from lognormal P(Δ B/ B) with the assumption that vectors undergo pure rotations (in red). The separations shown are Δ t ∈ {1, 16, 256, 4096} · 3 s.

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