Figure 5 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 5.

Comparison of the pdf's of Δθ for MHD turbulence (in red) with Δ x/ L ∈ {4, 16, 64}/1024 and for the solar wind (in blue) with Δ t ∈ {5, 64, 830} · 9 s, consistent with the relation Δ t ~ (Δ x) ^1.85. There is generally good agreement in the pdf's for both cases.

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