Figure 1 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 1.

pdf of rotations in the magnetic field direction, P(Δθ), for the solar wind with measurement intervals of Δ t ∈ {1, 16, 256, 4096} · 3 s (measured by the WIND spacecraft). While part of the tail (Δθ > 60°) may be fit by an exponential function (straight line in the plot), the bulk of the pdf (Δθ < 60°) varies drastically with Δ t.

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