Figure 3 from Three-dimensional Simulation of the Fast Solar Wind Driven by Compressible Magnetohydrodynamic Turbulence

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Three-dimensional Simulation of the Fast Solar Wind Driven by Compressible Magnetohydrodynamic Turbulence

Authors: Munehito Shoda, Takeru Ken Suzuki, Mahboubeh Asgari-Targhi, and Takaaki Yokoyama

2019 The Astrophysical Journal Letters 880 L2.

Provider: AAS Journals

Caption: Figure 3.

Second-order structure function of antisunward (﹩{\mathrm{SF}}_{2}^{+}﹩, top) and sunward (﹩{\mathrm{SF}}_{2}^{-}﹩, bottom) Elsässer variables measured in the vicinity of r/R_⊙ = 10. Embedded white lines represent the contour lines.

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