Figure 3 from The Parametric Decay Instability of Alfvén Waves in Turbulent Plasmas and the Applications in the Solar Wind

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The Parametric Decay Instability of Alfvén Waves in Turbulent Plasmas and the Applications in the Solar Wind

Authors: Mijie Shi, Hui Li, Chijie Xiao, and Xiaogang Wang

2017 The Astrophysical Journal 842 63.

Provider: AAS Journals

Caption: Figure 3.

Evolution of density distribution in the ﹩\{x,y\}﹩ plane (﹩z=\pi ﹩) for a turbulence case with ﹩\delta B=0.2﹩ at (a) t = 0.08, (b) t = 1.15, (c) t = 2.39, and (d) t = 3.98. An Alfvén wave is injected at t = 1.2.

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