Figure 1 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 1.

Power spectrum of B_z component at different times of one turbulence simulation (﹩\delta {B}_{\mathrm{turb}}=\delta {v}_{\mathrm{turb}}=0.15﹩). The spectrum is normalized by the grids size. At t = 1.2, an Alfvén wave with ﹩\delta B=0.2﹩ is injected into the simulation domain.

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