Figure 5 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 5.

Growth rate comparison of PDI modes for turbulence simulations (⋆) (﹩\delta {B}_{\mathrm{turb}}=\delta {v}_{\mathrm{turb}}=0.05﹩), non-turbulence simulations (+), and theoretical predictions (o) from Equation (5), with different amplitudes of circularly polarized Alfvén waves. The plasma ﹩\beta =0.5﹩.

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