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Radial Evolution of Alfvén Wave Parametric Decay Instability in the Near-Sun Solar Wind: Effects of Temperature Anisotropy
Hayato Saguchi et al 2026 The Astrophysical Journal 1005 .
Caption: Figure 5.
Maximum growth rate in MHD (black dots) and in CGL (red dots) as a function of β, evaluated for ﹩{\hat{B}}_{\perp }=0.1﹩ and ξ = 1.
© 2026. The Author(s). Published by the American Astronomical Society.
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