Measured non-Maxwellian velocity distribution functions in the solar wind lower ion-acoustic wave damping rates and can trigger instability where bi-Maxwellian approximations predict strong damping.
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A new MHD model of transonic sub-Alfvenic turbulence shows it remains nearly-incompressible with 2D+slab geometry when sub-Alfvenic, consistent with simulations and extending NI theories for solar wind and space plasmas.
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The Damping and Instability of Ion-acoustic Waves in the Solar Wind: Solar Orbiter Observations
Measured non-Maxwellian velocity distribution functions in the solar wind lower ion-acoustic wave damping rates and can trigger instability where bi-Maxwellian approximations predict strong damping.
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Nature of Transonic Sub-Alfv\'enic Turbulence and Density Fluctuations in the Near-Sun Solar Wind: Insights from Magnetohydrodynamic Simulations and Nearly-Incompressible Models
A new MHD model of transonic sub-Alfvenic turbulence shows it remains nearly-incompressible with 2D+slab geometry when sub-Alfvenic, consistent with simulations and extending NI theories for solar wind and space plasmas.