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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Skewness parameter δ in Skew-Kappa electron distributions for solar wind scales as δ ∼ K_N, the effective Knudsen number, via a collision-modified Boltzmann equation.
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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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Knudsen number as a non-thermal parameter: possible origin of skewness in space plasma distributions
Skewness parameter δ in Skew-Kappa electron distributions for solar wind scales as δ ∼ K_N, the effective Knudsen number, via a collision-modified Boltzmann equation.