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.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
physics.plasm-ph 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
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.