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Knudsen Number as a Nonthermal Parameter: Possible Origin of Skewness in Space Plasma Distributions

  • Authors: Iván Gallo-Méndez, Adolfo F. Viñas, Pablo S. Moya

Iván Gallo-Méndez et al 2026 The Astrophysical Journal 1003 .

  • Provider: AAS Journals

Caption: Figure 3.

Comparative plot of the Ψα factor, for two different values of α. The dashed curve in red is for α = 0, and the solid black line is for α = 3/2. We can observe, independent of the value of α, how the Ψα function saturates quickly for high values of κ.

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