On the physical meaning of n-distributions in solar flares

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Fig. 6

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Moving Maxwellian distributions showing a change of their derivatives in the interval in 1–4 keV. The full line means the distribution for the temperature T = 4 × 10⁶ K and v₀/v_T = 0, dotted line for T = 2 × 10⁶ K and v₀/v_T = 1.4, dashed line for T = 10⁶ K and v₀/v_T = 3, and dash-dotted line for T = 0.5 × 10⁶ K and v₀/v_T = 5.

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