On the physical meaning of n-distributions in solar flares

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Fig. 3

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a) Moving Maxwellian distribution for T = 10⁶ K and for v₀/v_T = 1.4 (dotted line) and the Maxwellian distribution for v₀/v_T = 0 with the same energy (full line). b) Moving Maxwellian distribution for T = 10⁶ K and for v₀/v_T = 1.4 (dotted line) and the n-distribution with the same energy, for n = 3.

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