Figure 1 from The Origin of Non-Maxwellian Solar Wind Electron Velocity Distribution Function: Connection to Nanoflares in the Solar Corona

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The Origin of Non-Maxwellian Solar Wind Electron Velocity Distribution Function: Connection to Nanoflares in the Solar Corona

Authors: H. Che and M. L. Goldstein

Che & Goldstein 2014 The Astrophysical Journal Letters 795 L38.

Provider: AAS Journals

Caption: Figure 1.

EVDFs f(v_x) = ∫f(v_x, v_y)dv_y (a) and f(v_y) = ∫f(v_x, v_y)dv_x (b) at Ω_it = 0 (black solid line), 0.32, two-stream instability nearly saturates and slowly decay (green dashed), 0.64, the Weibel instability is near the peak (red dash-dotted), and 10.56, turbulence is in full saturation (blue dot-dashed).

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