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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 2.

1D EVDFs f(vx, vy = 0) (parallel to B0) and f(vx = 0, vy) (perpendicular to B0) at Ωit = 10.56. The dot-dashed lines delineate the core Maxwellian distribution functions with and the dashed lines represent the halo distribution functions with .

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