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Simulating the Effects of Initial Pitch-angle Distributions on Solar Flares

  • Authors: Henry D. Winter, Petrus Martens, and Katharine K. Reeves

Winter, Martens, & Reeves 2011 The Astrophysical Journal 735 103.

  • Provider: AAS Journals

Caption: Figure 6.

Plot of the number of non-thermal particles as a function of energy. The energy distribution follows the power law F( E) = F 0 E −δ with the electron spectral index, δ, set equal to 3 and a low energy cutoff of 15 keV. Each run consists of 2 × 10 4 test particles. Each simulation is made from 50 runs yielding 1 × 10 6 test particles in total.

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