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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 12.

Apex to footpoint emission ratio for three XRT filter channels for the γ PA = −4 (red), γ PA = 0 (green), and γ PA = 4 (blue) cases with 1σ errors shown (Bevington 1969). While the ratios differ slightly in magnitude from filter to filter, the differences in the timing of the peaks provide a clear signature.

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