Image Details

Choose export citation format:

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 7.

Plot showing pitch-angle cosine distributions, f(cos θ PA), corresponding to γ PA = −4 (top), γ PA = 0 (middle), and γ PA = 4 (bottom). A value of cos θ PA of 1 (− 1) corresponds to the non-thermal particle's momentum being directed parallel (anti-parallel) to the loop axis. A pitch-angle cosine of zero corresponds to the non-thermal particle's momentum being directed perpendicular to the loop axis.

Other Images in This Article

Show More

Copyright and Terms & Conditions