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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 1.

Visual representation of the staggered grid system. The energy and electron number densities, epsilon and  n e , are defined in N volumes. Other quantities, such as velocity, v, magnetic field strength, B, area, A, and parallel component of acceleration due to gravity, g, are defined on N − 1 surfaces. The first and last volumes serve as static boundary conditions for the grids and are not altered by the simulation.

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