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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 5.

Field lines from the Green current sheet model. The vertical line represents the current sheet in the half-plane. The thick gray line illustrates the field line chosen for the basis of the simulated loop's geometry. From this figure it is easy to see why this geometry is called Y-type. The current sheet connects with the separatrix field lines, just above the gray line, to form an inverted Y.

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