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Density Fluctuations and the Acceleration of Electrons by Beam-generated Langmuir Waves in the Solar Corona

  • Authors: H. Ratcliffe, N. H. Bian, and E. P. Kontar

Ratcliffe, Bian, & Kontar 2012 The Astrophysical Journal 761 176.

  • Provider: AAS Journals

Caption: Figure 2.

Total energy of beam (left) and tail (middle) electrons, both normalized to the initial beam energy E 0, and the average energy of a tail electron (right), all evaluated at t = 100τ ql, against the parameter R = τ D ql, which gives a measure of the degree of inhomogeneity. Beam and plasma parameters, and ranges for and v 0 are as given in the text. The asterisks mark the three levels of inhomogeneity shown in Figure 1. The dashed lines are polynomial fits to the data to illustrate its general trends.

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