Image Details

Choose export citation format:

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 1.

Electron distribution f( v) (upper plots), and Langmuir wave spectral energy density W( k) (lower plots) for homogeneous (top left) and inhomogeneous plasma, with q 0 = 10 −4 k de , v 0/ v Te = 0.3 and of 3.7 × 10 −4 (top right), 3.7 × 10 −3 (bottom left), and 1.2 × 10 −2 (bottom right). Lines from dark (blue in online version) to light show the beam relaxation during the first 10 quasilinear times, while the thick line (red in online version) shows the state reached at t = 100τ ql.

Other Images in This Article
Copyright and Terms & Conditions