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Acceleration and Enrichment of 3He in Impulsive Solar Flares by Electron Firehose Waves

  • Authors: G. Paesold, R. Kallenbach, and A. O. Benz

Paesold, Kallenbach, & Benz 2003 The Astrophysical Journal 582 495.

  • Provider: AAS Journals

Caption: Fig. 1.

Dispersion relation of EF waves calculated from linear theory. The frequency ωr (solid curve) and growth rate γ (dashed curve) of the EF waves are shown normalized to the proton gyrofrequency as a function of parallel wavenumber k normalized to the inertial length of the protons. The plasma parameters are ﹩T^{e}_{\parallel }/ T^{e}_{\perp }=15﹩, ﹩T^{p}_{\parallel }/ T^{p}_{\perp }=2﹩, ﹩T^{e}_{\perp }=T^{p}_{\perp }=1\times 10^{7}﹩ K, ﹩n_{e}=n_{p}=5\times 10^{10}﹩ cm−3, and ﹩B_{0}=100﹩ G. The sign convention is that ﹩k> 0﹩ and ﹩\omega > 0﹩ mean left‐hand circularly polarized; ﹩\gamma > 0﹩ refers to growing modes. The dotted horizontal lines indicate the gyrofrequency of the corresponding ion species.

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