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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. 3.

Maximum growth rate γmaxH vs. frequency ω/ΩH. For each of the three lines the electron anisotropy is constant and the proton anisotropy is varied. The uppermost line with triangles depicts ﹩T^{e}_{\parallel }/ T^{e}_{\perp }=20﹩, the middle line with diamonds ﹩T^{e}_{\parallel }/ T^{e}_{\perp }=15﹩, and the bottom line with asterisks ﹩T^{e}_{\parallel }/ T^{e}_{\perp }=14﹩. The small numbers refer to the corresponding values of ﹩T^{p}_{\parallel }/ T^{p}_{\perp }﹩. The vertical dotted line indicates the 3He+2 gyrofrequency.

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