Particle scattering in turbulent plasmas with amplified wave modes



: Lange S, Spanier F, Battarbee M, Vainio R, Laitinen T

Publisher: EDP SCIENCES S A

: 2013

: Astronomy and Astrophysics

: ASTRONOMY & ASTROPHYSICS

: ASTRON ASTROPHYS

: UNSP A129

: 553

: 15

: 0004-6361

DOI: https://doi.org/10.1051/0004-6361/201220804


Our calculations show a good agreement of particle simulations and the QLT for broad-band turbulent spectra; for higher turbulence levels and particle beam driven plasmas, the QLT approximation gets worse. Especially the resonance gap at mu = 0 poses a well-known problem for QLT for steep turbulence spectra, whereas test-particle computations show no problems for the particles to scatter across this region. The reason is that the sharp resonant wave-particle interactions in QLT are an oversimplification of the broader resonances in test-particle calculations, which result from nonlinear effects not included in the QLT. We emphasise the importance of these results for both numerical simulations and analytical particle transport approaches, especially the validity of the QLT.

Last updated on 2024-26-11 at 22:57