Physics – Plasma Physics
Scientific paper
Dec 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsm22a..01g&link_type=abstract
American Geophysical Union, Fall Meeting 2011, abstract #SM22A-01
Physics
Plasma Physics
[7839] Space Plasma Physics / Nonlinear Phenomena, [7867] Space Plasma Physics / Wave/Particle Interactions
Scientific paper
The nonlinear whistler mode instability associated with magnetospheric chorus and VLF triggered emissions is known to be a key driver in magnetospheric dynamics. Nevertheless, despite many years of dedicated experiments, observations, theories, and simulations, the process continues to be poorly understood. We present a review of key observations and following up on recent formulations of other authors, we give a new analytical exploration of the stability of the phenomenon. This exploration derives an additional requirement on the anisotropy of the energetic electron distribution relative to the linear treatment of the instability, and shows that the nonlinear instability is strongest when electrons become initially trapped in the wave potential. These results imply that the initiation of the nonlinear instability at the equator requires a positive frequency sweep rate, while the initiation of the instability by a constant frequency triggering wave must occur at a location upstream of the geomagnetic equator.
Gibby A. R.
Golkowski M.
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