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Detailed Reference Information |
Clark, A.E. and Seyler, C.E. (1999). Electron beam formation by small-scale oblique inertial Alfvén waves. Journal of Geophysical Research 104: doi: 10.1029/1999JA900212. issn: 0148-0227. |
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Particle-in-cell simulations reveal characteristics of small-scale nearly perpendicular nonlinear inertial Alfv¿n waves in the electrostatic limit, during wave steepening and electron beam generation. These electrostatic inertial Alfv¿n waves (ESIAW) propagate with only weak electron Landau damping for Ti/Te≫1. Nonlinear amplitude initial conditions convectively steepen and evolve higher wavenumber structures similar in morphology and magnitude to previous results from a fluid-kinetic model. Shorter wavelength acoustic waves emergent during steepened ESIAW wave evolution are found to be instrumental in exciting cold electron beams possessing kinetic energies a few hundred times that of the thermal electron population. This mechanism is one possible explanation for suprathermal electron bursts observed in and near auroral inverted-V events. ¿ 1999 American Geophysical Union |
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Abstract |
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Keywords
Magnetospheric Physics, Auroral phenomena, Magnetospheric Physics, Electric fields, Ionosphere, Particle acceleration, Magnetospheric Physics, Numerical modeling, Magnetospheric Physics, Polar cap phenomena, Space Plasma Physics, Waves and instabilities |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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