|
Detailed Reference Information |
Gary, S.P., Winske, D. and Hesse, M. (2000). Electron temperature anisotropy instabilities: Computer simulations. Journal of Geophysical Research 105: doi: 10.1029/1999JA000322. issn: 0148-0227. |
|
An electron temperature anisotropy T⊥e/T∥e>1 leads to excitation of three distinct modes, the whistler, the electrostatic, and the Z-mode instabilities, in collision-less plasmas at frequencies below the electron cyclotron frequency |&OHgr;e|. (Here perpendicular and parallel subscripts denote directions relative to the background magnetic field.) Two-and-one-half-dimensional particle-in-cell simulations are used to study the nonlinear consequences of the growth of these modes in homogeneous plasmas with &ohgr;e~|&OHgr;e|, where &ohgr;e is the electron plasma frequency. The simulations show that wave-particle scattering by enhanced fluctuations from the whistler and electrostatic anisotropy instabilities imposes a &bgr;-dependent upper bound on the electron temperature anisotropy at &bgr;∥e≤0.10. The simulations also demonstrate that the maximum value of the dimensionless fluctuating magnetic fields increases with &bgr;∥e and that at sufficiently low &bgr; the electrostatic instability leads to non-Maxwellian suprathermal enhancements on the reduced electron velocity distribution fe(&ngr;∥). ¿ 2000 American Geophysical Union |
|
|
|
BACKGROUND DATA FILES |
|
|
Abstract |
|
|
|
|
|
Keywords
Magnetospheric Physics, Plasma waves and instabilities, Space Plasma Physics, Numerical simulation studies, Space Plasma Physics, Wave/particle interactions, Space Plasma Physics, Waves and instabilities |
|
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 |
|
|
|