Chaotic scattering of trapped relativistic electrons in the magnetosphere by whistler waves

• Published in: The 31st IEEE International Conference on Plasma Science, 2004. ICOPS 2004. IEEE Conference Record - Abstracts p. 425
• Main Authors: Kuo, S.P., Kossey, P., Huyhn, J.T., Kuo, S.S.
• Format: Conference Proceeding
• Language: English
• Published: IEEE 2004
• Subjects: Belts; Chaos; Charge carrier processes; Earth; Electron traps; Geomagnetism; Magnetic fields; Magnetosphere; Satellites; Scattering
• ISBN: 0780383346; 9780780383340
• ISSN: 0730-9244; 2576-7208
• DOI: 10.1109/PLASMA.2004.1340220

Summary form only given. In the magnetosphere, energetic electrons in the radiation belts are trapped by the Earth's dipole magnetic field and undergo bouncing motion about the geomagnetic equator. Those very energetic electrons (at the MeV level) have a strong impact on passing satellites. The behaviors of the trajectories of these electrons interacting with a large amplitude whistler wave are explored, with the electron energy and wave amplitude as variable parameters. A surface of section technique is used to examine chaoticity of the system graphically. Once the trajectory of an electron becomes chaotic, it can wander into the loss cone and subsequently precipitates into the ionosphere and/or the upper atmosphere. The bouncing motion of the electron is a key cause of chaotic behavior in the interaction. However, the commencement of chaotic behavior in the electron trajectories also requires the whistler wave field to exceed a threshold. The threshold wave magnetic field for the onset of chaos can be as low as 0.25% of the geomagnetic field for those energetic electrons having kinetic energies larger than 250 keV, i.e., /spl gamma//sub 0/>1.5. Waves with amplitudes at this level have been observed propagating between hemispheres. This threshold increases slightly with /spl gamma//sub 0//spl sim/3, i.e., for those MeV energetic electrons.