Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Nonlinear electron acceleration by oblique whistler waves: Landau resonance vs. cyclotron resonance

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.4836595· OSTI ID:22224185
; ;  [1];  [2];  [3]
  1. LPC2E/CNRS—University of Orleans, Orleans (France)
  2. Space Research Institute, RAS, Moscow (Russian Federation)
  3. CEA, DAM, DIF, Arpajon (France)

This paper is devoted to the study of the nonlinear interaction of relativistic electrons and high amplitude strongly oblique whistler waves in the Earth's radiation belts. We consider electron trapping into Landau and fundamental cyclotron resonances in a simplified model of dipolar magnetic field. Trapping into the Landau resonance corresponds to a decrease of electron equatorial pitch-angles, while trapping into the first cyclotron resonance increases electron equatorial pitch-angles. For 100 keV electrons, the energy gained due to trapping is similar for both resonances. For electrons with smaller energy, acceleration is more effective when considering the Landau resonance. Moreover, trapping into the Landau resonance is accessible for a wider range of initial pitch-angles and initial energies in comparison with the fundamental resonance. Thus, we can conclude that for intense and strongly oblique waves propagating in the quasi-electrostatic mode, the Landau resonance is generally more important than the fundamental one.

OSTI ID:
22224185
Journal Information:
Physics of Plasmas, Journal Name: Physics of Plasmas Journal Issue: 12 Vol. 20; ISSN PHPAEN; ISSN 1070-664X
Country of Publication:
United States
Language:
English

Similar Records

Pitch angle scattering of energetic particles by oblique whistler waves
Journal Article · Mon Dec 31 23:00:00 EST 1990 · Geophysical Research Letters (American Geophysical Union); (United States) · OSTI ID:5152711

Resonant excitation of whistler waves by a helical electron beam
Journal Article · Sun Jan 24 23:00:00 EST 2016 · Geophysical Research Letters · OSTI ID:1467653