Laboratory experiment on the excitation of whistler-mode chorus waves

ORAL

Abstract

Whistler-mode chorus waves play an important role in accelerating electrons to relativistic energies in the heart of the outer radiation belt, as well as in precipitating electrons to the atmosphere. An experiment in the Large Plasma Device at UCLA generates both broadband and discrete chirping whistler-mode emissions using a gyrating electron beam injected into a cold background plasma. The mode structure of these emissions is identified using a phase-correlation technique. The emission forms of the whistler waves depend on plasma density, beam density and magnetic field profiles. A kinetic simulation in accordance with the experiment shows an initial relaxation of the electron beam by Langmuir waves and subsequently growing whistler waves through cyclotron resonance and Landau resonance.

*The research was funded by the Department of Energy and the National Science Foundation by grant DE-SC0010578 and was also funded by NASA grant NNX16AG21G.

Authors

  • Xin An

    • University of California, Los Angeles
  • Bart Van Compernolle

    • University of California, Los Angeles
  • Jacob Bortnik

    • University of California, Los Angeles
  • Viktor Decyk

    • University of California, Los Angeles
  • Richard Thorne

    • University of California, Los Angeles