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Direct Detection of Resonant Electron Pitch Angle Scattering by Whistler Waves in a Laboratory Plasma

B. Van Compernolle, J. Bortnik, P. Pribyl, W. Gekelman, M. Nakamoto, X. Tao, and R. M. Thorne
Phys. Rev. Lett. 112, 145006 – Published 10 April 2014
Physics logo See Synopsis: Radiation-Belt Scattering in the Lab

Abstract

Resonant interactions between energetic electrons and whistler mode waves are an essential ingredient in the space environment, and in particular in controlling the dynamic variability of Earth’s natural radiation belts, which is a topic of extreme interest at the moment. Although the theory describing resonant wave-particle interaction has been present for several decades, it has not been hitherto tested in a controlled laboratory setting. In the present Letter we report on the first laboratory experiment to directly detect resonant pitch angle scattering of energetic (keV) electrons due to whistler mode waves. We show that the whistler mode wave deflects energetic electrons at precisely the predicted resonant energy, and that varying both the maximum beam energy, and the wave frequency, alters the energetic electron beam very close to the resonant energy.

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  • Received 9 August 2013

DOI:https://doi.org/10.1103/PhysRevLett.112.145006

© 2014 American Physical Society

Synopsis

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Radiation-Belt Scattering in the Lab

Published 10 April 2014

Experiments in a laboratory recreate an interaction between electrons and plasma waves that may be responsible for large electron-flux variability in the Earth’s radiation belts.

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Authors & Affiliations

B. Van Compernolle1,*, J. Bortnik2, P. Pribyl1, W. Gekelman1, M. Nakamoto1, X. Tao2, and R. M. Thorne2

  • 1Department of Physics, University of California, Los Angeles, California 90095, USA
  • 2Department of Atmospheric and Oceanic Sciences, University of California, Los Angeles, California 90095, USA

  • *bvcomper@physics.ucla.edu

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Issue

Vol. 112, Iss. 14 — 11 April 2014

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