Radio and Plasma Wave Generation by an Electron Beam in a Laboratory Plasma
POSTER
Abstract
Interaction between relativistic electron beams and magnetized plasma is a fundamental and practical problem relevant to many challenging issues in space physics and astrophysics. We present results from a 20 keV beam experiment on the Large Plasma Device (LAPD) at UCLA motivated by the problem of how naturally occurring electron beams may produce type II/III solar radio emissions as well as recent proposals to place compact high-energy electron beam sources on future spacecraft. These spacecraft-borne beams may be used to map magnetic field lines in the Earth's magnetosphere or to generate waves for radiation belt remediation. In the LAPD experiments, electromagnetic emission between the plasma and upper hybrid frequencies is observed by both in-situ probes and by an antenna outside of the plasma. The parallel phase speed of the excited waves is measured to be consistent with generation via a resonance process at the point on the dispersion relation where the beam mode and Z-mode couple. Kinetic modeling suggests that the apparent absence of strong instabilities is due to velocity dispersion imposed by the beam injection conditions. Consistent with this, A 15-45% perturbation of the beam density is estimated from the parallel electric field measurements.
Presenters
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Seth E Dorfman
Space Science Institute, Space Science Institute; University of California Los Angeles
Authors
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Seth E Dorfman
Space Science Institute, Space Science Institute; University of California Los Angeles
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Vadim S Roytershteyn
Space Science Institute
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Gian Luca Delzanno
Los Alamos National Laboratory
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Cynthia Cattell
University Of Minnesota, University of Minnesota
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Quinn Marksteiner
Los Alamos National Laboratory
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Christopher Colpitts
University of Minnesota
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Haoran Xu
Los Alamos National Laboratory
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Jesus A Perez
University of California, Los Angeles