Interaction of a Relativistic Electron Beam with Magnetized Plasma

ORAL

Abstract

The interaction between relativistic electron beams and a magnetized plasma is a fundamental and practical problem that is relevant to many challenging issues in space physics and astrophysics. For example, it is well known that energetic particles in the Earth’s radiation belts pose a danger to communication satellites. Compact electron beam sources may be used on future spacecraft to generate waves that would remove the energetic particles from the radiation belt region. A full understanding of the physics of these waves may also shed light on the mechanism for type II/III solar radio emissions. This talk will discuss experiments proposed to further advance understanding of the physical mechanisms governing beam-plasma interactions. The experiments and supporting simulations will investigate in detail the types of waves (whistler, Langmuir, etc.) produced by high-energy beams, beam stability, and feasibility for future space-based experiments. Experiments will be conducted on the Large Plasma Device (LAPD) at UCLA using a unique variable-energy electron beam recently developed at Los Alamos. We will discuss the proposed experimental setup as well as ongoing feasibility studies conducted using theoretical estimates and kinetic simulations.

Authors

  • Seth Dorfman

    University of California, Los Angeles, University of California Los Angeles

  • Vadim Roytershteyn

    Space Science Institute

  • Cynthia Cattell

    University of Minnesota, School of Physics and Astronomy, University of Minnesota

  • Bart Van Compernolle

    University of California, Los Angeles, UCLA, Department of Physics, University of California, Los Angeles

  • Gian Luca Delzanno

    Los Alamos National Laboratory