Measurement and Simulation of Source-Generated Halos in the University of Maryland Electron Ring (UMER)

POSTER

Abstract

An area of nonlinear beam physics that is important in a number of beam systems, and is inadequately understood, is the generation and evolution of beam halos. Study of beam halos therefore has served as one rationale for recent research on UMER. While it was expected that halo formation would primarily result from nonlinear dynamics during beam propagation, recent experiments and simulations have instead identified imperfections in the source geometry, particularly in the region near the emitter edge, as a potentially significant source of halo particles. The edge-generated halo particles, both in the experiments and the simulations are found to pass through the center of the beam a short distance downstream of the anode plane. Understanding the detailed evolution of these particle orbits is therefore important to designing any aperture to remove the beam halo. Both experimental data and simulations will be presented to illustrate the details of this process, as well as proposed means of mitigation.

Authors

  • Irving Haber

    University of Maryland, Institute for Research in Electronics and Applied Physics

  • S. Bernal

    University of Maryland

  • R.B. Feldman

    University of Maryland

  • Rami Kishek

    University of Maryland, College Park, University of Maryland, Institute for Research in Electronics and Applied Physics

  • Patrick O'Shea

    University of Maryland, Institute for Research in Electronics and Applied Physics

  • Christos Papadopoulos

    University of Maryland, University of Maryland, College Park

  • M. Reiser

    University of Maryland

  • Diktys Stratakis

    University of Maryland, Institute for Research in Electronics and Applied Physics

  • Mark Walter

    University of Maryland, Institute for Research in Electronics and Applied Physics

  • A. Friedman

    LLNL

  • D.P. Grote

    LLNL

  • J.-L. Vay

    Lawrence Berkeley National Laboratory, LBNL