Whistler Waves Driven by Runaway Electrons

POSTER

Abstract

In quiescent runaway electron plasmas, whistler waves with frequencies between 90-190 MHz are driven unstable in plasmas with appreciable hard x-ray and non-thermal electron cyclotron emission (ECE). Narrow (δf < 50 kHz) discrete modes are observed at erratically spaced frequencies, likely due to the bounding of the plasma [1]. The dependency of the frequency on field and density implies a wavenumber k ≈ 140 m-1 with kparallel much less than k. Reducing the gap between the plasma and the wall increases the number of detected modes. The high intensity gamma ray bremsstrahlung and synchrotron emission measurements suggest the waves are driven by electrons of several MeV through the anomalous Doppler resonance. The ECE signals often jump at whistler bursts, suggesting that the modes pitch-angle scatter the runaways via nonlinear predator-prey dynamics, implying that whistler waves can potentially be used to mitigate reactor damage from runaways.

[1] D.A. Spong et at., Phys. Rev. Lett. 120 (2018) 155002.

*Work supported by US DOE DE-FC02-04ER54698.

Presenters

  • Kenneth Gage

    • Univ of California - Irvine

Authors

  • Kenneth Gage

    • Univ of California - Irvine
  • Xiaodi Du

    • Univ of California - Irvine
  • William Walter Heidbrink

    • Univ of California - Irvine
    • University of California, Irvine
  • C. Alberto Paz-Soldan

    • General Atomics - San Diego
    • General Atomics
    • GA
  • Kathreen Thome

    • General Atomics - San Diego
  • Michael A Van Zeeland

    • General Atomics - San Diego
    • General Atomics
    • GA
  • Donald Spong

    • Oak Ridge National Lab
  • Andrey Lvovskiy

    • Oak Ridge Assoc Univ
  • R.A. A Moyer

    • Univ of California - San Diego
    • University of California San Diego
    • UCSD
  • Max E. Austin

    • University of Texas at Austin, Institute for Fusion Studies
    • Univ of Texas, Austin
    • Univ. of Texas, Austin
    • U. Texas-Austin
    • The University of Texas at Austin