Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session NP11: Poster Session V: Laser-plasma Particle Acceleration; HEDP; Turbulence and Transport; DIII-D Tokamak; Machine Learning, Data Science (9:30am-12:30pm)
Wednesday, November 7, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.NP11.118
Abstract: NP11.00118 : Whistler Waves Driven by Runaway Electrons*
Presenter:
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)
Carlos Alberto Paz-Soldan
(General Atomics - San Diego)
Kathreen Thome
(General Atomics - San Diego)
Michael A Van Zeeland
(General Atomics - San Diego)
Donald Spong
(Oak Ridge National Lab)
Andrey Lvovskiy
(Oak Ridge Assoc Univ)
Richard A Moyer
(Univ of California - San Diego)
Max E Austin
(Univ of Texas, Austin)
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.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.NP11.118
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