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Title: Loss of relativistic electrons when magnetic surfaces are broken

Abstract

Relativistic runaway electrons in ITER could be confined in a broad annulus of stochastic magnetic field lines bounded by an annulus of magnetic surfaces. The outer confining annulus can be broken by either an evolution of the magnetic field or by the drift of the plasma into the walls. Both possibilities are studied, and in both cases, the relativistic electrons in the stochastic region are lost to the walls in a short pulse of length $$\tau$$ along a narrow tube, which carries a flux fψst, where f ~ 10-3 and ψst is the toroidal flux in stochastic annulus. Both $$\tau$$ and f are determined by two parameters: the time it takes for a toroidal transit of a relativistic electron $$\tau$$t = 2πR/c, which is approximately 0.1 μs in ITER, and the evolution time $$\tau$$ev, which is of order 100 ms in most conditions of interest for ITER. The concept of turnstiles in Hamiltonian mechanics is then used to obtain the relation between $$\tau$$ and f and $$\tau$$t and $$\tau$$ev. The turnstile concept is also important in the theory of divertors for stellarators.

Authors:
 [1]; ORCiD logo [2]
  1. Columbia Univ., New York, NY (United States). Dept. of Applied Physics and Applied Mathematics
  2. Hampton Univ., Hampton, VA (United States). Dept. of Mathematics
Publication Date:
Research Org.:
Columbia Univ., New York, NY (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Fusion Energy Sciences (FES)
Contributing Org.:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
OSTI Identifier:
1465170
Alternate Identifier(s):
OSTI ID: 1330119
Grant/Contract Number:  
FG02-03ER54696; FG02-04ER54793; AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
Physics of Plasmas
Additional Journal Information:
Journal Volume: 23; Journal Issue: 10; Journal ID: ISSN 1070-664X
Publisher:
American Institute of Physics (AIP)
Country of Publication:
United States
Language:
English
Subject:
70 PLASMA PHYSICS AND FUSION TECHNOLOGY; runaway electrons; Hamiltonian mechanics; magnetic flux; relativistic plasmas; tokamaks; toroidal plasma confinement; plasma transport properties; stellar spectral lines; magnetic fields; surface magnetism

Citation Formats

Boozer, Allen H., and Punjabi, Alkesh. Loss of relativistic electrons when magnetic surfaces are broken. United States: N. p., 2016. Web. doi:10.1063/1.4966046.
Boozer, Allen H., & Punjabi, Alkesh. Loss of relativistic electrons when magnetic surfaces are broken. United States. https://doi.org/10.1063/1.4966046
Boozer, Allen H., and Punjabi, Alkesh. Wed . "Loss of relativistic electrons when magnetic surfaces are broken". United States. https://doi.org/10.1063/1.4966046. https://www.osti.gov/servlets/purl/1465170.
@article{osti_1465170,
title = {Loss of relativistic electrons when magnetic surfaces are broken},
author = {Boozer, Allen H. and Punjabi, Alkesh},
abstractNote = {Relativistic runaway electrons in ITER could be confined in a broad annulus of stochastic magnetic field lines bounded by an annulus of magnetic surfaces. The outer confining annulus can be broken by either an evolution of the magnetic field or by the drift of the plasma into the walls. Both possibilities are studied, and in both cases, the relativistic electrons in the stochastic region are lost to the walls in a short pulse of length $\tau$ℓ along a narrow tube, which carries a flux fψst, where f ~ 10-3 and ψst is the toroidal flux in stochastic annulus. Both $\tau$ℓ and f are determined by two parameters: the time it takes for a toroidal transit of a relativistic electron $\tau$t = 2πR/c, which is approximately 0.1 μs in ITER, and the evolution time $\tau$ev, which is of order 100 ms in most conditions of interest for ITER. The concept of turnstiles in Hamiltonian mechanics is then used to obtain the relation between $\tau$ℓ and f and $\tau$t and $\tau$ev. The turnstile concept is also important in the theory of divertors for stellarators.},
doi = {10.1063/1.4966046},
journal = {Physics of Plasmas},
number = 10,
volume = 23,
place = {United States},
year = {Wed Oct 26 00:00:00 EDT 2016},
month = {Wed Oct 26 00:00:00 EDT 2016}
}

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Cited by: 19 works
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Works referencing / citing this record:

Simulation of stellarator divertors
journal, September 2018

  • Boozer, Allen H.; Punjabi, Alkesh
  • Physics of Plasmas, Vol. 25, Issue 9
  • DOI: 10.1063/1.5042666

Simulations of the effects of pre-seeded magnetic islands on the generation of runaway current during disruption on J-TEXT
journal, June 2019

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  • DOI: 10.1063/1.5100093

Simulation of non-resonant stellarator divertor
journal, January 2020

  • Punjabi, Alkesh; Boozer, Allen H.
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  • DOI: 10.1063/1.5113907

Magnetic surface loss and electron runaway
journal, January 2019


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journal, March 2019

  • Paz-Soldan, C.; Eidietis, N. W.; Liu, Y. Q.
  • Plasma Physics and Controlled Fusion, Vol. 61, Issue 5
  • DOI: 10.1088/1361-6587/aafd15

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journal, December 2017


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journal, August 2018


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journal, June 2019

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MARS-F modeling of post-disruption runaway beam loss by magnetohydrodynamic instabilities in DIII-D
journal, October 2019


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text, January 2018


Simulation of non-resonant stellarator divertor
text, January 2021