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Title: Nonlinear growth of zonal flows by secondary instability in general magnetic geometry

Abstract

Here we present a theory of the nonlinear growth of zonal flows in magnetized plasma turbulence, by the mechanism of secondary instability. The theory is derived for general magnetic geometry, and is thus applicable to both tokamaks and stellarators. The predicted growth rate is shown to compare favorably with nonlinear gyrokinetic simulations, with the error scaling as expected with the small parameter of the theory.

Authors:
;
Publication Date:
Research Org.:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC); European Union (EU)
OSTI Identifier:
1437702
Alternate Identifier(s):
OSTI ID: 1393855
Grant/Contract Number:  
DEAC02-05CH11231; AC02-05CH11231; 277870
Resource Type:
Published Article
Journal Name:
New Journal of Physics
Additional Journal Information:
Journal Name: New Journal of Physics Journal Volume: 19 Journal Issue: 2; Journal ID: ISSN 1367-2630
Publisher:
IOP Publishing
Country of Publication:
United Kingdom
Language:
English
Subject:
70 PLASMA PHYSICS AND FUSION TECHNOLOGY; stellarators; magnetic confinement fusion; plasma turbulence; zonal flows; nonlinear stability

Citation Formats

Plunk, G. G., and Navarro, A. Bañón. Nonlinear growth of zonal flows by secondary instability in general magnetic geometry. United Kingdom: N. p., 2017. Web. doi:10.1088/1367-2630/aa5fdf.
Plunk, G. G., & Navarro, A. Bañón. Nonlinear growth of zonal flows by secondary instability in general magnetic geometry. United Kingdom. https://doi.org/10.1088/1367-2630/aa5fdf
Plunk, G. G., and Navarro, A. Bañón. Wed . "Nonlinear growth of zonal flows by secondary instability in general magnetic geometry". United Kingdom. https://doi.org/10.1088/1367-2630/aa5fdf.
@article{osti_1437702,
title = {Nonlinear growth of zonal flows by secondary instability in general magnetic geometry},
author = {Plunk, G. G. and Navarro, A. Bañón},
abstractNote = {Here we present a theory of the nonlinear growth of zonal flows in magnetized plasma turbulence, by the mechanism of secondary instability. The theory is derived for general magnetic geometry, and is thus applicable to both tokamaks and stellarators. The predicted growth rate is shown to compare favorably with nonlinear gyrokinetic simulations, with the error scaling as expected with the small parameter of the theory.},
doi = {10.1088/1367-2630/aa5fdf},
journal = {New Journal of Physics},
number = 2,
volume = 19,
place = {United Kingdom},
year = {Wed Feb 01 00:00:00 EST 2017},
month = {Wed Feb 01 00:00:00 EST 2017}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record
https://doi.org/10.1088/1367-2630/aa5fdf

Citation Metrics:
Cited by: 1 work
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