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}
}
Free Publicly Available Full Text
Publisher's Version of Record
https://doi.org/10.1088/1367-2630/aa5fdf
https://doi.org/10.1088/1367-2630/aa5fdf
Other availability
Cited by: 1 work
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