Global linear gyrokinetic simulation of energetic particledriven instabilities in the LHD stellarator
Abstract
Energetic particles are inherent to toroidal fusion systems and can drive instabilities in the Alfvén frequency range, leading to decreased heating efficiency, high heat fluxes on plasmafacing components, and decreased ignition margin. The applicability of global gyrokinetic simulation methods to macroscopic instabilities has now been demonstrated and it is natural to extend these methods to 3D configurations such as stellarators, tokamaks with 3D coils and reversed field pinch helical states. This has been achieved by coupling the GTC global gyrokinetic PIC model to the VMEC equilibrium model, including 3D effects in the field solvers and particle push. Here, this paper demonstrates the application of this new capability to the linearized analysis of Alfvénic instabilities in the LHD stellarator. For normal shear iota profiles, toroidal Alfvén instabilities in the n = 1 and 2 toroidal mode families are unstable with frequencies in the 75 to 110 kHz range. Also, an LHD case with nonmonotonic shear is considered, indicating reductions in growth rate for the same energetic particle drive. Finally, since 3D magnetic fields will be present to some extent in all fusion devices, the extension of gyrokinetic models to 3D configurations is an important step for the simulation of future fusionmore »
 Authors:

 Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
 Univ. of California, Irvine, CA (United States). Dept. of Physics and Astronomy; Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
 National Inst. for Fusion Science, Toki (Japan)
 Publication Date:
 Research Org.:
 Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States). Oak Ridge Leadership Computing Facility (OLCF); Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
 Sponsoring Org.:
 USDOE Office of Science (SC); USDOE National Nuclear Security Administration (NNSA)
 OSTI Identifier:
 1366391
 Alternate Identifier(s):
 OSTI ID: 1497274
 Report Number(s):
 LLNLJRNL748842
Journal ID: ISSN 00295515; AT1030100; ERAT021
 Grant/Contract Number:
 AC0500OR22725; AC0205CH11231; AC5207NA27344
 Resource Type:
 Accepted Manuscript
 Journal Name:
 Nuclear Fusion
 Additional Journal Information:
 Journal Volume: 57; Journal Issue: 8; Journal ID: ISSN 00295515
 Publisher:
 IOP Science
 Country of Publication:
 United States
 Language:
 English
 Subject:
 70 PLASMA PHYSICS AND FUSION TECHNOLOGY; stellarator; LHD; gyrokinetics; Alfven wave; energetic particles; fast ion instability linear
Citation Formats
Spong, Donald A., Holod, Ihor, Todo, Y., and Osakabe, M. Global linear gyrokinetic simulation of energetic particledriven instabilities in the LHD stellarator. United States: N. p., 2017.
Web. doi:10.1088/17414326/aa7601.
Spong, Donald A., Holod, Ihor, Todo, Y., & Osakabe, M. Global linear gyrokinetic simulation of energetic particledriven instabilities in the LHD stellarator. United States. doi:10.1088/17414326/aa7601.
Spong, Donald A., Holod, Ihor, Todo, Y., and Osakabe, M. Fri .
"Global linear gyrokinetic simulation of energetic particledriven instabilities in the LHD stellarator". United States. doi:10.1088/17414326/aa7601. https://www.osti.gov/servlets/purl/1366391.
@article{osti_1366391,
title = {Global linear gyrokinetic simulation of energetic particledriven instabilities in the LHD stellarator},
author = {Spong, Donald A. and Holod, Ihor and Todo, Y. and Osakabe, M.},
abstractNote = {Energetic particles are inherent to toroidal fusion systems and can drive instabilities in the Alfvén frequency range, leading to decreased heating efficiency, high heat fluxes on plasmafacing components, and decreased ignition margin. The applicability of global gyrokinetic simulation methods to macroscopic instabilities has now been demonstrated and it is natural to extend these methods to 3D configurations such as stellarators, tokamaks with 3D coils and reversed field pinch helical states. This has been achieved by coupling the GTC global gyrokinetic PIC model to the VMEC equilibrium model, including 3D effects in the field solvers and particle push. Here, this paper demonstrates the application of this new capability to the linearized analysis of Alfvénic instabilities in the LHD stellarator. For normal shear iota profiles, toroidal Alfvén instabilities in the n = 1 and 2 toroidal mode families are unstable with frequencies in the 75 to 110 kHz range. Also, an LHD case with nonmonotonic shear is considered, indicating reductions in growth rate for the same energetic particle drive. Finally, since 3D magnetic fields will be present to some extent in all fusion devices, the extension of gyrokinetic models to 3D configurations is an important step for the simulation of future fusion systems.},
doi = {10.1088/17414326/aa7601},
journal = {Nuclear Fusion},
number = 8,
volume = 57,
place = {United States},
year = {2017},
month = {6}
}
Web of Science
Figures / Tables:
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