Analysis of ELM stability with extended MHD models in JET, JT-60U and future JT-60SA tokamak plasmas
The stability with respect to a peeling–ballooning mode (PBM) was investigated numerically with extended MHD simulation codes in JET, JT-60U and future JT-60SA plasmas. The MINERVA-DI code was used to analyze the linear stability, including the effects of rotation and ion diamagnetic drift ( *w i),...
| Autores: | , , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2018 |
| País: | España |
| Institución: | Universidad de Sevilla (US) |
| Repositorio: | idUS. Depósito de Investigación de la Universidad de Sevilla |
| OAI Identifier: | oai:idus.us.es:11441/99695 |
| Acceso en línea: | https://hdl.handle.net/11441/99695 https://doi.org/10.1088/1361-6587/aa8bec |
| Access Level: | acceso abierto |
| Palabra clave: | ELM Extended MHD model Rotation Tokamaks H-mode |
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Analysis of ELM stability with extended MHD models in JET, JT-60U and future JT-60SA tokamak plasmasAiba, N.Pamela, S.Honda, M.Urano, H.Giroud, C.Jet ContributorsGarcía Muñoz, ManuelAyllón Guerola, Juan ManuelELMExtended MHD modelRotationTokamaksH-modeThe stability with respect to a peeling–ballooning mode (PBM) was investigated numerically with extended MHD simulation codes in JET, JT-60U and future JT-60SA plasmas. The MINERVA-DI code was used to analyze the linear stability, including the effects of rotation and ion diamagnetic drift ( *w i), in JET-ILW and JT-60SA plasmas, and the JOREK code was used to simulate nonlinear dynamics with rotation, viscosity and resistivity in JT-60U plasmas. It was validated quantitatively that the ELM trigger condition in JET-ILW plasmas can be reasonably explained by taking into account both the rotation and *w i effects in the numerical analysis. When deuterium poloidal rotation is evaluated based on neoclassical theory, an increase in the effective charge of plasma destabilizes the PBM because of an acceleration of rotation and a decrease in *w i. The difference in the amount of ELM energy loss in JT-60U plasmas rotating in opposite directions was reproduced qualitatively with JOREK. By comparing the ELM affected areas with linear eigenfunctions, it was confirmed that the difference in the linear stability property, due not to the rotation direction but to the plasma density profile, is thought to be responsible for changing the ELM energy loss just after the ELM crash. A predictive study to determine the pedestal profiles in JT-60SA was performed by updating the EPED1 model to include the rotation and *w i effects in the PBM stability analysis. It was shown that the plasma rotation predicted with the neoclassical toroidal viscosity degrades the pedestal performance by about 10% by destabilizing the PBM, but the pressure pedestal height will be high enough to achieve the target parameters required for the ITER-like shape inductive scenario in JT-60SA.JSPS KAKENHI 15K06656EURATOM 633053IOP PublishingFísica Atómica, Molecular y NuclearRNM138: Física Nuclear Aplicada2018info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionapplication/pdfapplication/pdfhttps://hdl.handle.net/11441/99695https://doi.org/10.1088/1361-6587/aa8becreponame:idUS. Depósito de Investigación de la Universidad de Sevillainstname:Universidad de Sevilla (US)InglésPlasma Physics and Controlled Fusion, 60 (1), 1-11.15K06656633053https://doi.org/10.1088/1361-6587/aa8becinfo:eu-repo/semantics/openAccessoai:idus.us.es:11441/996952026-06-17T12:51:07Z |
| dc.title.none.fl_str_mv |
Analysis of ELM stability with extended MHD models in JET, JT-60U and future JT-60SA tokamak plasmas |
| title |
Analysis of ELM stability with extended MHD models in JET, JT-60U and future JT-60SA tokamak plasmas |
| spellingShingle |
Analysis of ELM stability with extended MHD models in JET, JT-60U and future JT-60SA tokamak plasmas Aiba, N. ELM Extended MHD model Rotation Tokamaks H-mode |
| title_short |
Analysis of ELM stability with extended MHD models in JET, JT-60U and future JT-60SA tokamak plasmas |
| title_full |
Analysis of ELM stability with extended MHD models in JET, JT-60U and future JT-60SA tokamak plasmas |
| title_fullStr |
Analysis of ELM stability with extended MHD models in JET, JT-60U and future JT-60SA tokamak plasmas |
| title_full_unstemmed |
Analysis of ELM stability with extended MHD models in JET, JT-60U and future JT-60SA tokamak plasmas |
| title_sort |
Analysis of ELM stability with extended MHD models in JET, JT-60U and future JT-60SA tokamak plasmas |
| dc.creator.none.fl_str_mv |
Aiba, N. Pamela, S. Honda, M. Urano, H. Giroud, C. Jet Contributors García Muñoz, Manuel Ayllón Guerola, Juan Manuel |
| author |
Aiba, N. |
| author_facet |
Aiba, N. Pamela, S. Honda, M. Urano, H. Giroud, C. Jet Contributors García Muñoz, Manuel Ayllón Guerola, Juan Manuel |
| author_role |
author |
| author2 |
Pamela, S. Honda, M. Urano, H. Giroud, C. Jet Contributors García Muñoz, Manuel Ayllón Guerola, Juan Manuel |
| author2_role |
author author author author author author author |
| dc.contributor.none.fl_str_mv |
Física Atómica, Molecular y Nuclear RNM138: Física Nuclear Aplicada |
| dc.subject.none.fl_str_mv |
ELM Extended MHD model Rotation Tokamaks H-mode |
| topic |
ELM Extended MHD model Rotation Tokamaks H-mode |
| description |
The stability with respect to a peeling–ballooning mode (PBM) was investigated numerically with extended MHD simulation codes in JET, JT-60U and future JT-60SA plasmas. The MINERVA-DI code was used to analyze the linear stability, including the effects of rotation and ion diamagnetic drift ( *w i), in JET-ILW and JT-60SA plasmas, and the JOREK code was used to simulate nonlinear dynamics with rotation, viscosity and resistivity in JT-60U plasmas. It was validated quantitatively that the ELM trigger condition in JET-ILW plasmas can be reasonably explained by taking into account both the rotation and *w i effects in the numerical analysis. When deuterium poloidal rotation is evaluated based on neoclassical theory, an increase in the effective charge of plasma destabilizes the PBM because of an acceleration of rotation and a decrease in *w i. The difference in the amount of ELM energy loss in JT-60U plasmas rotating in opposite directions was reproduced qualitatively with JOREK. By comparing the ELM affected areas with linear eigenfunctions, it was confirmed that the difference in the linear stability property, due not to the rotation direction but to the plasma density profile, is thought to be responsible for changing the ELM energy loss just after the ELM crash. A predictive study to determine the pedestal profiles in JT-60SA was performed by updating the EPED1 model to include the rotation and *w i effects in the PBM stability analysis. It was shown that the plasma rotation predicted with the neoclassical toroidal viscosity degrades the pedestal performance by about 10% by destabilizing the PBM, but the pressure pedestal height will be high enough to achieve the target parameters required for the ITER-like shape inductive scenario in JT-60SA. |
| publishDate |
2018 |
| dc.date.none.fl_str_mv |
2018 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
https://hdl.handle.net/11441/99695 https://doi.org/10.1088/1361-6587/aa8bec |
| url |
https://hdl.handle.net/11441/99695 https://doi.org/10.1088/1361-6587/aa8bec |
| dc.language.none.fl_str_mv |
Inglés |
| language_invalid_str_mv |
Inglés |
| dc.relation.none.fl_str_mv |
Plasma Physics and Controlled Fusion, 60 (1), 1-11. 15K06656 633053 https://doi.org/10.1088/1361-6587/aa8bec |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess |
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openAccess |
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application/pdf application/pdf |
| dc.publisher.none.fl_str_mv |
IOP Publishing |
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IOP Publishing |
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reponame:idUS. Depósito de Investigación de la Universidad de Sevilla instname:Universidad de Sevilla (US) |
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Universidad de Sevilla (US) |
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idUS. Depósito de Investigación de la Universidad de Sevilla |
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idUS. Depósito de Investigación de la Universidad de Sevilla |
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15.300724 |