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Configuration characteristics of the Chinese First Quasi-axisymmetric Stellarator
The Chinese First Quasi-axisymmetric Stellarator (CFQS) will be the first operational quasi-axially symmetric stellarator in the world. The physical and engineering complexities led to the cancellation of two famous quasi-axisymmetric stellarators, CHS-qa and NCSX. Therefore, the major mission of th...
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Published in: | Nuclear fusion 2021-01, Vol.61 (1), p.16014 |
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creator | Liu, Haifeng Shimizu, Akihiro Xu, Yuhong Okamura, Shoichi Kinoshita, Shigeyoshi Isobe, Mitsutaka Li, Yangbo Xiong, Guozheng Wang, Xianqu Huang, Jie Cheng, Jun Liu, Hai Zhang, Xin Yin, Dapeng Wang, Y Murase, Takanori Nakagawa, Sho Tang, Changjian |
description | The Chinese First Quasi-axisymmetric Stellarator (CFQS) will be the first operational quasi-axially symmetric stellarator in the world. The physical and engineering complexities led to the cancellation of two famous quasi-axisymmetric stellarators, CHS-qa and NCSX. Therefore, the major mission of the CFQS is to experimentally achieve the canonical quasi-axisymmetric configuration. The CFQS has been designed to possess a number of advanced features in fixed and free-boundary equilibria. It is a compact stellarator with an aspect ratio R/a ∼4.0. The neoclassical diffusion coefficient is similar to that of tokamaks in the collisionless regime. The MHD equilibrium of the CFQS configuration is stable up to volume-averaged normalized pressure β ∼1.1%. A region of the second ballooning stability exists in this facility with a large region of plasma, becoming second stable for β ∼2.7% in free-boundary equilibria. The gap between the first and second stability boundaries is very narrow, which is greatly beneficial for the CFQS operation in the second stable regime with high β plasma. A modular coil system with 16 coils is designed which robustly reproduces the standard quasi-axisymmetric magnetic field. |
doi_str_mv | 10.1088/1741-4326/abbc85 |
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The physical and engineering complexities led to the cancellation of two famous quasi-axisymmetric stellarators, CHS-qa and NCSX. Therefore, the major mission of the CFQS is to experimentally achieve the canonical quasi-axisymmetric configuration. The CFQS has been designed to possess a number of advanced features in fixed and free-boundary equilibria. It is a compact stellarator with an aspect ratio R/a ∼4.0. The neoclassical diffusion coefficient is similar to that of tokamaks in the collisionless regime. The MHD equilibrium of the CFQS configuration is stable up to volume-averaged normalized pressure β ∼1.1%. A region of the second ballooning stability exists in this facility with a large region of plasma, becoming second stable for β ∼2.7% in free-boundary equilibria. The gap between the first and second stability boundaries is very narrow, which is greatly beneficial for the CFQS operation in the second stable regime with high β plasma. 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Fusion</addtitle><description>The Chinese First Quasi-axisymmetric Stellarator (CFQS) will be the first operational quasi-axially symmetric stellarator in the world. The physical and engineering complexities led to the cancellation of two famous quasi-axisymmetric stellarators, CHS-qa and NCSX. Therefore, the major mission of the CFQS is to experimentally achieve the canonical quasi-axisymmetric configuration. The CFQS has been designed to possess a number of advanced features in fixed and free-boundary equilibria. It is a compact stellarator with an aspect ratio R/a ∼4.0. The neoclassical diffusion coefficient is similar to that of tokamaks in the collisionless regime. The MHD equilibrium of the CFQS configuration is stable up to volume-averaged normalized pressure β ∼1.1%. A region of the second ballooning stability exists in this facility with a large region of plasma, becoming second stable for β ∼2.7% in free-boundary equilibria. The gap between the first and second stability boundaries is very narrow, which is greatly beneficial for the CFQS operation in the second stable regime with high β plasma. A modular coil system with 16 coils is designed which robustly reproduces the standard quasi-axisymmetric magnetic field.</description><subject>MHD stability</subject><subject>Quasi-axisymmetric configuration</subject><subject>Stellarator design</subject><issn>0029-5515</issn><issn>1741-4326</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNp1UMFKAzEUDKJgrd495uTJtXnZTXZzlMVWoSBFPYdsNrEp7aYkWbB_b0rFk57e8JgZZgahWyAPQJpmBnUFRVVSPlNdpxt2hia_r3M0IYSKgjFgl-gqxg0hUEFZTtCq9YN1n2NQyfkB67UKSicTXExOR-wtTmuD27UbTDR47kJMeDWq6Ar15eJhtzMpOI3fktluszT5cI0urNpGc_Nzp-hj_vTePhfL18VL-7gsdMXLVFCrLVWmqVlfirqpq74mnFItDO2oyNkytsJUve0Y04yLDggjFEB0HBrRl1NETr46-BiDsXIf3E6FgwQij5PIY3957C9Pk2TJ3Uni_F5u_BiGHFAOVnKQIAnwvIrc9zYT7_8g_uv7DY2AcF8</recordid><startdate>20210101</startdate><enddate>20210101</enddate><creator>Liu, Haifeng</creator><creator>Shimizu, Akihiro</creator><creator>Xu, Yuhong</creator><creator>Okamura, Shoichi</creator><creator>Kinoshita, Shigeyoshi</creator><creator>Isobe, Mitsutaka</creator><creator>Li, Yangbo</creator><creator>Xiong, Guozheng</creator><creator>Wang, Xianqu</creator><creator>Huang, Jie</creator><creator>Cheng, Jun</creator><creator>Liu, Hai</creator><creator>Zhang, Xin</creator><creator>Yin, Dapeng</creator><creator>Wang, Y</creator><creator>Murase, Takanori</creator><creator>Nakagawa, Sho</creator><creator>Tang, Changjian</creator><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0002-0424-645X</orcidid><orcidid>https://orcid.org/0000-0002-7635-2905</orcidid><orcidid>https://orcid.org/0000-0001-6407-5958</orcidid><orcidid>https://orcid.org/0000-0001-8603-4356</orcidid><orcidid>https://orcid.org/0000-0003-4882-647X</orcidid><orcidid>https://orcid.org/0000-0001-8485-895X</orcidid><orcidid>https://orcid.org/0000-0003-4179-943X</orcidid><orcidid>https://orcid.org/0000-0003-3764-3184</orcidid><orcidid>https://orcid.org/0000-0002-8156-8233</orcidid></search><sort><creationdate>20210101</creationdate><title>Configuration characteristics of the Chinese First Quasi-axisymmetric Stellarator</title><author>Liu, Haifeng ; Shimizu, Akihiro ; Xu, Yuhong ; Okamura, Shoichi ; Kinoshita, Shigeyoshi ; Isobe, Mitsutaka ; Li, Yangbo ; Xiong, Guozheng ; Wang, Xianqu ; Huang, Jie ; Cheng, Jun ; Liu, Hai ; Zhang, Xin ; Yin, Dapeng ; Wang, Y ; Murase, Takanori ; Nakagawa, Sho ; Tang, Changjian</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c463t-2fcf2ae875d397874d70622c9e2b2913322cf9e4dfb55c569b10502119b6189d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>MHD stability</topic><topic>Quasi-axisymmetric configuration</topic><topic>Stellarator design</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Liu, Haifeng</creatorcontrib><creatorcontrib>Shimizu, Akihiro</creatorcontrib><creatorcontrib>Xu, Yuhong</creatorcontrib><creatorcontrib>Okamura, Shoichi</creatorcontrib><creatorcontrib>Kinoshita, Shigeyoshi</creatorcontrib><creatorcontrib>Isobe, Mitsutaka</creatorcontrib><creatorcontrib>Li, Yangbo</creatorcontrib><creatorcontrib>Xiong, Guozheng</creatorcontrib><creatorcontrib>Wang, Xianqu</creatorcontrib><creatorcontrib>Huang, Jie</creatorcontrib><creatorcontrib>Cheng, Jun</creatorcontrib><creatorcontrib>Liu, Hai</creatorcontrib><creatorcontrib>Zhang, Xin</creatorcontrib><creatorcontrib>Yin, Dapeng</creatorcontrib><creatorcontrib>Wang, Y</creatorcontrib><creatorcontrib>Murase, Takanori</creatorcontrib><creatorcontrib>Nakagawa, Sho</creatorcontrib><creatorcontrib>Tang, Changjian</creatorcontrib><collection>CrossRef</collection><jtitle>Nuclear fusion</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Liu, Haifeng</au><au>Shimizu, Akihiro</au><au>Xu, Yuhong</au><au>Okamura, Shoichi</au><au>Kinoshita, Shigeyoshi</au><au>Isobe, Mitsutaka</au><au>Li, Yangbo</au><au>Xiong, Guozheng</au><au>Wang, Xianqu</au><au>Huang, Jie</au><au>Cheng, Jun</au><au>Liu, Hai</au><au>Zhang, Xin</au><au>Yin, Dapeng</au><au>Wang, Y</au><au>Murase, Takanori</au><au>Nakagawa, Sho</au><au>Tang, Changjian</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Configuration characteristics of the Chinese First Quasi-axisymmetric Stellarator</atitle><jtitle>Nuclear fusion</jtitle><stitle>NF</stitle><addtitle>Nucl. Fusion</addtitle><date>2021-01-01</date><risdate>2021</risdate><volume>61</volume><issue>1</issue><spage>16014</spage><pages>16014-</pages><issn>0029-5515</issn><eissn>1741-4326</eissn><coden>NUFUAU</coden><abstract>The Chinese First Quasi-axisymmetric Stellarator (CFQS) will be the first operational quasi-axially symmetric stellarator in the world. The physical and engineering complexities led to the cancellation of two famous quasi-axisymmetric stellarators, CHS-qa and NCSX. Therefore, the major mission of the CFQS is to experimentally achieve the canonical quasi-axisymmetric configuration. The CFQS has been designed to possess a number of advanced features in fixed and free-boundary equilibria. It is a compact stellarator with an aspect ratio R/a ∼4.0. The neoclassical diffusion coefficient is similar to that of tokamaks in the collisionless regime. The MHD equilibrium of the CFQS configuration is stable up to volume-averaged normalized pressure β ∼1.1%. A region of the second ballooning stability exists in this facility with a large region of plasma, becoming second stable for β ∼2.7% in free-boundary equilibria. The gap between the first and second stability boundaries is very narrow, which is greatly beneficial for the CFQS operation in the second stable regime with high β plasma. 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subjects | MHD stability Quasi-axisymmetric configuration Stellarator design |
title | Configuration characteristics of the Chinese First Quasi-axisymmetric Stellarator |
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