Numerical study of minority ion heating scenarios in CN-H1 stellarator plasma
A preliminary simulation of ion cyclotron resonance heating (ICRH) in the poloidal cross-section at the antenna location of the CN-H1 (Chinese Heliac 1) stellarator has been conducted for the first time using the full-wave solver TORIC. The heating scheme employed focuses on minority ion heating of...
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Veröffentlicht in: | Physica scripta 2025-02, Vol.100 (2), p.25602 |
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description | A preliminary simulation of ion cyclotron resonance heating (ICRH) in the poloidal cross-section at the antenna location of the CN-H1 (Chinese Heliac 1) stellarator has been conducted for the first time using the full-wave solver TORIC. The heating scheme employed focuses on minority ion heating of He 4 (H), with an independent investigation into the effects of wave frequency, toroidal mode number, and minority ion concentration on ICRH. Preliminary simulation results indicate that, under the conditions of wave frequency f = 4.7MHz, central magnetic field B 0 = 0.32T and low-temperature, low-density plasma (with density on the order of 10 18 m −3 and temperature in the range of tens of eV), more efficient minority-ion heating can be achieved when the toroidal mode number is in the range of 10–20 and the minority ion concentration is between 15% and 30%. This simulation provides theoretical insights and delineates the parameter space for prospective ICRH experiments in CN-H1. |
doi_str_mv | 10.1088/1402-4896/ad9c33 |
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The heating scheme employed focuses on minority ion heating of He 4 (H), with an independent investigation into the effects of wave frequency, toroidal mode number, and minority ion concentration on ICRH. Preliminary simulation results indicate that, under the conditions of wave frequency f = 4.7MHz, central magnetic field B 0 = 0.32T and low-temperature, low-density plasma (with density on the order of 10 18 m −3 and temperature in the range of tens of eV), more efficient minority-ion heating can be achieved when the toroidal mode number is in the range of 10–20 and the minority ion concentration is between 15% and 30%. This simulation provides theoretical insights and delineates the parameter space for prospective ICRH experiments in CN-H1.</description><identifier>ISSN: 0031-8949</identifier><identifier>EISSN: 1402-4896</identifier><identifier>DOI: 10.1088/1402-4896/ad9c33</identifier><identifier>CODEN: PHSTBO</identifier><language>eng</language><publisher>IOP Publishing</publisher><subject>ICRF ; minority ion heating ; stellarator</subject><ispartof>Physica scripta, 2025-02, Vol.100 (2), p.25602</ispartof><rights>2025 IOP Publishing Ltd. All rights, including for text and data mining, AI training, and similar technologies, are reserved.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c1461-4f5e1d2122fffbdcf57d3ce049a5a8c8362dcdbbfb0d6eb69f6618526b3b23ad3</cites><orcidid>0000-0003-2459-0749 ; 0009-0004-1352-5516 ; 0009-0005-4826-0084</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1088/1402-4896/ad9c33/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>314,776,780,27901,27902,53821,53868</link.rule.ids></links><search><creatorcontrib>Wang, Shuangshuang</creatorcontrib><creatorcontrib>Yin, Lan</creatorcontrib><creatorcontrib>Chen, You</creatorcontrib><creatorcontrib>Gong, Xueyu</creatorcontrib><creatorcontrib>Peng, Yaoyi</creatorcontrib><creatorcontrib>Zheng, Pingwei</creatorcontrib><creatorcontrib>Ma, Wankun</creatorcontrib><creatorcontrib>Ou, Qi</creatorcontrib><title>Numerical study of minority ion heating scenarios in CN-H1 stellarator plasma</title><title>Physica scripta</title><addtitle>PS</addtitle><addtitle>Phys. 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This simulation provides theoretical insights and delineates the parameter space for prospective ICRH experiments in CN-H1.</description><subject>ICRF</subject><subject>minority ion heating</subject><subject>stellarator</subject><issn>0031-8949</issn><issn>1402-4896</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2025</creationdate><recordtype>article</recordtype><recordid>eNp9kD1PwzAYhC0EEqGwM3pjIdQfibFHVAFFKmWB2fInuEriyE6G_nsSBTEhppNe3fPq7gC4xugOI87XuEKkrLhga2WFofQEFL-nU1AgRHHJRSXOwUXOB4QII0wU4HU_ti4FoxqYh9EeYfSwDV1MYTjCEDv45dQQuk-YjetUCjHD0MHNvtziCXBNo5IaYoJ9o3KrLsGZV012Vz-6Ah9Pj--bbbl7e37ZPOxKgyuGy8rXDluCCfHea2t8fW-pcagSqlbccMqINVZrr5FlTjPhGcO8JkxTTaiydAXQ8tekmHNyXvYptCodJUZynkPO3eXcXS5zTMjtgoTYy0McUzcF_M9-84e9nwkkiUSkZhPRW0-_AXxCb1Q</recordid><startdate>20250201</startdate><enddate>20250201</enddate><creator>Wang, Shuangshuang</creator><creator>Yin, Lan</creator><creator>Chen, You</creator><creator>Gong, Xueyu</creator><creator>Peng, Yaoyi</creator><creator>Zheng, Pingwei</creator><creator>Ma, Wankun</creator><creator>Ou, Qi</creator><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0003-2459-0749</orcidid><orcidid>https://orcid.org/0009-0004-1352-5516</orcidid><orcidid>https://orcid.org/0009-0005-4826-0084</orcidid></search><sort><creationdate>20250201</creationdate><title>Numerical study of minority ion heating scenarios in CN-H1 stellarator plasma</title><author>Wang, Shuangshuang ; Yin, Lan ; Chen, You ; Gong, Xueyu ; Peng, Yaoyi ; Zheng, Pingwei ; Ma, Wankun ; Ou, Qi</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c1461-4f5e1d2122fffbdcf57d3ce049a5a8c8362dcdbbfb0d6eb69f6618526b3b23ad3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2025</creationdate><topic>ICRF</topic><topic>minority ion heating</topic><topic>stellarator</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Wang, Shuangshuang</creatorcontrib><creatorcontrib>Yin, Lan</creatorcontrib><creatorcontrib>Chen, You</creatorcontrib><creatorcontrib>Gong, Xueyu</creatorcontrib><creatorcontrib>Peng, Yaoyi</creatorcontrib><creatorcontrib>Zheng, Pingwei</creatorcontrib><creatorcontrib>Ma, Wankun</creatorcontrib><creatorcontrib>Ou, Qi</creatorcontrib><collection>CrossRef</collection><jtitle>Physica scripta</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Wang, Shuangshuang</au><au>Yin, Lan</au><au>Chen, You</au><au>Gong, Xueyu</au><au>Peng, Yaoyi</au><au>Zheng, Pingwei</au><au>Ma, Wankun</au><au>Ou, Qi</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Numerical study of minority ion heating scenarios in CN-H1 stellarator plasma</atitle><jtitle>Physica scripta</jtitle><stitle>PS</stitle><addtitle>Phys. Scr</addtitle><date>2025-02-01</date><risdate>2025</risdate><volume>100</volume><issue>2</issue><spage>25602</spage><pages>25602-</pages><issn>0031-8949</issn><eissn>1402-4896</eissn><coden>PHSTBO</coden><abstract>A preliminary simulation of ion cyclotron resonance heating (ICRH) in the poloidal cross-section at the antenna location of the CN-H1 (Chinese Heliac 1) stellarator has been conducted for the first time using the full-wave solver TORIC. The heating scheme employed focuses on minority ion heating of He 4 (H), with an independent investigation into the effects of wave frequency, toroidal mode number, and minority ion concentration on ICRH. Preliminary simulation results indicate that, under the conditions of wave frequency f = 4.7MHz, central magnetic field B 0 = 0.32T and low-temperature, low-density plasma (with density on the order of 10 18 m −3 and temperature in the range of tens of eV), more efficient minority-ion heating can be achieved when the toroidal mode number is in the range of 10–20 and the minority ion concentration is between 15% and 30%. This simulation provides theoretical insights and delineates the parameter space for prospective ICRH experiments in CN-H1.</abstract><pub>IOP Publishing</pub><doi>10.1088/1402-4896/ad9c33</doi><tpages>13</tpages><orcidid>https://orcid.org/0000-0003-2459-0749</orcidid><orcidid>https://orcid.org/0009-0004-1352-5516</orcidid><orcidid>https://orcid.org/0009-0005-4826-0084</orcidid></addata></record> |
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title | Numerical study of minority ion heating scenarios in CN-H1 stellarator plasma |
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