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Suppression of non-axisymmetric field-induced α-particle loss channels in a quasi-axisymmetric stellarator
In future fusion reactors, the confinement of α-particles is a crucial issue. The perfect omnigenity may be difficult to achieve in the quasi-isodynamic and quasi-symmetric stellarators when a multi-objective optimization is considered. Non-axisymmetric field can result in collisionless particles’ t...
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Published in: | AIP advances 2022-05, Vol.12 (5), p.055214-055214-10 |
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creator | Zhang, Yichao Liu, Haifeng Huang, Jie Xu, Yuhong Zhang, Jian Shimizu, Akihiro Satake, Shinsuke Isobe, Mitsutaka Wang, Xianqu Cheng, Jun Liu, Hai Zhang, Xin Tang, Changjian |
description | In future fusion reactors, the confinement of α-particles is a crucial issue. The perfect omnigenity may be difficult to achieve in the quasi-isodynamic and quasi-symmetric stellarators when a multi-objective optimization is considered. Non-axisymmetric field can result in collisionless particles’ transport via localized trapping by ripples. Specific loss channels have been revealed to essentially exist in quasi-axisymmetric stellarators [Yang et al., Europhys. Lett. 129, 35001 (2020)] and W7-X [J. M. Faustin et al., Nucl. Fusion 56, 092006 (2016)]. It indicates a drastic loss of collisionless ions through these channels. This paper is devoted to investigate the effects of axisymmetry-breaking magnetic fields on collisionless α-particle transport in the CFQS (Chinese First Quasi-axisymmetric Stellarator) -like reactor configuration. A semi-analytic representation of radial and poloidal drifts in Boozer coordinates is given, by which we found an effective route to mitigate α-particle losses, i.e., adjusting the location of the quasi-axisymmetric radial position. Such a route enables the enhancement of the poloidal drift and decrease of radial drift in peripheral regions of the identified loss channels. The particles launched inside the quasi-axisymmetric radial surface can be well confined because localized particles that may fall in loss channels can transit into blocked particles near the quasi-axisymmetric surface, escaping from loss channels, which is beneficial for the improvement of the particle confinement. Moreover, this paper may provide a set of proxy functions for suppression of energetic particle losses to optimize stellarator configurations. |
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The perfect omnigenity may be difficult to achieve in the quasi-isodynamic and quasi-symmetric stellarators when a multi-objective optimization is considered. Non-axisymmetric field can result in collisionless particles’ transport via localized trapping by ripples. Specific loss channels have been revealed to essentially exist in quasi-axisymmetric stellarators [Yang et al., Europhys. Lett. 129, 35001 (2020)] and W7-X [J. M. Faustin et al., Nucl. Fusion 56, 092006 (2016)]. It indicates a drastic loss of collisionless ions through these channels. This paper is devoted to investigate the effects of axisymmetry-breaking magnetic fields on collisionless α-particle transport in the CFQS (Chinese First Quasi-axisymmetric Stellarator) -like reactor configuration. A semi-analytic representation of radial and poloidal drifts in Boozer coordinates is given, by which we found an effective route to mitigate α-particle losses, i.e., adjusting the location of the quasi-axisymmetric radial position. Such a route enables the enhancement of the poloidal drift and decrease of radial drift in peripheral regions of the identified loss channels. The particles launched inside the quasi-axisymmetric radial surface can be well confined because localized particles that may fall in loss channels can transit into blocked particles near the quasi-axisymmetric surface, escaping from loss channels, which is beneficial for the improvement of the particle confinement. Moreover, this paper may provide a set of proxy functions for suppression of energetic particle losses to optimize stellarator configurations.</description><identifier>ISSN: 2158-3226</identifier><identifier>EISSN: 2158-3226</identifier><identifier>DOI: 10.1063/5.0079827</identifier><identifier>CODEN: AAIDBI</identifier><language>eng</language><publisher>Melville: American Institute of Physics</publisher><subject>Channels ; Configurations ; Confinement ; Drift ; Energetic particles ; Fusion reactors ; Mathematical analysis ; Multiple objective analysis ; Optimization ; Position (location) ; Stellarators</subject><ispartof>AIP advances, 2022-05, Vol.12 (5), p.055214-055214-10</ispartof><rights>Author(s)</rights><rights>2022 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c428t-340569a5d1a2bed0532bd2b32c6b8dadd5aa140fcbe489103b390ff80ce7cf2a3</citedby><cites>FETCH-LOGICAL-c428t-340569a5d1a2bed0532bd2b32c6b8dadd5aa140fcbe489103b390ff80ce7cf2a3</cites><orcidid>0000-0002-9387-9987 ; 0000-0002-3572-1882 ; 0000-0002-0496-5542 ; 0000-0001-8485-895X ; 0000-0003-4882-647X ; 0000-0001-6407-5958 ; 0000-0002-0424-645X</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://pubs.aip.org/adv/article-lookup/doi/10.1063/5.0079827$$EHTML$$P50$$Gscitation$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,27890,27924,27925,76408</link.rule.ids></links><search><creatorcontrib>Zhang, Yichao</creatorcontrib><creatorcontrib>Liu, Haifeng</creatorcontrib><creatorcontrib>Huang, Jie</creatorcontrib><creatorcontrib>Xu, Yuhong</creatorcontrib><creatorcontrib>Zhang, Jian</creatorcontrib><creatorcontrib>Shimizu, Akihiro</creatorcontrib><creatorcontrib>Satake, Shinsuke</creatorcontrib><creatorcontrib>Isobe, Mitsutaka</creatorcontrib><creatorcontrib>Wang, Xianqu</creatorcontrib><creatorcontrib>Cheng, Jun</creatorcontrib><creatorcontrib>Liu, Hai</creatorcontrib><creatorcontrib>Zhang, Xin</creatorcontrib><creatorcontrib>Tang, Changjian</creatorcontrib><title>Suppression of non-axisymmetric field-induced α-particle loss channels in a quasi-axisymmetric stellarator</title><title>AIP advances</title><description>In future fusion reactors, the confinement of α-particles is a crucial issue. The perfect omnigenity may be difficult to achieve in the quasi-isodynamic and quasi-symmetric stellarators when a multi-objective optimization is considered. Non-axisymmetric field can result in collisionless particles’ transport via localized trapping by ripples. Specific loss channels have been revealed to essentially exist in quasi-axisymmetric stellarators [Yang et al., Europhys. Lett. 129, 35001 (2020)] and W7-X [J. M. Faustin et al., Nucl. Fusion 56, 092006 (2016)]. It indicates a drastic loss of collisionless ions through these channels. This paper is devoted to investigate the effects of axisymmetry-breaking magnetic fields on collisionless α-particle transport in the CFQS (Chinese First Quasi-axisymmetric Stellarator) -like reactor configuration. A semi-analytic representation of radial and poloidal drifts in Boozer coordinates is given, by which we found an effective route to mitigate α-particle losses, i.e., adjusting the location of the quasi-axisymmetric radial position. Such a route enables the enhancement of the poloidal drift and decrease of radial drift in peripheral regions of the identified loss channels. The particles launched inside the quasi-axisymmetric radial surface can be well confined because localized particles that may fall in loss channels can transit into blocked particles near the quasi-axisymmetric surface, escaping from loss channels, which is beneficial for the improvement of the particle confinement. Moreover, this paper may provide a set of proxy functions for suppression of energetic particle losses to optimize stellarator configurations.</description><subject>Channels</subject><subject>Configurations</subject><subject>Confinement</subject><subject>Drift</subject><subject>Energetic particles</subject><subject>Fusion reactors</subject><subject>Mathematical analysis</subject><subject>Multiple objective analysis</subject><subject>Optimization</subject><subject>Position (location)</subject><subject>Stellarators</subject><issn>2158-3226</issn><issn>2158-3226</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>AJDQP</sourceid><sourceid>DOA</sourceid><recordid>eNqdkclKBDEQhhtRcFAPvkHAk0Jr1u7MUcQNBjyo51CdRTP2dNqkW5zH8kV8JqMzuFytSxXFV39tRbFP8DHBFTsRxxjXU0nrjWJCiZAlo7Ta_BVvF3spzXE2PiVY8knxdDv2fbQp-dCh4FAXuhJefVouFnaIXiPnbWtK35lRW4Pe38oe4uB1a1EbUkL6EbrOtgn5DgF6HiH5v_VpsG0LEYYQd4stB22ye2u_U9xfnN-dXZWzm8vrs9NZqTmVQ8k4FtUUhCFAG2uwYLQxtGFUV400YIwAIBw73Vgu8xqsYVPsnMTa1tpRYDvF9UrXBJirPvoFxKUK4NVXIsQHtd5BSVpZzggxdS24kKapDCZNHqDOvXnNs9bBSquP4Xm0aVDzMMYuj69oVRFKSZbI1OGK0jEfJVr33ZVg9fkaJdT6NZk9WrFJ-wGGfPf_wS8h_oCqN459AAAHnkg</recordid><startdate>20220501</startdate><enddate>20220501</enddate><creator>Zhang, Yichao</creator><creator>Liu, Haifeng</creator><creator>Huang, Jie</creator><creator>Xu, Yuhong</creator><creator>Zhang, Jian</creator><creator>Shimizu, Akihiro</creator><creator>Satake, Shinsuke</creator><creator>Isobe, Mitsutaka</creator><creator>Wang, Xianqu</creator><creator>Cheng, Jun</creator><creator>Liu, Hai</creator><creator>Zhang, Xin</creator><creator>Tang, Changjian</creator><general>American Institute of Physics</general><general>AIP Publishing LLC</general><scope>AJDQP</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>DOA</scope><orcidid>https://orcid.org/0000-0002-9387-9987</orcidid><orcidid>https://orcid.org/0000-0002-3572-1882</orcidid><orcidid>https://orcid.org/0000-0002-0496-5542</orcidid><orcidid>https://orcid.org/0000-0001-8485-895X</orcidid><orcidid>https://orcid.org/0000-0003-4882-647X</orcidid><orcidid>https://orcid.org/0000-0001-6407-5958</orcidid><orcidid>https://orcid.org/0000-0002-0424-645X</orcidid></search><sort><creationdate>20220501</creationdate><title>Suppression of non-axisymmetric field-induced α-particle loss channels in a quasi-axisymmetric stellarator</title><author>Zhang, Yichao ; Liu, Haifeng ; Huang, Jie ; Xu, Yuhong ; Zhang, Jian ; Shimizu, Akihiro ; Satake, Shinsuke ; Isobe, Mitsutaka ; Wang, Xianqu ; Cheng, Jun ; Liu, Hai ; Zhang, Xin ; Tang, Changjian</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c428t-340569a5d1a2bed0532bd2b32c6b8dadd5aa140fcbe489103b390ff80ce7cf2a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Channels</topic><topic>Configurations</topic><topic>Confinement</topic><topic>Drift</topic><topic>Energetic particles</topic><topic>Fusion reactors</topic><topic>Mathematical analysis</topic><topic>Multiple objective analysis</topic><topic>Optimization</topic><topic>Position (location)</topic><topic>Stellarators</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Zhang, Yichao</creatorcontrib><creatorcontrib>Liu, Haifeng</creatorcontrib><creatorcontrib>Huang, Jie</creatorcontrib><creatorcontrib>Xu, Yuhong</creatorcontrib><creatorcontrib>Zhang, Jian</creatorcontrib><creatorcontrib>Shimizu, Akihiro</creatorcontrib><creatorcontrib>Satake, Shinsuke</creatorcontrib><creatorcontrib>Isobe, Mitsutaka</creatorcontrib><creatorcontrib>Wang, Xianqu</creatorcontrib><creatorcontrib>Cheng, Jun</creatorcontrib><creatorcontrib>Liu, Hai</creatorcontrib><creatorcontrib>Zhang, Xin</creatorcontrib><creatorcontrib>Tang, Changjian</creatorcontrib><collection>AIP Open Access Journals</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>DOAJ Directory of Open Access Journals</collection><jtitle>AIP advances</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Zhang, Yichao</au><au>Liu, Haifeng</au><au>Huang, Jie</au><au>Xu, Yuhong</au><au>Zhang, Jian</au><au>Shimizu, Akihiro</au><au>Satake, Shinsuke</au><au>Isobe, Mitsutaka</au><au>Wang, Xianqu</au><au>Cheng, Jun</au><au>Liu, Hai</au><au>Zhang, Xin</au><au>Tang, Changjian</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Suppression of non-axisymmetric field-induced α-particle loss channels in a quasi-axisymmetric stellarator</atitle><jtitle>AIP advances</jtitle><date>2022-05-01</date><risdate>2022</risdate><volume>12</volume><issue>5</issue><spage>055214</spage><epage>055214-10</epage><pages>055214-055214-10</pages><issn>2158-3226</issn><eissn>2158-3226</eissn><coden>AAIDBI</coden><abstract>In future fusion reactors, the confinement of α-particles is a crucial issue. The perfect omnigenity may be difficult to achieve in the quasi-isodynamic and quasi-symmetric stellarators when a multi-objective optimization is considered. Non-axisymmetric field can result in collisionless particles’ transport via localized trapping by ripples. Specific loss channels have been revealed to essentially exist in quasi-axisymmetric stellarators [Yang et al., Europhys. Lett. 129, 35001 (2020)] and W7-X [J. M. Faustin et al., Nucl. Fusion 56, 092006 (2016)]. It indicates a drastic loss of collisionless ions through these channels. This paper is devoted to investigate the effects of axisymmetry-breaking magnetic fields on collisionless α-particle transport in the CFQS (Chinese First Quasi-axisymmetric Stellarator) -like reactor configuration. A semi-analytic representation of radial and poloidal drifts in Boozer coordinates is given, by which we found an effective route to mitigate α-particle losses, i.e., adjusting the location of the quasi-axisymmetric radial position. Such a route enables the enhancement of the poloidal drift and decrease of radial drift in peripheral regions of the identified loss channels. The particles launched inside the quasi-axisymmetric radial surface can be well confined because localized particles that may fall in loss channels can transit into blocked particles near the quasi-axisymmetric surface, escaping from loss channels, which is beneficial for the improvement of the particle confinement. Moreover, this paper may provide a set of proxy functions for suppression of energetic particle losses to optimize stellarator configurations.</abstract><cop>Melville</cop><pub>American Institute of Physics</pub><doi>10.1063/5.0079827</doi><tpages>10</tpages><orcidid>https://orcid.org/0000-0002-9387-9987</orcidid><orcidid>https://orcid.org/0000-0002-3572-1882</orcidid><orcidid>https://orcid.org/0000-0002-0496-5542</orcidid><orcidid>https://orcid.org/0000-0001-8485-895X</orcidid><orcidid>https://orcid.org/0000-0003-4882-647X</orcidid><orcidid>https://orcid.org/0000-0001-6407-5958</orcidid><orcidid>https://orcid.org/0000-0002-0424-645X</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Channels Configurations Confinement Drift Energetic particles Fusion reactors Mathematical analysis Multiple objective analysis Optimization Position (location) Stellarators |
title | Suppression of non-axisymmetric field-induced α-particle loss channels in a quasi-axisymmetric stellarator |
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