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A power-balance model, with radiation losses from impurities and neutrals, gives a unified description of the density limit (DL) of the stellarator, the L-mode tokamak, and the reversed field pinch (RFP). The model predicts a Sudo-like scaling for the stellarator, a Greenwald- like scaling, alpha I-p(8/9), for the RFP and the ohmic tokamak, a mixed scaling, alpha (PIp4/9)-I-4/9, for the additionally heated L-mode tokamak. In a previous paper (Zanca et al 2017 Nucl. Fusion 57 056010) the model was compared with ohmic tokamak, RFP and stellarator experiments. Here, we address the issue of the DL dependence on heating power in the L-mode tokamak. Experimental data from high-density disrupted L-mode discharges performed at JET, as well as in other machines, arc taken as a term of comparison. The model fits the observed maximum densities better than the pure Greenwald limit.
A power-balance model of the density limit in fusion plasmas: application to the L-mode tokamak
Zanca P;Sattin F;Escande D F;Abduallev S;Abhangi M;Abreu P;Afzal M;Aggarwal K M;Ahlgren T;Ahn J H;AhoMantila L;Aiba N;Airila M;Albanese R;Aldred V;Alegre D;Alessi E;Aleynikov P;Alfier A;Alkseev A;Allinson M;Alper B;Alves E;Ambrosino G;Ambrosino R;Amicucci L;Amosov V;Sunden E Andersson;Angelone M;Anghel M;Angioni C;Appel L;Appelbee C;Arena P;Ariola M;Arnichand H;Arshad S;Ash A;Ashikawa N;Aslanyan V;Asunta O;Auriemma F;Austin Y;Avotina L;Axton M D;Ayres C;Bacharis M;Baciero A;Baiao D;Bailey S;Baker A;Balboa I;Balden M;Balshaw N;Bament R;Banks J W;Baranov Y F;Barnard M A;Barnes D;Barnes M;Barnsley R;Wiechec A Baron;Orte L Barrera;Baruzzo M;Basiuk V;Bassan M;Bastow R;Batista A;Batistoni P;Baughan R;Bauvir B;Baylor L;Bazylev B;Beal J;Beaumont P S;Beckers M;Beckett B;Becoulet A;Bekris N;Beldishevski M;Bell K;Belli F;Bellinger M;Belonohy E;Ben Ayed N;Benterman N A;Bergsaker H;Bernardo J;Bernert M;Berry M;Bertalot L;Besliu C;Beurskens M;Bieg B;Bielecki J;Biewer T;Bigi M;Bilkova P;Binda F;Bisoffi A;Bizarro J P S;Bjorkas C;Blackburn J;Blackman K;Blackman T R;Blanchard P;Blatchford P;Bobkov V;Boboc A;Bodnar G;Bogar O;Bolshakova I;Bolzonella T;Bonanomi N;Bonelli F;Boom J;Booth J;Borba D;Borodin D;Borodkina I;Botrugno A;Bottereau C;Boulting P;Bourdelle C;Bowden M;Bower C;Bowman C;Boyce T;Boyd C;Boyer H J;Bradshaw J M A;Braic V;Bravanec R;Breizman B;Bremond S;Brennan P D;Breton S;Brett A;Brezinsek S;Bright M D J;Brix M;Broeckx W;Brombin M;Broslawski A;Brown D P D;Brown M;Bruno E;Bucalossi J;Buch J;Buchanan J;Buckley M A;Budny R;Bufferand H;Bulman M;Bulmer N;Bunting P;Buratti P;Burckhart A;Buscarino A;Busse A;Butler N K;Bykov I;Byrne J;Cahyna P;Calabro G;Calvo I;Camenen Y;Camp P;Campling D C;Cane J;Cannas B;Capel A J;Card P J;Cardinali A;Carman P;Carr M;Carralero D;Carraro L;Carvalho B B;Carvalho I;Carvalho P;Casson F J;Castaldo C;Catarino N;Caumont J;Causa F;Cavazzana R;CaveAyland K;Cavinato M;Cecconello M;Ceccuzzi S;Cecil E;Cenedese A;Cesario R;Challis C D;Chandler M;Chandra D;Chang C S;Chankin A;Chapman I T;Chapman S C;Chernyshova M;Chitarin G;Ciraolo G;Ciric D;Citrin J;Clairet F;Clark E;Clark M;Clarkson R;Clatworthy D;Clements C;Cleverly M;Coad J P;Coates P A;Cobalt A;Coccorese V;Cocilovo V;Coda S;Coelho R;Coenen J W;Coffey I;Colas L;Collins S;Conka D;Conroy S;Conway N;Coombs D;Cooper D;Cooper S R;Corradino C;Corre Y;Corrigan G;Cortes S;Coster D;Couchman A S;Cox M P;Craciunescu T;Cramp S;Craven R;Crisanti F;Croci G;Croft D;Crombe K;Crowe R;Cruz N;Cseh G;Cufar A;Cullen A;Curuia M;Czarnecka A;Dabirikhah H;Dalgliesh P;Dalley S;Dankowski J;Darrow D;Davies O;Davis W;Day C;Day I E;De Bock M;de Castro A;de la Cal E;de la Luna E;De Masi G;de Pablos J L;De Temmerman G;De Tommasi G;de Vries P;Deakin K;Deane J;Agostini F Degli;Dejarnac R;Delabie E;den Harder N;Dendy R O;Denis J;Denner P;Devaux S;Devynck P;Di Maio F;Di Siena A;Di Troia C;Dinca P;D'Inca R;Ding B;Dittmar T;Doerk H;Doerner R P;Donne T;Dorling S E;DormidoCanto S;Doswon S;Douai D;Doyle P T;Drenik A;Drewelow P;Drews P;Duckworth Ph;Dumont R;Dumortier P;Dunai D;Dunne M;Duran I;Durodie F;Dutta P;Duval B P;Dux R;Dylst K;Dzysiuk N;Edappala P V;Edmond J;Edwards A M;Edwards J;Eich Th;Ekedahl A;ElJorf R;Elsmore C G;Enachescu M;Ericsson G;Eriksson F;Eriksson J;Eriksson L G;Esposito B;Esquembri S;Esser H G;Esteve D;Evans B;Evans G E;Evison G;Ewart G D;Fagan D;Faitsch M;Falie D;Fanni A;Fasoli A;Faustin J M;Fawlk N;Fazendeiro L;Fedorczak N;Felton R C;Fenton K;Fernades A;Fernandes H;Ferreira J;Fessey J A;Fevrier O;Ficker O;Field A;Fietz S;Figueiredo A;Figueiredo J;Fil A;Finburg P;Firdaouss M;Fischer U;Fittill L;Fitzgerald M;Flammini D;Flanagan J;Fleming C;Flinders K;Fonnesu N;Fontdecaba J M;Formisano A;Forsythe L;Fortuna L;FortunaZalesna E;Fortune M;Foster S;Franke T;Franklin T;Frasca M;Frassinetti L;Freisinger M;Fresa R;Frigione D;Fuchs V;Fuller D;Futatani S;Fyvie J;Gal K;Galassi D;Galazka K;GaldonQuiroga J;Gallagher J;Gallart D;Galvao R;Gao X;Gao Y;Garcia J;GarciaCarrasco A;GarciaMunoz M;Gardarein J L;Garzotti L;Gaudio P;Gauthier E;Gear D F;Gee S J;Geiger B;Gelfusa M;Gerasimov S;Gervasini G;Gethins M;Ghani Z;Ghate M;Gherendi M;Giacalone J C;Giacomelli L;Gibson C S;Giegerich T;Gil C;Gil L;Gilligan S;Gin D;Giovannozzi E;Girardo J B;Giroud C;Giruzzi G;Gloeggler S;Godwin J;Goff J;Gohil P;Goloborod'ko V;Gomes R;Goncalves B;Goniche M;Goodliffe M;Goodyear A;Gorini G;Gosk M;Goulding R;Goussarov A;Gowland R;Graham B;Graham M E;Graves J P;Grazier N;Grazier P;Green N R;Greuner H;Grierson B;Griph F S;Grisolia C;Grist D;Groth M;Grove R;Grundy C N;Grzonka J;Guard D;Guerard C;Guillemaut C;Guirlet R;Gurl C;Utoh H H;Hackett L J;Hacquin S;Hagar A;Hager R;Hakola A;Halitovs M;Hall S J;Cook S P Hallworth;HamlynHarris C;Hammond K;Harrington C;Harrison J;Harting D;Hasenbeck F;Hatano Y;Hatch D R;Haupt T D V;Hawes J;Hawkes N C;Hawkins J;Hawkins P;Haydon P W;Hayter N;Hazel S;Heesterman P J L;Heinola K;Hellesen C;Hellsten T;Helou W;Hemming O N;Hender T C;Henderson M;Henderson S S;Henriques R;Hepple D;Hermon G;Hertout P;Hidalgo C;Highcock E G;Hill M;Hillairet J;Hillesheim J;Hillis D;Hizanidis K;Hjalmarsson A;Hobirk J;Hodille E;Hogben C H A;Hogeweij G M D;Hollingsworth A;Hollis S;Homfray D A;Horacek J;Hornung G;Horton A R;Horton L D;Horvath L;Hotchin S P;Hough M R;Howarth P J;Hubbard A;Huber A;Huber V;Huddleston T M;Hughes M;Huijsmans G T A;Hunter C L;Huynh P;Hynes A M;Iglesias D;Imazawa N;Imbeaux F;Imrisek M;Incelli M;Innocente P;Irishkin M;IvanovaStanik I;Jachmich S;Jacobsen A S;Jacquet P;Jansons J;Jardin A;Jarvinen A;Jaulmes F;Jednorog S;Jenkins I;Jeong C;Jepu I;Joffrin E;Johnson R;Johnson T;Johnston Jane;Joita L;Jones G;Jones T T C;Hoshino K K;Kallenbach A;Kamiya K;Kaniewski J;Kantor A;Kappatou A;Karhunen J;Karkinsky D;Karnowska I;Kaufman M;Kaveney G;Kazakov Y;Kazantzidis V;Keeling D L;Keenan T;Keep J;Kempenaars M;Kennedy C;Kenny D;Kent J;Kent O N;Khilkevich E;Kim H T;Kim H S;Kinch A;King C;King D;King R F;Kinna D J;Kiptily V;Kirk A;Kirov K;Kirschner A;Kizane G;Klepper C;Klix A;Knight P;Knipe S J;Knott S;Kobuchi T;Koechl F;Kocsis G;Kodeli I;Kogan L;Kogut D;Koivuranta S;Kominis Y;Koeppen M;Kos B;Koskela T;Koslowski H R;Koubiti M;Kovari M;KowalskaStrzeciwilk E;Krasilnikov A;Krasilnikov V;Krawczyk N;Kresina M;Krieger K;Krivska A;Kruezi U;Ksiazek I;Kukushkin A;Kundu A;KurkiSuonio T;Kwak S;Kwiatkowski R;Kwon O J;Laguardia L;Lahtinen A;Laing A;Lam N;Lambertz H T;Lane C;Lang P T;Lanthaler S;Lapins J;Lasa A;Last J R;Laszynska E;Lawless R;Lawson A;Lawson K D;Lazaros A;Lazzaro E;Leddy J;Lee S;Lefebvre X;Leggate H J;Lehmann J;Lehnen M;Leichtle D;Leichuer P;Leipold F;Lengar I;Lennholm M;Lerche E;Lescinskis A;Lesnoj S;Letellier E;Leyland M;Leysen W;Li L;Liang Y;Likonen J;Linke J;Linsmeier Ch;Lipschultz B;Liu G;Liu Y;Lo Schiavo V P;Loarer T;Loarte A;Lobel R C;Lomanowski B;Lomas P J;Lonnroth J;Lopez J M;LopezRazola J;Lorenzini R;Losada U;Lovell J J;Loving A B;Lowry C;Luce T;Lucock R M A;Lukin A;Luna C;Lungaroni M;Lungu C P;Lungu M;Lunniss A;Lupelli I;Lyssoivan A;Macdonald N;Macheta P;Maczewa K;Magesh B;Maget P;Maggi C;Maier H;Mailloux J;Makkonen T;Makwana R;Malaquias A;Malizia A;Manas P;Manning A;Manso M E;Mantica P;Mantsinen M;Manzanares A;Maquet Ph;Marandet Y;Marcenko N;Marchetto C;Marchuk O;Marinelli M;Marinucci M;Markovic T;Marocco D;Marot L;Marren C A;Marshal R;Martin A;Martin Y;Martin de Aguilera A;Martinez F J;MartinSolis J R;Martynova Y;Maruyama S;Masiello A;Maslov M;Matejcik S;Mattei M;Matthews G F;Maviglia F;Mayer M;Mayoral M L;MaySmith T;Mazon D;Mazzotta C;McAdams R;McCarthy P J;McClements K G;McCormack O;McCullen P A;McDonald D;McIntosh S;McKean R;McKehon J;Meadows R C;Meakins A;Medina F;Medland M;Medley S;Meigh S;Meigs A G;Meisl G;Meitner S;Meneses L;Menmuir S;Mergia K;Merrigan I R;Mertens Ph;Meshchaninov S;Messiaen A;Meyer H;Mianowski S;Michling R;MiddletonGear D;Miettunen J;Militello F;MilitelloAsp E;Miloshevsky G;Mink F;Minucci S;Miyoshi Y;Mlynar J;Molina D;Monakhov I;Moneti M;Mooney R;Moradi S;Mordijck 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M;Wang E;Wang N;Warder S;Warren R J;Waterhouse J;Watkins N W;Watts C;Wauters T;Weckmann A;Weiland J;Weisen H;Weiszflog M;Wellstood C;West A T;Wheatley M R;Whetham S;Whitehead A M;Whitehead B D;Widdowson A M;Wiesen S;Wilkinson J;Williams J;Williams M;Wilson A R;Wilson D J;Wilson H R;Wilson J;Wischmeier M;Withenshaw G;Withycombe A;Witts D M;Wood D;Wood R;Woodley C;Wray S;Wright J;Wright J C;Wu J;Wukitch S;Wynn A;Xu T;Yadikin D;Yanling W;Yao L;Yavorskij V;Yoo M G;Young C;Young D;Young I D;Young R;Zacks J;Zagorski R;Zaitsev F S;Zanino R;Zarins A;Zastrow K D;Zerbini M;Zhang W;Zhou Y;Zilli E;Zoita V;Zoletnik S;Zychor I
2019
Abstract
A power-balance model, with radiation losses from impurities and neutrals, gives a unified description of the density limit (DL) of the stellarator, the L-mode tokamak, and the reversed field pinch (RFP). The model predicts a Sudo-like scaling for the stellarator, a Greenwald- like scaling, alpha I-p(8/9), for the RFP and the ohmic tokamak, a mixed scaling, alpha (PIp4/9)-I-4/9, for the additionally heated L-mode tokamak. In a previous paper (Zanca et al 2017 Nucl. Fusion 57 056010) the model was compared with ohmic tokamak, RFP and stellarator experiments. Here, we address the issue of the DL dependence on heating power in the L-mode tokamak. Experimental data from high-density disrupted L-mode discharges performed at JET, as well as in other machines, arc taken as a term of comparison. The model fits the observed maximum densities better than the pure Greenwald limit.
Istituto di fisica del plasma - IFP - Sede Milano Istituto gas ionizzati - IGI - Sede Padova Istituto dei Sistemi Complessi - ISC Istituto per la Scienza e Tecnologia dei Plasmi - ISTP
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/381247
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