Nuclear Fushion,2022年
E. Militello Asp, G. Corrigan, P. da Silva Aresta Belo, L. Garzotti, D.M. Harting, F. Köchl, V. Parail, M. Cavinato, A. Loarte, M. Romanelli, R. Sartori
LicenseType:Unknown |
We have modelled self-consistently how to most efficiently fuel ITER hydrogen (H), helium (He) and deuterium–tritium (DT) plasmas with gas and/or pellets with the integrated core and 2D SOL/divertor suite of codes JINTRAC. This paper presents the first overview of full integrated simulations from core to divertor of ITER scenarios following their evolution fromX -point formation, through L-mode, L–H transition, steady-state H-mode, H–L transition and current ramp-down. Our simulations respect all ITER operational limits, maintaining the target power loads below 10 MW m−2 by timely gas fuelling or Ne seeding. For the pre-fusion plasma operation (PFPO) phase our aim was to develop robust scenarios and our simulations show that commissioning and operation of the ITER neutral beam (NB) to full power should be possible in 15 MA/5.3 T L-mode H plasmas with pellet fuelling and 20 MW of ECRH. For He plasmas gas fuelling alone allows access to H-mode at 7.5 MA/2.65 T with 53–73 MW of additional heating, since after application of NB and during the L–H transition, the modelled density build-up quickly reduces the NB shine-through losses to acceptable levels. This should allow the characterisation of ITER H-mode plasmas and the demonstration of ELM control schemes in PFPO-2. In ITER DT plasmas we varied the fuelling and heating schemes to achieve a target fusion gain ofQ= 10 and to exit the plasma from such conditions with acceptable divertor loads. The use of pellets in DT can provide a faster increase of the density in L-modes, but it is not essential for unrestricted NB operation due to the lower shine-through losses compared to H. During the H–L transition and current ramp-down, gas fuelling and Ne seeding are required to keep the divertor power loads under the engineering limits but accurate control over radiation is crucial to prevent the plasma becoming thermally unstable.
Nuclear Fushion,2022年
D. Alegre, S. Aleiferis, A. Aleksa, A.G. Alekseev, E. Alessi, P. Aleynikov, J. Algualcil, M. Ali, M. Allinson, B. Alper, E. Alves, G. Ambrosino, R. Ambrosino, V. Amosov, E.Andersson Sundén, P. Andrew, B.M. Angelini, C. Angioni, I. Antoniou, L.C. Appel, C. Appelbee, S. Aria, M. Ariola, G. Artaserse, W. Arter, V. Artigues, N. Asakura, A. Ash, N. Ashikawa, V. Aslanyan, M. Astrain, O. Asztalos, D. Auld, F. Auriemma, Y. Austin, L. Avotina, E. Aymerich, A. Lyssoivan, M. Machielsen, E. Macusova, R. Mäenpää, C.F. Maggi, R. Maggiora, M. Magness, S. Mahesan, H. Maier, R. Maingi, K. Malinowski, P. Manas, P. Mantica, M.J. Mantsinen, J. Manyer, A. Manzanares, Ph. Maquet, G. Marceca, N. Marcenko, C. Marchetto, O. Marchuk, A. Mariani, G. Mariano, M. Marin, M. Marinelli, T. Markovič, D. Marocco, L. Marot, S. Marsden, J. Marsh, R. Marshall, L. Martellucci, A. Martin, A.J. Martin, R. Martone, S. Maruyama, G. Ramogida, D. Rasmussen, J.J. Rasmussen, G. Rattá, S. Ratynskaia, M. Rebai, D. Réfy, R. Reichle, M. Reinke, D. Reiser, C. Reux, S. Reynolds, M.L. Richiusa, S. Richyal, D. Rigamonti, F.G. Rimini, J. Risner, M. Riva, J. Rivero-Rodriguez, C.M. Roach, R. Robins, S. Robinson, D. Robson, R. Rodionov, P. Rodrigues, M.Rodriguez Ramos, P. Rodriguez-Fernandez, F. Romanelli, M. Romanelli, S. Romanelli, J. Romazanov, R. Rossi, S. Rowe, D. Rowlands, M. Rubel, G. Rubinacci, G. Rubino, L. Ruchko, M. Ruiz, J.Ruiz Ruiz, C. Ruset, J. Rzadkiewicz, S. Saarelma, E. Safi, A. Sahlberg, M. Salewski, A. Salmi, R. Salmon, F. Salzedas, I. Sanders, D. Sandiford, B. Santos, A. Santucci, K. Särkimäki, R. Sarwar, I. Sarychev, O. Sauter, P. Sauwan, N. Scapin, F. Schluck, K. Schmid, S. Schmuck, M. Schneider, P.A. Schneider, D. Schwörer, G. Scott, M. Scott, D. Scraggs, S. Scully, M. Segato, Jaemin Seo, G. Sergienko, M. Sertoli, S.E. Sharapov, A. Shaw, H. Sheikh, U. Sheikh, A. Shepherd, A. Shevelev, P. Shigin, K. Shinohara, S. Shiraiwa, D. Shiraki, M. Short, G. Sias, S.A. Silburn, A. Silva, C. Silva, J. Silva, D. Silvagni, D. Simfukwe, J. Simpson, D. Sinclair, S.K. Sipilä, A.C.C. Sips, P. Sirén, A. Sirinelli, H. Sjöstrand, N. Skinner, J. Slater, N. Smith, P. Smith, J. Snell, G. Snoep, L. Snoj, P. Snyder, S. Soare, E.R. Solano, H.J. Sun, T.E. Susts, J. Svensson, J. Svoboda, R. Sweeney, D. Sytnykov, T. Szabolics, G. Szepesi, B. Tabia, T. Tadić, B. Tál, T. Tala, A. Tallargio, P. Tamain, H. Tan, K. Tanaka, W. Tang, M. Tardocchi, D. Taylor, A.S. Teimane, G. Telesca, N. Teplova, A. Teplukhina, D. Terentyev, A. Terra, D. Terranova, N. Terranova, D. Testa, E. Tholerus, J. Thomas, E. Thoren, A. Thorman, W. Tierens, R.A. Tinguely, A. Tipton, H. Todd, J. Mailloux, N. Abid, K. Abraham, P. Abreu, O. Adabonyan, P. Adrich, V. Afanasev, M. Afzal, T. Ahlgren, L. Aho-Mantila, N. Aiba, M. Airila, M. Akhtar, R. Albanese, M. Alderson-Martin, A. Baciero, F. Bairaktaris, J. Balbin, L. Balbinot, I. Balboa, M. Balden, C. Balshaw, N. Balshaw, V.K. Bandaru, J. Banks, Yu.F. Baranov, C. Barcellona, A. Barnard, M. Barnard, R. Barnsley, A. Barth, M. Baruzzo, S. Barwell, M. Bassan, A. Batista, P. Batistoni, L. Baumane, B. Bauvir, L. Baylor, P.S. Beaumont, D. Beckett, A. Begolli, M. Beidler, N. Bekris, M. Beldishevski, E. Belli, F. Belli, É. Belonohy, M. Ben Yaala, J. Benayas, J. Bentley, H. Bergsåker, J. Bernardo, M. Bernert, M. Berry, L. Bertalot, H. Betar, M. Beurskens, S. Bickerton, B. Bieg, J. Bielecki, A. Bierwage, T. Biewer, R. Bilato, P. Bílková, G. Birkenmeier, H. Bishop, J.P.S. Bizarro, J. Blackburn, P. Blanchard, P. Blatchford, V. Bobkov, A. Boboc, P. Bohm, T. Bohm, I. Bolshakova, T. Bolzonella, N. Bonanomi, D. Bonfiglio, X. Bonnin, P. Bonofiglo, S. Boocock, A. Booth, J. Booth, D. Borba, D. Borodin, I. Borodkina, C. Boulbe, C. Bourdelle, M. Bowden, K. Boyd, I.Božičević Mihalić, S.C. Bradnam, V. Braic, L. Brandt, R. Bravanec, B. Breizman, A. Brett, S. Brezinsek, M. Brix, K. Bromley, B. Brown, D. Brunetti, R. Buckingham, M. Buckley, R. Budny, J. Buermans, H. Bufferand, P. Buratti, A. Burgess, A. Buscarino, A. Busse, D. Butcher, E.de la Cal, G. Calabrò, L. Calacci, R. Calado, Y. Camenen, G. Canal, B. Cannas, M. Cappelli, S. Carcangiu, P. Card, A. Cardinali, P. Carman, D. Carnevale, M. Carr, D. Carralero, L. Carraro, I.S. Carvalho, P. Carvalho, I. Casiraghi, F.J. Casson, C. Castaldo, J.P. Catalan, N. Catarino, F. Causa, M. Cavedon, M. Cecconello, C.D. Challis, B. Chamberlain, C.S. Chang, A. Chankin, B. Chapman, M. Chernyshova, A. Chiariello, P. Chmielewski, A. Chomiczewska, L. Chone, G. Ciraolo, D. Ciric, J. Citrin, Ł. Ciupinski, M. Clark, R. Clarkson, C. Clements, M. Cleverly, J.P. Coad, P. Coates, A. Cobalt, V. Coccorese, R. Coelho, J.W. Coenen, I.H. Coffey, A. Colangeli, L. Colas, C. Collins, J. Collins, S. Collins, D. Conka, S. Conroy, B. Conway, N.J. Conway, D. Coombs, P. Cooper, S. Cooper, C. Corradino, G. Corrigan, D. Coster, P. Cox, T. Craciunescu, S. Cramp, C. Crapper, D. Craven, R. Craven, M.Crialesi Esposito, G. Croci, D. Croft, A. Croitoru, K. Crombé, T. Cronin, N. Cruz, C. Crystal, G. Cseh, A. Cufar, A. Cullen, M. Curuia, T. Czarski, H. Dabirikhah, A.Dal Molin, E. Dale, P. Dalgliesh, S. Dalley, J. Dankowski, P. David, A. Davies, S. Davies, G. Davis, K. Dawson, S. Dawson, I.E. Day, M. De Bock, G. De Temmerman, G. De Tommasi, K. Deakin, J. Deane, R. Dejarnac, D. Del Sarto, E. Delabie, D. Del-Castillo-Negrete, A. Dempsey, R.O. Dendy, P. Devynck, A. Di Siena, C. Di Troia, T. Dickson, P. Dinca, T. Dittmar, J. Dobrashian, R.P. Doerner, A.J.H. Donné, S. Dorling, S. Dormido-Canto, D. Douai, S. Dowson, R. Doyle, M. Dreval, P. Drewelow, P. Drews, G. Drummond, Ph. Duckworth, H. Dudding, R. Dumont, P. Dumortier, D. Dunai, T. Dunatov, M. Dunne, I. Ďuran, F. Durodié, R. Dux, A. Dvornova, R. Eastham, J. Edwards, Th. Eich, A. Eichorn, N. Eidietis, A. Eksaeva, H. El Haroun, G. Ellwood, C. Elsmore, O. Embreus, S. Emery, G. Ericsson, B. Eriksson, F. Eriksson, J. Eriksson, L.G. Eriksson, S. Ertmer, S. Esquembri, A.L. Esquisabel, T. Estrada, G. Evans, S. Evans, E. Fable, D. Fagan, M. Faitsch, M. Falessi, A. Fanni, A. Farahani, I. Farquhar, A. Fasoli, B. Faugeras, S. Fazinić, F. Felici, R. Felton, A. Fernandes, H. Fernandes, J. Ferrand, D.R. Ferreira, J. Ferreira, G. Ferrò, J. Fessey, O. Ficker, A.R. Field, A. Figueiredo, J. Figueiredo, A. Fil, N. Fil, P. Finburg, D. Fiorucci, U. Fischer, G. Fishpool, L. Fittill, M. Fitzgerald, D. Flammini, J. Flanagan, K. Flinders, S. Foley, N. Fonnesu, M. Fontana, J.M. Fontdecaba, S. Forbes, A. Formisano, T. Fornal, L. Fortuna, E. Fortuna-Zalesna, M. Fortune, C. Fowler, E. Fransson, L. Frassinetti, M. Freisinger, R. Fresa, R. Fridström, D. Frigione, T. Fülöp, M. Furseman, V. Fusco, S. Futatani, D. Gadariya, K. Gál, D. Galassi, K. Gałązka, S. Galeani, D. Gallart, R. Galvão, Y. Gao, J. Garcia, M. García-Muñoz, M. Gardener, L. Garzotti, J. Gaspar, R. Gatto, P. Gaudio, D. Gear, T. Gebhart, S. Gee, M. Gelfusa, R. George, S.N. Gerasimov, G. Gervasini, M. Gethins, Z. Ghani, M. Gherendi, F. Ghezzi, J.C. Giacalone, L. Giacomelli, G. Giacometti, C. Gibson, K.J. Gibson, L. Gil, A. Gillgren, D. Gin, E. Giovannozzi, C. Giroud, R. Glen, S. Glöggler, J. Goff, P. Gohil, V. Goloborodko, R. Gomes, B. Gonçalves, M. Goniche, A. Goodyear, S. Gore, G. Gorini, T. Görler, N. Gotts, R. Goulding, E. Gow, B. Graham, J.P. Graves, H. Greuner, B. Grierson, J. Griffiths, S. Griph, D. Grist, W. Gromelski, M. Groth, R. Grove, M. Gruca, D. Guard, N. Gupta, C. Gurl, A. Gusarov, L. Hackett, S. Hacquin, R. Hager, L. Hägg, A. Hakola, M. Halitovs, S. Hall, S.A. Hall, S. Hallworth-Cook, C.J. Ham, D. Hamaguchi, M. Hamed, C. Hamlyn-Harris, K. Hammond, E. Harford, J.R. Harrison, D. Harting, Y. Hatano, D.R. Hatch, T. Haupt, J. Hawes, N.C. Hawkes, J. Hawkins, T. Hayashi, S. Hazael, S. Hazel, P. Heesterman, B. Heidbrink, W. Helou, O. Hemming, S.S. Henderson, R.B. Henriques, D. Hepple, J. Herfindal, G. Hermon, J. Hill, J.C. Hillesheim, K. Hizanidis, A. Hjalmarsson, A. Ho, J. Hobirk, O. Hoenen, C. Hogben, A. Hollingsworth, S. Hollis, E. Hollmann, M. Hölzl, B. Homan, M. Hook, D. Hopley, J. Horáček, D. Horsley, N. Horsten, A. Horton, L.D. Horton, L. Horvath, S. Hotchin, R. Howell, Z. Hu, A. Huber, V. Huber, T. Huddleston, G.T.A. Huijsmans, P. Huynh, A. Hynes, M. Iliasova, D. Imrie, M. Imríšek, J. Ingleby, P. Innocente, K. Insulander Björk, N. Isernia, I. Ivanova-Stanik, E. Ivings, S. Jablonski, S. Jachmich, T. Jackson, P. Jacquet, H. Järleblad, F. Jaulmes, J.Jenaro Rodriguez, I. Jepu, E. Joffrin, R. Johnson, T. Johnson, J. Johnston, C. Jones, G. Jones, L. Jones, N. Jones, T. Jones, A. Joyce, R. Juarez, M. Juvonen, P. Kalniņa, T. Kaltiaisenaho, J. Kaniewski, A. Kantor, A. Kappatou, J. Karhunen, D. Karkinsky, Yu Kashchuk, M. Kaufman, G. Kaveney, Ye.O. Kazakov, V. Kazantzidis, D.L. Keeling, R. Kelly, M. Kempenaars, C. Kennedy, D. Kennedy, J. Kent, K. Khan, E. Khilkevich, C. Kiefer, J. Kilpeläinen, C. Kim, Hyun-Tae Kim, S.H. Kim, D.B. King, R. King, D. Kinna, V.G. Kiptily, A. Kirjasuo, K.K. Kirov, A. Kirschner, T. kiviniemi, G. Kizane, M. Klas, C. Klepper, A. Klix, G. Kneale, M. Knight, P. Knight, R. Knights, S. Knipe, M. Knolker, S. Knott, M. Kocan, F. Köchl, I. Kodeli, Y. Kolesnichenko, Y. Kominis, M. Kong, V. Korovin, B. Kos, D. Kos, H.R. Koslowski, M. Kotschenreuther, M. Koubiti, E. Kowalska-Strzęciwilk, K. Koziol, A. Krasilnikov, V. Krasilnikov, M. Kresina, K. Krieger, N. Krishnan, A. Krivska, U. Kruezi, I. Książek, A.B. Kukushkin, H. Kumpulainen, T. Kurki-Suonio, H. Kurotaki, S. Kwak, O.J. Kwon, L. Laguardia, E. Lagzdina, A. Lahtinen, A. Laing, N. Lam, H.T. Lambertz, B. Lane, C. Lane, E.Lascas Neto, E. Łaszyńska, K.D. Lawson, A. Lazaros, E. Lazzaro, G. Learoyd, Chanyoung Lee, S.E. Lee, S. Leerink, T. Leeson, X. Lefebvre, H.J. Leggate, J. Lehmann, M. Lehnen, D. Leichtle, F. Leipold, I. Lengar, M. Lennholm, E. Leon Gutierrez, B. Lepiavko, J. Leppänen, E. Lerche, A. Lescinskis, J. Lewis, W. Leysen, L. Li, Y. Li, J. Likonen, Ch. Linsmeier, B. Lipschultz, X. Litaudon, E. Litherland-Smith, F. Liu, T. Loarer, A. Loarte, R. Lobel, B. Lomanowski, P.J. Lomas, J.M. López, R. Lorenzini, S. Loreti, U. Losada, V.P. Loschiavo, M. Loughlin, Z. Louka, J. Lovell, T. Lowe, C. Lowry, S. Lubbad, T. Luce, R. Lucock, A. Lukin, C. Luna, E.de la Luna, M. Lungaroni, C.P. Lungu, T. Lunt, V. Lutsenko, B. Lyons, M. Maslov, S. Masuzaki, S. Matejcik, M. Mattei, G.F. Matthews, D. Matveev, E. Matveeva, A. Mauriya, F. Maviglia, M. Mayer, M.-L. Mayoral, S. Mazzi, C. Mazzotta, R. McAdams, P.J. McCarthy, K.G. McClements, J. McClenaghan, P. McCullen, D.C. McDonald, D. McGuckin, D. McHugh, G. McIntyre, R. McKean, J. McKehon, B. McMillan, L. McNamee, A. McShee, A. Meakins, S. Medley, C.J. Meekes, K. Meghani, A.G. Meigs, G. Meisl, S. Meitner, S. Menmuir, K. Mergia, S. Merriman, Ph. Mertens, S. Meshchaninov, A. Messiaen, R. Michling, P. Middleton, D. Middleton-Gear, J. Mietelski, D. Milanesio, E. Milani, F. Militello, A.Militello Asp, J. Milnes, A. Milocco, G. Miloshevsky, C. Minghao, S. Minucci, I. Miron, M. Miyamoto, J. Mlynář, V. Moiseenko, P. Monaghan, I. Monakhov, T. Moody, S. Moon, R. Mooney, S. Moradi, J. Morales, R.B. Morales, S. Mordijck, L. Moreira, L. Morgan, F. Moro, J. Morris, K.-M. Morrison, L. Msero, D. Moulton, T. Mrowetz, T. Mundy, M. Muraglia, A. Murari, A. Muraro, N. Muthusonai, B. N’Konga, Yong-Su Na, F. Nabais, M. Naden, J. Naish, R. Naish, F. Napoli, E. Nardon, V. Naulin, M.F.F. Nave, I. Nedzelskiy, G. Nemtsev, V. Nesenevich, I. Nestoras, R. Neu, V.S. Neverov, S. Ng, M. Nicassio, A.H. Nielsen, D. Nina, D. Nishijima, C. Noble, C.R. Nobs, M. Nocente, D. Nodwell, K. Nordlund, H. Nordman, R. Normanton, J.M. Noterdaeme, S. Nowak, E. Nunn, H. Nyström, M. Oberparleiter, B. Obryk, J. O'Callaghan, T. Odupitan, H.J.C. Oliver, R. Olney, M. O’Mullane, J. Ongena, E. Organ, F. Orsitto, J. Orszagh, T. Osborne, R. Otin, T. Otsuka, A. Owen, Y. Oya, M. Oyaizu, R. Paccagnella, N. Pace, L.W. Packer, S. Paige, E. Pajuste, D. Palade, S.J.P. Pamela, N. Panadero, E. Panontin, A. Papadopoulos, G. Papp, P. Papp, V.V. Parail, C. Pardanaud, J. Parisi, F.Parra Diaz, A. Parsloe, M. Parsons, N. Parsons, M. Passeri, A. Patel, A. Pau, G. Pautasso, R. Pavlichenko, A. Pavone, E. Pawelec, C.Paz Soldan, A. Peacock, M. Pearce, E. Peluso, C. Penot, K. Pepperell, R. Pereira, T. Pereira, E.Perelli Cippo, P. Pereslavtsev, C. Perez von Thun, V. Pericoli, D. Perry, M. Peterka, P. Petersson, G. Petravich, N. Petrella, M. Peyman, M. Pillon, S. Pinches, G. Pintsuk, W. Pires de Sá, A. Pires dos Reis, C. Piron, L. Pionr, A. Pironti, R. Pitts, K.L. van de Plassche, N. Platt, V. Plyusnin, M. Podesta, G. Pokol, F.M. Poli, O.G. Pompilian, S. Popovichev, M. Poradziński, M.T. Porfiri, M. Porkolab, C. Porosnicu, M. Porton, G. Poulipoulis, I. Predebon, G. Prestopino, C. Price, D. Price, M. Price, D. Primetzhofer, P. Prior, G. Provatas, G. Pucella, P. Puglia, K. Purahoo, I. Pusztai, O. Putignano, T. Pütterich, A. Quercia, E. Rachlew, G. Radulescu, V. Radulovic, M. Rainford, P. Raj, G. Ralph, V. Solokha, A. Somers, C. Sommariva, K. Soni, E. Sorokovoy, M. Sos, J. Sousa, C. Sozzi, S. Spagnolo, T. Spelzini, F. Spineanu, D. Spong, D. Sprada, S. Sridhar, C. Srinivasan, G. Stables, G. Staebler, I. Stamatelatos, Z. Stancar, P. Staniec, G. Stankūnas, M. Stead, E. Stefanikova, A. Stephen, J. Stephens, P. Stevenson, M. Stojanov, P. Strand, H.R. Strauss, S. Strikwerda, P. Ström, C.I. Stuart, W. Studholme, M. Subramani, E. Suchkov, S. Sumida, M. Tokitani, P. Tolias, M. Tomeš, A. Tookey, Y. Torikai, U. von Toussaint, P. Tsavalas, D. Tskhakaya, I. Turner, M. Turner, M.M. Turner, M. Turnyanskiy, G. Tvalashvili, S. Tyrrell, M. Tyshchenko, A. Uccello, V. Udintsev, G. Urbanczyk, A. Vadgama, D. Valcarcel, M. Valisa, P.Vallejos Olivares, O. Vallhagen, M. Valovič, D. Van Eester, J. Varje, S. Vartanian, T. Vasilopoulou, G. Vayakis, M. Vecsei, J. Vega, S. Ventre, G. Verdoolaege, C. Verona, G.Verona Rinati, E. Veshchev, N. Vianello, E. Viezzer, L. Vignitchouk, R. Vila, R. Villari, F. Villone, P. Vincenzi, I. Vinyar, B. Viola, A.J. Virtanen, A. Vitins, Z. Vizvary, G. Vlad, M. Vlad, P. Vondráček, P.de Vries, B. Wakeling, N.R. Walkden, M. Walker, R. Walker, M. Walsh, E. Wang, N. Wang, S. Warder, R. Warren, J. Waterhouse, C. Watts, T. Wauters, A. Weckmann, H.Wedderburn Maxwell, M. Weiland, H. Weisen, M. Weiszflog, P. Welch, N. Wendler, A. West, M. Wheatley, S. Wheeler, A. Whitehead, D. Whittaker, A. Widdowson, S. Wiesen, J. Wilkinson, J.C. Williams, D. Willoughby, I. Wilson, J. Wilson, T. Wilson, M. Wischmeier, P. Wise, G. Withenshaw, A. Withycombe, D. Witts, A. Wojcik-Gargula, E. Wolfrum, R. Wood, C. Woodley, R. Woodley, B. Woods, J. Wright, J.C. Wright, T. Xu, D. Yadikin, M. Yajima, Y. Yakovenko, Y. Yang, W. Yanling, V. Yanovskiy, I. Young, R. Young, R.J. Zabolockis, J. Zacks, R. Zagorski, F.S. Zaitsev, L. Zakharov, A. Zarins, D. Zarzoso Fernandez, K.-D. Zastrow, Y. Zayachuk, M. Zerbini, W. Zhang, Y. Zhou, M. Zlobinski, A. Zocco, A. Zohar, V. Zoita, S. Zoletnik, V.K. Zotta, I. Zoulias, W. Zwingmann, I. Zychor
LicenseType:Unknown |
The JET 2019–2020 scientific and technological programme exploited the results of years of concerted scientific and engineering work, including the ITER-like wall (ILW: Be wall and W divertor) installed in 2010, improved diagnostic capabilities now fully available, a major neutral beam injection upgrade providing record power in 2019–2020, and tested the technical and procedural preparation for safe operation with tritium. Research along three complementary axes yielded a wealth of new results. Firstly, the JET plasma programme delivered scenarios suitable for high fusion power and alpha particle ( α ) physics in the coming D–T campaign (DTE2), with record sustained neutron rates, as well as plasmas for clarifying the impact of isotope mass on plasma core, edge and plasma-wall interactions, and for ITER pre-fusion power operation. The efficacy of the newly installed shattered pellet injector for mitigating disruption forces and runaway electrons was demonstrated. Secondly, research on the consequences of long-term exposure to JET-ILW plasma was completed, with emphasis on wall damage and fuel retention, and with analyses of wall materials and dust particles that will help validate assumptions and codes for design and operation of ITER and DEMO. Thirdly, the nuclear technology programme aiming to deliver maximum technological return from operations in D, T and D–T benefited from the highest D–D neutron yield in years, securing results for validating radiation transport and activation codes, and nuclear data for ITER.
Nuclear Fushion,2022年
F.J. Artola, A. Loarte, M. Hoelzl, M. Lehnen, N. Schwarz
LicenseType:Unknown |
Non-axisymmetric simulations of the current quench phase of ITER disruptions are key to predict asymmetric forces acting into the ITER wall. We present for the first time such simulations for ITER mitigated disruptions at realistic Lundquist numbers. For these strongly mitigated disruptions, we find that the safety factor remains above 2 and the maximal integral horizontal forces remain below 1 MN. The maximal integral vertical force is found to be 13 MN and arises in a time scale given by the resistive wall time as expected from theoretical considerations. In this respect, the vertical force arises after the plasma current has completely decayed, showing the importance of continuing the simulations also in the absence of plasma current. We conclude that the horizontal wall force rotation is not a concern for these strongly mitigated disruptions in ITER, since when the wall forces form, there are no remaining sources of rotation.
Nuclear Fushion,2022年
J. Adamek, F.J. Artola, A. Loarte, E. Matveeva, J. Cavalier, R.A. Pitts, R. Roccella, M. Lehnen, J. Havlicek, M. Hron, R. Panek
LicenseType:Unknown |
The presented experimental study realized in the COMPASS tokamak demonstrates, for the first time, that the current density that flows from the plasma into the vacuum vessel during disruptions is limited by the ion particle flux. Such a limitation shows that, at least in COMPASS, the sheath that forms between the plasma and the first wall dominates the halo current flow. This observation is achieved by measuring simultaneously the ion saturation current with negatively biased Langmuir probes and the halo current with grounded probes to the vacuum vessel. These comparative measurements, which were never performed during disruptions in other machines, directly confirm that the halo current density remains below the ion particle flux in COMPASS. The study also shows, using Mirnov coils measurement, that the total electric current entering the wall grows with the plasma current while the current density obtained by Langmuir probes remains unaffected. This, together with the current density limitation, leads to a novel finding that the halo current width increases with the pre-disruptive plasma current, which limits the local forces. The new findings reported here could also provide potential constraints on the modeling of disruption-induced loads on future reactor scale tokamaks and motivation for further experiments on existing devices.
Nuclear Fushion,2022年
J.R. Martín-Solís, J.A. Mier, M. Lehnen, A. Loarte
LicenseType:Unknown |
A simple 0D model which mimics the plasma surrounded by the conducting structures (Kiramov and Breizman 2017Phys. Plasmas24100702) and including self-consistently the vertical plasma motion and the generation of runaway electrons during the disruption is used for an assessment of the effect of vertical displacement events on the runaway current formation and termination. The total plasma current and runaway current at the time the plasma hits the wall is estimated and the effect of injecting impurities into the plasma is evaluated. In the case of ITER, with a highly conducting wall, although the total plasma current when the plasma touches the wall is the same for any number of injected impurities, however the fraction of the plasma current carried by runaway electrons can significantly decrease for large enough amounts of impurities. The plasma velocity is larger and the time when the plasma hits the wall shorter for lower runaway currents, which are obtained when larger amounts of impurities are injected. When the plasma reaches the wall, the scraping-off of the runaway beam occurs and the current is terminated. During this phase, the plasma vertical displacement velocity and electric field can substantially increase leading to the deposition of a noticeable amount of energy on the runaway electrons (∼hundreds of MJ). It is found that an early second impurity injection reduces somewhat the amount of energy deposited by the runaways. Also larger temperatures of the companion plasma during the scraping-off might be efficient in reducing the power fluxes due to the runaways onto the PFCs. The plasma reaches theq a = 2 limit before the runaway electron current is terminated and by that time the amount of energy deposited on the runaway electrons can be substantially lower than that expected until the beam is fully terminated. Negligible additional conversion of magnetic into runaway kinetic energy is predicted during the runaway deconfinement following the large magnetic fluctuations afterq a = 2 is crossed for characteristic deconfinement times lower than 0.1 ms which is a characteristic timescale for ideal MHD instabilities to develop.
6 LOCUST-GPU predictions of fast-ion transport and power loads due to ELM-control coils in ITER [期刊论文]
Nuclear Fushion,2022年
S.H. Ward, R. Akers, L. Li, Y.Q. Liu, A. Loarte, S.D. Pinches, A. R. Polevoi, R.G.L. Vann, M.A. Van Zeeland
LicenseType:Unknown |
The graphics processing unit (GPU) version of the Lorentz-orbit code for use in stellarators and tokamaks ( LOCUST ) has been applied to study the fast-ion transport and loss caused by resonant magnetic perturbations in the high-performanceQ= 10 ITER baseline scenario. The unique computational efficiency of the code is exploited to calculate the impact of the application of ITER's edge-localised mode (ELM) control coil system on neutral beam heating efficiency, as well as producing detailed predictions of the resulting plasma-facing component power loads, for a variety of operational parameters—the applied fundamental toroidal mode numbern 0, mode spectrum and absolute toroidal phase of the imposed perturbation. The feasibility of continually rotating the perturbations is assessed and shown to be effective at reducing the time-averaged power loads. Through careful adjustment of the relative phase of the applied perturbation in the three rows of coils, peak power loads are found to correlate with reductions in neutral beam injection (NBI) heating efficiency forn 0 = 3 fields. Adjusting the phase this way can increase total NBI system efficiency by approximately 2%–3% and reduce peak power loads by up to 0.43 MW m−2. From the point of view of fast-ion confinement,n 0 = 3 ELM control fields are preferred overall ton 0 = 4 fields. In addition, the implementation of 3D magnetic fields inLOCUSTis also verified by comparison with theSPIRALcode for a DIII-D discharge with ITER-similar shaping andn 0 = 3 perturbation.