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Numerical scan at constant β shows that core and scrape-off layer (SOL) radiations do not depend on the plasma current (Ip). Whereas the SOL radiation increases with seeding, the core radiation, however, does not continue to increase with seeding but rolls over at higher seeding rates in the simulations. The core plasma contamination by W ions is low, cW≪ 10−4. When the seeding starts, an increase in radiation power leading to a reduction in Ploss= (Paux− Prad) is observed, influencing the plasma confinement. The power scan at constant Ipindicates that the core radiation, Pplate, PSOL(and even SOL radiation), saturates with seeding. In addition, strong dilution with increasing seeding (Zeff≫ 3) and large W concentrations with increasing power are found. Comparing neon with nitrogen seeding, it is seen that neon leads to slightly larger total radiation than nitrogen. However, that is achieved with much higher plasma contamination (Zeff∼ 4–5) and dilution in the case of Ne, and simultaneously the power crossing the separatrix is lower for Ne than for N, indicating better H-mode performance in N2-seeded discharges.
Modelling of JET DT experiments in ILW configurations
Zagórski, R.;Czarnecka, A.;Ivanova-Stanik, I.;Challis, C.;X. Litaudon;S. Abduallev;M. Abhangi;P. Abreu;M. Afzal;K. M. Aggarwal;T. Ahlgren;J. H. Ahn;L. Aho-Mantila;N. Aiba;M. Airila;R. Albanese;V. Aldred;D. Alegre;E. Alessi;P. Aleynikov;A. Alfier;A. Alkseev;M. Allinson;B. Alper;E. Alves;G. Ambrosino;R. Ambrosino;L. Amicucci;V. Amosov;E. Andersson Sundén;M. Angelone;M. Anghel;C. Angioni;L. Appel;C. Appelbee;P. Arena;M. Ariola;H. Arnichand;S. Arshad;A. Ash;N. Ashikawa;V. Aslanyan;O. Asunta;F. Auriemma;Y. Austin;L. Avotina;M. D. Axton;C. Ayres;M. Bacharis;A. Baciero;D. Baião;S. Bailey;A. Baker;I. Balboa;M. Balden;N. Balshaw;R. Bament;J. W. Banks;Y. F. Baranov;M. A. Barnard;D. Barnes;M. Barnes;R. Barnsley;A. Baron Wiechec;L. Barrera Orte;M. Baruzzo;V. Basiuk;M. Bassan;R. Bastow;A. Batista;P. Batistoni;R. Baughan;B. Bauvir;L. Baylor;B. Bazylev;J. Beal;P. S. Beaumont;M. Beckers;B. Beckett;A. Becoulet;N. Bekris;M. Beldishevski;K. Bell;F. Belli;M. Bellinger;É. Belonohy;N. Ben Ayed;N. A. 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D. Young;R. Young;J. Zacks;R. Zagorski;F. S. Zaitsev;R. Zanino;A. Zarins;K. D. Zastrow;M. Zerbini;W. Zhang;Y. Zhou;E. Zilli;V. Zoita;S. Zoletnik;I. Zychor
2018-01-01
Abstract
Numerical scan at constant β shows that core and scrape-off layer (SOL) radiations do not depend on the plasma current (Ip). Whereas the SOL radiation increases with seeding, the core radiation, however, does not continue to increase with seeding but rolls over at higher seeding rates in the simulations. The core plasma contamination by W ions is low, cW≪ 10−4. When the seeding starts, an increase in radiation power leading to a reduction in Ploss= (Paux− Prad) is observed, influencing the plasma confinement. The power scan at constant Ipindicates that the core radiation, Pplate, PSOL(and even SOL radiation), saturates with seeding. In addition, strong dilution with increasing seeding (Zeff≫ 3) and large W concentrations with increasing power are found. Comparing neon with nitrogen seeding, it is seen that neon leads to slightly larger total radiation than nitrogen. However, that is achieved with much higher plasma contamination (Zeff∼ 4–5) and dilution in the case of Ne, and simultaneously the power crossing the separatrix is lower for Ne than for N, indicating better H-mode performance in N2-seeded discharges.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11563/134663
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simulazione ASN
Il report seguente simula gli indicatori relativi alla propria produzione scientifica in relazione alle soglie ASN 2023-2025 del proprio SC/SSD. Si ricorda che il superamento dei valori soglia (almeno 2 su 3) è requisito necessario ma non sufficiente al conseguimento dell'abilitazione. La simulazione si basa sui dati IRIS e sugli indicatori bibliometrici alla data indicata e non tiene conto di eventuali periodi di congedo obbligatorio, che in sede di domanda ASN danno diritto a incrementi percentuali dei valori. La simulazione può differire dall'esito di un’eventuale domanda ASN sia per errori di catalogazione e/o dati mancanti in IRIS, sia per la variabilità dei dati bibliometrici nel tempo. Si consideri che Anvur calcola i valori degli indicatori all'ultima data utile per la presentazione delle domande.
La presente simulazione è stata realizzata sulla base delle specifiche raccolte sul tavolo ER del Focus Group IRIS coordinato dall’Università di Modena e Reggio Emilia e delle regole riportate nel DM 589/2018 e allegata Tabella A. Cineca, l’Università di Modena e Reggio Emilia e il Focus Group IRIS non si assumono alcuna responsabilità in merito all’uso che il diretto interessato o terzi faranno della simulazione. Si specifica inoltre che la simulazione contiene calcoli effettuati con dati e algoritmi di pubblico dominio e deve quindi essere considerata come un mero ausilio al calcolo svolgibile manualmente o con strumenti equivalenti.