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research article

Modelling of JET DT experiments in ILW configurations

Zagorski, R.
•
Czarnecka, A.
•
Ivanova-Stanik, I.
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July 1, 2018
Contributions To Plasma Physics

Numerical scan at constant shows that core and scrape-off layer (SOL) radiations do not depend on the plasma current (I-p). 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, c(W) << 10(-4). When the seeding starts, an increase in radiation power leading to a reduction in P-loss = (P-aux - P-rad) is observed, influencing the plasma confinement. The power scan at constant I-p indicates that the core radiation, P-plate, P-SOL (and even SOL radiation), saturates with seeding. In addition, strong dilution with increasing seeding (Z(eff) >> 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 (Z(eff) approximate to 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 N-2-seeded discharges.

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Type
research article
DOI
10.1002/ctpp.201700118
Web of Science ID

WOS:000443937100045

Author(s)
Zagorski, R.
Czarnecka, A.
Ivanova-Stanik, I.
Challis, C.
Abduallev, S.
Abhangi, M.
Abreu, P.
Afzal, M.
Aggarwal, K. M.
Ahlgren, T.
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Date Issued

2018-07-01

Published in
Contributions To Plasma Physics
Volume

58

Issue

6-8

Start page

739

End page

745

Subjects

Physics, Fluids & Plasmas

•

Physics

•

core plasma

•

edge plasma

•

integrated modelling

•

jet seeding discharges

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h-mode

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discharges

•

tritium

Note

16th International Workshop on Plasma Edge Theory in Fusion Devices (PET), Sep 27-29, 2017, Marseille, FRANCE

Editorial or Peer reviewed

REVIEWED

Written at

EPFL

EPFL units
SPC  
Available on Infoscience
September 20, 2019
Use this identifier to reference this record
https://infoscience.epfl.ch/handle/20.500.14299/161376
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