2014
DOI: 10.1088/0029-5515/54/3/033002
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On the challenge of plasma heating with the JET metallic wall

Abstract: The major aspects linked to the use of the JET auxiliary heating systems: NBI, ICRF and LHCD, in the new JET ITER-like wall (JET-ILW) are presented. We show that although there were issues related to the operation of each system, efficient and safe plasma heating was obtained with room for higher power. For the NBI up to 25.7MW was safely injected; issues that had to be tackled were mainly the beam shine-through and beam re-ionisation before its entrance into the plasma. For the ICRF system, 5MW were coupled i… Show more

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Cited by 21 publications
(25 citation statements)
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“…1 in Refs. [28] and [29], respectively) have been modelled in detail in BBNBI as described in Sec. 2.1.…”
Section: Comparisons Against Established Nbi Codesmentioning
confidence: 99%
“…1 in Refs. [28] and [29], respectively) have been modelled in detail in BBNBI as described in Sec. 2.1.…”
Section: Comparisons Against Established Nbi Codesmentioning
confidence: 99%
“…It is essential to adapt the heating systems to the WEST configuration, and also to verify the adequacy of these heating schemes with H-mode operation in terms of power coupling, fast particle confinement and ELM resilience in a metallic environment. It will complement active efforts carried out in metallic environments on JET-ILW [13], ASDEX Upgrade [14,15], Alcator C-Mod [16] and FTU [17].…”
Section: High Frequency Plasma Heatingmentioning
confidence: 85%
“…The ideal MHD stability limit in the WEST scenarios studied has been calculated using the linear MHD code MISHKA [13]. The pedestal width is assumed to be around 5% of the minor radius such that ped = 2.3 cm.…”
Section: L-h Power Threshold Pedestal and Elmsmentioning
confidence: 99%
“…At present, numerous codes 35,36 are capable of iterating between the first two, mostly considering an isotropic background equilibrium and ignoring finite orbit e ects, although significant e orts to circumvent these limitations have recently been developed 37 . The most di cult challenges that remain in simulating ICRH in tokamaks and stellarators relate to the coupling between the antenna and the edge plasma, which involves strongly nonlinear e ects associated with the large radiofrequency (RF) voltages (tens of kilovolts) present at the antenna surface, and the turbulent nature of the edge-plasma region 38 . This coupling strongly influences not only the e ectiveness of the heating, but also the integrity of the antenna, which is subject to electrical arcs and ion bombardment due to the rectification of the RF voltage in the plasma sheath close to the antenna, and can strongly modify the properties of the edge plasma.…”
Section: Heating and Current Drive By Wavesmentioning
confidence: 99%