2021
DOI: 10.1088/1741-4326/abea56
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Measurements and modelling of diamagnetic flux in ASDEX Upgrade

Abstract: The reproducibility of diamagnetic flux measurements in vacuum field shots for the internal and external diamagnetic flux measurements in the ASDEX Upgrade tokamak is investigated. A comparison of diamagnetic flux measurements and predictions from equilibrium reconstruction, including pressure constraints from thermal and fast-ion contributions, is reported. The ideal magnetohydrodynamic model involved in interpreting diamagnetic flux measurements in a tokamak with anisotropic pressure is summarised. The plasm… Show more

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Cited by 8 publications
(5 citation statements)
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“…The diamagnetic energy is calculated as part of the equilibrium reconstruction with EFIT++. W dia is not output by TRANSP by default and is derived from the computed thermal W th and fast ion perpendicular W f⊥ energy components as W dia = W th + 1.5 W f⊥ [63].…”
Section: Consistency Checksmentioning
confidence: 99%
“…The diamagnetic energy is calculated as part of the equilibrium reconstruction with EFIT++. W dia is not output by TRANSP by default and is derived from the computed thermal W th and fast ion perpendicular W f⊥ energy components as W dia = W th + 1.5 W f⊥ [63].…”
Section: Consistency Checksmentioning
confidence: 99%
“…The main reason the absorbed NBI power is significantly below the nominal power are FI prompt losses, which are significant when counter-injection beams are used, as is the case here. Hence, while the total heating power is increased by 43% by the addition of NBI (from 7 MW to 10 MW), the plasma energy, as calculated by the integrated data analysis (IDA) for equilibrium reconstruction [32,33] and measured via the diamagnetic loop [34], increases only by about 23% (0.26 MJ to 0.32 MJ). This hints to increased transport (worse confinement) at increasing heating powers, which is usually referred to as power degradation, a common observation in both tokamaks and stellarators [35][36][37][38].…”
Section: Negative Triangulariy Plasmas In Asdex Upgradementioning
confidence: 99%
“…The measured neutron emission rate signal (blue) approaches the classical neutron rate (TRANSP) when the TAEs are mitigated and suppressed after t ∼ 5.4 s. Also, the stored energy rises significantly and the difference between W DIA and W MHD increases while the TAEs are stabilized. This discrepancy with the condition of W MHD > W DIA indicates the beam-ion stored energy increases [51] since the beam-injection geometry of KSTAR is mainly parallel.…”
Section: Change In Spectral and Kinetic Profilesmentioning
confidence: 74%
“…Stored energy (W DIA ) is measured by the diamagnetic loop [50] and compared with the calculated energy (W MHD ) from the equilibrium reconstruction. In particular, as the geometry of NBI in KSTAR is mainly parallel, the parallel fast-ion energy produced by the parallel beam injection has a significant contribution to the W MHD when the beam-ion confinement is enhanced [51].…”
Section: Heating Current Drive and Diagnosticsmentioning
confidence: 99%