2023
DOI: 10.1088/1361-6587/ad1654
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Initial Fulcher band observations from high resolution spectroscopy in the MAST-U divertor

N Osborne,
K Verhaegh,
M D Bowden
et al.

Abstract: High resolution D 2 ∗ Fulcher band spectroscopy was used in the MAST-U divertors during Super-X and… Show more

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Cited by 4 publications
(2 citation statements)
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“…Predictive SOLPS-ITER [9] simulations have shown that the characteristic extended SOL magnetic field paths and increased flux expansion-which lead to increased radiative cooling and increased plasma wetted area-of the Super-X divertor can drastically reduce exhaust particle and heat flux on divertor tiles [10][11][12]. Recent experimental results are in line with the SOLPS-ITER predictions, showing significantly reduced heat loading on the divertor target [13,14] and migration of hydrogenic [15,16] and impurity [16] radiation fronts upstream of the target. The Super-X divertor configuration also expands the parameter region in which stable diverted plasmas can be obtained [14,17], which could enable longer pulses and improved core confinement.…”
Section: Introductionmentioning
confidence: 58%
“…Predictive SOLPS-ITER [9] simulations have shown that the characteristic extended SOL magnetic field paths and increased flux expansion-which lead to increased radiative cooling and increased plasma wetted area-of the Super-X divertor can drastically reduce exhaust particle and heat flux on divertor tiles [10][11][12]. Recent experimental results are in line with the SOLPS-ITER predictions, showing significantly reduced heat loading on the divertor target [13,14] and migration of hydrogenic [15,16] and impurity [16] radiation fronts upstream of the target. The Super-X divertor configuration also expands the parameter region in which stable diverted plasmas can be obtained [14,17], which could enable longer pulses and improved core confinement.…”
Section: Introductionmentioning
confidence: 58%
“…where, I ki is the spectral intensity of the optical emission from the upper-level n = k to the lower-level n = i, λ ki is the wavelength of the spectral emission line, g k is the statistical weight of the upper level and A ki is the Einstein coefficient for spontaneous emission. The Q-branch of the Fulcher-α band for the hydrogen molecular is a suitable option for obtaining the rovibrational population due to its relatively strong spectral intensity and minimal perturbations [21,22]. The Q-branch comprises the rovibrational spectral transitions from the d 3 Π − u state to the a 3 Σ + g state.…”
Section: Diagnostic Results Of Oesmentioning
confidence: 99%