Explaining the lack of power degradation of energy confinement in wide pedestal quiescent H-modes via transport modeling

Wide pedestal quiescent H (WPQH)-mode is an attractive scenario for future burning plasmas as they operate without ELMs. WPQH is characterized by formation of a wider and higher pedestal (than quiescent H-mode), and broadband fluctuations in the pedestal. Unlike conventional H-modes, where the energ...

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Veröffentlicht in:Nuclear fusion 2022-05, Vol.62 (5), p.56024
Hauptverfasser: Houshmandyar, Saeid, Burrell, K.H., Grierson, B.A., McClenaghan, J., Staebler, G.M., Chrystal, C., Halfmoon, M.R., Hatch, D.R., Zeng, L., Austin, M.E.
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Sprache:eng
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Zusammenfassung:Wide pedestal quiescent H (WPQH)-mode is an attractive scenario for future burning plasmas as they operate without ELMs. WPQH is characterized by formation of a wider and higher pedestal (than quiescent H-mode), and broadband fluctuations in the pedestal. Unlike conventional H-modes, where the energy confinement time reduces with increasing heating power, the WPQH plasmas reported in this paper do not show power degradation of the energy confinement. As the injected neutral beam power was increased, reduced core ( ρ ⩽ 0.45) transport calculated by transp , as well as increased core temperatures, pressure gradient and diamagnetic E × B shear rate were observed. The reduction in the heat transport and rapid decrease in the ion temperature gradient scale length suggest the formation of an ion internal transport barrier (ITB) that was accompanied by increased stored energy in the core. Quasilinear turbulent transport modeling using the trapped gyro Landau fluid ( tglf ) code was used to predict the ITB and its turbulence stability properties. By using profiles and equilibria produced by matching the transp transport fluxes with the tglf transport model within the tgyro transport solver, the energy confinement time captures the experimentally observed insensitivity to the increased P NBI . Linear stability analysis reveals that drift-wave instabilities in the core are stabilized by E × B shear, T i / T e ratio and Shafranov shift; the latter was found to have the strongest effect on the turbulence suppression at the highest heating level.
ISSN:0029-5515
1741-4326
DOI:10.1088/1741-4326/ac583b