MHD simulations of small ELMs at low triangularity in ASDEX Upgrade

A. Cathey (Corresponding author), M. Hoelzl, G. Harrer, M.G. Dunne, G.T.A. Huijsmans, K. Lackner, S.J.P. Pamela, E. Wolfrum, S. Günter, JOREK team

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Samenvatting

The development of small and no-ELM regimes for ITER is a high priority topic due to the risks associated with type-I ELMs. By considering non-linear extended magnetohydrodynamic (MHD) simulations of the ASDEX Upgrade tokamak with the JOREK code, we probe a regime that avoids type-I ELMs completely, provided that the separatrix density is high enough. The dynamics of the pedestal in this regime are observed to be qualitatively similar to the so-called quasi-continuous exhaust regime in several ways. Repetitive type-I ELMs are substituted by roughly constant levels of outward transport, caused by peeling-ballooning modes (with dominant ballooning characteristics) which are localised in the last 5% of the confined region (in normalised poloidal flux). The simulated low triangularity plasma transitions to a type-I ELMy H-mode if the separatrix density is sufficiently reduced or if the input heating power is sufficiently increased. The stabilising factors that play a role in the suppression of the small ELMs are also investigated by analysing the simulations, and the importance of including diamagnetic effects in the simulations is highlighted. By considering a scan in the pedestal resistivity and by comparing the poloidal velocity of the modes to theoretical estimates for ideal and resistive modes, we identify the underlying instabilities as resistive peeling-ballooning modes. Decreasing the resistivity below experimentally-relevant conditions (i.e. going towards ideal MHD), the peeling-ballooning modes that constrain the pedestal below the type-I ELM stability boundary display sharply decreasing growth rates.

Originele taal-2Engels
Artikelnummer054011
Aantal pagina's15
TijdschriftPlasma Physics and Controlled Fusion
Volume64
Nummer van het tijdschrift5
DOI's
StatusGepubliceerd - 13 apr. 2022

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© 2022 Max-Planck-Institut fur Plasmaphysik.

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