2023
DOI: 10.1088/1741-4326/ad0599
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How fluctuation intensity flux drives SOL expansion

Nami Li,
X.Q. Xu,
P.H. Diamond
et al.

Abstract: Predictions of heat load widths λ_q based on particle orbits alone are very pessimistic. This paper shows that pedestal peeling-ballooning (P-B) MHD turbulence broadens the stable SOL by the transport, or spreading, of fluctuation energy from the pedestal. λ_q is seen to increase with Γ_ε, the fluctuation energy density flux. We elucidate the fundamental physics of the spreading process. Γ_ε increases with pressure fluctuation correlation length. P-B turbulence is seen to be especially effective at spreading,… Show more

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Cited by 6 publications
(1 citation statement)
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“…The grassy-ELM λ js is larger than the inter large-ELM λ js is probably due to that the turbulence in pedestal is largely suppressed during the inter-ELM phase and strong turbulent fluctuations for the grassy-ELM pedestal enhance the cross-field transports of particles and heat into the SOL, which should broaden λ js in principle. This is supported by BOUT++ 3D turbulence simulations in the recent study [40]. To further confirm this theory, dedicated experiments with sufficient diagnostic measurements in the edge and SOL are required.…”
Section: Comparison Of the Sol Particle Flux Width For Different Elm ...mentioning
confidence: 58%
“…The grassy-ELM λ js is larger than the inter large-ELM λ js is probably due to that the turbulence in pedestal is largely suppressed during the inter-ELM phase and strong turbulent fluctuations for the grassy-ELM pedestal enhance the cross-field transports of particles and heat into the SOL, which should broaden λ js in principle. This is supported by BOUT++ 3D turbulence simulations in the recent study [40]. To further confirm this theory, dedicated experiments with sufficient diagnostic measurements in the edge and SOL are required.…”
Section: Comparison Of the Sol Particle Flux Width For Different Elm ...mentioning
confidence: 58%