Pith. sign in

REVIEW

Gyrokinetic simulations of the effects of magnetic islands on microturbulence in KSTAR

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2412.09522 v2 pith:Z5S6GKTR submitted 2024-12-12 physics.plasm-ph

classification physics.plasm-ph
keywords transportmagneticsimulationsislandskstardirectioneffectsflows
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Gyrokinetic simulations are utilized to study effects of magnetic islands on the ion temperature gradient (ITG) turbulence in the KSTAR tokamak with resonant magnetic perturbations. Simulations show that the transport is controlled by the nonlinear interactions between the ITG turbulence and self-generated vortex flows and zonal flows, leading to an anisotropic structure of fluctuation and transport on the poloidal plane and in the toroidal direction. Magnetic islands greatly enhance turbulent transport of both particle and heat. The turbulent transport exhibits variations in the toroidal direction, with transport through the resonant layer near the island X-point being enhanced when the X-point is located at the outer mid-plane. A quantitative agreement is shown between simulations and KSTAR experiments in terms of time frequency and perpendicular wavevector spectrum.

Discussion (0). Continue with ORCID to comment.

Pith tools