First achievement of high poloidal beta scenario with KSTAR-like constraints on DIII-D
ORAL
Abstract
The high poloidal beta (βP) scenario, recognized as a promising solution for achieving steady-state operation in future fusion devices, has been well established in DIII-D. Recently, initiatives have been taken to demonstrate its feasibility for long-pulse operation in a tungsten environment like KSTAR. As an initial step towards this goal, a collaborative DIII-D-KSTAR team was formed to conduct experiments during the FY24-25 campaign aimed at establishing a high-βP scenario with KSTAR-like constraints. These constraints include considerations such as the latest plasma shape optimized for a new W-divertor, limited IP ramp-up rates, and restrictions on auxiliary heating.
The initial experimental results showed that achieving and sustaining a high qmin early in the discharge, a critical element for accessing high-βP regime, was challenging. Consequently, achieving a large radius ITB formation was initially unsuccessful. However, through optimizations in plasma shape, density, and beta evolutions, and in heating power waveforms, high-performance high-βP plasmas with ITB at large radius (ρ~0.7), βN~3.0, H98y2~1.5, and ƒGW~0.8, were eventually achieved. In the presentation, additional improvement strategies will be discussed through more detailed analysis.
The initial experimental results showed that achieving and sustaining a high qmin early in the discharge, a critical element for accessing high-βP regime, was challenging. Consequently, achieving a large radius ITB formation was initially unsuccessful. However, through optimizations in plasma shape, density, and beta evolutions, and in heating power waveforms, high-performance high-βP plasmas with ITB at large radius (ρ~0.7), βN~3.0, H98y2~1.5, and ƒGW~0.8, were eventually achieved. In the presentation, additional improvement strategies will be discussed through more detailed analysis.
*This research was supported by R&D Program of "KSTAR Experimental Collaboration and Fusion Plasma Research (EN2401-15)" through the Korea Institute of Fusion Energy (KFE) funded by the Government (Republic of Korea), and by the Department of Energy under Award Number(s) DE-FC02-04ER54698, DE-AC0209CH11466.
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Presenters
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YoungMu Jeon
- Korea Institute of Fusion Energy