Transport Modeling of NSTX/NSTX-U discharges
POSTER
Abstract
The spherical tokamak (ST) provides critical information required for the optimization of the
design and operation of steady-state compact fusion pilot plants (CFPP). The National
Spherical Torus Experiment Upgrade (NSTX-U) will advance the physics basis by producing
unique non-inductive regimes at low-aspect ratio that operate at large normalized beta,
bootstrap fraction and toroidal field utilization. However, in order to extrapolate the results
obtained on current STs to next-step devices, a better physics understanding of transport,
stability, and non-inductive start-up is required, as well as the development of predictive
capabilities that span aspect ratio. This work describes the results of plasma transport
modeling performed using the OMFIT framework on previous relevant NSTX/NSTX-U
discharges. Simulations are carried out with the TRANSP and TGYRO modules of OMFIT,
and comparisons between calculated and measured plasma quantities indicate the validity of
these predictive tools. To better understand the underlying transport mechanisms, we have
performed linear turbulence mode analysis using the TGLF model and identified conditions
where this model might be applicable for NSTX plasmas.
design and operation of steady-state compact fusion pilot plants (CFPP). The National
Spherical Torus Experiment Upgrade (NSTX-U) will advance the physics basis by producing
unique non-inductive regimes at low-aspect ratio that operate at large normalized beta,
bootstrap fraction and toroidal field utilization. However, in order to extrapolate the results
obtained on current STs to next-step devices, a better physics understanding of transport,
stability, and non-inductive start-up is required, as well as the development of predictive
capabilities that span aspect ratio. This work describes the results of plasma transport
modeling performed using the OMFIT framework on previous relevant NSTX/NSTX-U
discharges. Simulations are carried out with the TRANSP and TGYRO modules of OMFIT,
and comparisons between calculated and measured plasma quantities indicate the validity of
these predictive tools. To better understand the underlying transport mechanisms, we have
performed linear turbulence mode analysis using the TGLF model and identified conditions
where this model might be applicable for NSTX plasmas.
Presenters
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Galina Avdeeva
General Atomics - San Diego
Authors
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Galina Avdeeva
General Atomics - San Diego
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Kathreen E Thome
General Atomics - San Diego, General Atomics
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Sterling P Smith
General Atomics - San Diego, General Atomics, General Atomics, San Diego, CA, US
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Orso-Maria O Meneghini
General Atomics - San Diego, General Atomics
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Joseph T Mcclenaghan
General Atomics, General Atomics - San Diego, Oak Ridge National Laboratory
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Devon J Battaglia
Princeton Plasma Physics Laboratory, PPPL
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Walter Guttenfelder
Princeton Plasma Physics Laboratory
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Stanley M Kaye
Princeton Plasma Physics Laboratory