Available energy of trapped electrons in Miller tokamak equilibria
R.J.J. Mackenbach, J.H.E. Proll, G. Snoep, P. Helander

TL;DR
This paper investigates the available energy (AE{}) in Miller tokamak equilibria, demonstrating its potential to predict turbulence trends and optimize device geometry for stability, especially considering effects like triangularity and shear.
Contribution
It introduces a detailed analysis of AE{} in Miller equilibria, linking it to experimental trends, and explores how geometry and gradients influence stability and turbulence predictions.
Findings
AE{} correlates with experimental turbulence trends.
Negative triangularity stabilizes by reducing AE{} in certain configurations.
Optimal device parameters depend strongly on equilibrium conditions.
Abstract
Available energy (\AE{}), which quantifies the maximum amount of thermal energy that may be liberated and converted into instabilities and turbulence, has shown to be a useful metric for predicting saturated energy fluxes in trapped-electron-mode-driven turbulence. Here, we calculate and investigate the \AE{} in the analytical tokamak equilibria introduced by \citet{Miller1998NoncircularModel}. The \AE{} of trapped electrons reproduces various trends also observed in experiments; negative shear, increasing Shafranov shift, vertical elongation, and negative triangularity can all be stabilising, as indicated by a reduction in \AE{}, although it is strongly dependent on the chosen equilibrium. Comparing \AE{} with saturated energy flux estimates from the \textsc{tglf} model, we find fairly good correspondence, showcasing that \AE{} can be useful to predict trends. We go on to investigate…
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Taxonomy
TopicsMagnetic confinement fusion research · Ionosphere and magnetosphere dynamics · Physics of Superconductivity and Magnetism
