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Turbulence and transport in mirror geometries in the Large Plasma Device

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arxiv 2409.11557 v2 pith:QSCPNHNH submitted 2024-09-17 physics.plasm-ph

Turbulence and transport in mirror geometries in the Large Plasma Device

classification physics.plasm-ph
keywords mirrorweredensityincreasedmagneticplasmainterchangepower
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Thanks to advances in plasma science and enabling technology, mirror machines are being reconsidered for fusion power plants and as possible fusion volumetric neutron sources. However cross-field transport and turbulence in mirrors remains relatively understudied compared to toroidal devices. Turbulence and transport in mirror configurations were studied utilizing the flexible magnetic geometry of the Large Plasma Device (LAPD). Multiple mirror ratios from $ M = 1 $ to $ M = 2.68 $ and three mirror-cell lengths from $L = 3.51 $m to $ L = 10.86 $m were examined. Langmuir and magnetic probes were used to measure profiles of density, temperature, potential, and magnetic field. The fluctuation-driven $ \tilde{ E } \times B $ particle flux was calculated from these quantities. Two probe correlation techniques were used to infer wavenumbers and two-dimensional structure. Cross-field particle flux and density fluctuation power decreased with increased mirror ratio. Core density and temperatures remain similar with mirror ratio, but radial line-integrated density increased. The physical expansion of the plasma in the mirror cell by using a higher field in the source region may have led to reduced density fluctuation power through the increased gradient scale length. This increased scale length reduced the growth rate and saturation level of rotational interchange and drift-like instabilities. Despite the introduction of magnetic curvature, no evidence of mirror driven instabilities -- interchange, velocity space, or otherwise -- were observed. For curvature-induced interchange, many possible stabilization mechanisms were present, suppressing the visibility of the instability.

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