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The use of flexures to achieve fibre positioner motion is being actively investigated by several institutes, for example at the UK Astronomy Technology Centre (UKATC) and Leibniz-Institute for Astrophysics Potsdam. One challenge when designing with flexures is the large number of degrees of freedom available which makes it difficult or impossible to optimise their motion by hand. In this paper we demonstrate two approaches for optimising flexure geometry to follow arbitrary focal surface curvature and to orient the optical fibre with arbitrary tilt. These approaches are: analytical using MATLAB models and FEA based using Ansys. The approaches are complementary allowing the designer to efficiently explore the parameter space and then do precise optimisation of the flexure geometry. We demonstrate the applicability both to the UKATCs preferred design for WST, and to flexure-based fibre positioner designs generally. We also present a sensitivity analysis relating small changes in design parameters to changes in fibre tip motion. Finally we briefly present the UKATCs preferred geometry for the WST fibre positioner., Comment: 17 pages, 13 figures, submitted to SPIE Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation VI, Tokyo, 16-21/06/2024

We report on simulations of counter-propagating laser-produced plasmas in an inertial confinement fusion (ICF) hohlraum surrogate, aiming to replicate observations reported by Le Pape et. al in recent work. The conditions of the colliding plasmas are relevant to ICF hohlraums used for indirect-drive ignition, and are obtained both with and without low-density He-gas fill. We compare experimental diagnostics to outputs from simulations using the 1D-2V Vlasov-Fokker-Planck kinetic code iFP and the xRAGE radiation-hydrodynamics code. These include the inferred radial lineouts of inferred ion number fraction and ion and electron temperatures, as well as the reported experimental Thomson-scattering (TS) spectra (compared via synthetic TS diagnostics). We observe that 1D kinetic simulations capture the plasma states reported in the experimental diagnostics quite well. Counter-intuitively, the kinetic simulations capture the gas-fill experiment (expected to be more `hydro-like') better than the vacuum experiment, while the reverse is observed for hydrodynamic simulations. This is attributed to the presence of non-trivial multi-dimensional hydrodynamic effects which are more dominant in the vacuum experiment. These effects are somewhat inhibited in the gas-fill experiment, permitting quasi-1D kinetic plasma transport to play more of a role in producing plasma interpenetration. Differences between the effects of Maxwellian vs. non-Maxwellian (`full f') synthetic TS diagnostics are investigated for the kinetic simulations. We find non-Maxwellian TS spectra differ non-trivially from Maxwellian spectra, which suggests caution may be warranted when applying Maxwellian TS models to infer plasma conditions via backward modeling when kinetic effects may be present.

Shock-bubble interactions (SBI) are important across a wide range of physical systems. In inertial confinement fusion, interactions between laser-driven shocks and micro-voids in both ablators and foam targets generate instabilities that are a major obstacle in achieving ignition. Experiments imaging the collapse of such voids at high energy densities (HED) are constrained by spatial and temporal resolution, making simulations a vital tool in understanding these systems. In this study, we benchmark several radiation and thermal transport models in the xRAGE hydrodynamic code against experimental images of a collapsing mesoscale void during the passage of a 300 GPa shock. We also quantitatively examine the role of transport physics in the evolution of the SBI. This allows us to understand the dynamics of the interaction at timescales shorter than experimental imaging framerates. We find that all radiation models examined reproduce empirical shock velocities within experimental error. Radiation transport is found to reduce shock pressures by providing an additional energy pathway in the ablation region, but this effect is small ($\sim$1\% of total shock pressure). Employing a flux-limited Spitzer model for heat conduction, we find that flux limiters between 0.03 and 0.10 produce agreement with experimental velocities, suggesting that the system is well-within the Spitzer regime. Higher heat conduction is found to lower temperatures in the ablated plasma and to prevent secondary shocks at the ablation front, resulting in weaker primary shocks. Finally, we confirm that the SBI-driven instabilities observed in the HED regime are baroclinically driven, as in the low energy case., Comment: 14 pages, 12 figures