The Large Binocular Telescope Interferometer is a high contrast imager and interferometer that sits at the combined bent Gregorian focus of the LBTs dual 8.4~m apertures. The interferometric science drivers dictate 0.1 resolution with $10^3-10^4$ contrast at $10~mu m$, while the $4~mu m$ imaging science drivers require even greater contrasts, but at scales $>$0.2. In imaging mode, LBTIs Adaptive Optics system is already delivering $4~mu m$ contrast of $10^4-10^5$ at $0.3-0.75$ in good conditions. Even in poor seeing, it can deliver up to 90% Strehl Ratio at this wavelength. However, the performance could be further improved by mitigating Non-Common Path Aberrations. Any NCPA remedy must be feasible using only the current hardware: the science camera, the wavefront sensor, and the adaptive secondary mirror. In preliminary testing, we have implemented an ``eye doctor grid search approach for astigmatism and trefoil, achieving 5% improvement in Strehl Ratio at $4~mu m$, with future plans to test at shorter wavelengths and with more modes. We find evidence of NCPA variability on short timescales and discuss possible upgrades to ameliorate time-variable effects
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