Characterization of Aerogel with Spectral Domain Optical Coherence Tomography & Preliminary Analysis of HELIX RICH Flight Data Investigation

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This thesis characterizes the refractive index and thickness of aerogel tiles and analyzes preliminary flight data from the High Energy Light Isotope eXperiment (HELIX), a balloon-borne detector. Accurate velocity measurements from HELIX's Ring Imaging Cherenkov (RICH) detector are essential to achieve a 3% cosmic-ray isotope mass resolution for Z≤4. This requires aerogel radiators with n = 1.15 at 405 nm to be characterized to the order of 10⁻³ in thickness and 10⁻⁴ in refractive index. Spectral Domain Optical Coherence Tomography (SD-OCT) is introduced here as a non-contact method to simultaneously determine both parameters. The technique meets the experimental requirements, achieving a thickness precision of ±2.1 μm and a group refractive index precision of ±0.0003. A procedure to derive the phase refractive index is also demonstrated. Finally, a preliminary analysis of HELIX flight data is presented here, applying a clustering algorithm (DBSCAN) to identify event morphology in the RICH.

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Cosmic Rays, Optical Coherence Tomography

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