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We present a segment-level wavefront stability error budget for the LUVOIR A architecture essential for exoplanet detection. We start with a detailed finite element model to relate the temperature and gravity gradients at the location of the primary mirror to wavefront variations for each segment, and propagate the elements through a diffractive model of the observatory and coronagraphic instrument. Segment level errors are measured via a model of the WFS&C architecture in combination with a Zernike phase sensor and science camera. These sensitivities are used to relate semi-analytically the open and closed loop variance of the segments’ thermo-mechanical modes.
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Ananya Sahoo, Iva Laginja, Laurent Pueyo, Remi Soummer, Laura E. Coyle, J. Scott Knight, Matthew East, "LUVOIR A Segment level thermo-mechanical stability requirements," Proc. SPIE 11823, Techniques and Instrumentation for Detection of Exoplanets X, 118231N (1 August 2021); https://doi.org/10.1117/12.2594636