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For the BepiColombo mission, the extreme thermal environment around Mercury requires good heat shields for the instruments. The BepiColombo Laser altimeter (BELA) Receiver will be equipped with a specular reflective baffle in order to limit the solar power impact. The design uses a Stavroudis geometry with alternating elliptical and hyperbolic vanes to reflect radiation at angles >38° back into space. The thermal loads on the baffle lead to deformations, and the resulting changes in the optical performance can be modeled by ray-tracing. Conventional interfaces, such as Zernike surface fitting, fail to provide a proper import of the mechanical distortions into optical models. We have studied alternative models such as free form surface representations and compared them to a simple modeling approach with straight segments. The performance merit is presented in terms of the power rejection ratio and the absence of specular stray-light.
E. Heesel,T. Weigel,P. Lochmatter, andE. Rugi Grond
"Coupled thermo-elastic and optical performance analyses of a reflective baffle for the BepiColombo laser altimeter (BELA) receiver", Proc. SPIE 10566, International Conference on Space Optics — ICSO 2008, 105661W (21 November 2017); https://doi.org/10.1117/12.2308252
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E. Heesel, T. Weigel, P. Lochmatter, E. Rugi Grond, "Coupled thermo-elastic and optical performance analyses of a reflective baffle for the BepiColombo laser altimeter (BELA) receiver," Proc. SPIE 10566, International Conference on Space Optics — ICSO 2008, 105661W (21 November 2017); https://doi.org/10.1117/12.2308252