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Polarization compensating protective coatings for TPF-Coronagraph optics to control contrast degrading cross polarization leakage

机译:用于TPF-Coronagraph光学器件的偏振补偿保护膜,可控制对比度降低的交叉偏振泄漏

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摘要

The Terrestrial Planet Finder Coronagraph (TPF-C) for observing and characterizing exo-solar planets requiring star light suppression to 10~(-10) level demands optical aberrations and instrument stability to sub-nm levels. Additionally, wavefront polarization has to be tightly controlled over the 8m x 3.5m primary mirror aperture and 500nm — 500nm minimum bandwidth because the Deformable Mirror (DM) employed to control the wavefront can not correct simultaneously for the different wavefronts presented by two orthogonal uncorrected polarization fields. Further, leakage of cross polarization fields introduced by the various optical surfaces can degrade the image contrast. The study reported here shows mirror coating designs that reduce the phase difference between orthogonal polarizations reflected by a mirror surface to less than 0.6 deg over the bandwidth and aperture which may encounter a maximum angle of incidence of about 12 deg at a curved mirror. Such designs mitigate the contrast degradation due to cross polarization leakage. Simulations show that required contrast levels can be achieved with such coatings.
机译:用于观测和表征需要将恒星光抑制到10〜(-10)级的太阳系外行星的地球行星探测仪日冕仪(TPF-C),要求光学像差和仪器稳定性达到亚纳米级。此外,必须严格控制8m x 3.5m主镜孔径和500nm-500nm最小带宽的波前偏振,因为用于控制波前的可变形镜(DM)不能同时针对两个正交未校正偏振所呈现的不同波前进行校正。领域。此外,由各种光学表面引入的交叉偏振场的泄漏会降低图像对比度。此处报道的研究表明,镜面涂层设计可将镜面反射的正交偏振之间的相位差在带宽和孔径上减小到小于0.6度,而在弯曲镜处可能会遇到约12度的最大入射角。这样的设计减轻了由于交叉极化泄漏引起的对比度下降。仿真表明,使用这种涂料可以达到所需的对比度水平。

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