作者
JB Breckinridge, JE Harvey, R Irvin, R Chipman, M Kupinski, J Davis, DW Kim, E Douglas, CF Lillie, T Hull
发表日期
2019/9/9
研讨会论文
UV/Optical/IR Space Telescopes and Instruments: Innovative Technologies and Concepts IX
卷号
11115
页码范围
98-108
出版商
SPIE
简介
In this paper we examine several contrast-degrading static signature sources present in current terrestrial exoplanet Lyot Coronagraph/Telescope optical systems. These are: - Unnecessary optical surfaces, which increase cost, absorption, scatter, wavefront control and alignment issues. A suggested solution is to make every effort to investigate innovative solutions to reduce the number of optical surfaces during the early design phase. Consider free-form optics. - Diffraction from secondary support systems and classical hexagon segmented apertures, which masks the low IWA terrestrial exoplanets. A suggested mitigation is to investigate curved secondary support systems and a pinwheel architecture for the deployable primary aperture. - Polarization Fresnel and form birefringence aberrations, which distort the system PSF, introduce absorption, scatter and wavefront control issues. Mitigation is to reduce all ray …
引用总数
20202021202220233241
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