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Optical designs of snapshot interferometer for coronagraphy

机译:Coronagraphy快照干涉仪的光学设计

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摘要

Following the idea developed in (Boccaletti et al. 2000), a snapshot imaging interferometer is proposed as an alternative to the NASA Origin project: "Terrestrial Planet Finder". This concept is based on densified pupil imaging and phase-mask coronagraphy by (Rouan et al. 2000). The so-called Four-Quadrant Phase-Mask features a large starlight attenuation (10~(-8)). Thorough calculations indicate that the detection of Earth like planets amidst zodiacal and exo-zodiacal clouds is faster with an imaging system than with a nulling interferometer as originally proposed for the TPF design. Detailed numerical simulations have been carried out taking into account several sources of noise and as a result we found that Earth-like planets can be imaged up to about 25 pc with a large interferometer in the thermal infrared. Finally this concept seems promising for discovering life hints with medium resolution spectra in both the visible (O_2, CH_4, H_2O and Chlorophylla signature) and the thermal infra-red (CH_4, H_2O, O_3, CO_2, NH_3).
机译:在(Boccaletti等,2000)中发育的想法之后,提出了一种快照成像干涉仪作为美国宇航局起源项目的替代品:“地面行星发现者”。该概念基于致密化的瞳孔成像和相位掩模Coronagraphy(Rouan等人。2000)。所谓的四象限相位掩模具有大的星光衰减(10〜(-8))。彻底的计算表明,在Zodiacal和Exo-Zodiacal云中的图像中的地球检测是具有比成像系统更快的速度,而不是最初提出用于TPF设计的无效干涉仪。已经考虑了详细的数值模拟,考虑了几种噪声来源,因此我们发现,在热红外线中,地球状行星可以在大约25台上成像,在热红外线中具有大的干涉仪。最后,这种概念似乎有希望在可见(O_2,CH_4,H_2O和叶绿素签名中的中等分辨率光谱中发现生命暗示)和热红外(CH_4,H_2O,O_3,CO_2,NH_3)。

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