Polarization interferometric nulling coronagraph for high-contrast imaging

被引:13
|
作者
Murakami, Naoshi [1 ]
Yokochi, Kaito [2 ,3 ]
Nishikawa, Jun [3 ]
Tamura, Motohide [3 ]
Kurokawa, Takashi [2 ]
Takeda, Mitsuo [4 ]
Baba, Naoshi [1 ]
机构
[1] Hokkaido Univ, Grad Sch Engn, Kita Ku, Sapporo, Hokkaido 0608588, Japan
[2] Tokyo Univ Agr & Technol, Grad Sch Engn, Koganei, Tokyo 1848588, Japan
[3] Natl Inst Nat Sci, Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan
[4] Univ Electrocommun, Dept Informat & Commun Engn, Tokyo 1828585, Japan
基金
日本学术振兴会;
关键词
PHASE-MASK CORONAGRAPH; GEOMETRIC PHASE; PLANETS; TELESCOPE; LIGHT; APERTURE; IMAGES; PUPIL;
D O I
10.1364/AO.49.00D106
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
We propose a novel, high-contrast imager called a polarization interferometric nulling coronagraph (PINC) for direct detection of extrasolar planets. The PINC uses achromatic half-wave plates (HWPs) installed in a fully symmetric beam combiner based on polarizing beam splitters. Jones calculus suggests that a stellar halo suppression level of 10(-10) can be achieved at 5 lambda/D for a broad wavelength range from 1.6 to 2.2 mu m by using Fresnel-rhomb HWPs made of BK7. Laboratory experiments on the PINC used two laser light sources (wavelengths of lambda = 532 and 671 nm), and we obtained a halo suppression level of approximately 10(-6) at 5 lambda/D for both wavelengths. (C) 2010 Optical Society of America
引用
收藏
页码:D106 / D114
页数:9
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