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Polarization interferometric nulling coronagraph for high-contrast imaging

机译:用于高对比度成像的偏振干涉零位冠冕仪

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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 velence 532 and 671 nm), and we obtained a halo suppression level of approximately 10~(-6) at 5 lambda/D for both wavelengths.
机译:我们提出了一种新颖的,高对比度的成像器,称为极化干涉零点日冕仪(PINC),用于直接探测太阳系外行星。 PINC使用安装在基于偏振分束器的完全对称光束组合器中的消色差半波片(HWP)。琼斯演算表明,通过使用由BK7制成的菲涅耳-rhomb HWP,可以在5λ/ D的情况下在1.6至2.2μm的宽波长范围内实现10〜(-10)的恒星晕抑制水平。在PINC上进行的实验室实验使用了两个激光光源(λvelence 532和671 nm的波长),并且在5λ/ D下,两个波长的光晕抑制水平大约为10〜(-6)。

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