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用于消光干涉测量的中红外宽带消色差天文光束组合器。

Midinfrared broadband achromatic astronomical beam combiner for nulling interferometry.

作者信息

Hsiao Hsien-kai, Winick Kim A, Monnier John D

机构信息

Department of Electrical Engineering and Computer Science, University of Michigan, 1301 Beal Avenue, Ann Arbor, Michigan 48109, USA.

出版信息

Appl Opt. 2010 Dec 10;49(35):6675-88. doi: 10.1364/AO.49.006675.

Abstract

Integrated optic beam combiners offer many advantages over conventional bulk optic implementations for astronomical imaging. To our knowledge, integrated optic beam combiners have only been demonstrated at operating wavelengths below 4 μm. Operation in the midinfrared wavelength region, however, is highly desirable. In this paper, a theoretical design technique based on three coupled waveguides is developed to achieve fully achromatic, broadband, polarization-insensitive, lossless beam combining. This design may make it possible to achieve the very deep broadband nulls needed for exoplanet searching.

摘要

与传统的体光学实现方式相比,集成光学光束组合器在天文成像方面具有许多优势。据我们所知,集成光学光束组合器仅在低于4μm的工作波长下得到了验证。然而,在中红外波长区域工作是非常有必要的。在本文中,我们开发了一种基于三个耦合波导的理论设计技术,以实现全消色差、宽带、偏振不敏感、无损的光束组合。这种设计可能使实现系外行星搜索所需的极深宽带零值成为可能。

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