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Integrated optics for astronomical interferometry. I. Concept and astronomical applications

机译:用于天文干涉测量的集成光学系统。一,概念和   天文应用

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摘要

We propose a new instrumental concept for long-baseline optical single-modeinterferometry using integrated optics which were developed fortelecommunication. Visible and infrared multi-aperture interferometry requiresmany optical functions (spatial filtering, beam combination, photometriccalibration, polarization control) to detect astronomical signals at very highangular resolution. Since the 80's, integrated optics on planar substrate havebecome available for telecommunication applications with multiple opticalfunctions like power dividing, coupling, multiplexing, etc. We present theconcept of an optical / infrared interferometric instrument based on this newtechnology. The main advantage is to provide an interferometric combinationunit on a single optical chip. Integrated optics are compact, providestability, low sensitivity to external constrains like temperature, pressure ormechanical stresses, no optical alignment except for coupling, simplicity andintrinsic polarization control. The integrated optics devices are inexpensivecompared to devices that have the same functionalities in bulk optics. We thinkintegrated optics will fundamentally change single-mode interferometry.Integrated optics devices are in particular well-suited for interferometriccombination of numerous beams to achieve aperture synthesis imaging or forspace-based interferometers where stability and a minimum of optical alignmentsare wished.
机译:我们提出了一种新的仪器概念,用于使用为电信业开发的集成光学器件进行长基线光学单模干涉测量。可见光和红外多孔径干涉仪需要许多光学功能(空间滤波,光束组合,光度校准,偏振控制),才能以很高的角度分辨率检测天文信号。自80年代以来,平面基板上的集成光学元件已可用于具有多种光学功能(如功率分配,耦合,复用等)的电信应用。我们提出了基于这种新技术的光学/红外干涉仪的概念。主要优点是在单个光学芯片上提供干涉式组合单元。集成光学器件紧凑,可提供性,对诸如温度,压力或机械应力等外部约束的灵敏度低,除了耦合,简单和本征偏振控制外,没有光学对准。与大批量光学器件中具有相同功能的器件相比,集成光学器件价格便宜。我们认为集成光学将从根本上改变单模干涉仪。集成光学器件特别适合于众多光束的干涉组合,以实现孔径合成成像或希望获得稳定性和最小光学对准的基于空间的干涉仪。

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