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A SPECS Update: Engineering and Technology Requirements for a Space-based Far-IR Imaging Interferometer

机译:SPECS更新:天基远红外成像干涉仪的工程和技术要求

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The Submillimeter Probe of the Evolution of Cosmic Structure (SPECS) is a space-based imaging and spectral ("double Fourier") interferometer with kilometer maximum baseline lengths for imaging. This NASA "vision mission" will provide spatial resolution in the far-IR and submillimeter spectral range comparable to that of the Hubble Space Telescope, enabling astrophysicists to extend the legacy of current and planned far-IR observatories. The astrophysical information uniquely available with SPECS and its pathfinder mission SPIRIT will be briefly described, but that is more the focus of a companion paper in the Proceedings of the Optical, Infrared, and Millimeter Space Telescopes conference. Here we present an updated design concept for SPECS and for the pathfinder interferometer SPIRIT (Space Infrared Interferometric Telescope) and focus on the engineering and technology requirements for far-IR double Fourier interferometry. We compare the SPECS optical system requirements with those of existing ground-based and other planned space-based interferometers, such as SIM and TPF-I/Darwin.
机译:宇宙结构演化的亚毫米探针(SPECS)是一种基于空间的成像和光谱(“双傅立叶”)干涉仪,具有用于成像的千米最大基线长度。这项NASA的“视觉任务”将提供与哈勃太空望远镜相当的远红外和亚毫米波光谱范围内的空间分辨率,从而使天体物理学家能够扩展当前和计划中的远红外观测站的遗产。将简要介绍SPECS及其探路任务SPIRIT独有的天体信息,但这将是光学,红外和毫米波空间望远镜会议论文集的另一篇重点论文。在这里,我们为SPECS和探路仪干涉仪SPIRIT(空间红外干涉望远镜)提供了更新的设计概念,并着重介绍了远红外双傅立叶干涉仪的工程和技术要求。我们将SPECS光学系统要求与现有的地面和其他计划中的空间干涉仪(例如SIM和TPF-I / Darwin)的要求进行了比较。

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