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Design of a Mid-IR Polarimeter for SOFIA

机译:SOFIA中红外旋光仪的设计

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摘要

Mid-infrared polarimetry remains an underexploited technique; where available it is limited in spectral coverage from the ground, and conspicuously absent from the Spitzer, JWST and Herschel instrument suites. The unique characteristics of SOFIA afford unprecedented spectral coverage and sensitivity in the mid-infrared waveband. We discuss the preliminary optical design for a 5-40μm spectro-polarimeter for use on SOFIA, the SOFIA Mid-InfraRed Polarimeter (SMIRPh). The design furthers the existing 5-40μm imaging and spectroscopic capabilities of SOFIA, and draws on experience gained through the University of Florida's mid-IR imagers, spectrometer and polarimeter designs of T-ReCS and CanariCam. We pay special attention to the challenges of obtaining polarimetric materials suitable at both these wavelengths and cryogenic temperatures. Finally, we (briefly) present an overview of science highlights that could be performed from a 5-40μm imaging- and spectro-polarimeter on SOFIA. Combined with the synergy between the possible future far-IR polarimeter, Hale, this instrument would provide the SOFIA community with unique and exciting science capabilities, leaving a unique scientific legacy.
机译:中红外旋光法仍然是一种尚未被充分利用的技术。在可用的情况下,它的地面光谱覆盖范围有限,而Spitzer,JWST和Herschel仪器套件则明显缺乏。 SOFIA的独特特性在中红外波段提供了空前的光谱覆盖范围和灵敏度。我们讨论了用于SOFIA的5-40μm分光偏振仪的初步光学设计,即SOFIA中红外旋光仪(SMIRPh)。该设计进一步完善了SOFIA现有的5-40μm成像和光谱功能,并借鉴了佛罗里达大学T-ReCS和CanariCam的中红外成像仪,光谱仪和偏振计的设计经验。我们特别注意获得在这些波长和低温下均适用的偏振材料的挑战。最后,我们简要介绍了可以在SOFIA上使用5-40μm成像和分光偏振计执行的科学亮点的概述。结合未来可能的远红外旋光仪Hale之间的协同作用,该仪器将为SOFIA社区提供独特而令人兴奋的科学能力,从而留下独特的科学遗产。

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