用于支持大气研究的高分辨率测量的冷却光学光谱仪

L. Strow, C. Korb, B. Gentry
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摘要

本文研制了一种高分辨率、3米焦距的液氮冷却有序光学光栅光谱仪,用于2 ~ 30 μm光谱区域大气成分的实验室光谱分析,该光谱仪采用Littrow光学设计,可允许25 cm梯级光栅进行2次或4次衍射。双通道的理论分辨率为0.011 cm−1,四通道的理论分辨率为0.006 cm−1。在红外光栅光谱中实现高分辨率的根本限制是高室温背景下的高噪声问题。为了进行具有足够的信噪比的测量,光栅光谱仪通常必须使狭缝宽度大大大于衍射极限。这导致信号增加,但分辨率下降。在黑体背景光子通量相对较低的近红外波段,使用了分辨率高达0.015 cm−1的光谱仪。然而,在热红外中,由于该区域存在高黑体背景,光栅光谱仪的分辨率被限制在0.05 ~ 0.10 cm−1左右。
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A Cooled Optics Spectrometer for High Resolution Measurements in Support of Atmospheric Research
A high resolution, 3 meter focal length grating spectrometer utilizing liquid nitrogen cooled order sorting optics has been developed for laboratory spectroscopy of atmospheric constituents in the 2 μm to 30 μm spectral region, the spectrometer uses a Littrow optical design modified to allow either two or four diffractions off the 25 cm echelle grating. The theoretical resolution is 0.011 cm−1 for double pass and 0.006 cm−1 for four pass operation. The fundamental limitation in achieving high resolution in infrared grating spectroscopy has been the problem of high noise associated with high room temperature background. In order to perform measurements with sufficient signal to noise, grating spectrometers must generally be operated with slit widths substantially greater than the diffraction limit. This results in an increase in signal but with a loss in resolution. In the near infrared, where relatively low blackbody background photon fluxes occur, spectrometers with resolutions as high as 0.015 cm−1 have been used. In the thermal infrared, however, the resolution of grating spectrometers has been limited to about 0.05 to 0.10 cm−1 by the high blackbody backgrounds occurring in this region.
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