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Impact of atmospheric clutter on Doppler-limited gas sensors in the submillimeter/terahertz

机译:大气杂波对亚毫米/太赫兹多普勒限制气体传感器的影响

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摘要

It is well known that clutter (spectral interference) from atmospheric constituents can be a severe limit for spectroscopic point sensors, especially where high sensitivity and specificity are required. In this paper, we will show for submillimeter/terahertz (SMM/THz) sensors that use cw electronic techniques the clutter limit for the detection of common target gases with absolute specificity (probability of false alarm 10~(-10)) is in the ppt (1 part in 10~(12)) range or lower. This is because the most abundant atmospheric gases are either transparent to SMM/THz radiation (e.g., CO_(2)) or have spectra that are very sparse relative to the 10~(5) Doppler-limited resolution elements available (e.g., H_(2)O). Moreover, the low clutter limit demonstrated for cw electronic systems in the SMM/THz is independent of system size and complexity.
机译:众所周知,来自大气成分的杂波(光谱干扰)可能是光谱点传感器的严重限制,尤其是在需要高灵敏度和特异性的情况下。在本文中,我们将显示对于使用连续电子技术的亚毫米/太赫兹(SMM / THz)传感器,以绝对特异性检测杂散极限的常见目标气体的检测限(误报警的可能性 10〜(-10))为在ppt(10〜(12)中的1个部分)范围内或更低。这是因为最丰富的大气对SMM / THz辐射是透明的(例如CO_(2)),或者具有相对于可用的10〜(5)多普勒限制的分辨率元素非常稀疏的光谱(例如H_( 2)O)。此外,在SMM / THz中为连续电子系统演示的低杂波限制与系统大小和复杂性无关。

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