使用fm调制可调谐二极管激光吸收光谱仪测量平流层中痕量气体的光谱问题

S. Poultney, A. Pires, D. Chen
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引用次数: 0

摘要

在平流层条件下,fm调制的可调谐二极管激光吸收光谱仪已被证明能够检测到NO的分数吸收率为1 / 105这种能力意味着可以在32公里处检测到低至108分子/ cm3的痕量物质浓度,同时吸收路径长度为100米。调频/二次谐波检测技术的滤波特性使这些测量成为可能,但也会扭曲被检测的红外特征,并使测量校准成为必要。分数吸收的校准通常是通过在已知的恒定条件下使用含有已知气体量的校准池来完成的。在平流层中所研究的微量气体受到各种压力和温度条件的影响。畸变、环境条件的变化和校准技术的相互作用使得对检测到的信号的解释变得复杂。在可能的情况下,通过选择合适的谱线,记录每次测量的环境条件,并利用所研究的每种物种的高分辨率光谱数据库,可以使这种解释更加确定。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Spectroscopic Issues Related to Trace Gas Measurements in the Stratosphere Using the FM-Modulated Tunable Diode Laser Absorption Spectrometer
The fm-modulated tunable diode laser absorption spectrometer has been shown to be capable of detecting fractional absorptions of 1 part in 105 for NO under stratospheric conditions.1 This capability implies that trace species concentrations as low as 108 molecules/ cm3 can be detected at 32 Km in conjunction with absorption path lengths of 100m. The filtering properties of the fm/2nd harmonic detection tech nique which make these measurements possible2 also distort the IR signature being detected and make calibration of the measurement necessary. Calibration of fractional absorption is most generally accomplished through the use of calibration cells containing a known amount of gas under known, constant conditions. The trace gases being studied in the stratosphere are subject to a wide range of pressure and temperature conditions. The interplay of distortion, variation of ambient conditions, and calibration technique make interpretation of detected signatures complex. This interpretation can be made more certain by selecting appropriate lines when possible, by recording the ambient conditions of each measurement, and by drawing upon a high resolution spectroscopic data base for each species being studied.
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