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[基于前向散射近红外光谱法的雾雨大气消光测量研究]

[Study on the measurement of the atmospheric extinction of fog and rain by forward-scattering near infrared spectroscopy].

作者信息

Wang Mian, Liu Wen-qing, Lu Yi-huai, Zhao Xue-song, Song Bing-chao, Zhang Yu-jun, Wang Ya-ping, Lian Cui-hua, Chen Jun, Cheng Yin, Liu Jian-guo, Wei Qing-nong

机构信息

Key Laboratory of Environmental Optics & Technology, Anhui Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Hefei 230031, China.

出版信息

Guang Pu Xue Yu Guang Pu Fen Xi. 2008 Aug;28(8):1776-80.

Abstract

In the visible and near IR, absorption is negligible so that the atmospheric extinction can be derived by atmospheric scattering which is mainly contributed by fog droplet, rain droplet, another types of droplet and small articles. The forward-scattering visibility meter (FVM) works by illuminating with near IR light a small sample volume of about 100 mL of air and measuring the intensity scattered in the angular range of 30 to 36 degrees. The scattered intensity is proportional to the extinction coefficient regardless of the article size distribution and after wavelength calibration. The ratio of scattered signal to extinction coefficient of fog and haze can be achieved by comparative test of FVM outputs and manual observations. Nevertheless, as a result of the application of the measurement during rain with the ratio of fog and haze, an unacceptable error is raised. To obtain an accuracy extinction measurement during rain, an appropriated ratio of scattered signal to extinction coefficient of rain would be found. The calculation for different size distributions of fog and rain with Mie theory has been made in this paper. And a comparison of extinction measurements made with two FVMs and manual observations during fog and rain has been made. The result shows that during rain the FVM extinction coefficient is from 20% to 60% greater than that of manual observations. This result can be used to define correction factors so that the FVM using forward-scattering near IR spectroscopy not only can be used to estimate extinction during fog and haze as well as during rain.

摘要

在可见光和近红外波段,吸收可以忽略不计,因此大气消光可以通过大气散射来推导,大气散射主要由雾滴、雨滴、其他类型的液滴和小颗粒造成。前向散射能见度仪(FVM)的工作原理是用近红外光照射大约100毫升的小体积空气样本,并测量在30至36度角范围内散射的强度。无论颗粒尺寸分布如何,经过波长校准后,散射强度与消光系数成正比。通过FVM输出与人工观测的对比测试,可以得到雾和霾的散射信号与消光系数的比值。然而,由于在降雨期间应用该测量方法时涉及雾和霾的比值,会产生不可接受的误差。为了在降雨期间获得准确的消光测量结果,需要找到合适的降雨散射信号与消光系数的比值。本文利用米氏理论对不同尺寸分布的雾和雨进行了计算。并对两台FVM在雾和雨期间进行的消光测量与人工观测进行了比较。结果表明,在降雨期间,FVM消光系数比人工观测结果大20%至60%。该结果可用于定义校正因子,这样使用前向散射近红外光谱的FVM不仅可用于估计雾和霾期间的消光,也可用于降雨期间的消光估计。

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