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EARLINET项目框架下的气溶胶激光雷达相互比对。1. 仪器

Aerosol lidar intercomparison in the framework of the EARLINET project. 1. Instruments.

作者信息

Matthais Volker, Freudenthaler Volker, Amodeo Aldo, Balin Ioan, Balis Dimitris, Bösenberg Jens, Chaikovsky Anatoly, Chourdakis Georgius, Comeron Adolfo, Delaval Arnaud, De Tomasi Ferdinando, Eixmann Ronald, Hågård Arne, Komguem Leonce, Kreipl Stephan, Matthey Renaud, Rizi Vincenzo, Rodrigues José António, Wandinger Ulla, Wang Xuan

机构信息

Max-Planck-Institut für Meteorologie, Bundesstrasse 55, 20146 Hamburg, Germany.

出版信息

Appl Opt. 2004 Feb 1;43(4):961-76. doi: 10.1364/ao.43.000961.

Abstract

In the framework of the European Aerosol Research Lidar Network to Establish an Aerosol Climatology (EARLINET), 19 aerosol lidar systems from 11 European countries were compared. Aerosol extinction or backscatter coefficient profiles were measured by at least two systems for each comparison. Aerosol extinction coefficients were derived from Raman lidar measurements in the UV (351 or 355 nm), and aerosol backscatter profiles were calculated from pure elastic backscatter measurements at 351 or 355, 532, or 1064 nm. The results were compared for height ranges with high and low aerosol content. Some systems were additionally compared with sunphotometers and starphotometers. Predefined maximum deviations were used for quality control of the results. Lidar systems with results outside those limits could not meet the quality assurance criterion. The algorithms for deriving aerosol backscatter profiles from elastic lidar measurements were tested separately, and the results are described in Part 2 of this series of papers [Appl. Opt. 43, 977-989 (2004)]. In the end, all systems were quality assured, although some had to be modified to improve their performance. Typical deviations between aerosol backscatter profiles were 10% in the planetary boundary layer and 0.1 x 10(-6) m(-1) sr(-1) in the free troposphere.

摘要

在欧洲建立气溶胶气候学激光雷达网络(EARLINET)的框架内,对来自11个欧洲国家的19台气溶胶激光雷达系统进行了比较。每次比较中,至少有两个系统测量气溶胶消光或后向散射系数剖面。气溶胶消光系数由紫外波段(351或355纳米)的拉曼激光雷达测量得出,气溶胶后向散射剖面则根据351或355、532或1064纳米处的纯弹性后向散射测量计算得出。对高气溶胶含量和低气溶胶含量的高度范围的结果进行了比较。一些系统还与太阳光度计和恒星光度计进行了比较。使用预定义的最大偏差对结果进行质量控制。结果超出这些限制的激光雷达系统不符合质量保证标准。从弹性激光雷达测量中推导出气溶胶后向散射剖面的算法进行了单独测试,结果在本系列论文的第2部分中描述[《应用光学》43, 977 - 989 (2004)]。最后,所有系统都通过了质量保证,尽管有些系统必须进行改进以提高其性能。气溶胶后向散射剖面之间的典型偏差在行星边界层为10%,在自由对流层为0.1×10⁻⁶米⁻¹球面度⁻¹。

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