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Changes in atmospheric composition discerned from long-term NDACC measurements: trends in direct greenhouse gases derived from infrared solar absorption spectra recorded at the Jungfraujoch station

机译:长期NDACC测量可发现大气成分的变化:少女峰站记录的红外太阳吸收光谱得出的直接温室气体趋势

摘要

The University of Liège (ULg) is operating -under clear sky conditions- two state-of-the-art Fourier Transform Infrared (FTIR) spectrometers at the high-altitude research station of the Jungfraujoch (Swiss Alps, 46.5ºN, 3580m asl), within the framework of the Network for the Detection of Atmospheric Composition Changes (NDACC). Routine FTIR operation started in 1984. Since then, it has been continued without disruption, allowing collecting more than 45000 high-resolution broadband IR solar absorption spectra, between 2 and 16 µm, using either HgCdTe or InSb detectors as well as a suite of optical filters. Typically, the spectral resolutions achieved lie in the 0.003 to 0.009 cm-1 interval while signal-to-noise ratios of 1000 and more are reached. Numerous narrow-band IR spectra essentially recorded from 1976 to 1989 with grating instruments are also available. Their analyses with modern tools have recently started [Bader et al., 2011] and will be pursued to consistently extend our datasets back in the 1970s. Geophysical parameters are deduced from the ULg observational database either with the SFIT-1, SFIT-2 or PROFFIT-9 algorithm, allowing producing total column time series of the target gases. In addition, information on their vertical distributions with altitude can generally be derived when using SFIT-2 or PROFFIT-9 which both implement the Optimal Estimation Method of Rodgers [1990]. Presently, more than two dozen atmospheric species are systematically retrieved from the Jungfraujoch observations, allowing the monitoring of key constituents of the Earth's atmosphere which play important roles in stratospheric ozone depletion and/or in global warming. This communication will focus on the direct and major greenhouse gases available from our database, namely water vapor, CO2, CH4, N2O, tropospheric ozone, CFC-11, CFC-12, HCFC-22, CCl4, SF6, as well as CF4 which has recently been added to our targets list [Duchatelet et al., 2011]. Trends and associated uncertainties characterizing the available -and often multi-decadal- time series have been derived or updated with a statistical bootstrap resampling tool [Gardiner et al., 2008], they will be presented and critically compared with data available from the literature.
机译:列日大学(ULg)在晴朗的天空条件下,在少女峰高空研究站(瑞士阿尔卑斯山,46.5ºN,3580m asl)上运行着两个最新的傅立叶变换红外(FTIR)光谱仪在大气成分变化检测网络(NDACC)的框架内。 FTIR的常规操作始于1984年。此后一直持续运行,没有中断,使用HgCdTe或InSb探测器以及一套光学装置就可以收集25000至16 µm的45000高分辨率高分辨率宽带红外太阳吸收光谱。过滤器。通常,获得的光谱分辨率在0.003至0.009 cm-1的区间内,而信噪比则达到1000以上。还提供了从1976年到1989年使用光栅仪器记录的大量窄带IR光谱。他们最近开始使用现代工具进行分析[Bader et al。,2011],并将继续将其数据集扩展到1970年代。使用SFIT-1,SFIT-2或PROFFIT-9算法从ULg观测数据库推导出地球物理参数,从而可以生成目标气体的总色谱柱时间序列。另外,使用SFIT-2或PROFFIT-9时,通常都可以得出关于它们的垂直分布随高度的信息,这两种方法均实现了Rodgers [1990]的最佳估计方法。目前,从少女峰的观测中系统地检索了二十多种大气物种,从而可以监测地球大气的关键成分,这些成分在平流层臭氧消耗和/或全球变暖中起着重要作用。本交流将重点关注可从我们的数据库中获得的直接和主要温室气体,即水蒸气,CO2,CH4,N2O,对流层臭氧,CFC-11,CFC-12,HCFC-22,CCl4,SF6以及CF4,最近已添加到我们的目标列表中[Duchatelet等,2011]。趋势和相关的不确定性表征了可用的(通常是数十年时间序列)的特征,并已使用统计自举重采样工具[Gardiner et al。,2008]进行了更新或更新,将对它们进行介绍并与文献中的可用数据进行严格比较。

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