ATMOS/ATLAS 3 infrared profile measurements of trace gases in the November 1994 tropical and subtropical upper troposphere

被引:29
作者
Rinsland, CP [1 ]
Gunson, MR
Wang, PH
Arduini, RF
Baum, BA
Minnis, P
Goldman, A
Abrams, MC
Zander, R
Mahieu, E
Salawitch, RJ
Michelsen, HA
Irion, FW
Newchurch, MJ
机构
[1] NASA, Langley Res Ctr, Div Atmospher Sci, Hampton, VA 23681 USA
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[3] Sci & Technol Corp, Hampton, VA 23666 USA
[4] Sci Applicat Int Corp, Hampton, VA 23666 USA
[5] Univ Denver, Dept Phys, Denver, CO 80208 USA
[6] ITT Def & Elect, Ft Wayne, IN 46801 USA
[7] Univ Liege, Inst Astrophys, B-4000 Liege, Belgium
[8] Harvard Univ, Div Appl Sci, Cambridge, MA 02138 USA
[9] Univ Alabama, Dept Atmospher Sci, Huntsville, AL 35899 USA
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
D O I
10.1016/S0022-4073(98)00092-2
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Vertical mixing ratio profiles of four relatively long-lives gases, HCN, C2H2, CO, and C2H6, have been retrieved from 0.01 cm(-1) resolution infrared solar occultation spectra recorded between latitudes of 5.3 degrees N and 31.4 degrees N. The observations were obtained by the Atmospheric Trace Molecule Spectroscopy (ATMOS) Fourier transform spectrometer during the Atmospheric Laboratory for Applications and Science (ATLAS) 3 shuttle flight, 3-12 November 1994. Elevated mixing ratios below the tropopause were measured for these gases during several of the occultations. The positive correlations obtained between the simultaneously measured mixing ratios suggest that the enhancements are likely the result of surface emissions, most likely biomass burning and/or urban industrial activities, followed by common injection via deep convective transport of the gases to the upper troposphere. The elevated levels of HCN may account for at least part of the "missing NOy" in the upper troposphere. Comparisons of the observations with values measured during a recent aircraft campaign are presented. Published by Elsevier Science Ltd.
引用
收藏
页码:891 / 901
页数:11
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