Stratospheric HBr mixing ratio obtained from far infrared emission spectra
Emission features of HBr isotopes have been identified in high-resolution FIR emission spectra obtained with a balloon-borne Fourier-transform spectrometer in the spring of 1979 at 32 deg N latitude. When six single-scan spectra at a zenith angle of 93.2 deg were averaged, two features of HBr isotop...
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Published in | Geophysical research letters Vol. 16; no. 8; pp. 787 - 790 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Legacy CDMS
Blackwell Publishing Ltd
01.08.1989
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Subjects | |
Online Access | Get full text |
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Summary: | Emission features of HBr isotopes have been identified in high-resolution FIR emission spectra obtained with a balloon-borne Fourier-transform spectrometer in the spring of 1979 at 32 deg N latitude. When six single-scan spectra at a zenith angle of 93.2 deg were averaged, two features of HBr isotopes at 50.054 and 50.069/cm were obtained with a signal-to-noise ratio of 2.5. The volume mixing ratio retrieved from the average spectrum is 2.0 x 10 to the -11th, which is assumed to be constant above 28 km, with an uncertainty of 35 percent. This stratospheric amount of HBr is about the same as the current level of tropospheric organic bromine compounds, 25 pptv. Thus HBr could be the major stratospheric bromine species. |
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Bibliography: | istex:1AF28DC78AC7082E05B04271905140E5D4083C73 ArticleID:89GL01195 ark:/67375/WNG-P82F2MCX-L CDMS Legacy CDMS ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 ObjectType-Article-2 ObjectType-Feature-1 |
ISSN: | 0094-8276 1944-8007 |
DOI: | 10.1029/GL016i008p00787 |