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 inGeophysical research letters Vol. 16; no. 8; pp. 787 - 790
Main Authors Park, J. H., Carli, B., Barbis, A.
Format Journal Article
LanguageEnglish
Published Legacy CDMS Blackwell Publishing Ltd 01.08.1989
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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.
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