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Stratospheric HBr mixing ratio obtained from far infrared emission spectra

Journal Article · · Geophysical Research Letters (American Geophysical Union); (USA)
 [1];  [2];  [3]
  1. NASA Langley Research Center, Hampton, VA (USA)
  2. Instituto Ricerca Onde Electromagnetiche, CNR, Firenze (Italy)
  3. Universita di Firenze (Italy)
Emission features of HBr isotopes have been identified in high-resolution far-infrared emission spectra obtained with a balloon-born Fourier transform spectrometer in the spring of 1979 at 32{degree}N latitude. When six single-scan spectra at a zenith angle of 93.2{degree} were averaged, two features of HBr isotopes at 50.054 and 50.069 cm{sup {minus}1} were obtained with a signal-to-noise ratio of 2.5. The volume mixing ratio retrieved from the average spectrum is 2.0 {times} 10{sub {minus}11}, which is assumed to be constant above 28 km, with an uncertainty of 35%. 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.
OSTI ID:
5548974
Journal Information:
Geophysical Research Letters (American Geophysical Union); (USA), Journal Name: Geophysical Research Letters (American Geophysical Union); (USA) Vol. 16:8; ISSN 0094-8276; ISSN GPRLA
Country of Publication:
United States
Language:
English