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Weak ozone isotopic absorption in the 5 μm region from high resolution FTIR solar spectra

  • A. Goldman
  • , T. M. Stephen
  • , C. P. Rinsland
  • , M. A.H. Smith
  • , A. Perrin
  • , J. M. Flaud
  • , A. Barbe
  • , C. Camy-Peyret
  • , M. T. Coffey
  • , W. G. Mankin
  • , J. W. Hannigan
  • , V. Malathy Devi
  • University of Denver
  • NASA Langley Research Center
  • CNRS
  • Groupe de Spectrométrie Moléculaire et Atmosphérique, URM CNRS 7331, UFR Sciences Exactes et Naturelles, Moulin de la Housse
  • Sorbonne Université
  • National Center for Atmospheric Research
  • College of William and Mary

Research output: Contribution to journalArticlepeer-review

10 Scopus citations

Abstract

Isotopic ozone lines of 16O16O17O and 16O17O16O in the 5 μm region are identified for the first time in balloon-borne high-resolution (0.003 cm-1) solar absorption spectra. A few of these lines also are observed in ground-based spectra. These lines need to be included in analysis of atmospheric absorption spectra, in addition to the recently identified 16O16O18O, 16O18O16O and 16O12C34S lines in this region.

Original languageEnglish
Pages (from-to)133-138
Number of pages6
JournalJournal of Quantitative Spectroscopy and Radiative Transfer
Volume74
Issue number1
DOIs
StatePublished - Jul 1 2002

Keywords

  • Atmospheric ozone isotopomers
  • Infrared Fourier transform atmospheric spectroscopy
  • Solar spectra

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