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Stratospheric minor constituent distributions from far-infrared thermal emission spectra

Journal Article · · Journal of Geophysical Research; (United States)
DOI:https://doi.org/10.1029/92JD02083· OSTI ID:6848294
 [1];  [2]
  1. NASA Marshall Space Flight Center, Huntsville, AL (United States)
  2. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
We retrieve mixing ratio profiles of O[sub 3], H[sub 2][sup 16], H[sub 2][sup 17]O,H[sub 2][sup 18]O, HF, and HCl from far-infrared thermal emission observations of the limb in the 80-220 cm[sup [minus]1] spectral region. The observations were made with a balloon-borne Fourier transform spectrometer as a part of the 1983 Balloon Intercomparison Campaign (BIC-2). A subset of the data was analyzed previously using the method in the work of Throb et at [1982, 1991]; in the present paper we use an alternative method of calibration and analysis, given by Abbes et al. [1985]. The retrieved constituent profiles are compared with the measurements made with other instruments on the BIC-2 flights. The results for the concentrations of H[sup 2][sup 17]O and H[sub 2][sup 18]O obtained in this study indicate no isotopic enhancement or depletion with a standard deviation of about 20%. 34 refs., 15 figs., 1 tab.
OSTI ID:
6848294
Journal Information:
Journal of Geophysical Research; (United States), Journal Name: Journal of Geophysical Research; (United States) Vol. 97:D16; ISSN JGREA2; ISSN 0148-0227
Country of Publication:
United States
Language:
English