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Airborne observations of the composition of the 1992 tropical stratosphere by FTIR solar absorption spectrometry

Journal Article · · Geophysical Research Letters (American Geophysical Union); (United States)
DOI:https://doi.org/10.1029/93GL01962· OSTI ID:5108336
; ; ;  [1]
  1. California Institute of Technology, Pasadena, CA (United States)
Vertical column measurements of the gaseous composition of the tropical stratosphere were made from the NASA DC-8 aircraft early in 1992. As anticipated, the burdens of the stratospheric source gases (e.g., O[sub 3], HF, HCl, ClNO[sub 3], HNO[sub 3]) were reduced from their mid-latitude values due to increased uplift and photolysis. The tracers revealed considerably more uplift near the equator than the sub-tropics. For example, the HF burdens at [+-]20[degrees] latitude (0.50[times]10[sup 15] molec.cm[sup [minus]2]) were nearly double those at 5[degrees]N (0.27[times]10[sup 15] molec.cm[sup [minus]2]). This, together with results obtained from other long-lived gases (e.g., N[sub 2]O, CH[sub 4], CF[sub 2]Cl[sub 2]) indicates that volume mixing ratios found at 22 km altitude at mid-latitudes occurred at 26 km in the sub-tropics and at 30 km in the equatorial zone. This zone of uplift was symmetrical about the equator even though the sun was overhead at 20[degrees]S. 14 refs., 4 figs., 1 tab.
OSTI ID:
5108336
Journal Information:
Geophysical Research Letters (American Geophysical Union); (United States), Journal Name: Geophysical Research Letters (American Geophysical Union); (United States) Vol. 20:22; ISSN GPRLAJ; ISSN 0094-8276
Country of Publication:
United States
Language:
English