Ozone isotopologue measurements from the Atmospheric Chemistry Experiment (ACE)
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作者:
Fernando, Anton M.
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Old Dominion Univ, Dept Phys, Norfolk, VA 23529 USAOld Dominion Univ, Dept Phys, Norfolk, VA 23529 USA
Fernando, Anton M.
[1
]
Bernath, Peter E.
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Old Dominion Univ, Dept Phys, Norfolk, VA 23529 USA
Old Dominion Univ, Dept Chem & Biochem, Norfolk, VA 23529 USAOld Dominion Univ, Dept Phys, Norfolk, VA 23529 USA
Bernath, Peter E.
[1
,2
]
Boone, Christopher D.
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Univ Waterloo, Dept Chem, Waterloo, ON, CanadaOld Dominion Univ, Dept Phys, Norfolk, VA 23529 USA
Boone, Christopher D.
[3
]
机构:
[1] Old Dominion Univ, Dept Phys, Norfolk, VA 23529 USA
[2] Old Dominion Univ, Dept Chem & Biochem, Norfolk, VA 23529 USA
[3] Univ Waterloo, Dept Chem, Waterloo, ON, Canada
Near global ozone isotopologue distributions have been determined from infrared solar occultation measurements of the Atmospheric Chemistry Experiment (ACE) satellite mission. ACE measurements are made with a high resolution Fourier transform spectrometer. Annual and seasonal latitudinal fractionation (delta value) distributions of the ozone isotopologues (OOO)-O-16-O-16-O-18, (OOO)-O-16-O-18-O-16 and (OOO)-O-16-O-17-O-16 were obtained. Asymmetric ozone ((OOO)-O-16-O-1-O-6-O-18) shows higher fractionation compared to symmetric ozone ((OOO)-O-16-O-18-O-16). The maximum ozone fractionation occurs in the tropical stratosphere as expected from the contribution of photolysis to the enrichment of heavy isotopologues. An enhancement of the heavy ozone isotopologues is also seen in the upper stratosphere of the Antarctic polar vortex. (C) 2019 Elsevier Ltd. All rights reserved.