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AGU: Geophysical Research Letters

 

Index Terms

  • Atmospheric Composition and Structure: Chemical kinetic and photochemical properties
  • Atmospheric Composition and Structure
  • Atmospheric Composition and Structure: Geochemical cycles

Abstract

GEOPHYSICAL RESEARCH LETTERS, VOL. 29, 1456, 4 PP., 2002
doi:10.1029/2001GL013851

High resolution spectroscopy of the OIO radical: Implications for the ozone-depleting potential of iodine

Stephen H. Ashworth

School of Chemical Sciences, University of East Anglia, Norwich, UK

Beverley J. Allan

School of Environmental Sciences, University of East Anglia, Norwich, UK

John M. C. Plane

School of Environmental Sciences, University of East Anglia, Norwich, UK

The absorption spectrum of iodine dioxide (OIO), obtained at high resolution between 540 and 605 nm by cavity ring-down spectroscopy, exhibits no evidence of coarse rotational structure. Furthermore, a laser induced fluorescence spectrum was not observed when pumping the molecule in this region of the visible spectrum. Ab initio quantum calculations were performed on the ground and first excited states of OIO. The rotational envelopes of the observed absorption bands are very satisfactorily simulated if the lifetime of the excited state is 200 ± 50 fs, indicating prompt predissociation. Quantum calculations indicate photolysis to I + O2, rather than O + IO. The estimated photodissociation rate of OIO in daylight ranges from 0.36 to 2.2 s−1, depending on the choice of absolute cross-section, which explains why OIO has only been observed in the atmosphere after sunset. Photolysis to yield atomic I will enhance the O3-depleting potential of iodine in the remote marine boundary layer.

Published 25 May 2002.

Citation: Ashworth, S. H., B. J. Allan, and J. M. C. Plane (2002), High resolution spectroscopy of the OIO radical: Implications for the ozone-depleting potential of iodine, Geophys. Res. Lett., 29(10), 1456, doi:10.1029/2001GL013851.

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