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GEOPHYSICAL RESEARCH LETTERS,
VOL. 26, NO. 10,
PAGES 1373–1376,
1999
Twilight Observations Suggest Unknown Sources of HOx
P. O. Wennberg
California Institute of Technology, Pasadena
R. J. Salawitch
Jet Propulsion Laboratory, California Inst. of Tech., Pasadena
D. J. Donaldson
Department of Chemistry, University of Toronto, Canada
T. F. Hanisco
Department of Chemistry, Harvard University, Cambridge, MA
E. J. Lanzendorf
Department of Chemistry, Harvard University, Cambridge, MA
K. K. Perkins
Department of Chemistry, Harvard University, Cambridge, MA
S. A. Lloyd
Applied Physics Lab., Johns Hopkins Univ., Laurel, MD
V. Vaida
Department of Chemistry, University of Colorado, Boulder
R. S. Gao
NOAA Aeronomy Laboratory, Boulder, CO
E. J. Hintsa
Department of Chemistry, Harvard University, Cambridge, MA
R. C. Cohen
Department of Chemistry, University of California, Berkeley
W. H. Swartz
Applied Physics Lab., Johns Hopkins Univ., Laurel, MD
T. L. Kusterer
Applied Physics Lab., Johns Hopkins Univ., Laurel, MD
D. E. Anderson
Applied Physics Lab., Johns Hopkins Univ., Laurel, MD
Abstract
Measurements of the concentrations of OH and HO2 (HOx) in the high-latitude lower stratosphere imply the existence of unknown photolytic sources of HOx. The strength of the additional HOx source required to match the observations depends only weakly on solar zenith angle (SZA) for 80° < SZA < 93°. The wavelengths
responsible for producing this HOx must be longer than 650 nm because the flux at shorter wavelengths is significantly attenuated at high SZA by scattering
and absorption. Provided that the sources involve only a single photon, the strength of the bonds being broken must be < 45
kcal mole−1. We speculate that peroxynitric acid (HNO4) dissociates after excitation to an unknown excited state with an integrated band cross section of 2-3 × 10−20 cm² molecule−1 nm (650 < λ < 1250 nm).
Received 21
December
1998;
accepted 24
March
1999.
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Citation: Wennberg, P. O., et al.
(1999),
Twilight Observations Suggest Unknown Sources of HOx,
Geophys. Res. Lett.,
26(10),
1373–1376.
Copyright 1999 by the American Geophysical Union.
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