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Observations of stratospheric hydrogen fluoride by halogen occultation experiment (HALOE)
Author(s) -
Luo M.,
Cicerone R. J.,
Russell J. M.,
Huang T. Y. W.
Publication year - 1994
Publication title -
journal of geophysical research: atmospheres
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/94jd01246
Subject(s) - hydrogen fluoride , atmospheric sciences , occultation , environmental science , latitude , atmosphere (unit) , polar vortex , altitude (triangle) , stratosphere , climatology , meteorology , geology , physics , chemistry , geodesy , astronomy , inorganic chemistry , geometry , mathematics
The Halogen Occultation Experiment (HALOE) Hydrogen Fluoride (HF) channel on the Upper Atmospheric Research Satellite is providing the first global measurements of stratospheric HF, the dominant fluorine reservoir in the atmosphere. This paper describes the latitudinal and seasonal variations of HALOE‐observed HF in terms of vertical profiles, altitude/latitude cross sections, and column abundances. The HF global distribution shows a “tracerlike” structure and its column amount increases with latitude, in agreement with previous aircraft measurements of the HF column amount. A comparison between the HALOE HF column above 20 km and the ATMOS 1985 measurements is used to estimate the annual rate of increase of stratospheric HF. Exponential rates of 4.9–6.6% yr −1 and linear growth rates of 6–8.6% yr −1 in 1985 and 4.3–5.5% yr −1 in 1992–1993 are found. HALOE HF measurements during the 1993 Antarctic spring are briefly described. This species behaves like a conserved tracer and its distribution shows an area of enhanced mixing ratios correlated with the polar vortex that has a clear latitude boundary. Finally, simulated HF distributions by the National Center for Atmospheric Research two‐dimensional model are used to compare with HALOE observations of HF. Reasonable agreements in the global structure and the absolute amount of HF are found. The differences between the model and the observed results indicate the need for improving treatment of atmospheric dynamics and fluorine‐related chemical parameters in the model simulations.

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