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Satellite observations of stratospheric hydrogen fluoride and comparisons with SLIMCAT calculations

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posted on 2016-11-15, 10:04 authored by Jeremy J. Harrison, M. P. Chipperfield, C. D. Boone, S. S. Dhomse, P. F. Bernath, L. Froidevaux, J. Anderson, J. Russell
The vast majority of emissions of fluorine-containing molecules are anthropogenic in nature, e.g. chlorofluorocarbons (CFCs), hydrochlorofluorocarbons (HCFCs), and hydrofluorocarbons (HFCs). Many of these fluorine-containing species deplete stratospheric ozone and are regulated by the Montreal Protocol. Once in the atmosphere they slowly degrade, ultimately leading to the formation of hydrogen fluoride (HF), the dominant reservoir of stratospheric fluorine due to its extreme stability. Monitoring the growth of stratospheric HF is therefore an important marker for the success of the Montreal Protocol. We report the comparison of global distributions and trends of HF measured in the Earth's atmosphere by the satellite remote-sensing instruments ACE-FTS (Atmospheric Chemistry Experiment Fourier transform spectrometer), which has been recording atmospheric spectra since 2004, and HALOE (HALogen Occultation Experiment), which recorded atmospheric spectra between 1991 and 2005, with the output of SLIMCAT, a state-of-the-art three-dimensional chemical transport model. In general the agreement between observation and model is good, although the ACE-FTS measurements are biased high by ~10% relative to HALOE. The observed global HF trends reveal a substantial slowing down in the rate of increase of HF since the 1990s: 4.97±0.12%year-1 (1991-1997; HALOE), 1.12±0.08%year-1 (1998-2005; HALOE), and 0.52±0.03%year-1 (2004-2012; ACE-FTS). In comparison, SLIMCAT calculates trends of 4.01, 1.10, and 0.48%year-1, respectively, for the same periods; the agreement is very good for all but the earlier of the two HALOE periods. Furthermore, the observations reveal variations in the HF trends with latitude and altitude; for example, between 2004 and 2012 HF actually decreased in the Southern Hemisphere below 35km. An additional SLIMCAT simulation with repeating meteorology for the year 2000 produces much cleaner trends in HF with minimal variations with latitude and altitude. Therefore, the variations with latitude and altitude in the observed HF trends are due to variability in stratospheric dynamics on the timescale of a few years. Overall, the agreement between observation and model points towards the ongoing success of the Montreal Protocol and the usefulness of HF as a metric for stratospheric fluorine.

Funding

The authors wish to thank the UK Natural Environment Research Council (NERC) for supporting Jeremy J. Harrison through grant NE/I022663/1 and through the National Centre for Earth Observation (NCEO). The ACE satellite mission is funded primarily by the Canadian Space Agency (CSA). HALOE was funded by NASA. Martyn P. Chipperfield and Sandip S. Dhomse thank Wuhu Feng (the National Centre for Atmospheric Science; NCAS) for help with SLIMCAT. Martyn P. Chipperfield is a Royal Society Wolfson Research Merit Award holder. Work at the Jet Propulsion Laboratory was performed under contract with the National Aeronautics and Space Administration (NASA). We thank the ECMWF for providing the ERA-Interim reanalyses used by the SLIMCAT model.

History

Citation

Atmospheric Chemistry and Physics, 2016, 16 (16), pp. 10501-10519

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy

Version

  • VoR (Version of Record)

Published in

Atmospheric Chemistry and Physics

Publisher

European Geosciences Union (EGU), Copernicus Publications

issn

1680-7316

eissn

1680-7324

Acceptance date

2016-07-18

Copyright date

2016

Available date

2016-11-15

Publisher version

http://www.atmos-chem-phys.net/16/10501/2016/

Notes

ACE-FTS data were obtained from https://databace.scisat.ca/ level2/ace_v3.0/ and https://databace.scisat.ca/level2/ace_ v3.5/. HALOE data were obtained from http://haloe.gats-inc. com/home/index.php. The GOZCARDS data used in this work have not been officially released, but will become available via the GOZCARDS website (https://gozcards.jpl.nasa. gov/index.php) at a later date.

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en

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