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Deriving Global OH Abundance and Atmospheric Lifetimes for Long-Lived Gases: A Search for CH3CCl3 Alternatives.
Liang, Qing; Chipperfield, Martyn P; Fleming, Eric L; Abraham, N Luke; Braesicke, Peter; Burkholder, James B; Daniel, John S; Dhomse, Sandip; Fraser, Paul J; Hardiman, Steven C; Jackman, Charles H; Kinnison, Douglas E; Krummel, Paul B; Montzka, Stephen A; Morgenstern, Olaf; McCulloch, Archie; Mühle, Jens; Newman, Paul A; Orkin, Vladimir L; Pitari, Giovanni; Prinn, Ronald G; Rigby, Matthew; Rozanov, Eugene; Stenke, Andrea; Tummon, Fiona; Velders, Guus J M; Visioni, Daniele; Weiss, Ray F.
  • Liang Q; Atmospheric Chemistry and Dynamics Laboratory, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA.
  • Chipperfield MP; Universities Space Research Association, GESTAR, Columbia, Maryland, USA.
  • Fleming EL; National Centre for Earth Observation, School of Earth and Environment, University of Leeds, Leeds, UK.
  • Abraham NL; Atmospheric Chemistry and Dynamics Laboratory, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA.
  • Braesicke P; Science Systems and Applications, Inc, Lanham, Maryland, USA.
  • Burkholder JB; National Centre for Atmospheric Science, Leeds, UK.
  • Daniel JS; Department of Chemistry, University of Cambridge, Cambridge, UK.
  • Dhomse S; Karlsruhe Institute of Technology, Karlsruhe, Germany.
  • Fraser PJ; Chemical Sciences Division, NOAA Earth System Research Laboratory, Boulder, Colorado, USA.
  • Hardiman SC; Chemical Sciences Division, NOAA Earth System Research Laboratory, Boulder, Colorado, USA.
  • Jackman CH; National Centre for Earth Observation, School of Earth and Environment, University of Leeds, Leeds, UK.
  • Kinnison DE; Climate Science Centre, CSIRO Oceans and Atmosphere, Aspendale, Vic, Australia.
  • Krummel PB; Met Office Hadley Centre, Exeter, UK.
  • Montzka SA; Atmospheric Chemistry and Dynamics Laboratory, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA.
  • Morgenstern O; National Center for Atmospheric Research, Boulder, Colorado, USA.
  • McCulloch A; Climate Science Centre, CSIRO Oceans and Atmosphere, Aspendale, Vic, Australia.
  • Mühle J; Global Monitoring Division, NOAA Earth System Research Laboratory, Boulder, Colorado, USA.
  • Newman PA; National Institute of Water and Atmospheric Research, Wellington, New Zealand.
  • Orkin VL; School of Chemistry, University of Bristol, Bristol, UK.
  • Pitari G; Scripps Institution of Oceanography, University of California, San Diego, La Jolla, California, USA.
  • Prinn RG; Atmospheric Chemistry and Dynamics Laboratory, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA.
  • Rigby M; National Institute of Standards and Technology, Gaithersburg, Maryland, USA.
  • Rozanov E; Department of Physical and Chemical Sciences, Università dell'Aquila, L'Aquila, Italy.
  • Stenke A; Massachusetts Institute of Technology, Cambridge, Massachusetts, USA.
  • Tummon F; School of Chemistry, University of Bristol, Bristol, UK.
  • Velders GJM; Institute for Atmospheric and Climate Science, ETH Zurich, Zurich, Switzerland.
  • Visioni D; Physikalisch-Meteorologisches Observatorium Davos World Radiation Centre, Davos Dorf, Switzerland.
  • Weiss RF; Institute for Atmospheric and Climate Science, ETH Zurich, Zurich, Switzerland.
J Geophys Res Atmos ; 122(21): 11914-11933, 2017 Nov 16.
Article en En | MEDLINE | ID: mdl-38515436
ABSTRACT
An accurate estimate of global hydroxyl radical (OH) abundance is important for projections of air quality, climate, and stratospheric ozone recovery. As the atmospheric mixing ratios of methyl chloroform (CH3CCl3) (MCF), the commonly used OH reference gas, approaches zero, it is important to find alternative approaches to infer atmospheric OH abundance and variability. The lack of global bottom-up emission inventories is the primary obstacle in choosing a MCF alternative. We illustrate that global emissions of long-lived trace gases can be inferred from their observed mixing ratio differences between the Northern Hemisphere (NH) and Southern Hemisphere (SH), given realistic estimates of their NH-SH exchange time, the emission partitioning between the two hemispheres, and the NH versus SH OH abundance ratio. Using the observed long-term trend and emissions derived from the measured hemispheric gradient, the combination of HFC-32 (CH2F2), HFC-134a (CH2FCF3, HFC-152a (CH3CHF2), and HCFC-22 (CHClF2), instead of a single gas, will be useful as a MCF alternative to infer global and hemispheric OH abundance and trace gas lifetimes. The primary assumption on which this multispecies approach relies is that the OH lifetimes can be estimated by scaling the thermal reaction rates of a reference gas at 272 K on global and hemispheric scales. Thus, the derived hemispheric and global OH estimates are forced to reconcile the observed trends and gradient for all four compounds simultaneously. However, currently, observations of these gases from the surface networks do not provide more accurate OH abundance estimate than that from MCF.