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Analysis of present day and future OH and methane lifetime in the ACCMIP simulations

Research output: Contribution to journalJournal article

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  • A. Voulgarakis
  • Vaishali Naik
  • J. F. Lamarque
  • Drew T. Shindell
  • Michael J. Prather
  • R. D. Field
  • D. Bergmann
  • Philip Cameron-Smith
  • I Cionni
  • William J. Collins
  • Stig B Dalsoren
  • R. M. Doherty
  • V. Eyring
  • G. Folberth
  • L. W. Horowitz
  • B Josse
  • Ian A. MacKenzie
  • T Nagashima
  • David A Plummer
  • M Righi
  • S Rumbold
  • D. S. Stevenson
  • Sarah Strode
  • K. Sudo
  • Sophie Szopa
  • Guang Zeng
Journal publication date5/03/2013
JournalAtmospheric Chemistry and Physics
Journal number5
Volume13
Number of pages25
Pages2563-2587
Original languageEnglish

Abstract

Results from simulations performed for the Atmospheric Chemistry and Climate Modeling Intercomparison Project (ACCMIP) are analysed to examine how OH and methane lifetime may change from present day to the future, under different climate and emissions scenarios. Present day (2000) mean tropospheric chemical lifetime derived from the ACCMIP multi-model mean is 9.8±1.6 yr (9.3±0.9 yr when only including selected models), lower than a recent observationally-based estimate but with a similar range to previous multi-model estimates. Future model projections are based on the four Representative Concentration Pathways (RCPs), and the results also exhibit a large range. Decreases in global methane lifetime of 4.5±9.1% are simulated for the scenario with lowest radiative forcing by 2100 (RCP 2.6), while increases of 8.5±10.4% are simulated for the scenario with highest radiative forcing (RCP 8.5). In this scenario, the key driver of the evolution of OH and methane lifetime is methane itself, since its concentration more than doubles by 2100 and it consumes much of the OH that exists in the troposphere. Stratospheric ozone recovery, which drives tropospheric OH decreases through photolysis modifications, also plays a partial role. In the other scenarios, where methane changes are less drastic, the interplay between various competing drivers leads to smaller and more diverse OH and methane lifetime responses, which are difficult to attribute. For all scenarios, regional OH changes are even more variable, with the most robust feature being the large decreases over the remote oceans in RCP8.5. Through a regression analysis, we suggest that differences in emissions of non-methane volatile organic compounds and in the simulation of photolysis rates may be the main factors causing the differences in simulated present day OH and methane lifetime. Diversity in predicted changes between present day and future OH was found to be associated more strongly with differences in modelled temperature and stratospheric ozone changes. Finally, through perturbation experiments we calculated an OH feedback factor (F) of 1.24 from present day conditions (1.50 from 2100 RCP8.5 conditions) and a climate feedback on methane lifetime of 0.33±0.13 yr K−1 , on average. Models that did not include interactive stratospheric ozone effects on photolysis showed a stronger sensitivity to climate, as they did not account for negative effects of climate-driven stratospheric ozone recovery on tropospheric OH, which would have partly offset the overall OH/methane lifetime response to climate change.

Bibliographic note

© Author(s) 2013. This work is distributed under the Creative Commons Attribution 3.0 License.

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