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Volume 16, issue 5
Atmos. Chem. Phys., 16, 3265-3278, 2016
https://doi.org/10.5194/acp-16-3265-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.
Atmos. Chem. Phys., 16, 3265-3278, 2016
https://doi.org/10.5194/acp-16-3265-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.

Research article 11 Mar 2016

Research article | 11 Mar 2016

Upper tropospheric water vapour variability at high latitudes – Part 1: Influence of the annular modes

Christopher E. Sioris1, Jason Zou2, David A. Plummer3, Chris D. Boone4, C. Thomas McElroy1, Patrick E. Sheese2, Omid Moeini1, and Peter F. Bernath4,5 Christopher E. Sioris et al.
  • 1Department of Earth and Space Science and Engineering, York University, 4700 Keele St., Toronto, ON, M3J 1P3, Canada
  • 2Department of Physics, University of Toronto, 60 St. George Street, Toronto, ON, M5S 1A7, Canada
  • 3Canadian Centre for Climate Modelling and Analysis, Environment Canada, Victoria, BC, Canada
  • 4Department of Chemistry, University of Waterloo, 200 University Ave. W, Waterloo, ON, N2L 3G1, Canada
  • 5Department of Chemistry & Biochemistry, Old Dominion University, 4541 Hampton Blvd., Norfolk, VA 23529, USA

Abstract. Seasonal and monthly zonal medians of water vapour in the upper troposphere and lower stratosphere (UTLS) are calculated for both Atmospheric Chemistry Experiment (ACE) instruments for the northern and southern high-latitude regions (60–90°N and 60–90°S). Chosen for the purpose of observing high-latitude processes, the ACE orbit provides sampling of both regions in 8 of 12 months of the year, with coverage in all seasons. The ACE water vapour sensors, namely MAESTRO (Measurements of Aerosol Extinction in the Stratosphere and Troposphere Retrieved by Occultation) and the Fourier Transform Spectrometer (ACE-FTS) are currently the only satellite instruments that can probe from the lower stratosphere down to the mid-troposphere to study the vertical profile of the response of UTLS water vapour to the annular modes.

The Arctic oscillation (AO), also known as the northern annular mode (NAM), explains 64 % (r = −0.80) of the monthly variability in water vapour at northern high latitudes observed by ACE-MAESTRO between 5 and 7 km using only winter months (January to March, 2004–2013). Using a seasonal time step and all seasons, 45% of the variability is explained by the AO at 6.5±0.5 km, similar to the 46 % value obtained for southern high latitudes at 7.5±0.5 km explained by the Antarctic oscillation or southern annular mode (SAM). A large negative AO event in March 2013 produced the largest relative water vapour anomaly at 5.5km (+70 %) over the ACE record. A similarly large event in the 2010 boreal winter, which was the largest negative AO event in the record (1950–2015), led to >50 % increases in water vapour observed by MAESTRO and ACE-FTS at 7.5 km.

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The AM (annular mode) is the most important internal mode of climatic variability at high latitudes. Upper tropospheric water vapour (UTWV) at high latitudes increases by up to ~ 50 % during the negative phase of the AMs. The response of water vapour to the AMs vanishes above the tropopause. The ultimate goal of the study was to improve UTWV trend uncertainties by explaining shorter-term variability, and this was achieved by accounting for the AM-related response in a multiple linear regression.
The AM (annular mode) is the most important internal mode of climatic variability at high...
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