Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
Menu
Juno Jupiter image

Professor Lesley Gray

Emeritus

Research theme

  • Climate physics

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Climate dynamics
lesley.gray@retired.ox.ac.uk
Telephone: 01865 (2)72909
Atmospheric Physics Clarendon Laboratory, room 109
  • About
  • Publications

Uncertainty in the response of sudden stratospheric warmings and stratosphere‐troposphere coupling to quadrupled CO2 concentrations in CMIP6 models

Journal of Geophysical Research: Atmospheres American Geophysical Union 125:6 (2020) e2019JD032345

Authors:

B Ayarzagüena, AJ Charlton-Perez, AH Butler, P Hitchcock, IR Simpson, LM Polvani, N Butchart, EP Gerber, L Gray, B Hassler, P Lin, F Lott, E Manzini, R Mizuta, C Orbe, S Osprey, D Saint-Martin, M Sigmond, M Taguchi, EM Volodin, S Watanabe

Abstract:

Major sudden stratospheric warmings (SSWs), vortex formation and final breakdown dates are key highlight points of the stratospheric polar vortex. These phenomena are relevant for stratosphere‐troposphere coupling, which explains the interest in understanding their future changes. However, up to now, there is not a clear consensus on which projected changes to the polar vortex are robust, particularly in the Northern Hemisphere, possibly due to short data record or relatively moderate CO2 forcing. The new simulations performed under the Coupled Model Intercomparison Project, Phase 6, together with the long daily data requirements of the DynVarMIP project in preindustrial and quadrupled CO2 (4xCO2) forcing simulations provide a new opportunity to revisit this topic by overcoming the limitations mentioned above. In this study, we analyze this new model output to document the change, if any, in the frequency of SSWs under 4xCO2 forcing. Our analysis reveals a large disagreement across the models as to the sign of this change, even though most models show a statistically significant change. As for the near‐surface response to SSWs, the models, however, are in good agreement as to this signal over the North Atlantic: there is no indication of a change under 4xCO2 forcing. Over the Pacific, however, the change is more uncertain, with some indication that there will be a larger mean response. Finally, the models show robust changes to the seasonal cycle in the stratosphere. Specifically, we find a longer duration of the stratospheric polar vortex, and thus a longer season of stratosphere‐troposphere coupling.
More details from the publisher
Details from ORA
More details

Evaluation of the Quasi‐Biennial Oscillation in global climate models for the SPARC QBO‐initiative

Quarterly Journal of the Royal Meteorological Society Wiley (2020) qj.3765

Authors:

AC Bushell, JA Anstey, N Butchart, Y Kawatani, SM Osprey, JH Richter, F Serva, P Braesicke, C Cagnazzo, C‐C Chen, H‐Y Chun, RR Garcia, LJ Gray, K Hamilton, T Kerzenmacher, Y‐H Kim, F Lott, C McLandress, H Naoe, J Scinocca, AK Smith, TN Stockdale, S Versick, S Watanabe, K Yoshida, S Yukimoto
More details from the publisher
More details

The equatorial stratospheric semiannual oscillation and time‐mean winds in QBOi models

Quarterly Journal of the Royal Meteorological Society Wiley 148:744A (2020) 1593-1609

Authors:

AK Smith, LA Holt, RR Garcia, JA Anstey, F Serva, N Butchart, Scott Osprey, AC Bushell, Y Kawatani, Y Kim, F Lott, P Braesicke, C Cagnazzo, C Chen, H Chun, L Gray, T Kerzenmacher, H Naoe, J Richter, S Versick, V Schenzinger, S Watanabe, K Yoshida

Abstract:

The Quasi‐Biennial Oscillation initiative (QBOi) is a model intercomparison programme that specifically targets simulation of the QBO in current global climate models. Eleven of the models or model versions that participated in a QBOi intercomparison study have upper boundaries in or above the mesosphere and therefore simulate the region where the stratopause semiannual oscillation (SAO) is the dominant mode of variability of zonal winds in the tropical upper stratosphere. Comparisons of the SAO simulations in these models are presented here. These show that the model simulations of the amplitudes and phases of the SAO in zonal‐mean zonal wind near the stratopause agree well with the information derived from available observations. However, most of the models simulate time‐average zonal winds that are more westward than determined from observations, in some cases by several tens of m·s–1. Validation of wave activity in the models is hampered by the limited observations of tropical waves in the upper stratosphere but suggests a deficit of eastward forcing either by large‐scale waves, such as Kelvin waves, or by gravity waves.
More details from the publisher
Details from ORA
More details

Extreme weather events in early summer 2018 connected by a recurrent hemispheric wave-7 pattern

Environmental Research Letters IOP Publishing 14:5 (2019) 054002

Authors:

K Kornhuber, Scott Osprey, D Coumou, S Petri, V Petoukhov, S Rahmstorf, L Gray

Abstract:

The summer of 2018 witnessed a number of extreme weather events such as heatwaves in North America, Western Europe and the Caspian Sea region, and rainfall extremes in South-East Europe and Japan that occurred near-simultaneously. Here we show that some of these extremes were connected by an amplified hemisphere-wide wavenumber 7 circulation pattern. We show that this pattern constitutes an important teleconnection in Northern Hemisphere summer associated with prolonged and above-normal temperatures in North America, Western Europe and the Caspian Sea region. This pattern was also observed during the European heatwaves of 2003, 2006 and 2015 among others. We show that the occurrence of this wave 7 pattern has increased over recent decades.
More details from the publisher
Details from ORA
More details

Slowdown of the Walker circulation at solar cycle maximum

Proceedings of the National Academy of Sciences National Academy of Sciences 116:15 (2019) 7186-7191

Authors:

S Misios, Lesley Gray, M Knudsen, C Karoff, H Schmidt, J Haigh

Abstract:

The Pacific Walker Circulation (PWC) fluctuates on interannual and multidecadal timescales under the influence of internal variability and external forcings. Here, we provide observational evidence that the 11-y solar cycle (SC) affects the PWC on decadal timescales. We observe a robust reduction of east–west sea-level pressure gradients over the Indo-Pacific Ocean during solar maxima and the following 1–2 y. This reduction is associated with westerly wind anomalies at the surface and throughout the equatorial troposphere in the western/central Pacific paired with an eastward shift of convective precipitation that brings more rainfall to the central Pacific. We show that this is initiated by a thermodynamical response of the global hydrological cycle to surface warming, further amplified by atmosphere–ocean coupling, leading to larger positive ocean temperature anomalies in the equatorial Pacific than expected from simple radiative forcing considerations. The observed solar modulation of the PWC is supported by a set of coupled ocean–atmosphere climate model simulations forced only by SC irradiance variations. We highlight the importance of a muted hydrology mechanism that acts to weaken the PWC. Demonstration of this mechanism acting on the 11-y SC timescale adds confidence in model predictions that the same mechanism also weakens the PWC under increasing greenhouse gas forcing.
More details from the publisher
Details from ORA
More details
More details

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 2
  • Page 3
  • Page 4
  • Page 5
  • Current page 6
  • Page 7
  • Page 8
  • Page 9
  • Page 10
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Current students
  • Staff intranet