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Dr Scott Osprey FRMetS

Senior NCAS Research Scientist

Research theme

  • Climate physics

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Climate dynamics
  • Predictability of weather and climate
Scott.Osprey@physics.ox.ac.uk
Telephone: 01865 (2)82434,01865 (2)72923
Atmospheric Physics Clarendon Laboratory, room 111
National Centre for Atmospheric Science
SPARC QBOi
Explaining & Predicting Earth System Change
  • About
  • Publications

Toward Improved Understanding and Attribution of Large-Scale Circulation Changes and Associated Extremes: Challenges and Opportunities

Bulletin of the American Meteorological Society American Meteorological Society (2026)

Authors:

Kirsten L Findell, Chaim Garfinkel, June-Yi Lee, Erik Behrens, Leonard Borchert, Lijing Cheng, Annalisa Cherchi, Leandro B Diaz, Andrea Dittus, Stephanie Fiedler, Erich Fischer, Alexia Karwat, Yukiko Imada, Fei Luop, Shoshiro Minobe, Suyeon Moon, Scott Osprey, James Risbey, Tiffany A Shaw, Doug Smith, Andrea K Steiner, Zhuo Wang, Maureen Wanzala, Jonathon S Wright, Jeong-Eun Yun
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Supplementary material to "Revisiting the surface impacts of the QBO in the Large Ensemble Single Forcing MIP simulations: are teleconnections still too weak?"

(2026)

Authors:

Chaim I Garfinkel, David Avisar, Scott M Osprey, Doug Smith, Jian Rao, Jonathon S Wright
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Relative roles of different tropical oceans on the weakening of the stratospheric equatorial quasi-biennial oscillation

npj Climate and Atmospheric Science Nature Research (2026)

Authors:

Yue Wang, Jian Rao, Chaim I Garfinkel, Rongcai Ren, Scott M Osprey, Yixiong Lu

Abstract:

The Quasi-Biennial Oscillation (QBO) is the dominant mode of tropical stratospheric variability that modulates global circulation and climate. Although a long-term weakening of QBO amplitude has been observed under global warming, the relative roles of different tropical oceans remain unclear. We perform sensitivity experiments forced by sea surface temperature perturbations over the tropical Pacific, Atlantic, and Indian Oceans, as well as their combined warming, to separate individual and joint effects. Pacific warming produces the strongest weakening and slowest descent of the QBO, whereas Atlantic warming slightly strengthens the amplitude and extends the vertical structure. Indian Ocean warming slightly weakens the amplitude and accelerates the descent. When all three oceans warm simultaneously, the QBO exhibits a weaker amplitude and faster descent, consistent in sign with the combined single-basin responses but with a reduced magnitude owing to diminished zonal and inter-basin SST gradients. Momentum budget analyses further show that basin-dependent competition between equatorial wave forcing and tropical upwelling underlies these contrasting responses.
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QBOi El Niño Southern Oscillation experiments: assessing relationships between ENSO, MJO, and QBO

Weather and Climate Dynamics Copernicus Publications 7:1 (2026) 317-339

Authors:

Dillon Elsbury, Federico Serva, Julie M Caron, Seung-Yoon Back, Clara Orbe, Jadwiga H Richter, James A Anstey, Neal Butchart, Chih-Chieh Chen, Javier García-Serrano, Anne Glanville, Yoshio Kawatani, Tobias Kerzenmacher, Francois Lott, Hiroaki Naoe, Scott Osprey, Froila M Palmeiro, Seok-Woo Son, Masakazu Taguchi, Stefan Versick, Shingo Watanabe, Kohei Yoshida

Abstract:

Abstract. This study uses an ensemble of climate model experiments coordinated by the Quasi-Biennial Oscillation initiative (QBOi) to analyze the Madden-Julian Oscillation (MJO) in the presence of either perpetual El Niño or La Niña sea surface temperatures during boreal winter. In addition to the prescribed El Niño Southern Oscillation (ENSO) conditions, the nine models internally generate QBOs, meaning each may influence the MJO. Objectives of our analyses are to assess the response of the MJO to strong idealized ENSO forcing and look for evidence of a QBO influence on the MJO in a multi-model context. The diagnostics used include wavenumber-frequency spectra of tropical convective and dynamical fields, measures of MJO lifetime, an evaluation of MJO diversity and visualization of MJO vertical structure, as well as an assessment of QBO morphology and the QBO's impact on tropical convection. Kelvin wave spectral power increases in the El Niño simulations whereas equatorial Rossby waves power is stronger in the La Niña simulations. All models simulate faster MJO propagation under El Niño conditions. This change in speed is corroborated by the MJO diversity analysis, which reveals that models better reproduce the observed “fast propagating” and “standing” MJO archetypes given perpetual El Niño and La Niña, respectively. Regardless of ENSO, QBO descent into the lower stratosphere is underestimated and we detect little QBO influence on tropical tropopause stability and MJO activity. With little influence from the QBO on the MJO activity in these runs, we can be confident that the aforementioned changes in the MJO indeed arise from the different ENSO boundary conditions.
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On complex network techniques for atmospheric flow analysis: a polar vortex case study

Journal of Physics: Complexity IOP Publishing (2025)

Authors:

María Reboredo Prado, Renaud Lambiotte, Irene Moroz, Scott Osprey

Abstract:

<jats:title>Abstract</jats:title> <jats:p>Atmospheric flow underpins virtually all meteorological and climatological phenomena, yet extracting meaningful features from its dynamics remains a major scientific challenge due to its high dimensionality, multi-scale behaviour, and inherent nonlinearity. In this study, we investigate the potential of a network-based framework to reveal the relationships between distinct flow structures. Specifically, we apply three techniques, independent of any particular phenomenon or model, to explore patterns of coherence and information transfer, vortical interactions, and Lagrangian coherent structures. We assess their utility using a rotating shallow-water model of the stratospheric polar vortex, which reproduces key aspects of wintertime dynamics, including sudden stratospheric warming split events. Our results support three central claims. First, the transformation of fluid flow data into a network representation preserves essential dynamical information. Second, this representation enables a more accessible and structured analysis of the underlying dynamical structures. Third, multiple types of networks can be constructed from atmospheric flow data, each offering distinct yet complementary insights into the system’s collective behaviour. Together, these findings highlight the potential of network-based approaches as valuable tools in atmospheric research.</jats:p>
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