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Dynamics of the Remarkable Southern Hemisphere Winter of 2024Typical Southern Hemisphere (SH) stratospheric winters are characterized by relatively weak planetary wave dynamics when compared to the Northern Hemisphere winter, especially in early and mid-winter. However, the SH stratospheric winter 2024 saw the development of two large wave events in July. These wave events were associated with the slowing of the polar vortex winds and positive polar temperature anomalies. The second of these two events saw the development of a zonal wavenumber two that was larger in amplitude than seen in the 1980-present record from the Modern Era Retrospective Analysis for Research and Applications – version 2 (MERRA-2). Here we present diagnostics characterizing the wave and mean circulation such as EP (Eliassen-Palm Flux) and residual mean meridional circulation during these events and trace the origin of these stratospheric disturbances to the troposphere. Results show the increase in wave activity associated with the slowing of the zonal wind and the increase in the strength of the poleward and downward circulation associated with the warm anomaly. Analysis of the wave and circulation anomalies will continue through September 2024.
Document ID
20240015660
Acquisition Source
Goddard Space Flight Center
Document Type
Presentation
Authors
Lawrence Coy
(Science Systems and Applications (United States) Lanham, Maryland, United States)
Paul A Newman
(Goddard Space Flight Center Greenbelt, United States)
Steven Pawson
(Goddard Space Flight Center Greenbelt, United States)
Date Acquired
December 6, 2024
Subject Category
Earth Resources and Remote Sensing
Meeting Information
Meeting: AGU Fall Meeting 2024
Location: Washington, DC
Country: US
Start Date: December 9, 2024
End Date: December 13, 2024
Sponsors: American Geophysical Union
Funding Number(s)
CONTRACT_GRANT: NNG17HP01C
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
NASA Peer Committee
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