On the Abnormally Strong Westward Phase of the Mesospheric Semiannual Oscillation at Low Latitudes During March Equinox 2023

Abstract Different meteor radars at low latitudes observed abnormally strong westward mesospheric winds around the March Equinox of 2023, that is, during the first phase of the Mesospheric Semiannual Oscillation. This event was the strongest of at least the last decade (2014–2023). The westward winds reached −80 m/s at 82 km of altitude in late March, and decreased with increasing altitude and latitude. A considerable increase in the diurnal tide amplitude was also observed. The Whole Atmosphere Community Climate Model with thermosphere‐ionosphere eXtension constrained to meteorological reanalysis up to ∼50 km does not capture the observed low‐latitude behavior. Additionally, these strong mesospheric winds developed during the westerly phase of the Quasi‐Biennial Oscillation, in accordance with the filtering mechanism of gravity waves in the stratosphere proposed in previous works. Finally, analysis of SABER temperatures strongly suggests that the breaking of the migrating diurnal tide may be the main driver of these strong winds.

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Publication Details

Journal
Geophysical Research Letters
Published
2024-08-13
DOI
https://doi.org/10.1029/2024gl110331
Citations
5
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
1.66

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article

On the Abnormally Strong Westward Phase of the Mesospheric Semiannual Oscillation at Low Latitudes During March Equinox 2023

Danny Scipión, N. M. Pedatella, S. Vijaya Bhaskara Rao, M. Venkat Ratnam et al.
5 citations
Geophysical Research Letters
Ionosphere and magnetosphere dynamics
1.66
article

On the Abnormally Strong Westward Phase of the Mesospheric Semiannual Oscillation at Low Latitudes During March Equinox 2023

Danny Scipión, N. M. Pedatella, S. Vijaya Bhaskara Rao, M. Venkat Ratnam, Guozhu Li, J. Federico Conte, Rodolfo Rodríguez, Rolando R. García, Lourivaldo Mota Lima, José Suclupe, Jorge L. Chau, Kaoru Sato, Christoph Zülicke
article en
5 citations

Abstract

Abstract Different meteor radars at low latitudes observed abnormally strong westward mesospheric winds around the March Equinox of 2023, that is, during the first phase of the Mesospheric Semiannual Oscillation. This event was the strongest of at least the last decade (2014–2023). The westward winds reached −80 m/s at 82 km of altitude in late March, and decreased with increasing altitude and latitude. A considerable increase in the diurnal tide amplitude was also observed. The Whole Atmosphere Community Climate Model with thermosphere‐ionosphere eXtension constrained to meteorological reanalysis up to ∼50 km does not capture the observed low‐latitude behavior. Additionally, these strong mesospheric winds developed during the westerly phase of the Quasi‐Biennial Oscillation, in accordance with the filtering mechanism of gravity waves in the stratosphere proposed in previous works. Finally, analysis of SABER temperatures strongly suggests that the breaking of the migrating diurnal tide may be the main driver of these strong winds.

Geophysical Research LettersVol. 51(16)
NSF National Center for Atmospheric Research (US), NSF NCAR High Altitude Observatory (US), Universidade Estadual da Paraíba (BR), National Atmospheric Research Laboratory (IN), University of Piura (PE), Sri Venkateswara University (IN), Chinese Academy of Sciences (CN), Institute of Geology and Geophysics (CN), Leibniz Institute of Atmospheric Physics at the Rostock University (DE), Instituto Geofísico del Perú (PE), University of Rostock (DE), The University of Tokyo (JP)
National Science Foundation, National Aeronautics and Space Administration, National Natural Science Foundation of China, Nuclear Safety and Security Commission, Leibniz-Gemeinschaft, Japan Society for the Promotion of Science
Climate action
Openalex Percentile: Top 17%
Ionosphere and magnetosphere dynamics
1.66
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