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Abstract
An unusual sudden stratospheric warming (SSW) event occurred in the Southern Hemisphere in September 2019. Ground-based and satellite observations show the presence of transient eastward- and westward-propagating quasi-10 day planetary waves (Q10DWs) during the SSW. The planetary wave activity maximizes in the mesosphere and lower thermosphere region approximately 10 days after the SSW onset. Analysis indicates that the westward-propagating Q10DW with zonal wave number s = 1 is mainly symmetric about the equator, which is contrary to theory which predicts the presence of an antisymmetric normal mode for such planetary wave. Observations from microwave limb sounder and sounding of the atmosphere using broadband emission radiometry are combined with meteor radar wind measurements from Antarctica, providing a comprehensive view of Q10DW wave activity in the Southern Hemisphere during this SSW. Analysis suggests that the Q10DWs of various wavenumbers are potentially excited from nonlinear wave-wave interactions that also involve stationary planetary waves with s = 1 and s = 2. The Q10DWs are also found to couple the ionosphere with the neutral atmosphere. The timing of the quasi-10-day oscillations (Q10DOs) in the ionosphere are contemporaneous with the Q10DWs in the neutral atmosphere during a period of relatively low solar and geomagnetic activity, suggesting that the Q10DWs play a key role in driving the ionospheric Q10DOs during the Southern SSW event. This study provides observational evidence for coupling between the neutral atmosphere and ionosphere through the upward propagation of global scale planetary waves.
Original language | English |
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Article number | e2021JA029286 |
Journal | Journal of Geophysical Research: Space Physics |
Volume | 126 |
Issue number | 6 |
Early online date | 8 Jun 2021 |
DOIs | |
Publication status | Published - 30 Jun 2021 |
Funding
This research was supported by NSF grant AGS‐1552286, part of the CEDAR program under the direction of Dr. Scott Palo. The meteor radar located at McMurdo Station was supported by NSF grant OPP‐1543446. J.M. Forbes was supported under Award AGS‐1630177 from the NSF Aeronomy Program. T. Moffat‐Griffin and N.J. Mitchell are supported by the UK Natural Environment Research Council (grant nos. NE/R001391/1 and NE/R001235/1). This work was performed while J.C. Wang held a Government Scholarship for Study Abroad awarded by the Ministry of Education, Taiwan. J.C. Wang thanks to the high‐performance computing support on Cheyenne (ark:/85065/d7wd3xhc) provided by NCAR's Computational and Information Systems Laboratory. J.C. Wang also acknowledges Dr. Han‐Li Liu for his valuable discussions and comments. The National Center for Atmospheric Research is a major facility sponsored by the National Science Foundation under Cooperative Agreement No. 1852977.
ASJC Scopus subject areas
- Space and Planetary Science
- Geophysics
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- 1 Finished
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DRAGON-WEX: The Drake Passage and Southern Ocean Wave Experiment
Mitchell, N. (PI), Wright, C. (CoI) & Hindley, N. (Researcher)
Natural Environment Research Council
21/10/17 → 20/10/20
Project: Research council