JOURNAL ARTICLE

Tidal Impact on Quiet‐Time Polar Thermosphere Zonal Winds During Northern Winter Sudden Stratospheric Warmings.

  • Published In: Journal of Geophysical Research. Space Physics, 2025, v. 130, n. 2. P. 1 1 of 3

  • Database: Applied Science & Technology Source Ultimate 2 of 3

  • Authored By: Kumari, Komal; Bossert, Katrina; Pedatella, Nicholas M.; Thorsen, Denise; Conde, Mark 3 of 3

Abstract

This study primarily examines the variability of zonal winds in the geomagnetic "quiet‐time" (AE index < 190 nT; Kp index < 2) thermosphere over Alaska (60–75°N) during the winter months from November 2018 to February 2019, and demonstrates a correlation of the meteor radar observed zonal winds at heights 82–98 km with Scanning Doppler Imager observed zonal wind variability at heights 120 and 250 km during nighttime. Notably, over Alaska following a mid‐winter sudden stratosphere warming (SSW) event, the zonal wind magnitudes on tidal timescale (difference between maximum eastward and minimum westward wind values over a 6‐hr interval during nighttime) in the thermosphere experience about two‐fold increase at observed thermosphere altitudes (98, 120, and 250 km). Additional validation of observational findings comes from SD‐WACCM‐X model simulations across solar‐minimum (2017–2021) winters, including both non‐SSW and SSW events (occurring in different winters). The model indicates that the SSW‐induced response in zonal wind tidal magnitudes may be indistinguishable from the seasonal trend in late winter, while it is more pronounced when the seasonal variations is minimal during mid‐winter months. By tidal diagnostics of zonal winds from meteor radar observations and SD‐WACCM‐X simulations at polar latitudes, a connection is established between the thermosphere zonal wind variations and the semidiurnal originating in the lower atmosphere following the SSW onset within the altitude range of 90–300 km (i.e., ionosphere‐thermosphere region). Additionally, the study highlights the migrating solar semidiurnal tides as a major contributor in the variability in the polar thermosphere region with minor contribution from lunar semidiurnal tides. Plain Language Summary: This study examines the effects of sudden stratosphere warmings (SSWs) on zonal wind variability in the high‐latitude thermosphere during the northern winter season. It specifically investigates the role of lower atmospheric waves in influencing wind variability during a SSW under quiet geomagnetic and solar minimum conditions. The study is significant because previous research has primarily focused on the impact of polar vortex disturbances on ionosphere‐thermosphere dynamics at low to mid latitudes. The findings of this study demonstrate that lower atmospheric dynamics play a substantial role in driving variability in the upper thermosphere at polar latitudes during SSW events, primarily influenced by semidiurnal tidal variabilities rather than diurnal or terdiurnal tidal variabilities. Further, the study discusses the potential relative contributions of lunar and solar semidiurnal tides in the polar thermosphere up to an altitude of 250 km during SSW events. Solar semidiurnal tides were never observed to influence polar thermosphere winds (>60°N) before thus emphasizing the need for further research to enhance our understanding of these complex dynamics. Key Points: After northern winter sudden stratosphere warming (SSW) onset, high‐latitude quiet‐time zonal wind on tidal timescales doubles from mesosphere to upper thermosphereDuring solar minimum, thermospheric zonal winds respond noticeably to SSW events in mid‐winter months when seasonal variability is smallZonal wind response following SSW is linked to enhanced solar migrating semidiurnal tides originating in the lower atmosphere [ABSTRACT FROM AUTHOR]

Additional Information

  • Source:Journal of Geophysical Research. Space Physics. 2025/02, Vol. 130, Issue 2, p1
  • Document Type:Article
  • Subject Area:Astronomy and Astrophysics
  • Publication Date:2025
  • ISSN:21699380
  • DOI:10.1029/2024JA033011
  • Accession Number:184019836
  • Copyright Statement:Copyright of Journal of Geophysical Research. Space Physics is the property of Wiley-Blackwell and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)

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