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dc.contributor.author | He M. | |
dc.contributor.author | Forbes J.M. | |
dc.contributor.author | Chau J.L. | |
dc.contributor.author | Li G. | |
dc.contributor.author | Wan W. | |
dc.contributor.author | Korotyshkin D.V. | |
dc.date.accessioned | 2021-02-25T20:33:34Z | |
dc.date.available | 2021-02-25T20:33:34Z | |
dc.date.issued | 2020 | |
dc.identifier.issn | 0094-8276 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/161731 | |
dc.description.abstract | ©2020. The Authors. Sudden stratospheric warming events (SSWs) are the most spectacular atmospheric vertical coupling processes, well-known for being associated with diverse wave activities in the upper atmosphere and ionosphere. The first four solar tidal harmonics have been reported as being engaged. Here, combining mesospheric winds detected by three midlatitude radars, we demonstrate at least the first six harmonics that occurred during SSW 2018. Wave number diagnosis demonstrates that all six harmonics are dominated by migrating components. Wavelet analyses reveal that the fourth, fifth, and sixth harmonics quench after the SSW onset. The six harmonics and the quenching appear also in a statistical analysis based on near-12-year observations from one of the radars. We attribute the quenching to reversal of the background eastward wind. | |
dc.relation.ispartofseries | Geophysical Research Letters | |
dc.subject | mesosphere | |
dc.subject | migrating solar tides | |
dc.subject | sudden stratospheric warming (SSW) | |
dc.subject | zonal wavenumber | |
dc.title | High-Order Solar Migrating Tides Quench at SSW Onsets | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 6 | |
dc.relation.ispartofseries-volume | 47 | |
dc.collection | Публикации сотрудников КФУ | |
dc.source.id | SCOPUS00948276-2020-47-6-SID85082514400 |