IGGCAS OpenIR  > 地球与行星物理院重点实验室
Solar Tide-like Signatures in the Ionospheric Total Electron Content During the 2018 Sudden Stratospheric Warming Event
Ma, Han1,2,3; He, Maosheng; Liu, Libo1,2,3; Li, Wenbo1,2,3; Yang, Yuyan1,2,3; Zhang, Ruilong1,2,3; Chen, Yiding1,3,4; Le, Huijun1,2,3; Zhang, Hui1,2,3; Li, Guozhu1,3,4
2022-09-01
Source PublicationSPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS
Volume20Issue:9Pages:11
AbstractAtmospheric waves play an important role in the vertical coupling of atmosphere and ionosphere. Recent studies revealed that the mesospheric wave activities associated with sudden stratospheric warming events (SSWs) are more complicated than previously thought. This study investigates the activities of the dominant solar tide-like harmonics in the ionosphere during SSWs. Significant tide-like harmonics are present in the residuals of total electron content (TEC) detected by five receivers at different latitudes using signals from BeiDou geostationary (BD-GEO) C3 satellite during the 2018 SSW. The results reveal that after the SSW onset, the third harmonic enhances and the fourth harmonic weakens at all selected receivers. However, the second harmonic exhibits a response varying with latitude. We then compare the ionospheric tide-like signatures with those in mesospheric winds observed by four meteor radars. A good agreement is found after the SSW onset. The measurements at Mohe (53.5 degrees N, 122.3 degrees E) show that the response of each specific ionospheric tide-like signature is similar to the tidal result in the mesospheric winds after the onset of three SSW events in 2017-2019. In addition, we suggest that besides the direct or indirect effects from the interactions of various waves in the lower atmosphere, the non-sinusoidal waveform of the ionospheric diurnal variation may also contribute to solar harmonic signatures in the ionosphere. Plain Language Summary Stratosphere sudden warming (SSW) is characterized by a dramatic increment of stratospheric atmospheric temperature within a few days during the polar winter. Although solar tides are the most predictably occurring waves in the upper atmosphere, their activities during SSWs become more complex than previously realized. To date, the observational studies of high-order solar tides have mainly focused on the lower thermosphere. We investigate the total electron content (TEC) data to extend our study to charged particles at ionospheric height. Results show that three solar tide-like harmonic peaks dominate during the 2018 SSW. In addition, the activities of the ionospheric harmonic signatures are similar to those in the neutral winds, suggesting a coupling between the lower thermosphere and the ionosphere.
DOI10.1029/2022SW003042
Funding OrganizationNational Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program
WOS KeywordTIRUNELVELI 8.7-DEGREES-N ; SEMIDIURNAL TIDES ; LUNAR ; VARIABILITY ; 77.8-DEGREES-E ; MESOSPHERE
Language英语
Funding ProjectNational Natural Science Foundation of China[42174204] ; National Key Research and Development Program[2017YFE0131400]
Funding OrganizationNational Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program ; National Key Research and Development Program
WOS Research AreaAstronomy & Astrophysics ; Geochemistry & Geophysics ; Meteorology & Atmospheric Sciences
WOS SubjectAstronomy & Astrophysics ; Geochemistry & Geophysics ; Meteorology & Atmospheric Sciences
WOS IDWOS:000859839600001
PublisherAMER GEOPHYSICAL UNION
Citation statistics
Document Type期刊论文
Identifierhttp://ir.iggcas.ac.cn/handle/132A11/108335
Collection地球与行星物理院重点实验室
Corresponding AuthorLiu, Libo
Affiliation1.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China
2.Chinese Acad Sci, Heilongjiang Mohe Observ Geophys, Inst Geol & Geophys, Beijing, Peoples R China
3.Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing, Peoples R China
4.Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing, Peoples R China
First Author AffilicationKey Laboratory of Earth and Planetary Physics, Chinese Academy of Sciences
Corresponding Author AffilicationKey Laboratory of Earth and Planetary Physics, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Ma, Han,He, Maosheng,Liu, Libo,et al. Solar Tide-like Signatures in the Ionospheric Total Electron Content During the 2018 Sudden Stratospheric Warming Event[J]. SPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS,2022,20(9):11.
APA Ma, Han.,He, Maosheng.,Liu, Libo.,Li, Wenbo.,Yang, Yuyan.,...&Li, Guozhu.(2022).Solar Tide-like Signatures in the Ionospheric Total Electron Content During the 2018 Sudden Stratospheric Warming Event.SPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS,20(9),11.
MLA Ma, Han,et al."Solar Tide-like Signatures in the Ionospheric Total Electron Content During the 2018 Sudden Stratospheric Warming Event".SPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS 20.9(2022):11.
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