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dc.contributor.authorZhang, Duan
dc.contributor.authorZhang, Qing-He
dc.contributor.authorOksavik, Kjellmar
dc.contributor.authorXing, Zan-Yang
dc.contributor.authorLyons, L.R.
dc.contributor.authorYang, Hui-Gen
dc.contributor.authorLi, Guo-Jun
dc.contributor.authorHosokawa, Keisuke
dc.contributor.authorShinbori, Atsuki
dc.contributor.authorMa, Yu-Zhang
dc.contributor.authorWang, Yong
dc.contributor.authorWang, Xiang-Yu
dc.date.accessioned2024-05-03T11:10:10Z
dc.date.available2024-05-03T11:10:10Z
dc.date.created2024-01-03T13:26:59Z
dc.date.issued2023
dc.identifier.issn2169-9380
dc.identifier.urihttps://hdl.handle.net/11250/3129010
dc.description.abstractSimultaneous observations from Defense Meteorological Satellite Program, Swarm, Resolute Bay all-sky imagers, GPS Total Electron Content and Super Dual Auroral Radar Network, are used to investigate the evolution and key characteristics of the Tongue of Ionization (TOI) being restructured into a polar cap patch. Six satellites crossed the TOI of patch as it moved from the dayside to the nightside. It was initially hot, then a mix of both cold and hot, and finally it became a cold patch. This suggests that cold patch is not only a result of solar extreme ultraviolet radiation, but may also develop when a hot patch cools down. Soft-electron precipitation and flow shears both contribute to the TOI restructuring and the appearance of polar cap patch. The plasma density of patch at ∼500 km was at least 4 times higher than at ∼800 km. The plasma density enhancement gradually decreased as the patch evolved due to decreased production and transport of cold nightside low-density plasma. Moreover, the duskward motion of the patch was influenced by changes in the ionospheric convection pattern.en_US
dc.language.isoengen_US
dc.publisherAGUen_US
dc.relation.urihttps://doi.org/10.1029/2023JA032176
dc.titleMulti-Instrument Observations of the Evolution of Polar Cap Patches Associated With Flow Shears and Particle Precipitationen_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2023 American Geophysical Union. All Rights Reserved.en_US
dc.source.articlenumbere2023JA032176en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.doi10.1029/2023JA032176
dc.identifier.cristin2219931
dc.source.journalJournal of Geophysical Research (JGR): Space Physicsen_US
dc.identifier.citationJournal of Geophysical Research (JGR): Space Physics. 2023, 128 (12), e2023JA032176.en_US
dc.source.volume128en_US
dc.source.issue12en_US


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