Matches in SemOpenAlex for { <https://semopenalex.org/work/W3208543245> ?p ?o ?g. }
- W3208543245 abstract "Abstract Recent studies revealed that the long-lasting daytime ionospheric enhancements of Total Electron Content (TEC) were sometimes observed in the Asian sector during the recovery phase of geomagnetic storms (e.g., Lei (J Geophys Res Space Phys 123: 3217–3232, 2018), Li (J Geophys Res Space Phys 125: e2020JA028238, 2020). However, they focused only on the dayside ionosphere, and no dedicated studies have been performed to investigate the nighttime ionospheric behavior during such kinds of storm recovery phases. In this study, we focused on two geomagnetic storms that happened on 7–8 September 2017 and 25–26 August 2018, which showed the prominent daytime TEC enhancements in the Asian sector during their recovery phases, to explore the nighttime large-scale ionospheric responses as well as the small-scale Equatorial Plasma Irregularities (EPIs). It is found that during the September 2017 storm recovery phase, the nighttime ionosphere in the American sector is largely depressed, which is similar to the daytime ionospheric response in the same longitude sector; while in the Asian sector, only a small TEC increase is observed at nighttime, which is much weaker than the prominent daytime TEC enhancement in this longitude sector. During the recovery phase of the August 2018 storm, a slight TEC increase is observed on the night side at all longitudes, which is also weaker than the prominent daytime TEC enhancement. For the small-scale EPIs, they are enhanced and extended to higher latitudes during the main phase of both storms. However, during the recovery phases of the first storm, the EPIs are largely enhanced and suppressed in the Asian and American sectors, respectively, while no prominent nighttime EPIs are observed during the second storm recovery phase. The clear north–south asymmetry of equatorial ionization anomaly crests during the second storm should be responsible for the suppression of EPIs during this storm. In addition, our results also suggest that the dusk side ionospheric response could be affected by the daytime ionospheric plasma density/TEC variations during the recovery phase of geomagnetic storms, which further modulates the vertical plasma drift and plasma gradient. As a result, the growth rate of post-sunset EPIs will be enhanced or inhibited." @default.
- W3208543245 created "2021-11-08" @default.
- W3208543245 creator A5007968052 @default.
- W3208543245 creator A5014531805 @default.
- W3208543245 creator A5043690784 @default.
- W3208543245 creator A5074747520 @default.
- W3208543245 creator A5080815893 @default.
- W3208543245 creator A5083585131 @default.
- W3208543245 creator A5084266744 @default.
- W3208543245 creator A5090137647 @default.
- W3208543245 date "2021-11-01" @default.
- W3208543245 modified "2023-10-02" @default.
- W3208543245 title "The nighttime ionospheric response and occurrence of equatorial plasma irregularities during geomagnetic storms: a case study" @default.
- W3208543245 cites W1516472442 @default.
- W3208543245 cites W1947642062 @default.
- W3208543245 cites W1957332219 @default.
- W3208543245 cites W1965611677 @default.
- W3208543245 cites W1968168798 @default.
- W3208543245 cites W1981483229 @default.
- W3208543245 cites W1982903954 @default.
- W3208543245 cites W1991378411 @default.
- W3208543245 cites W2012275826 @default.
- W3208543245 cites W2018554399 @default.
- W3208543245 cites W2026672454 @default.
- W3208543245 cites W2041528536 @default.
- W3208543245 cites W2042449366 @default.
- W3208543245 cites W2048429894 @default.
- W3208543245 cites W2058058461 @default.
- W3208543245 cites W2059807138 @default.
- W3208543245 cites W2077387669 @default.
- W3208543245 cites W2090065735 @default.
- W3208543245 cites W2109089487 @default.
- W3208543245 cites W2117233461 @default.
- W3208543245 cites W2141175170 @default.
- W3208543245 cites W2154825135 @default.
- W3208543245 cites W2161386319 @default.
- W3208543245 cites W2514458421 @default.
- W3208543245 cites W2563317537 @default.
- W3208543245 cites W2619159570 @default.
- W3208543245 cites W2778621041 @default.
- W3208543245 cites W2795541194 @default.
- W3208543245 cites W2801074251 @default.
- W3208543245 cites W2801918409 @default.
- W3208543245 cites W2802897558 @default.
- W3208543245 cites W2921894922 @default.
- W3208543245 cites W2924372663 @default.
- W3208543245 cites W2958399946 @default.
- W3208543245 cites W2972312558 @default.
- W3208543245 cites W3092272556 @default.
- W3208543245 cites W3096313931 @default.
- W3208543245 cites W3172788806 @default.
- W3208543245 cites W4245821960 @default.
- W3208543245 doi "https://doi.org/10.1186/s43020-021-00055-x" @default.
- W3208543245 hasPublicationYear "2021" @default.
- W3208543245 type Work @default.
- W3208543245 sameAs 3208543245 @default.
- W3208543245 citedByCount "13" @default.
- W3208543245 countsByYear W32085432452022 @default.
- W3208543245 countsByYear W32085432452023 @default.
- W3208543245 crossrefType "journal-article" @default.
- W3208543245 hasAuthorship W3208543245A5007968052 @default.
- W3208543245 hasAuthorship W3208543245A5014531805 @default.
- W3208543245 hasAuthorship W3208543245A5043690784 @default.
- W3208543245 hasAuthorship W3208543245A5074747520 @default.
- W3208543245 hasAuthorship W3208543245A5080815893 @default.
- W3208543245 hasAuthorship W3208543245A5083585131 @default.
- W3208543245 hasAuthorship W3208543245A5084266744 @default.
- W3208543245 hasAuthorship W3208543245A5090137647 @default.
- W3208543245 hasBestOaLocation W32085432451 @default.
- W3208543245 hasConcept C105306849 @default.
- W3208543245 hasConcept C105795698 @default.
- W3208543245 hasConcept C115260700 @default.
- W3208543245 hasConcept C116403925 @default.
- W3208543245 hasConcept C121332964 @default.
- W3208543245 hasConcept C122523270 @default.
- W3208543245 hasConcept C127313418 @default.
- W3208543245 hasConcept C13280743 @default.
- W3208543245 hasConcept C151325931 @default.
- W3208543245 hasConcept C153294291 @default.
- W3208543245 hasConcept C162725370 @default.
- W3208543245 hasConcept C165391973 @default.
- W3208543245 hasConcept C170641098 @default.
- W3208543245 hasConcept C176379880 @default.
- W3208543245 hasConcept C199635899 @default.
- W3208543245 hasConcept C2780554747 @default.
- W3208543245 hasConcept C33923547 @default.
- W3208543245 hasConcept C39432304 @default.
- W3208543245 hasConcept C41479618 @default.
- W3208543245 hasConcept C49204034 @default.
- W3208543245 hasConcept C62520636 @default.
- W3208543245 hasConcept C8058405 @default.
- W3208543245 hasConcept C91586092 @default.
- W3208543245 hasConceptScore W3208543245C105306849 @default.
- W3208543245 hasConceptScore W3208543245C105795698 @default.
- W3208543245 hasConceptScore W3208543245C115260700 @default.
- W3208543245 hasConceptScore W3208543245C116403925 @default.
- W3208543245 hasConceptScore W3208543245C121332964 @default.
- W3208543245 hasConceptScore W3208543245C122523270 @default.
- W3208543245 hasConceptScore W3208543245C127313418 @default.
- W3208543245 hasConceptScore W3208543245C13280743 @default.