FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2016355295> ?p ?o ?g. }

• W2016355295 endingPage "n/a" @default.
• W2016355295 startingPage "n/a" @default.
• W2016355295 abstract "[1] It took about 12 h for the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) satellite to fly from the outbound pass to inbound pass of every inner magnetosphere crossing. This provides a unique opportunity to study the nightside-to-dayside evolution of the corotating inner magnetosphere when the outbound pass is in the nighttime while the inbound pass is in the daytime because a flux tube observed on the nightside may be observed again on the dayside in such situation. The differences between the two observations may be caused by the evolution of the flux tube. By analyzing both the passive and active sounding measurements from the IMAGE Radio Plasma Imager, we study two cases concerning this evolution. One, under a quiet geomagnetic condition, shows a typical evolution process during which the plasmapause was observed on both the nightside and the dayside. The other, during the recovery phase of a magnetic storm, shows a different inner magnetospheric structure in which the distinct plasmapause observed on the nightside becomes unidentifiable on the dayside as the density in the nearly empty nightside plasmatrough increases to a level similar to that of the plasmasphere. It is shown that the evolutions of the inner magnetosphere in both cases were primarily controlled by the fast plasma refilling of the flux tubes from the ionosphere as the flux tubes drift from the nightside to the dayside. In the former case the fast refilling was confined inside L = ∼6.3, while in the latter case the fast refilling extended to at least L = 10. The present observations provide an example for fast refilling as a possible cause of the smooth density transition from the plasmasphere to the subauroral region and demonstrate the importance of the plasmasphere-ionosphere coupling in controlling the structures of the inner magnetosphere." @default.
• W2016355295 created "2016-06-24" @default.
• W2016355295 creator A5009663580 @default.
• W2016355295 creator A5023162083 @default.
• W2016355295 creator A5028826713 @default.
• W2016355295 creator A5048586965 @default.
• W2016355295 creator A5048632439 @default.
• W2016355295 creator A5051736289 @default.
• W2016355295 date "2010-04-01" @default.
• W2016355295 modified "2023-10-09" @default.
• W2016355295 title "The nightside-to-dayside evolution of the inner magnetosphere: Imager for Magnetopause-to-Aurora Global Exploration Radio Plasma Imager observations" @default.
• W2016355295 cites W139012307 @default.
• W2016355295 cites W1484914650 @default.
• W2016355295 cites W1834240855 @default.
• W2016355295 cites W1971202509 @default.
• W2016355295 cites W1975341957 @default.
• W2016355295 cites W1982564903 @default.
• W2016355295 cites W1987540124 @default.
• W2016355295 cites W1989724646 @default.
• W2016355295 cites W1991211860 @default.
• W2016355295 cites W1994657519 @default.
• W2016355295 cites W2001517082 @default.
• W2016355295 cites W2004654615 @default.
• W2016355295 cites W2006464963 @default.
• W2016355295 cites W2009852966 @default.
• W2016355295 cites W2020494970 @default.
• W2016355295 cites W2036136060 @default.
• W2016355295 cites W2038899595 @default.
• W2016355295 cites W2041966525 @default.
• W2016355295 cites W2042025349 @default.
• W2016355295 cites W2045105578 @default.
• W2016355295 cites W2050767790 @default.
• W2016355295 cites W2053164554 @default.
• W2016355295 cites W2055489564 @default.
• W2016355295 cites W2062598126 @default.
• W2016355295 cites W2067107034 @default.
• W2016355295 cites W2068987160 @default.
• W2016355295 cites W2069712756 @default.
• W2016355295 cites W2080294984 @default.
• W2016355295 cites W2085430190 @default.
• W2016355295 cites W2088262248 @default.
• W2016355295 cites W2093326740 @default.
• W2016355295 cites W2096527717 @default.
• W2016355295 cites W2110500430 @default.
• W2016355295 cites W2113199467 @default.
• W2016355295 cites W2122144241 @default.
• W2016355295 cites W2132372773 @default.
• W2016355295 cites W2148012574 @default.
• W2016355295 cites W2161501266 @default.
• W2016355295 cites W4231801625 @default.
• W2016355295 cites W4239729499 @default.
• W2016355295 cites W4249409233 @default.
• W2016355295 doi "https://doi.org/10.1029/2009ja014668" @default.
• W2016355295 hasPublicationYear "2010" @default.
• W2016355295 type Work @default.
• W2016355295 sameAs 2016355295 @default.
• W2016355295 citedByCount "28" @default.
• W2016355295 countsByYear W20163552952012 @default.
• W2016355295 countsByYear W20163552952013 @default.
• W2016355295 countsByYear W20163552952014 @default.
• W2016355295 countsByYear W20163552952015 @default.
• W2016355295 countsByYear W20163552952016 @default.
• W2016355295 countsByYear W20163552952017 @default.
• W2016355295 countsByYear W20163552952018 @default.
• W2016355295 countsByYear W20163552952019 @default.
• W2016355295 countsByYear W20163552952020 @default.
• W2016355295 countsByYear W20163552952021 @default.
• W2016355295 countsByYear W20163552952022 @default.
• W2016355295 countsByYear W20163552952023 @default.
• W2016355295 crossrefType "journal-article" @default.
• W2016355295 hasAuthorship W2016355295A5009663580 @default.
• W2016355295 hasAuthorship W2016355295A5023162083 @default.
• W2016355295 hasAuthorship W2016355295A5028826713 @default.
• W2016355295 hasAuthorship W2016355295A5048586965 @default.
• W2016355295 hasAuthorship W2016355295A5048632439 @default.
• W2016355295 hasAuthorship W2016355295A5051736289 @default.
• W2016355295 hasBestOaLocation W20163552951 @default.
• W2016355295 hasConcept C108411613 @default.
• W2016355295 hasConcept C115260700 @default.
• W2016355295 hasConcept C116403925 @default.
• W2016355295 hasConcept C118691173 @default.
• W2016355295 hasConcept C121332964 @default.
• W2016355295 hasConcept C130443932 @default.
• W2016355295 hasConcept C140161248 @default.
• W2016355295 hasConcept C157479481 @default.
• W2016355295 hasConcept C162725370 @default.
• W2016355295 hasConcept C170641098 @default.
• W2016355295 hasConcept C191897082 @default.
• W2016355295 hasConcept C192562407 @default.
• W2016355295 hasConcept C199635899 @default.
• W2016355295 hasConcept C2780379797 @default.
• W2016355295 hasConcept C44870925 @default.
• W2016355295 hasConcept C62520636 @default.
• W2016355295 hasConcept C68709404 @default.
• W2016355295 hasConcept C8058405 @default.
• W2016355295 hasConcept C82706917 @default.
• W2016355295 hasConcept C91586092 @default.
• W2016355295 hasConceptScore W2016355295C108411613 @default.

• next