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dc.contributor.authorNegrea, C.
dc.contributor.authorMunteanu, C.
dc.contributor.authorEchim, M.M.
dc.date2021
dc.date.accessioned2021-05-27T12:03:04Z
dc.date.available2021-05-27T12:03:04Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/7768
dc.descriptionIn this study, we investigate the global ionospheric impact of high‐speed solar wind streams/corotating interaction regions (HSS/CIR). A series of 10 such events are identified between December 1, 2007 and April 29, 2008, characterized in the frequency domain by the main spectral peaks corresponding to 27, 13.5, 9, and 6.75 days. The spectra of solar wind magnetic field, speed, and proton density, as well as those of the geomagnetic indices AE and SYM‐H, are solely dominated by these features. By contrast, the ionospheric NmF2 and to a lesser extent the hmF2 spectra have a much more complex structure, with secondary peaks adding to or replacing the main ones. We argue that this is evidence of the nonlinear nature of the magnetosphere‐ionosphere coupling, highlighted particularly in the NmF2 ionospheric response. Additionally, we show that hmF2 is more closely correlated than NmF2 to all parameters describing the solar wind and geomagnetic activity. Finally, the ionospheric response shows a higher correlation with Bz than any other solar wind parameter, and higher with SYM‐H than AE, indicating that for the low‐frequency part of the spectrum, high‐latitude Joule heating and particle precipitation play a secondary role to that of prompt penetration electric fields in dictating the ionospheric response to geomagnetic activity, in the case of this sequence of HSS/CIR events.
dc.languageeng
dc.titleGlobal ionospheric response to a periodic sequence of HSS/CIR events during the 2007-2008 solar minimum
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freecorrelation study
dc.subject.freeHSS/CIR
dc.subject.freeionospheric periodicities magnetosphere‐ionosphere coupling
dc.subject.freenonlinear interactions
dc.subject.freespectral analysis
dc.source.titleJournal of Geophysical Research: Space Physics
dc.source.volume126
dc.source.issue5
dc.source.pagee2020JA029071
Orfeo.peerreviewedYes
dc.identifier.doi10.1029/2020JA029071


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