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dc.contributor.authorHatch, Spencer Mark
dc.contributor.authorMoretto, Therese
dc.contributor.authorLynch, Kristina A.
dc.contributor.authorLaundal, Karl Magnus
dc.contributor.authorGjerloev, J.
dc.contributor.authorLund, Eric
dc.date.accessioned2021-04-28T08:50:25Z
dc.date.available2021-04-28T08:50:25Z
dc.date.created2020-03-19T11:28:32Z
dc.date.issued2020
dc.identifier.issn2169-9380
dc.identifier.urihttps://hdl.handle.net/11250/2740087
dc.description.abstractA number of interdependent conditions and processes contribute to ionospheric-origin energetic ( ∼ 10 eV to several keV) ion outflows. Due to these interdependences and the associated observational challenges, energetic ion outflows remain a poorly understood facet of atmosphere-ionosphere-magnetosphere coupling. Here we demonstrate the relationship between east-west magnetic field fluctuations ( ΔB EW ) and energetic outflows in the magnetosphere-ionosphere transition region. We use dayside cusp region FAST satellite observations made near apogee ( ∼ 4,180-km altitude) near fall equinox and solstices in both hemispheres to derive statistical relationships between ion upflow and ΔB EW spectral power as a function of spacecraft frame frequency bands between 0 and 4 Hz. Identification of ionospheric-origin energetic ion upflows is automated, and the spectral power P EW in each frequency band is obtained via integration of ΔB EW power spectral density. Derived relationships are of the γ form J ||,i = J 0,i P EW for upward ion flux J ||,i at 130-km altitude, with J 0,i the mapped upward ion flux for a nominal spectral power P EW = 1 nT 2 . The highest correlation coefficients are obtained for spacecraft frame frequencies ∼ 0.1–0.5 Hz. Summer solstice and fall equinox observations yield power law indices γ ≃ 0.9–1.3 and correlation coefficients r ≥ 0.92, while winter solstice observations yield γ ≃ 0.4–0.8 with r ≳ 0.8. Mass spectrometer observations reveal that the oxygen/hydrogen ion composition ratio near summer solstice is much greater than the corresponding ratio near winter. These results reinforce the importance of ion composition in outflow models. If observed ΔB EW perturbations result from Doppler-shifted wave structures with near-zero frequencies, we show that spacecraft frame frequencies ∼ 0.1–0.5 Hz correspond to perpendicular spatial scales of several to tens of kilometers.en_US
dc.language.isoengen_US
dc.publisherWileyen_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.titleThe Relationship Between Cusp Region Ion Outflows and East-West Magnetic Field Fluctuations at 4,000-km Altitudeen_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2020. The Authors.en_US
dc.source.articlenumbere2019JA027454en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.doi10.1029/2019JA027454
dc.identifier.cristin1802398
dc.source.journalJournal of Geophysical Research (JGR): Space Physicsen_US
dc.source.40125
dc.source.143
dc.relation.projectNorges forskningsråd: 223252en_US
dc.relation.projectESA - den europeiske romfartsorganisasjonen: 4000126731en_US
dc.identifier.citationJournal of Geophysical Research: Space Physics. 2020, 125 (3), e2019JA027454.en_US
dc.source.volume125en_US
dc.source.issue3en_US


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Navngivelse 4.0 Internasjonal
Except where otherwise noted, this item's license is described as Navngivelse 4.0 Internasjonal