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dc.contributor.authorZawedde, Annet Eva
dc.contributor.authorTyssøy, Hilde Nesse
dc.contributor.authorHibbins, Robert Edward
dc.contributor.authorEspy, Patrick Joseph
dc.contributor.authorDegaard, L-K.
dc.contributor.authorSandanger, Marit Irene
dc.contributor.authorStadsnes, Johan
dc.date.accessioned2016-12-30T08:36:03Z
dc.date.available2016-12-30T08:36:03Z
dc.date.issued2016-06
dc.PublishedJournal of Geophysical Research - Space Physics 2016, 121(6):5914–5929eng
dc.identifier.issn2169-9402en_US
dc.identifier.urihttps://hdl.handle.net/1956/15299
dc.description.abstractIn 2008 a sequence of geomagnetic storms occurred triggered by high-speed solar wind streams from coronal holes. Improved estimates of precipitating fluxes of energetic electrons are derived from measurements on board the NOAA/POES 18 satellite using a new analysis technique. These fluxes are used to quantify the direct impact of energetic electron precipitation (EEP) during solar minimum on middle atmospheric hydroxyl (OH) measured from the Aura satellite. During winter, localized longitudinal density enhancements in the OH are observed over northern Russia and North America at corrected geomagnetic latitudes poleward of 55°. Although the northern Russia OH enhancement is closely associated with increased EEP at these longitudes, the strength and location of the North America enhancement appear to be unrelated to EEP. This OH density enhancement is likely due to vertical motion induced by atmospheric wave dynamics that transports air rich in atomic oxygen and atomic hydrogen downward into the middle atmosphere, where it plays a role in the formation of OH. In the Southern Hemisphere, localized enhancements of the OH density over West Antarctica can be explained by a combination of enhanced EEP due to the local minimum in Earth's magnetic field strength and atmospheric dynamics. Our findings suggest that even during solar minimum, there is substantial EEP-driven OH production. However, to quantify this effect, a detailed knowledge of where and when the precipitation occurs is required in the context of the background atmospheric dynamics.en_US
dc.language.isoengeng
dc.publisherWileyen_US
dc.rightsAttribution CC BY-NC-NDeng
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/eng
dc.titleThe impact of energetic electron precipitation on mesospheric hydroxyl during a year of solar minimumen_US
dc.typePeer reviewed
dc.typeJournal article
dc.date.updated2016-12-15T15:17:54Z
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2016 The Author(s)en_US
dc.identifier.doihttps://doi.org/10.1002/2016ja022371
dc.identifier.cristin1398492
dc.relation.projectNorges forskningsråd: 223252/F50


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