Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/112261
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dc.contributor.authorYi, W.en
dc.contributor.authorReid, I.en
dc.contributor.authorXue, X.en
dc.contributor.authorMurphy, D.en
dc.contributor.authorHall, C.en
dc.contributor.authorTsutsumi, M.en
dc.contributor.authorNing, B.en
dc.contributor.authorLi, G.en
dc.contributor.authorYounger, J.en
dc.contributor.authorChen, T.en
dc.contributor.authorDou, X.en
dc.date.issued2018en
dc.identifier.citationGeophysical Research Letters, 2018; 45(1):436-444en
dc.identifier.issn0094-8276en
dc.identifier.issn1944-8007en
dc.identifier.urihttp://hdl.handle.net/2440/112261-
dc.descriptionPublished online 12 JAN 2018en
dc.description.abstractWe report the first observations of a high‐ and middle‐latitude neutral mesospheric density response to geomagnetic storms. Interhemisphere mesospheric densities are estimated using data from meteor radars at Davis Station (68.6°S, 77.9°E), Svalbard (78.3°N, 16°E) and Tromsø (69.6°N, 19.2°E), which are located under the auroral zone; the Mohe (53.5°N, 122.3°E), and Beijing (40.3°N, 116.2°E) meteor radars, located in northern midlatitudes, and the Microwave Limb Sounder (MLS) on the Aura satellite. Both case studies and a superposed epoch analysis indicate that geomagnetic storms can significantly influence mesospheric density, causing a greater than ~10% decrease in the auroral zones and a ~5% decrease at higher midlatitudes. With such large changes, it is reasonable to suspect that geomagnetic storms influence the dynamics of the high and middle latitudes mesosphere.en
dc.description.statementofresponsibilityWen Yi, Iain M. Reid, Xianghui Xue, Damian J. Murphy, Chris M. Hall, Masaki Tsutsumi, Baiqi Ning, Guozhu Li, Joel P. Younger, Tingdi Chen, and Xiankang Douen
dc.language.isoenen
dc.publisherAmerican Geophysical Unionen
dc.rights©2018. American Geophysical Union. All Rights Reserved.en
dc.titleHigh- and middle-latitude neutral mesospheric density response to geomagnetic stormsen
dc.typeJournal articleen
dc.identifier.rmid0030081364en
dc.identifier.doi10.1002/2017GL076282en
dc.identifier.pubid394573-
pubs.library.collectionPhysics publicationsen
pubs.library.teamDS03en
pubs.verification-statusVerifieden
pubs.publication-statusPublisheden
dc.identifier.orcidReid, I. [0000-0003-2340-9047]en
dc.identifier.orcidYounger, J. [0000-0003-2918-1709]en
Appears in Collections:Physics publications

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