Lunar tide in the equatorial F region vertical ion drift velocity

dc.contributor.authorStening, Robert J.
dc.contributor.authorFejer, Bela G.
dc.date.accessioned2018-10-22T16:56:12Z
dc.date.available2018-10-22T16:56:12Z
dc.date.issued2001-01-01
dc.description.abstractVertical ion drift velocity data from Jicamarca have been analyzed for a lunar semidiurnal tide using a least squares fitting method. Amplitudes of up to 6 m s−1 are obtained with phases in agreement with lunar tidal determinations of other associated physical parameters. Variations between season, solar activity, and day to night are also examined. Generally, amplitudes are larger in the southern summer. Much of the phase variation with season is very similar for solar maximum and minimum years. There is a summer to winter phase change that is most distinct at solar maximum nighttime. A day‐to‐night phase reversal can also been seen in some seasons. Hints of this are also found in the lunar tide in the F region height and in the magnetic variations at Huancayo.es_ES
dc.description.peer-reviewPor pareses_ES
dc.formatapplication/pdfes_ES
dc.identifier.citationStening, R. J., & Fejer, B. G. (2001). Lunar tide in the equatorial F region vertical ion drift velocity.==$Journal of Geophysical Research: Space Physics, 106$==(A1), 221-226. https://doi.org/10.1029/2000JA000175es_ES
dc.identifier.doihttps://doi.org/10.1029/2000JA000175es_ES
dc.identifier.journalJournal of Geophysical Research: Space Physicses_ES
dc.identifier.urihttp://hdl.handle.net/20.500.12816/3090
dc.language.isoenges_ES
dc.publisherAmerican Geophysical Uniones_ES
dc.relation.ispartofurn:issn:2169-9380
dc.rightsinfo:eu-repo/semantics/restrictedAccesses_ES
dc.subjectMoones_ES
dc.subjectSolar activityes_ES
dc.subjectRegion Fes_ES
dc.subjectIonospherees_ES
dc.subjectMagnetic fieldses_ES
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.05.01es_ES
dc.titleLunar tide in the equatorial F region vertical ion drift velocityes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES

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