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dc.contributor.author Araujo-Pradere, Eduardo A.
dc.contributor.author Fang, Tzu Wei
dc.contributor.author Anderson, David N.
dc.contributor.author Fedrizzi, Mariangel
dc.contributor.author Stoneback, Russell
dc.date.accessioned 2018-11-09T11:46:40Z
dc.date.available 2018-11-09T11:46:40Z
dc.date.issued 2012-04-26
dc.identifier.issn 1944-799X
dc.identifier.uri http://repositorio.igp.gob.pe/handle/IGP/3488
dc.description En: Radio Science, v. 47, n. 4, (August 2012), p. RS0L12 1-5.
dc.description.abstract Previous studies have quantified the longitude gradients in E × Bdrift associated with the four‐cell tidal structures and have confirmed that these sharp gradients exist on a day‐to‐day basis. For this paper, we incorporate the Ion Velocity Meter (IVM) sensor on the Communications/Navigation Outage Forecasting System satellite to obtain the daytime, verticalE × B drift velocities at the magnetic equator as a function of longitude, local time, and season and to theoretically calculate the F region ion densities as a function of altitude, latitude, longitude, and local time using the Global Ionosphere Plasmasphere model. We compare calculated ion densities assuming no longitude gradients in E × Bdrift velocities with calculated ion densities incorporating the IVM‐observedE × Bdrift at the boundaries of the four‐cell tidal structures in the Peruvian and the Atlantic longitude sectors. Incorporating the IVM‐observedE × B drift velocities, the ion density crests rapidly converge to the magnetic equator between 285 and 300°E geographic longitude, are absent between 300° and 305°, and move away from the magnetic equator between 305° and 340°. In essence, the steeper the longitude gradient in E × B drifts, the steeper the longitude gradient in the equatorial anomaly crest location". es_ES
dc.format application/pdf es_ES
dc.language.iso en es_ES
dc.publisher Radio Science es_ES
dc.rights info:eu-repo/semantics/restrictedAccess es_ES
dc.rights.uri http://creativecommons.org/licences/restrictedAccess es_ES
dc.source Repositorio institucional - IGP es_ES
dc.subject Iones es_ES
dc.subject Región F es_ES
dc.subject Ionósfera--Mediciones es_ES
dc.subject Satélites artificiales es_ES
dc.subject Ionósfera--Observaciones es_ES
dc.subject Campos magnéticos es_ES
dc.subject Geomagnetismo es_ES
dc.title Modeling the daytime, equatorial ionospheric ion densities associated with the observed, four‐cell longitude patterns in E × B drift velocities es_ES
dc.type info:eu-repo/semantics/article es_ES
dc.subject.ocde Densidad es_ES
dc.subject.ocde Atmósfera es_ES
dc.subject.ocde Modelos es_ES
dc.subject.ocde Observación es_ES
dc.subject.ocde Geofísica es_ES
dc.identifier.journal Radio science es_ES
dc.description.peer-review Por pares es_ES
dc.identifier.doi 10.1029/2011RS004930 es_ES

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