First successful prediction of a convective equatorial ionospheric storm using solar wind parameters

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dc.contributor.authorKelley, M. C.
dc.contributor.authorRetterer, J.
dc.date.accessioned2018-11-05T11:20:44Z
dc.date.available2018-11-05T11:20:44Z
dc.date.issued2008-08-28
dc.description.abstractOne of the major challenges of the National Space Weather Program in the United States is to predict the generation of intense turbulence in the equatorial and low‐latitude ionosphere. We term this a convective equatorial ionospheric storm since, much like a thunderstorm, low‐density media erupt upward, releasing stored gravitational energy. This is an important phenomenon since both communication and navigational systems can be severely affected by the associated turbulence. Here, for the first time, we use solar wind data obtained upstream of the Earth and a physics‐based assimilative model to successfully predict such an event during a strong magnetic storm in November 2004.es_ES
dc.description.peer-reviewPor pareses_ES
dc.formatapplication/pdfes_ES
dc.identifier.citationKelley, M. C., & Retterer, J. (2008). First successful prediction of a convective equatorial ionospheric storm using solar wind parameters.==$Space Weather, 6$==(8), S08003. https://doi.org/10.1029/2007SW000381es_ES
dc.identifier.doihttps://doi.org/10.1029/2007SW000381es_ES
dc.identifier.journalSpace Weatheres_ES
dc.identifier.urihttp://hdl.handle.net/20.500.12816/3274
dc.language.isoenges_ES
dc.publisherAmerican Geophysical Uniones_ES
dc.relation.ispartofurn:issn:1542-7390
dc.rightsinfo:eu-repo/semantics/restrictedAccesses_ES
dc.subjectPredicting CEISes_ES
dc.subjectPenetrating E Fieldses_ES
dc.subjectInstabilityes_ES
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.05.01es_ES
dc.titleFirst successful prediction of a convective equatorial ionospheric storm using solar wind parameterses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES

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