Theoretical relationship between maximum value of the post-sunset drift velocity and peak-to-valley ratio of anomaly TEC

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dc.contributor.authorBasu, B.
dc.contributor.authorRetterer, J. M.
dc.contributor.authorDe La Beaujardiére, O.
dc.contributor.authorValladares, C. E.
dc.contributor.authorKudeki, E.
dc.date.accessioned2018-07-13T15:39:19Z
dc.date.available2018-07-13T15:39:19Z
dc.date.issued2004-02-11
dc.description.abstractTheoretical study of electron density distribution in the nighttime equatorial ionosphere shows that linear relationships with statistically significant correlation coefficients exist between the maximum value of the post‐sunset plasma drift velocity and the peak‐to‐valley ratio of anomaly TEC. The study is based on the low‐latitude density model of Air Force Research Laboratory (AFRL) and the obtained relationships are valid for the longitudinal sector of Jicamarca incoherent scatter radar whose drift velocity measurements are used. The significance of this finding lies in the fact that the maximum value of the post‐sunset vertical plasma drift velocity is an important parameter for determining both the intensity and the latitudinal distribution of equatorial scintillation. When the parameter is not available from any direct measurement, the linear relationships may be used to estimate it from the measured peak‐to‐valley ratio of anomaly TEC.es_ES
dc.description.peer-reviewPor pareses_ES
dc.formatapplication/pdfes_ES
dc.identifier.citationBasu, B., Retterer, J. M., De La Beaujardiére, O., Valladares, C. E., & Kudeki, E. (2004). Theoretical relationship between maximum value of the post-sunset drift velocity and peak-to-valley ratio of anomaly TEC.==$Geophysical Research Letters, 31$==(3), L03807. https://doi.org/10.1029/2003GL018725es_ES
dc.identifier.doihttps://doi.org/10.1029/2003GL018725es_ES
dc.identifier.journalGeophysical Research Letterses_ES
dc.identifier.urihttp://hdl.handle.net/20.500.12816/1835
dc.language.isoenges_ES
dc.publisherAmerican Geophysical Uniones_ES
dc.relation.ispartofurn:issn:0094-8276
dc.rightsinfo:eu-repo/semantics/restrictedAccesses_ES
dc.subjectNighttime equatorial anomalyes_ES
dc.subjectTECes_ES
dc.subjectPost‐sunset drift velocityes_ES
dc.subjectScintillationes_ES
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.05.01es_ES
dc.titleTheoretical relationship between maximum value of the post-sunset drift velocity and peak-to-valley ratio of anomaly TECes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES

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