Radar scatter from equatorial electrojet waves: An explanation for the constancy of the Type I Doppler shift with zenith angle

dc.contributor.authorKelley, M. C.
dc.contributor.authorCuevas, R. A.
dc.contributor.authorHysell, D. L.
dc.date.accessioned2018-10-31T15:00:57Z
dc.date.available2018-10-31T15:00:57Z
dc.date.issued2008-02-26
dc.description.abstractThe first results from the 430 MHz Advanced Modular Incoherent Scatter Radar Prototype (AMISR‐P) at the Jicamarca Radio Observatory were reported by Hysell et al. (2007). We present additional data showing that the phase velocity of Type I echoes is independent of zenith angle, an unexplained property of these waves. We interpret the results using rocket data by predicting the total line‐of‐sight velocity at the four zenith angles used. We find that the radars preferentially detect waves within 10% of Cs in at least four range gates for all beams and up to eight range gates for the 51 JULIA beam. This result is consistent with recent auroral observations that Type I waves are only generated with k vectors near the electron flow velocity, where the latter is the vector sum of the zero‐order drift and the perturbation drift due to large‐scale waves in the equatorial case.es_ES
dc.description.peer-reviewPor pareses_ES
dc.formatapplication/pdfes_ES
dc.identifier.citationKelley, M. C., Cuevas, R. A., & Hysell, D. L. (2008). Radar scatter from equatorial electrojet waves: An explanation for the constancy of the Type I Doppler shift with zenith angle.==$Geophysical Research Letters, 35$==(4), L04106. https://doi.org/10.1029/2007GL032848es_ES
dc.identifier.doihttps://doi.org/10.1029/2007GL032848es_ES
dc.identifier.journalGeophysical Research Letterses_ES
dc.identifier.urihttp://hdl.handle.net/20.500.12816/3253
dc.language.isoenges_ES
dc.publisherAmerican Geophysical Uniones_ES
dc.relation.ispartofurn:issn:0094-8276
dc.rightsinfo:eu-repo/semantics/restrictedAccesses_ES
dc.subjectEquatorial electrojetes_ES
dc.subjectFarley‐Buneman waveses_ES
dc.subjectTwo‐stream instabilityes_ES
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.05.01es_ES
dc.titleRadar scatter from equatorial electrojet waves: An explanation for the constancy of the Type I Doppler shift with zenith anglees_ES
dc.typeinfo:eu-repo/semantics/articlees_ES

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