On the plasma instability mechanisms responsible for Esq

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dc.contributor.authorBalsley, Ben B.
dc.contributor.authorRey, Augusto
dc.contributor.authorWoodman Pollitt, Ronald Francisco
dc.date.accessioned2018-07-03T11:17:28Z
dc.date.available2018-07-03T11:17:28Z
dc.date.issued1976-03-01
dc.description.abstractEvidence is presented showing that the gradient drift (type 2) irregularities are the most probable scatterers responsible for equatorial sporadic E (Esq) echoes observed on conventional equatorial ionograms and that the two‐stream (type 1) irregularities are not detectable at ionosonde wavelengths (1–10 MHz).
dc.description.peer-reviewPor pares
dc.formatapplication/pdf
dc.identifier.citationBalsley, B., Rey, A., & Woodman, R. F. (1976). On the plasma instability mechanisms responsible for Esq.==$Journal Geophysical Research, 81$==(7), 1391-1396. https://doi.org/10.1029/JA081i007p01391
dc.identifier.doihttps://doi.org/10.1029/JA081i007p01391
dc.identifier.journalJournal de Geophysical Research
dc.identifier.urihttp://hdl.handle.net/20.500.12816/1644
dc.language.isoeng
dc.publisherAmerican Geophysical Union
dc.relation.ispartofurn:issn:0148-0227
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectPlasma instabilities
dc.subjectIonosphere
dc.subjectE Region
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.05.01
dc.titleOn the plasma instability mechanisms responsible for Esq
dc.typeinfo:eu-repo/semantics/article

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