Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10448
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dc.contributor.authorallTardelli, A.; Universidade do Vale do Paraíba (UNIVAP), São José dos Campos, Brazilen
dc.contributor.authorallFagundes, P. R.; Universidade do Vale do Paraíba (UNIVAP), São José dos Campos, Brazilen
dc.contributor.authorallPezzopane, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallPillat, V. G.; Universidade do Vale do Paraíba (UNIVAP), São José dos Campos, Brazilen
dc.contributor.authorallVenkatesh, K.; Universidade do Vale do Paraíba (UNIVAP), São José dos Campos, Brazilen
dc.date.accessioned2017-02-02T07:09:13Zen
dc.date.available2017-02-02T07:09:13Zen
dc.date.issued2016-12-20en
dc.identifier.urihttp://hdl.handle.net/2122/10448en
dc.description.abstractThe study of multiple stratification of the F layer has the initial records in the midtwentieth century. Since then, many studies were focused on F3 layer. The diurnal, seasonal, and solar activity variations of the F3 layer characteristics have been investigated by several researchers. Recently, investigations on multiple stratifications of F layer received an important boost after the quadruple stratification (StF-4) was observed at Palmas (10.3°S, 48.3°W; dip latitude 6.6°S—near-equatorial region), Brazil. The present study reports the latest findings related with the seasonal and solar activity characteristics of the F3 layer and StF-4 near the equatorial region during the period from 2002 to 2006. A significant connection between StF-4 and F3 layer has been noticed, since the StF-4 is always preceded and followed by a F3 layer appearance. However, the F3 layer and the StF-4 present different seasonal and solar cycle variations. At a near-equatorial station Palmas, the F3 layer shows the maximum and minimum occurrences during summer and winter seasons, respectively. On the contrary, the StF-4 presents the maximum and minimum occurrences during winter and summer seasons, respectively. While the F3 layer occurrence is not affected by solar cycle, the StF-4 appearance is instead more frequent during high solar activity.en
dc.language.isoEnglishen
dc.publisher.nameAmerican Geophysical Unionen
dc.relation.ispartofJournal of geophysical research - space physicsen
dc.relation.ispartofseries12/121(2016)en
dc.subjectIonogramen
dc.subjectF layeren
dc.subjectF3 layeren
dc.subjectF4 layeren
dc.subjectlow-latitude ionosphereen
dc.titleSeasonal and solar activity variations of F3 layer and quadruple stratification (StF-4) near the equatorial regionen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber12116–12125en
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.99. General or miscellaneousen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.02. Dynamicsen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.04. Plasma Physicsen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.05. Wave propagationen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniquesen
dc.identifier.doi10.1002/2016JA023580en
dc.description.obiettivoSpecifico2A. Fisica dell'alta atmosferaen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.relation.issn0148-0227en
dc.contributor.authorTardelli, A.en
dc.contributor.authorFagundes, P. R.en
dc.contributor.authorPezzopane, M.en
dc.contributor.authorPillat, V. G.en
dc.contributor.authorVenkatesh, K.en
dc.contributor.departmentUniversidade do Vale do Paraíba (UNIVAP), São José dos Campos, Brazilen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentUniversidade do Vale do Paraíba (UNIVAP), São José dos Campos, Brazilen
dc.contributor.departmentUniversidade do Vale do Paraíba (UNIVAP), São José dos Campos, Brazilen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptLaboratorio de FIsica e Astronomia, Universidade do Vale do Paraiba (UNIVAP)-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptLaboratorio de FIsica e Astronomia, Universidade do Vale do Paraiba (UNIVAP)-
crisitem.author.deptUniversidade do Vale do Paraíba (UNIVAP), São José dos Campos, Brazil-
crisitem.author.orcid0000-0003-4916-6012-
crisitem.author.orcid0000-0001-5800-2322-
crisitem.author.orcid0000-0002-5849-0597-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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