Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9092
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dc.contributor.authorallPezzopane, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.date.accessioned2014-09-11T06:48:55Zen
dc.date.available2014-09-11T06:48:55Zen
dc.date.issued2014-09en
dc.identifier.urihttp://hdl.handle.net/2122/9092en
dc.description.abstractUnusual nighttime impulsive electron density enhancements that are rarely observed at low latitudes on a wide region of South America are here investigated. These phenomena are very atypical because besides being of brief duration, they are characterized by a pronounced compression of the ionosphere. The events were studied and analyzed using both the F2 layer critical frequency (foF2) and the lowest virtual height of the ordinary trace of the F region (h'F) values recorded at five ionospheric stations widely distributed in space. A careful analysis of isoheight ionosonde plots suggests that traveling ionospheric disturbances (TIDs) caused by atmospheric gravity wave (AGW) propagation could play a significant role in causing these phenomena, both for quiet and for medium-high geomagnetic activity; in the latter case however a nocturnal recharging of the fountain effect, due to electric fields penetrating from the magnetosphere, plays an as much significant role.en
dc.language.isoEnglishen
dc.relation.ispartofIl Nuovo Cimento Cen
dc.relation.ispartofseries4/37(2014)en
dc.subjectEquatorial ionosphereen
dc.subjectIonosphere/atmospheric interactionsen
dc.subjectMagnetic storms, substormsen
dc.subjectIonosphere/magnetosphere interactionsen
dc.titleUnusual nighttime impulsive enhancements of electron density characterizing the low-latitude ionosphere: Phenomenology and possible mechanisms of triggeringen
dc.typearticleen
dc.description.statusPublisheden
dc.description.pagenumber145-154en
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::01.02.05. Wave propagationen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniquesen
dc.subject.INGV01. Atmosphere::01.03. Magnetosphere::01.03.02. Magnetic stormsen
dc.identifier.doi10.1393/ncc/i2014-11799-9en
dc.description.obiettivoSpecifico2A. Fisica dell'alta atmosferaen
dc.description.obiettivoSpecifico1IT. Reti di monitoraggio e Osservazionien
dc.description.journalTypeN/A or not JCRen
dc.description.fulltextrestricteden
dc.contributor.authorPezzopane, M.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.orcid0000-0001-5800-2322-
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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