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Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/1687
DC FieldValueLanguage
dc.contributor.authorallEzquer, R. G.; Laboratorio de Ionosfera, Instituto de Fisica, Universidad Nacional de Tucuman, Argentinaen
dc.contributor.authorallMosert de Gonzalez, M.; Member of the Argentine Scientific and Technological Research Council, Buenos Aires, Argentinaen
dc.contributor.authorallHeredia, T.; Laboratorio de Ionosfera, Instituto de Fisica, Universidad Nacional de Tucuman, Argentinaen
dc.date.accessioned2006-09-21T14:51:33Zen
dc.date.available2006-09-21T14:51:33Zen
dc.date.issued1996-05en
dc.identifier.urihttp://hdl.handle.net/2122/1687en
dc.description.abstractThe Base Point Model (BPM) is used to model the electron density (N) profile in the ionosphere, This model assumes two Chapman profile expressions one for the bottomside and one for the topside, and requires a characteristic point called "F region base point". The comparison among the modeled and experimental bottom-side N profiles obtained from Tucuman (26,9°S; 65.4°W) ionosonde shows that, in general, there is a very good agreement within 30 km below the height of the maximum N(hm). Cases with a very good agreement for the entire N-profile are observed. The study of the electron content below hm and the Total Electron Content (TEC) measured over Tucuman shows that, the difference among predicted and measured TEC is due to the disagreement in the topside N-profile more than that observed in the bottomside N-profile.en
dc.format.extent1112033 bytesen
dc.format.mimetypeapplication/pdfen
dc.language.isoEnglishen
dc.relation.ispartofseries3/39 (1996)en
dc.subjectIonosphereen
dc.subjectelectron densityen
dc.subjecttotal electron contenten
dc.titleElectron density profile modelingen
dc.typearticleen
dc.type.QualityControlPeer-revieweden
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.99. General or miscellaneousen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorEzquer, R. G.en
dc.contributor.authorMosert de Gonzalez, M.en
dc.contributor.authorHeredia, T.en
dc.contributor.departmentMember of the Argentine Scientific and Technological Research Council, Buenos Aires, Argentinaen
dc.contributor.departmentLaboratorio de Ionosfera, Instituto de Fisica, Universidad Nacional de Tucuman, Argentinaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptMember of the Argentine Scientific and Technological Research Council, Buenos Aires, Argentina-
crisitem.author.deptLaboratorio de Ionosfera, Instituto de Fisica, Universidad Nacional de Tucuman, Argentina-
crisitem.classification.parent01. Atmosphere-
Appears in Collections:Annals of Geophysics
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