Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/3983
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dc.contributor.authorallVillante, U.; Dipartimento di Fisica, Università dell'Aquila, L’Aquila, Italyen
dc.contributor.authorallLepidi, S.; Dipartimento di Fisica, Università dell'Aquila, L’Aquila, Italyen
dc.contributor.authorallFrancia, P.; Dipartimento di Fisica, Università dell'Aquila, L’Aquila, Italyen
dc.contributor.authorallMeloni, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallPalangio, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.date.accessioned2008-07-21T08:33:21Zen
dc.date.available2008-07-21T08:33:21Zen
dc.date.issued1997-06-15en
dc.identifier.urihttp://hdl.handle.net/2122/3983en
dc.description.abstractA statistical analysis of the power spectra (0.7 - 5 mHz) of the geomagnetic field components H and D recorded at Terra Nova Bay (Antarctica) during three austral summers close to the maximum of solar activity reveals power enhancements in the H componenta t = 3.3, 3.9 and 4.5 mHz, which become more evident during daytime intervals. During intervals characterized by higher solar wind speeds these spectral features more clearly emerge and are also accompanied by other enhancements at lower frequencies (= 1.2, 1.9 and 2.7 mHz). The observed frequencies are close to the ones detected both at auroral and low latitudes.en
dc.language.isoEnglishen
dc.publisher.nameAGUen
dc.relation.ispartofGeophysical Research Lettersen
dc.relation.ispartofseries12 / 24 (1997)en
dc.subjectmagnetic pulsationsen
dc.subjectAntarcticaen
dc.titleLong period geomagnetic field fluctuations at Terra Nova Bay (Antarctica)en
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber1443-1446en
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.04. Plasma Physicsen
dc.subject.INGV01. Atmosphere::01.03. Magnetosphere::01.03.03. Magnetospheric physicsen
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dc.description.journalTypeN/A or not JCRen
dc.description.fulltextreserveden
dc.contributor.authorVillante, U.en
dc.contributor.authorLepidi, S.en
dc.contributor.authorFrancia, P.en
dc.contributor.authorMeloni, A.en
dc.contributor.authorPalangio, P.en
dc.contributor.departmentDipartimento di Fisica, Università dell'Aquila, L’Aquila, Italyen
dc.contributor.departmentDipartimento di Fisica, Università dell'Aquila, L’Aquila, Italyen
dc.contributor.departmentDipartimento di Fisica, Università dell'Aquila, L’Aquila, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
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.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.orcid0000-0002-3630-7958-
crisitem.author.orcid0000-0002-5692-2560-
crisitem.author.orcid0000-0003-1155-401X-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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