Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/3932
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dc.contributor.authorallVillante, U.; Dipartimento di Fisica, Università dell'Aquila, L'Aquila, Italyen
dc.contributor.authorallLepidi, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallFrancia, P.; Dipartimento di Fisica, Università dell'Aquila, L'Aquila, Italyen
dc.contributor.authorallVellante, M.; 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.authorallLepping, R. P.; Laboratory for Extraterrestrial Physics, NASA/GSFC, Greenbelt, USAen
dc.contributor.authorallMariani, F.; Dipartimento di Fisica, Università di Roma-Tor Vergata, Italyen
dc.date.accessioned2008-07-07T08:35:09Zen
dc.date.available2008-07-07T08:35:09Zen
dc.date.issued1999en
dc.identifier.urihttp://hdl.handle.net/2122/3932en
dc.description.abstractPc3 geomagnetic field fluctuations detected at low latitude (L'Aquila, Italy) during the passage of a high velocity solar wind stream, characterized by variable interplanetary magnetic field conditions, are analyzed. Higher frequency resonant fluctuations and lower frequency phenomena are simultaneously observed; the intermittent appearance and the variable frequency of the longer period modes can be well interpreted in terms of the variable IMF elements; moreover their polarization characteristics are consistent with an origin related to external waves propagating in antisunward direction. A comparison with simultaneous observations performed at Terra Nova Bay (Antarctica) provides additional evidence for a clear relationship between the IMF and Pc3 pulsations also at very high latitudes.en
dc.language.isoEnglishen
dc.publisher.nameEGS - Springer-Verlagen
dc.relation.ispartofAnnales Geophysicaeen
dc.relation.ispartofseries4 / 17 (1999)en
dc.subjectMagnetospheric physicsen
dc.subjectMHD waves and instabilitiesen
dc.subjectSolar wind-magnetosphere interactionsen
dc.titlePc3 pulsations during variable IMF conditionsen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber490-496en
dc.subject.INGV01. Atmosphere::01.03. Magnetosphere::01.03.99. General or miscellaneousen
dc.subject.INGV01. Atmosphere::01.03. Magnetosphere::01.03.02. Magnetic stormsen
dc.subject.INGV01. Atmosphere::01.03. Magnetosphere::01.03.04. Structure and dynamicsen
dc.relation.referencesAnsari, I. A., and B. J. Fraser, A multistation study of low latitude Pc3 geomagnetic pulsations, Planet. Space Sci., 34, 519, 1986. Baransky, L. N., S. P. Belokris, U. E. Borovkov, and C. A. Green, Two simple methods for the determination of the resonance frequencies of magnetic ®eld lines, Planet. Space Sci., 38, 1573, 1990. Chen, L., and A. Hasegawa, A theory of long-period magnetic pulsations, 1, steady state excitation of ®eld line resonances, J. Geophys. Res., 79, 1024, 1974. Chi, P. J., C. T. Russell, and G. Le, Pc3 and Pc4 activity during a long period of low interplanetary magnetic ®eld cone angle as detected across the Institute of Geological Sciences array, J. Geophys. Res., 99, 11127, 1994. Engebretson M. J., C.-I. Meng, R. L. Arnoldy, and L. J. Cahill, Jr., Pc3 pulsations observed near the south polar cusp, J. Geophys. Res., 91, 8909, 1986. Engebretson M. J., B. J. Anderson, L. J. Cahill, Jr., R. L. Arnoldy, P. T. Newell, C.-I. Meng, L. J. Zanetti, and T. A. Potemra, A multipoint case study of high latitude daytime ULF pulsations, J. Geophys. Res., 94, 17 143, 1989. Engebretson M. J., L. J. Cahill, Jr., R. L. Arnoldy, B. J. Anderson, T. J. Rosenberg, D. L. Carpenter, U. S. Inan, and R. H. Eather, The role of the ionosphere in coupling upstream ULF wave power into the dayside magnetosphere, J. Geophys. Res., 96, 1527, 1991. Farrugia, C. J., M. P. Freeman, S. W. H. Cowley, D. J. Southwood, M. Lockwood, and A. Etemadi, Pressure driven magnetopause motions and attendant response on the ground, Planet. Space Sci., 37, 589, 1989. Green, A. W., E. W. Worthington, L. N. Baransky, E. N. Fedorov, N. A. Kurneva, V. A. Pilipenko, D. N. Shvetzov, A. A. Bektemirov, and G. V. Philipov, Alfve n ®eld line resonances at low-latitudes (L = 1.5), J. Geophys. Res., 98, 15 693, 1993. Greenstadt, E. W., and J. V. Olson, Pc3,4 activity and interplan- etary ®eld orientation, J. Geophys. Res., 81, 5911, 1976. Greenstadt, E. W., R. L. McPherron, and K. Takahashi, Solar wind control of daytime, midperiod geomagnetic pulsations, J. Geomagn Geoelectr., 32 (11), 89, 1980. Lanzerotti, L. J., L. V. Medford, C. G. Maclennan, T. Hasegawa, M. H. Acuna, and S. R. Dolce, Polarization characteristics of hydromagnetic waves at low geomagnetic latitudes, J. Geophys. Res., 86, 5500, 1981. Le, G., and C. T. Russell, Solar wind control of upstream wave frequency, J. Geophys. Res., 101, 2571, 1996. Lepidi, S., U. Villante, M. Vellante, P. Palangio, and A. Meloni, High resolution geomagnetic ®eld observations at Terra Nova Bay, Antarctica, Ann. Geo®s., 34, 519, 1996. Odera, T. J., Solar wind controlled pulsations: a review, Rev. Geophys., 24, 55, 1986. Russell, C. T., J. G. Luhmann, T. J. Odera, and W. F. Stuart, The rate of occurrence of dayside Pc3,4 pulsations: the L-value dependence of the IMF cone angle e ect, J. Geophys. Res., 10, 663, 1983. Southwood, D. J., Some features of ®eld-line resonances in the magnetosphere, Planet. Space Sci., 22, 483, 1974. Troitskaya, V. A., and O. V. Bolshakova, Diagnostics of the magnetosphere using multipoint measurements of ULF-waves, Adv. Space Res., 8, 413, 1988. Vellante, M., U. Villante, M. De Lauretis, and P. Cerulli-Irelli, An analysis of micropulsation events at a low-latitude station during 1985, Planet. Space Sci., 37, 767, 1989. Vellante, M., U. Villante, R. Core, A. Best, D. Lenners, and V. A. Pilipenko, Simultaneous geomagnetic pulsation observations at two latitudes: resonant mode characteristics, Ann. Geophysicae, 11, 734, 1993. Vellante, M., U. Villante, M. De Lauretis, G. Barchi, Solar cycle variation of the dominant frequencies of Pc3 geomagnetic pulsations at L = 1.6, Geophys. Res. Lett., 23, 1505, 1996. Villante, U., S. Lepidi, M. Vellante, A. J. Lazarus, and R. P. Lepping, Pc3 activity at low geomagnetic latitudes: a comparison with solar wind observations, Planet. Space Sci., 40, 1399, 1992. Villante, U., M. De Lauretis, P. Francia, S. Lepidi, L. Cafarella, A. Meloni, A. J. Lazarus, R. P. Lepping, and F. Mariani, Low frequency geomagnetic ®eld variations at low and high latitude during the January 10±11, 1997 magnetic cloud, Geophys. Res. Lett., 25, 2593, 1998. Waters, C. L., F. W. Menk, and B. J. Fraser, Low latitude geomagnetic ®eld line resonance: experiment and modeling, J. Geophys. Res., 99, 17 547, 1994. Webb, D., and D. Orr, Geomagnetic pulsations (5±50 mHz) and the interplanetary magnetic ®eld, J. Geophys. Res., 81, 5941, 1976. Yumoto, K., Generation and propagation mechanisms of low- latitude magnetic pulsations ± a review, J. Geophys., 60, 79, 1986. Yumoto, K., and T. Saito, Relation of compressional HM waves at GOES 2 to low-latitude Pc3 magnetic pulsations, J. Geophys. Res., 88, 10 041, 1983. Yumoto, K., T. Saito, and Y. Tanaka, Low-latitude Pc3 magnetic pulsations observed at conjugate stations (L 1.5), J. Geophys. Res., 90, 12 201, 1985. Yumoto, K., T. Saito, Y. Tanaka, K. J. W. Lynn, F. W. Menk, and B. J. Fraser, Polarization and amplitude characteristics of Pc3 pulsations in conjugate area around L = 1.3±2.1, J. Geophys. Res., 93, 7386, 1988.en
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.authorVellante, M.en
dc.contributor.authorMeloni, A.en
dc.contributor.authorLepping, R. P.en
dc.contributor.authorMariani, F.en
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.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.departmentLaboratory for Extraterrestrial Physics, NASA/GSFC, Greenbelt, USAen
dc.contributor.departmentDipartimento di Fisica, Università di Roma-Tor Vergata, Italyen
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.deptLaboratory for Extraterrestrial Physics, NASA/GSFC, Greenbelt, USA-
crisitem.author.deptDipartimento di Fisica, Università di Roma-Tor Vergata, Italy-
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.classification.parent01. Atmosphere-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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