Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/7272
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dc.contributor.authorallPrikryl, P.; Communications Research Centre Canada, Ottawa, ON, Canadaen
dc.contributor.authorallSpogli, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallJayachandran, P. T.; Physics Department, University of New Brunswick, Fredericton, NB, Canadaen
dc.contributor.authorallKinrade, J.; Department of Electronic and Electrical Engineering, University of Bath, Bath, UKen
dc.contributor.authorallMitchell, C. N.; Department of Electronic and Electrical Engineering, University of Bath, Bath, UKen
dc.contributor.authorallNing, B.; Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, Chinaen
dc.contributor.authorallLi, G.; Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, Chinaen
dc.contributor.authorallCilliers, P. J.; South African National Space Agency, Hermanus, South Africaen
dc.contributor.authorallTerkildsen, M.; IPS Radio and Space Services, Bureau of Meteorology, Haymarket, NSW, Australiaen
dc.contributor.authorallDanskin, D. W.; Geomagnetic Laboratory, Natural Resources Canada, ON, Canadaen
dc.contributor.authorallSpanswick, E.; Department of Physics and Astronomy, University of Calgary, AB, Canadaen
dc.contributor.authorallWeatherwax, A. T.; Department of Physics and Astronomy, Siena College, Loudonville, NY, USAen
dc.contributor.authorallBristow, W. A.; Geophysical Institute, University of Alaska Fairbanks, Fairbanks, AK, USAen
dc.contributor.authorallAlfonsi, Lu.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallDe Franceschi, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallRomano, V.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallNgwira, C. M.; South African National Space Agency, Hermanus, South Africaen
dc.contributor.authorallOpperman, B. D. L.; South African National Space Agency, Hermanus, South Africaen
dc.date.accessioned2011-12-23T09:55:58Zen
dc.date.available2011-12-23T09:55:58Zen
dc.date.issued2011-12-21en
dc.identifier.urihttp://hdl.handle.net/2122/7272en
dc.description.abstractArrays of GPS Ionospheric Scintillation and TEC Monitors (GISTMs) are used in a comparative scintillation study focusing on quasi-conjugate pairs of GPS receivers in the Arctic and Antarctic. Intense GPS phase scintillation and rapid variations in ionospheric total electron content (TEC) that can result in cycle slips were observed at high latitudes with dual-frequency GPS receivers during the first significant geomagnetic storm of solar cycle 24 on 5–7 April 2010. The impact of a bipolar magnetic cloud of north-south (NS) type embedded in high speed solar wind from a coronal hole caused a geomagnetic storm with maximum 3-hourly Kp = 8- and hourly ring current Dst =−73 nT. The interhemispheric comparison of phase scintillation reveals similarities but also asymmetries of the ionospheric response in the northern and southern auroral zones, cusps and polar caps. In the nightside auroral oval and in the cusp/cleft sectors the phase scintillation was observed in both hemispheres at about the same times and was correlated with geomagnetic activity. The scintillation level was very similar in approximately conjugate locations in Qiqiktarjuaq (75.4° N; 23.4° E CGM lat. and lon.) and South Pole (74.1° S; 18.9° E), in Longyearbyen (75.3° N; 111.2° E) and Zhongshan (74.7° S; 96.7° E), while it was significantly higher in Cambridge Bay (77.0° N; 310.1° E) than at Mario Zucchelli (80.0° S; 307.7° E). In the polar cap, when the interplanetary magnetic field (IMF) was strongly northward, the ionization due to energetic particle precipitation was a likely cause of scintillation that was stronger at Concordia (88.8° S; 54.4° E) in the dark ionosphere than in the sunlit ionosphere over Eureka (88.1° N; 333.4° E), due to a difference in ionospheric conductivity. When the IMF tilted southward, weak or no significant scintillation was detected in the northern polar cap, while in the southern polar cap rapidly varying TEC and strong phase scintillation persisted for many hours. This interhemispheric asymmetry is explained by the difference in the location of solar terminator relative to the cusps in the Northern and Southern Hemisphere. Solar terminator was in the immediate proximity of the cusp in the Southern Hemisphere where sunlit ionospheric plasma was readily convected into the central polar cap and a long series of patches was observed. In contrast, solar terminator was far poleward of the northern cusp thus reducing the entry of sunlit plasma and formation of dense patches. This is consistent with the observed and modeled seasonal variation in occurrence of polar cap patches. The GPS scintillation and TEC data analysis is supported by data from ground-based networks of magnetometers, riometers, ionosondes, HF radars and all-sky imagers, as well as particle flux measurements by DMSP satellites.en
dc.language.isoEnglishen
dc.publisher.nameCopernicus Publicationsen
dc.relation.ispartofAnnales Geophysicaeen
dc.relation.ispartofseries12/29 (2011)en
dc.subjectIonosphere (Ionospheric irregularities)en
dc.subjectMagnetospheric physics (Storms and substorms)en
dc.subjectRadio science (Space and satellite communication)en
dc.titleInterhemispheric comparison of GPS phase scintillation at high latitudes during the magnetic-cloud-induced geomagnetic storm of 5–7 April 2010en
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber2287-2304en
dc.identifier.URLwww.ann-geophys.net/29/2287/2011/en
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniquesen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.07. Scintillationsen
dc.subject.INGV05. General::05.04. Instrumentation and techniques of general interest::05.04.99. General or miscellaneousen
dc.subject.INGV05. General::05.08. Risk::05.08.01. Environmental risken
dc.identifier.doi10.5194/angeo-29-2287-2011en
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dc.description.obiettivoSpecifico1.7. Osservazioni di alta e media atmosferaen
dc.description.obiettivoSpecifico3.9. Fisica della magnetosfera, ionosfera e meteorologia spazialeen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorPrikryl, P.en
dc.contributor.authorSpogli, L.en
dc.contributor.authorJayachandran, P. T.en
dc.contributor.authorKinrade, J.en
dc.contributor.authorMitchell, C. N.en
dc.contributor.authorNing, B.en
dc.contributor.authorLi, G.en
dc.contributor.authorCilliers, P. J.en
dc.contributor.authorTerkildsen, M.en
dc.contributor.authorDanskin, D. W.en
dc.contributor.authorSpanswick, E.en
dc.contributor.authorWeatherwax, A. T.en
dc.contributor.authorBristow, W. A.en
dc.contributor.authorAlfonsi, Lu.en
dc.contributor.authorDe Franceschi, G.en
dc.contributor.authorRomano, V.en
dc.contributor.authorNgwira, C. M.en
dc.contributor.authorOpperman, B. D. L.en
dc.contributor.departmentCommunications Research Centre Canada, Ottawa, ON, Canadaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentPhysics Department, University of New Brunswick, Fredericton, NB, Canadaen
dc.contributor.departmentDepartment of Electronic and Electrical Engineering, University of Bath, Bath, UKen
dc.contributor.departmentDepartment of Electronic and Electrical Engineering, University of Bath, Bath, UKen
dc.contributor.departmentInstitute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, Chinaen
dc.contributor.departmentInstitute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, Chinaen
dc.contributor.departmentSouth African National Space Agency, Hermanus, South Africaen
dc.contributor.departmentIPS Radio and Space Services, Bureau of Meteorology, Haymarket, NSW, Australiaen
dc.contributor.departmentGeomagnetic Laboratory, Natural Resources Canada, ON, Canadaen
dc.contributor.departmentDepartment of Physics and Astronomy, University of Calgary, AB, Canadaen
dc.contributor.departmentDepartment of Physics and Astronomy, Siena College, Loudonville, NY, USAen
dc.contributor.departmentGeophysical Institute, University of Alaska Fairbanks, Fairbanks, AK, USAen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentSouth African National Space Agency, Hermanus, South Africaen
dc.contributor.departmentSouth African National Space Agency, Hermanus, South Africaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptCommunications Research Centre Canada-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptUniversity of New Brunswick-
crisitem.author.deptUniversity of Bath, Electronic and Electrical Engineering, Bath, United Kingdom-
crisitem.author.dept3Department of Electronic and Electrical Engineering, University of Bath-
crisitem.author.deptInstitute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China-
crisitem.author.deptInstitute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China-
crisitem.author.deptSpace Science Directorate, South African National Space Agency, Hermanus, South Africa-
crisitem.author.deptIPS Radio and Space Services, Bureau of Meteorology, Haymarket, NSW, Australia-
crisitem.author.deptGeomagnetic Laboratory, Natural Resources Canada, ON, Canada-
crisitem.author.deptUniversity of Calgary-
crisitem.author.deptDepartment of Physics and Astronomy, Siena College, Loudonville, NY, USA-
crisitem.author.deptGeophysical Institute, University of Alaska Fairbanks, Fairbanks, AK, USA-
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.deptSouth African National Space Agency, Hermanus, South Africa-
crisitem.author.deptSouth African National Space Agency, Hermanus, South Africa-
crisitem.author.orcid0000-0003-2310-0306-
crisitem.author.orcid0000-0003-3175-5134-
crisitem.author.orcid0000-0002-1806-9327-
crisitem.author.orcid0000-0002-3943-6798-
crisitem.author.orcid0000-0002-7532-4507-
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.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent05. General-
crisitem.classification.parent05. General-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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