Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/8731
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dc.contributor.authorallPrikryl, P.; Communications Research Centre, Ottawa, ON, Canadaen
dc.contributor.authorallZhang, Y.; Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United Statesen
dc.contributor.authorallEbihara, Y.; Research Institute for Sustainable Humanosphere, Kyoto University, Kyoto, Japanen
dc.contributor.authorallGhoddousi-Fard, R.; Natural Resources Canada, Geodetic Survey Division, Ottawa, ON, Canadaen
dc.contributor.authorallJayachandran, P. T.; University of New Brunswick, Physics Department, Fredericton, NB, Canadaen
dc.contributor.authorallKinrade, J.; University of Bath, Electronic and Electrical Engineering, Bath, United Kingdomen
dc.contributor.authorallMitchell, C. N.; University of Bath, Electronic and Electrical Engineering, Bath, United Kingdomen
dc.contributor.authorallWeatherwax, A. T.; Siena College, Physics and Astronomy, Loudonville, NY, United Statesen
dc.contributor.authorallBust, G.; Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United Statesen
dc.contributor.authorallCilliers, P. J.; South African National Space Agency, Space Science Directorate, Hermanus, South Africaen
dc.contributor.authorallSpogli, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallAlfonsi, Lu.; 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.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.authorallJarvis, M. J.; British Antarctic Survey, Physical Sciences Division, Cambridge, United Kingdomen
dc.contributor.authorallDanskin, D. W.; Natural Resources Canada, Geomagnetic Laboratory, Ottawa, ON, Canadaen
dc.contributor.authorallSpanswick, E.; University of Calgary, Department of Physics and Astronomy, AB, Canadaen
dc.contributor.authorallDonovan, E.; University of Calgary, Department of Physics and Astronomy, AB, Canadaen
dc.contributor.authorallTerkildsen, M.; IPS Radio and Space Services, Bureau of Meteorology, Haymarket, NSW, Australiaen
dc.date.accessioned2013-08-01T08:40:01Zen
dc.date.available2013-08-01T08:40:01Zen
dc.date.issued2013en
dc.identifier.urihttp://hdl.handle.net/2122/8731en
dc.description.abstractThe global positioning system (GPS) phase scintillation caused by highlatitude ionospheric irregularities during an intense high-speed stream (HSS) of the solar wind from April 29 to May 5, 2011, was observed using arrays of GPS ionospheric scintillation and total electron content monitors in the Arctic and Antarctica. The one-minute phase-scintillation index derived from the data sampled at 50 Hz was complemented by a proxy index (delta phase rate) obtained from 1-Hz GPS data. The scintillation occurrence coincided with the aurora borealis and aurora australis observed by an all-sky imager at the South Pole, and by special sensor ultraviolet scanning imagers on board satellites of the Defense Meteorological Satellites Program. The South Pole (SP) station is approximately conjugate with two Canadian High Arctic Ionospheric Network stations on Baffin Island, Canada, which provided the opportunity to study magnetic conjugacy of scintillation with support of riometers and magnetometers. The GPS ionospheric pierce points were mapped at their actual or conjugate locations, along with the auroral emission over the South Pole, assuming an altitude of 120 km. As the aurora brightened and/or drifted across the field of view of the all-sky imager, sequences of scintillation events were observed that indicated conjugate auroras as a locator of simultaneous or delayed bipolar scintillation events. In spite of the greater scintillation intensity in the auroral oval, where phase scintillation sometimes exceeded 1 radian during the auroral break-up and substorms, the percentage occurrence of moderate scintillation was highest in the cusp. Interhemispheric comparisons of bipolar scintillation maps show that the scintillation occurrence is significantly higher in the southern cusp and polar cap.en
dc.language.isoEnglishen
dc.publisher.nameINGVen
dc.relation.ispartofAnnals of Geophysicsen
dc.relation.ispartofseries2 / 56 (2013)en
dc.subjectScintillationsen
dc.subjectSolar-terrestrial interactionen
dc.subjectSpace weatheren
dc.subjectSolar variability and solar winden
dc.subjectMagnetic stormsen
dc.titleAn interhemispheric comparison of GPS phase scintillation with auroral emission observed at the South Pole and from the DMSP satelliteen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumberR0216en
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.99. General or miscellaneousen
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::01.02. Ionosphere::01.02.07. Scintillationsen
dc.subject.INGV05. General::05.07. Space and Planetary sciences::05.07.02. Space weatheren
dc.identifier.doi10.4401/ag-6227en
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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.authorZhang, Y.en
dc.contributor.authorEbihara, Y.en
dc.contributor.authorGhoddousi-Fard, R.en
dc.contributor.authorJayachandran, P. T.en
dc.contributor.authorKinrade, J.en
dc.contributor.authorMitchell, C. N.en
dc.contributor.authorWeatherwax, A. T.en
dc.contributor.authorBust, G.en
dc.contributor.authorCilliers, P. J.en
dc.contributor.authorSpogli, L.en
dc.contributor.authorAlfonsi, Lu.en
dc.contributor.authorRomano, V.en
dc.contributor.authorNing, B.en
dc.contributor.authorLi, G.en
dc.contributor.authorJarvis, M. J.en
dc.contributor.authorDanskin, D. W.en
dc.contributor.authorSpanswick, E.en
dc.contributor.authorDonovan, E.en
dc.contributor.authorTerkildsen, M.en
dc.contributor.departmentCommunications Research Centre, Ottawa, ON, Canadaen
dc.contributor.departmentJohns Hopkins University Applied Physics Laboratory, Laurel, MD, United Statesen
dc.contributor.departmentResearch Institute for Sustainable Humanosphere, Kyoto University, Kyoto, Japanen
dc.contributor.departmentNatural Resources Canada, Geodetic Survey Division, Ottawa, ON, Canadaen
dc.contributor.departmentUniversity of New Brunswick, Physics Department, Fredericton, NB, Canadaen
dc.contributor.departmentUniversity of Bath, Electronic and Electrical Engineering, Bath, United Kingdomen
dc.contributor.departmentUniversity of Bath, Electronic and Electrical Engineering, Bath, United Kingdomen
dc.contributor.departmentSiena College, Physics and Astronomy, Loudonville, NY, United Statesen
dc.contributor.departmentJohns Hopkins University Applied Physics Laboratory, Laurel, MD, United Statesen
dc.contributor.departmentSouth African National Space Agency, Space Science Directorate, Hermanus, South Africaen
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.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.departmentBritish Antarctic Survey, Physical Sciences Division, Cambridge, United Kingdomen
dc.contributor.departmentNatural Resources Canada, Geomagnetic Laboratory, Ottawa, ON, Canadaen
dc.contributor.departmentUniversity of Calgary, Department of Physics and Astronomy, AB, Canadaen
dc.contributor.departmentUniversity of Calgary, Department of Physics and Astronomy, AB, Canadaen
dc.contributor.departmentIPS Radio and Space Services, Bureau of Meteorology, Haymarket, NSW, Australiaen
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.deptDepartment of Geological Sciences, The University of Michigan, Ann Arbor (MI) USA-
crisitem.author.deptResearch Institute for Sustainable Humanosphere, Kyoto University, Kyoto, Japan-
crisitem.author.deptNatural Resources Canada, Geodetic Survey Division, Ottawa, ON, Canada-
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.deptDepartment of Physics and Astronomy, Siena College, Loudonville, NY, USA-
crisitem.author.deptApplied Research Laboratories, The University of Texas at Austin, TX, U.S.A.-
crisitem.author.deptSpace Science Directorate, South African National Space Agency, Hermanus, South Africa-
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.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.deptBritish Antarctic Survey, Physical Sciences Division, Cambridge, United Kingdom-
crisitem.author.deptGeomagnetic Laboratory, Natural Resources Canada, ON, Canada-
crisitem.author.deptUniversity of Calgary-
crisitem.author.deptUniversity of Calgary-
crisitem.author.deptIPS Radio and Space Services, Bureau of Meteorology, Haymarket, NSW, Australia-
crisitem.author.orcid0000-0003-3175-5134-
crisitem.author.orcid0000-0003-2310-0306-
crisitem.author.orcid0000-0002-1806-9327-
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.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
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-
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