Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/4542
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dc.contributor.authorallAlfonsi, Lu.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallKavanagh, A. J.; Space Plasma Environment and Radio Science Group, Department of Communication Systems, InfoLab 21, Lancaster University, Lancaster LA1 4WA, UKen
dc.contributor.authorallAmata, E.; Istituto di Fisica dello Spazio Interplanetario I.N.A.F., Via del fosso del cavaliere 100, 00133 Rome, Italyen
dc.contributor.authorallCilliers, P.; Hermanus Magnetic Observatory (HMO), P.O. Box 32, Hermanus, South Africaen
dc.contributor.authorallCorreia, E.; Instituto Nacional de Pesquisas Espaciais (INPE), São José dos Campos, Brazil and Centro de Rádio Astronomia e Astrofísica Mackenzie (CRAAM), Universidade Presbiteriana Mackenzie, Rua da Consolação 930, CEP: 01302-907 São Paulo, Brazilen
dc.contributor.authorallFreeman, M.; British Antarctic Survey, High Cross Madingley Road, Cambridge, UKen
dc.contributor.authorallKauristie, K.; Finnish Meteorological Institute, Erik Palménin aukio 1, Helsinki, Finlanden
dc.contributor.authorallLiu, R.; Polar Research Institute of China, Shanghai 200136, Chinaen
dc.contributor.authorallLuntama, J.-P.; Finnish Meteorological Institute, Erik Palménin aukio 1, Helsinki, Finlanden
dc.contributor.authorallMitchell, C. N.; Department of Electrical Engineering, University of Bath, Bath BA2 7AY, UKen
dc.contributor.authorallZherebtsov, G. A.; Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Science, Irkutsk, Russiaen
dc.date.accessioned2008-12-09T14:01:56Zen
dc.date.available2008-12-09T14:01:56Zen
dc.date.issued2008-12en
dc.identifier.urihttp://hdl.handle.net/2122/4542en
dc.description.abstractDuring the International Polar Year (IPY), one area of great interest is co-coordinated, multi-instrument probing of the ionosphere at high latitudes. This region is important not only for the applications that rely upon our understanding of it, but also because it contains the footprints of processes that have their origin in the interplanetary space. Many different techniques are now available for probing the ionosphere, from radar measurements to the analysis of very low frequency (VLF) wavepaths. Combining these methods provides the ability to study the ionosphere from high in the F-region to the bottom of the D-layer. Thus, coupling processes from the magnetosphere and to the neutral atmosphere can be considered. An additional dimension is through comparisons of the response of the two polar ionospheres to similar (or the same) geomagnetic activity. With more instruments available at the South Pole inter-hemispheric, studies have become easier to accomplish such that a fuller picture of the global response to Sun–Earth coupling can be painted. This paper presents a review of the current state of knowledge in ionospheric probing. It cannot provide a comprehensive guide of the work to date due to the scale of the topic.Rather it is intended to give an overview of the techniques and recent results from some of the instruments and facilities that are a part of the IPY cluster 63—Heliosphere Impact on Geospace. In this way it is hoped that the reader will gain a flavor of the recent research performed in this area and the potential for continuing collaboration and capabilities during the IPY (2007–2009).en
dc.language.isoEnglishen
dc.publisher.nameElsevier Ltd.en
dc.relation.ispartofJournal of Atmospheric and Solar-Terrestrial Physicsen
dc.relation.ispartofseries18 / 70 (2008)en
dc.subjectPolar ionosphereen
dc.subjectInternational polar yearen
dc.subjectConjugacyen
dc.subjectInterhemispheric studiesen
dc.titleProbing the high latitude ionosphere from ground-based observations: The state of current knowledge and capabilities during IPY (2007–2009)en
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber2293-2308en
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.02. Dynamicsen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniquesen
dc.subject.INGV05. General::05.07. Space and Planetary sciences::05.07.01. Solar-terrestrial interactionen
dc.subject.INGV05. General::05.07. Space and Planetary sciences::05.07.02. Space weatheren
dc.identifier.doi10.1016/j.jastp.2008.06.013en
dc.description.obiettivoSpecifico3.9. Fisica della magnetosfera, ionosfera e meteorologia spazialeen
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorAlfonsi, Lu.en
dc.contributor.authorKavanagh, A. J.en
dc.contributor.authorAmata, E.en
dc.contributor.authorCilliers, P.en
dc.contributor.authorCorreia, E.en
dc.contributor.authorFreeman, M.en
dc.contributor.authorKauristie, K.en
dc.contributor.authorLiu, R.en
dc.contributor.authorLuntama, J.-P.en
dc.contributor.authorMitchell, C. N.en
dc.contributor.authorZherebtsov, G. A.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentSpace Plasma Environment and Radio Science Group, Department of Communication Systems, InfoLab 21, Lancaster University, Lancaster LA1 4WA, UKen
dc.contributor.departmentIstituto di Fisica dello Spazio Interplanetario I.N.A.F., Via del fosso del cavaliere 100, 00133 Rome, Italyen
dc.contributor.departmentHermanus Magnetic Observatory (HMO), P.O. Box 32, Hermanus, South Africaen
dc.contributor.departmentInstituto Nacional de Pesquisas Espaciais (INPE), São José dos Campos, Brazil and Centro de Rádio Astronomia e Astrofísica Mackenzie (CRAAM), Universidade Presbiteriana Mackenzie, Rua da Consolação 930, CEP: 01302-907 São Paulo, Brazilen
dc.contributor.departmentBritish Antarctic Survey, High Cross Madingley Road, Cambridge, UKen
dc.contributor.departmentFinnish Meteorological Institute, Erik Palménin aukio 1, Helsinki, Finlanden
dc.contributor.departmentPolar Research Institute of China, Shanghai 200136, Chinaen
dc.contributor.departmentFinnish Meteorological Institute, Erik Palménin aukio 1, Helsinki, Finlanden
dc.contributor.departmentDepartment of Electrical Engineering, University of Bath, Bath BA2 7AY, UKen
dc.contributor.departmentInstitute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Science, Irkutsk, Russiaen
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.deptSpace Plasma Environment and Radio Science Group, Department of Communication Systems, InfoLab 21, Lancaster University, Lancaster LA1 4WA, UK-
crisitem.author.deptIstituto di Fisica dello Spazio Interplanetario I.N.A.F., Via del fosso del cavaliere 100, 00133 Rome, Italy-
crisitem.author.deptSpace Science Directorate, South African National Space Agency, Hermanus, South Africa-
crisitem.author.deptBritish Antarctic Survey, High Cross Madingley Road, Cambridge, UK-
crisitem.author.deptFinnish Meteorological Institute, Helsinki, Finland-
crisitem.author.deptPolar Research Institute of China, Shanghai 200136, China-
crisitem.author.deptFinnish Meteorological Institute, Erik Palménin aukio 1, Helsinki, Finland-
crisitem.author.dept3Department of Electronic and Electrical Engineering, University of Bath-
crisitem.author.deptInstitute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Science, Irkutsk, Russia-
crisitem.author.orcid0000-0002-1806-9327-
crisitem.author.orcid0000-0003-3175-5134-
crisitem.author.orcid0000-0003-4778-3834-
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-
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