Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/4009
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dc.contributor.authorallSchott, J. J.; Ecole et Observatoire des Sciences de la Terre, 5 rue Descartes F-67084 Strasbourg Franceen
dc.contributor.authorallDi Mauro, D.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallPérès, A.; Ecole et Observatoire des Sciences de la Terre, 5 rue Descartes F-67084 Strasbourg Franceen
dc.contributor.authorallCafarella, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallMagno, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallZirizzotti, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallMeloni, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.editorallYumoto, K.; Kakioka Magnetic Observatoryen
dc.date.accessioned2008-08-27T08:49:21Zen
dc.date.available2008-08-27T08:49:21Zen
dc.date.issued2004-11-09en
dc.identifier.urihttp://hdl.handle.net/2122/4009en
dc.description.abstractThe opening of a new magnetic observatory is one of the activities aimed at by the creation of a scientific base at DomeC, Antarctica (lat. 75° 06’S, long. 123° 21’E, elev. 3200m). There are many reasons supporting this objective: all Antarctic magnetic observatories providing absolute values are located along the shore and are therefore subject to coast effects and crustal field contamination. DomeC and Vostok will be so far the sole observatories free from these effects. On one hand, high latitude absolute observatories are very useful to global or regional modeling based upon satellite data, because, at high latitudes, only total field measurements can be used due to the strong influence of field aligned currents. On the other hand, the availability of magnetic data from the well distributed observatories of Terra Nova Bay (TNB), Scott Base (SBA), Dumont d’Urville (DRV), Casey (CSY) and Vostok (VOS) will provide strong support to auroral and polar cap ionosphere studies as well as asymmetry analyses between Northern and Southern hemispheres. This paper summarizes the results gathered during three summer campaigns, in 1999-2000, 2001 and 2003-2004.en
dc.language.isoEnglishen
dc.relation.ispartof11th IAGA Workshop on Geomagnetic Observatory Instruments, Data Acquisition and Processingen
dc.subjectAntarcticaen
dc.subjectMagnetic observatoryen
dc.subjectDome Cen
dc.titleTowards the Opening of a Magnetic Observatory at Dome C (Antarctica)en
dc.typeConference paperen
dc.description.statusPublisheden
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.08. Instruments and techniquesen
dc.description.ConferenceLocationKakioka Magnetic Observatory / Tsukuba Center for Institutes, Japanen
dc.relation.references[1] A. De Santis, J.M. Torta, L.R. Gaya-Piqué, (2002) The first Antarctic geomagnetic reference model (ARM), Geophys. Res. Lett., Vol. 29(8), 10.1029/2002GL0144675. [2] J.M. Torta, A. De Santis, M. Chiappini, R.R.B. von Frese (2002) A model of the secular change of the geomagnetic field for Antarctica, Tectonophysics, Vol. 347, pp 179-187. [3] S. Lepidi, L. Cafarella, P. Francia, A. Meloni, P. Palangio, J.J. Schott (2003) Low frequency geomagnetic field variations at Dome C (Antarctica), Annales Geophysicae, Vol. 21, pp 923-932. [4] L.R. Newitt, C.E. Barton, J. Bitterly (1996) Guide for magnetic repeat station surveys, International Association of Geomagnetism and Aeronomy. [5] J. Jankowski, C. Sucksdorff (1996) Guide for magnetic measurements and observatory practice, International Association of Geomagnetism and Aeronomy. [6] V.O. Papitashvili, N.E. Papitashvili, J.H. King (1997) Magnetospheric magnetic coordinate system for space physics data presentation and visualization, Adv. Space Res., Vol. 20, pp 1097-1100. [7] M. Mandea, B. Langlais (2002) Observatory crustal magnetic biases during MAGSAT and Orsted satellite missions, Geophysical Research Lett., Vol. 29(15), 10.1029/2001GL013693en
dc.description.obiettivoSpecifico1.6. Osservazioni di geomagnetismoen
dc.description.obiettivoSpecifico3.4. Geomagnetismoen
dc.description.fulltextopenen
dc.contributor.authorSchott, J. J.en
dc.contributor.authorDi Mauro, D.en
dc.contributor.authorPérès, A.en
dc.contributor.authorCafarella, L.en
dc.contributor.authorMagno, L.en
dc.contributor.authorZirizzotti, A.en
dc.contributor.authorMeloni, A.en
dc.contributor.departmentEcole et Observatoire des Sciences de la Terre, 5 rue Descartes F-67084 Strasbourg Franceen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentEcole et Observatoire des Sciences de la Terre, 5 rue Descartes F-67084 Strasbourg Franceen
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.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.editorYumoto, K.en
dc.contributor.editordepartmentKakioka Magnetic Observatoryen
item.openairetypeConference paper-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptEOST, IPG, Strasbourg, France-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptEcole et Observatoire des Sciences de la Terre, 5 rue Descartes F-67084 Strasbourg France-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, 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.orcid0000-0003-1757-9816-
crisitem.author.orcid0000-0003-2005-8923-
crisitem.author.orcid0000-0001-7586-9219-
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.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
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-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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