Towards the Opening of a Magnetic Observatory at Dome C (Antarctica)
The 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 lo...
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Format: | Conference Object |
Language: | English |
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2004
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Online Access: | http://hdl.handle.net/2122/4009 |
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ftingv:oai:www.earth-prints.org:2122/4009 |
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Earth-Prints (Istituto Nazionale di Geofisica e Vulcanologia) |
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ftingv |
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English |
topic |
Antarctica Magnetic observatory Dome C 04. Solid Earth::04.05. Geomagnetism::04.05.08. Instruments and techniques |
spellingShingle |
Antarctica Magnetic observatory Dome C 04. Solid Earth::04.05. Geomagnetism::04.05.08. Instruments and techniques Schott, J. J. Di Mauro, D. Pérès, A. Cafarella, L. Magno, L. Zirizzotti, A. Meloni, A. Towards the Opening of a Magnetic Observatory at Dome C (Antarctica) |
topic_facet |
Antarctica Magnetic observatory Dome C 04. Solid Earth::04.05. Geomagnetism::04.05.08. Instruments and techniques |
description |
The 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. Published Kakioka Magnetic Observatory / Tsukuba Center for Institutes, Japan 1.6. Osservazioni di geomagnetismo 3.4. Geomagnetismo open |
author2 |
Schott, J. J.; Ecole et Observatoire des Sciences de la Terre, 5 rue Descartes F-67084 Strasbourg France Di Mauro, D.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Pérès, A.; Ecole et Observatoire des Sciences de la Terre, 5 rue Descartes F-67084 Strasbourg France Cafarella, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Magno, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Zirizzotti, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Meloni, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Yumoto, K.; Kakioka Magnetic Observatory Ecole et Observatoire des Sciences de la Terre, 5 rue Descartes F-67084 Strasbourg France Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Yumoto, K. Kakioka Magnetic Observatory |
format |
Conference Object |
author |
Schott, J. J. Di Mauro, D. Pérès, A. Cafarella, L. Magno, L. Zirizzotti, A. Meloni, A. |
author_facet |
Schott, J. J. Di Mauro, D. Pérès, A. Cafarella, L. Magno, L. Zirizzotti, A. Meloni, A. |
author_sort |
Schott, J. J. |
title |
Towards the Opening of a Magnetic Observatory at Dome C (Antarctica) |
title_short |
Towards the Opening of a Magnetic Observatory at Dome C (Antarctica) |
title_full |
Towards the Opening of a Magnetic Observatory at Dome C (Antarctica) |
title_fullStr |
Towards the Opening of a Magnetic Observatory at Dome C (Antarctica) |
title_full_unstemmed |
Towards the Opening of a Magnetic Observatory at Dome C (Antarctica) |
title_sort |
towards the opening of a magnetic observatory at dome c (antarctica) |
publishDate |
2004 |
url |
http://hdl.handle.net/2122/4009 |
long_lat |
ENVELOPE(140.000,140.000,-66.667,-66.667) ENVELOPE(166.766,166.766,-77.849,-77.849) |
geographic |
Antarctic Dumont d’Urville Scott Base Terra Nova Bay |
geographic_facet |
Antarctic Dumont d’Urville Scott Base Terra Nova Bay |
genre |
Antarc* Antarctic Antarctica |
genre_facet |
Antarc* Antarctic Antarctica |
op_relation |
11th IAGA Workshop on Geomagnetic Observatory Instruments, Data Acquisition and Processing [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), 10.1029/2001GL013693 http://hdl.handle.net/2122/4009 |
op_rights |
open |
op_doi |
https://doi.org/10.1029/2002GL0144675. |
_version_ |
1766255664057810944 |
spelling |
ftingv:oai:www.earth-prints.org:2122/4009 2023-05-15T13:51:39+02:00 Towards the Opening of a Magnetic Observatory at Dome C (Antarctica) Schott, J. J. Di Mauro, D. Pérès, A. Cafarella, L. Magno, L. Zirizzotti, A. Meloni, A. Schott, J. J.; Ecole et Observatoire des Sciences de la Terre, 5 rue Descartes F-67084 Strasbourg France Di Mauro, D.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Pérès, A.; Ecole et Observatoire des Sciences de la Terre, 5 rue Descartes F-67084 Strasbourg France Cafarella, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Magno, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Zirizzotti, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Meloni, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Yumoto, K.; Kakioka Magnetic Observatory Ecole et Observatoire des Sciences de la Terre, 5 rue Descartes F-67084 Strasbourg France Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Yumoto, K. Kakioka Magnetic Observatory 2004-11-09 http://hdl.handle.net/2122/4009 en eng 11th IAGA Workshop on Geomagnetic Observatory Instruments, Data Acquisition and Processing [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), 10.1029/2001GL013693 http://hdl.handle.net/2122/4009 open Antarctica Magnetic observatory Dome C 04. Solid Earth::04.05. Geomagnetism::04.05.08. Instruments and techniques Conference paper 2004 ftingv https://doi.org/10.1029/2002GL0144675. 2022-07-29T06:04:57Z The 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. Published Kakioka Magnetic Observatory / Tsukuba Center for Institutes, Japan 1.6. Osservazioni di geomagnetismo 3.4. Geomagnetismo open Conference Object Antarc* Antarctic Antarctica Earth-Prints (Istituto Nazionale di Geofisica e Vulcanologia) Antarctic Dumont d’Urville ENVELOPE(140.000,140.000,-66.667,-66.667) Scott Base ENVELOPE(166.766,166.766,-77.849,-77.849) Terra Nova Bay |