A model of the secular change of the geomagnetic field for Antarctica
An improved model of geomagnetic secular change for the Antarctic was developed using observatory annual mean values measured in Antarctica during the last 40 years. Spherical cap harmonic analysis (SCHA) with a power series time dependence was used to model spatial and temporal variations of main f...
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Format: | Article in Journal/Newspaper |
Language: | English |
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Elsevier
2002
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Online Access: | http://hdl.handle.net/2122/3899 |
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ftingv:oai:www.earth-prints.org:2122/3899 |
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openpolar |
institution |
Open Polar |
collection |
Earth-Prints (Istituto Nazionale di Geofisica e Vulcanologia) |
op_collection_id |
ftingv |
language |
English |
topic |
Antarctica Spherical cap harmonic analysis Magnetic surveys Magnetic mapping Geomagnetic secular variation 04. Solid Earth::04.05. Geomagnetism::04.05.03. Global and regional models 04. Solid Earth::04.05. Geomagnetism::04.05.05. Main geomagnetic field 04. Solid Earth::04.07. Tectonophysics::04.07.99. General or miscellaneous |
spellingShingle |
Antarctica Spherical cap harmonic analysis Magnetic surveys Magnetic mapping Geomagnetic secular variation 04. Solid Earth::04.05. Geomagnetism::04.05.03. Global and regional models 04. Solid Earth::04.05. Geomagnetism::04.05.05. Main geomagnetic field 04. Solid Earth::04.07. Tectonophysics::04.07.99. General or miscellaneous Torta, J. M. De Santis, A. Chiappini, M. von Frese, R. R. B. A model of the secular change of the geomagnetic field for Antarctica |
topic_facet |
Antarctica Spherical cap harmonic analysis Magnetic surveys Magnetic mapping Geomagnetic secular variation 04. Solid Earth::04.05. Geomagnetism::04.05.03. Global and regional models 04. Solid Earth::04.05. Geomagnetism::04.05.05. Main geomagnetic field 04. Solid Earth::04.07. Tectonophysics::04.07.99. General or miscellaneous |
description |
An improved model of geomagnetic secular change for the Antarctic was developed using observatory annual mean values measured in Antarctica during the last 40 years. Spherical cap harmonic analysis (SCHA) with a power series time dependence was used to model spatial and temporal variations of main field differences at spatial wavelengths from 3000 to 13,000 km. The model was designed to facilitate merging satellite, airborne, marine and terrestrial magnetic data sets recorded at very different epochs in the Antarctic where significant annual geomagnetic changes have occurred. It improves the fit to observatory data by up to about 50% relative to the International Geomagnetic Reference Field. Published 179-187 JCR Journal reserved |
author2 |
Torta, J. M.; Observatori de l’Ebre, CSIC, 43520 Roquetes, Tarragona, Spain De Santis, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Chiappini, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia von Frese, R. R. B.; Department of Geological Sciences, and Byrd Polar Research Center, The Ohio State University, Columbus, OH 43210, USA Observatori de l’Ebre, CSIC, 43520 Roquetes, Tarragona, Spain Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Department of Geological Sciences, and Byrd Polar Research Center, The Ohio State University, Columbus, OH 43210, USA |
format |
Article in Journal/Newspaper |
author |
Torta, J. M. De Santis, A. Chiappini, M. von Frese, R. R. B. |
author_facet |
Torta, J. M. De Santis, A. Chiappini, M. von Frese, R. R. B. |
author_sort |
Torta, J. M. |
title |
A model of the secular change of the geomagnetic field for Antarctica |
title_short |
A model of the secular change of the geomagnetic field for Antarctica |
title_full |
A model of the secular change of the geomagnetic field for Antarctica |
title_fullStr |
A model of the secular change of the geomagnetic field for Antarctica |
title_full_unstemmed |
A model of the secular change of the geomagnetic field for Antarctica |
title_sort |
model of the secular change of the geomagnetic field for antarctica |
publisher |
Elsevier |
publishDate |
2002 |
url |
http://hdl.handle.net/2122/3899 |
geographic |
Antarctic The Antarctic |
geographic_facet |
Antarctic The Antarctic |
genre |
Antarc* Antarctic Antarctica |
genre_facet |
Antarc* Antarctic Antarctica |
op_relation |
Tectonophysics / 347 (2002) Alsdorf, D.E., von Frese, R.R.B., Arkani-Hamed, J., Noltimier, H.C., 1994. Separation of lithospheric, external, and core components of the south polar geomagnetic field at satellite altitudes. J. Geophys. Res. 99, 4655–4668. Barton, C.E., 1997. International geomagnetic reference field: the seventh generation. J. Geomagn. Geoelectr. 49, 123–148. Chiappini, M., von Frese, R.R.B., Ferris, J., 1998. Effort to develop magnetic anomaly database aids Antarctic research. EOS Trans. Am. Geophys. Union 79, 290. De Santis, A., Chiappini, M., Torta, J.M., von Frese, R.R.B., 1999. Development of an improved geomagnetic reference field of Antarctica. Ann. Geofis. 42, 265– 270. Haines, G.V., 1993. Modelling geomagnetic secular variation by main-field differences. Geophys. J. Int. 114, 490– 500. Haines, G.V., Newitt, L.R., 1986. Canadian geomagnetic reference field 1985. J. Geomagn. Geoelectr. 38, 895– 921. Haines, G.V., Newitt, L.R., 1997. The Canadian geomagnetic reference field 1995. J. Geomagn. Geoelectr. 49, 317– 336. Haines, G.V., Torta, J.M., 1994. Determination of equivalent current sources from spherical cap harmonic models of geomagnetic field variations. Geophys. J. Int. 118, 499–514. McLean, S.J., Meyers, K.D., Morris, L.D., Davis, W.M., 1995. A report on geomagnetic observatories. World Data Center-A for Solid Earth Geophysics, Rep. SE-53. Boulder, CO, 110 pp. Nevanlinna, H., Ryno¨ , J., 1991. Spherical cap harmonic model of the Scandinavian geomagnetic field for 1990. HHI-Rep. 22, 106. Nevanlinna, H., Ryno¨ , J., Haines, G.V., Borg, K., 1988. Spherical cap harmonic analysis applied to the Scandinavian geomagnetic field 1985.0. Deut. Hydro. Zeits. 41, 177– 186. Newitt, L.R., Haines, G.V., 1989. A Canadian geomagnetic reference field for epoch 1987.5. J. Geomagn. Geoelectr. 41, 249– 260. Newitt, L.R., Haines, G.V., 1991. The Canadian geomagnetic reference field 1990. Current Research, Part EGeological Survey of Canada, Paper 91-1E, 275– 281. Torta, J.M., Garcı´a, A., De Santis, A., 1993. A geomagnetic reference field for Spain at 1990. J. Geomagn. Geoelectr. 45, 573– 588. http://hdl.handle.net/2122/3899 |
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restricted |
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1766255658982703104 |
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ftingv:oai:www.earth-prints.org:2122/3899 2023-05-15T13:51:39+02:00 A model of the secular change of the geomagnetic field for Antarctica Torta, J. M. De Santis, A. Chiappini, M. von Frese, R. R. B. Torta, J. M.; Observatori de l’Ebre, CSIC, 43520 Roquetes, Tarragona, Spain De Santis, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Chiappini, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia von Frese, R. R. B.; Department of Geological Sciences, and Byrd Polar Research Center, The Ohio State University, Columbus, OH 43210, USA Observatori de l’Ebre, CSIC, 43520 Roquetes, Tarragona, Spain Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Department of Geological Sciences, and Byrd Polar Research Center, The Ohio State University, Columbus, OH 43210, USA 2002 http://hdl.handle.net/2122/3899 en eng Elsevier Tectonophysics / 347 (2002) Alsdorf, D.E., von Frese, R.R.B., Arkani-Hamed, J., Noltimier, H.C., 1994. Separation of lithospheric, external, and core components of the south polar geomagnetic field at satellite altitudes. J. Geophys. Res. 99, 4655–4668. Barton, C.E., 1997. International geomagnetic reference field: the seventh generation. J. Geomagn. Geoelectr. 49, 123–148. Chiappini, M., von Frese, R.R.B., Ferris, J., 1998. Effort to develop magnetic anomaly database aids Antarctic research. EOS Trans. Am. Geophys. Union 79, 290. De Santis, A., Chiappini, M., Torta, J.M., von Frese, R.R.B., 1999. Development of an improved geomagnetic reference field of Antarctica. Ann. Geofis. 42, 265– 270. Haines, G.V., 1993. Modelling geomagnetic secular variation by main-field differences. Geophys. J. Int. 114, 490– 500. Haines, G.V., Newitt, L.R., 1986. Canadian geomagnetic reference field 1985. J. Geomagn. Geoelectr. 38, 895– 921. Haines, G.V., Newitt, L.R., 1997. The Canadian geomagnetic reference field 1995. J. Geomagn. Geoelectr. 49, 317– 336. Haines, G.V., Torta, J.M., 1994. Determination of equivalent current sources from spherical cap harmonic models of geomagnetic field variations. Geophys. J. Int. 118, 499–514. McLean, S.J., Meyers, K.D., Morris, L.D., Davis, W.M., 1995. A report on geomagnetic observatories. World Data Center-A for Solid Earth Geophysics, Rep. SE-53. Boulder, CO, 110 pp. Nevanlinna, H., Ryno¨ , J., 1991. Spherical cap harmonic model of the Scandinavian geomagnetic field for 1990. HHI-Rep. 22, 106. Nevanlinna, H., Ryno¨ , J., Haines, G.V., Borg, K., 1988. Spherical cap harmonic analysis applied to the Scandinavian geomagnetic field 1985.0. Deut. Hydro. Zeits. 41, 177– 186. Newitt, L.R., Haines, G.V., 1989. A Canadian geomagnetic reference field for epoch 1987.5. J. Geomagn. Geoelectr. 41, 249– 260. Newitt, L.R., Haines, G.V., 1991. The Canadian geomagnetic reference field 1990. Current Research, Part EGeological Survey of Canada, Paper 91-1E, 275– 281. Torta, J.M., Garcı´a, A., De Santis, A., 1993. A geomagnetic reference field for Spain at 1990. J. Geomagn. Geoelectr. 45, 573– 588. http://hdl.handle.net/2122/3899 restricted Antarctica Spherical cap harmonic analysis Magnetic surveys Magnetic mapping Geomagnetic secular variation 04. Solid Earth::04.05. Geomagnetism::04.05.03. Global and regional models 04. Solid Earth::04.05. Geomagnetism::04.05.05. Main geomagnetic field 04. Solid Earth::04.07. Tectonophysics::04.07.99. General or miscellaneous article 2002 ftingv 2022-07-29T06:04:55Z An improved model of geomagnetic secular change for the Antarctic was developed using observatory annual mean values measured in Antarctica during the last 40 years. Spherical cap harmonic analysis (SCHA) with a power series time dependence was used to model spatial and temporal variations of main field differences at spatial wavelengths from 3000 to 13,000 km. The model was designed to facilitate merging satellite, airborne, marine and terrestrial magnetic data sets recorded at very different epochs in the Antarctic where significant annual geomagnetic changes have occurred. It improves the fit to observatory data by up to about 50% relative to the International Geomagnetic Reference Field. Published 179-187 JCR Journal reserved Article in Journal/Newspaper Antarc* Antarctic Antarctica Earth-Prints (Istituto Nazionale di Geofisica e Vulcanologia) Antarctic The Antarctic |