Two geomagnetic regional models for Albania and south-east Italy from 1990 to 2010 with prediction to 2012 and comparison with IGRF-11
Here we present a revised geomagnetic reference model for the region comprising Albanian territory, southeast part of Italian Peninsula and Ionian Sea from 1990 to 2010 with prediction to 2012. This study is based on the datasets of magnetic measurements taken during different campaigns in Albania a...
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Veröffentlicht in: | Earth, planets, and space planets, and space, 2010-10, Vol.62 (10), p.833-841 |
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creator | Qamili, Enkelejda De Santis, Angelo Cianchini, Gianfranco Duka, Bejo Gaya-Piqué, Luis R. Dominici, Guido Hyka, Niko |
description | Here we present a revised geomagnetic reference model for the region comprising Albanian territory, southeast part of Italian Peninsula and Ionian Sea from 1990 to 2010 with prediction to 2012. This study is based on the datasets of magnetic measurements taken during different campaigns in Albania and Italy in the time of concern, together with a total intensity data set from the ∅rsted and CHAMP satellite missions. The model is designed to represent the Cartesian components,
X, Y, Z
and the total intensity
F
of the main geomagnetic field (and its secular variation SV) for the period of interest. To develop the model, we applied a Spherical Cap Harmonic Analysis (SCHA) of the geomagnetic potential over a 16° cap with most of the observations concentrated in the central 4° half-angle. The use of a larger cap than that containing the data was made to reduce the typical problems in SV modelling over small regions. Also a new technique, called “Radially Simplified Spherical Cap Harmonic Analysis” (RS-SCHA), was developed to improve the model especially in the radial variation of the geomagnetic field components. Both these models provide an optimal representation of the geomagnetic field in the considered region compared with the International Geomagnetic Reference Field model (IGRF-11) and can be used as reference models to reduce magnetic surveys undertaken in the area during the time of validity of the model, or to extrapolate the field till 2012. |
doi_str_mv | 10.5047/eps.2010.07.011 |
format | Article |
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X, Y, Z
and the total intensity
F
of the main geomagnetic field (and its secular variation SV) for the period of interest. To develop the model, we applied a Spherical Cap Harmonic Analysis (SCHA) of the geomagnetic potential over a 16° cap with most of the observations concentrated in the central 4° half-angle. The use of a larger cap than that containing the data was made to reduce the typical problems in SV modelling over small regions. Also a new technique, called “Radially Simplified Spherical Cap Harmonic Analysis” (RS-SCHA), was developed to improve the model especially in the radial variation of the geomagnetic field components. Both these models provide an optimal representation of the geomagnetic field in the considered region compared with the International Geomagnetic Reference Field model (IGRF-11) and can be used as reference models to reduce magnetic surveys undertaken in the area during the time of validity of the model, or to extrapolate the field till 2012.</description><identifier>ISSN: 1343-8832</identifier><identifier>EISSN: 1880-5981</identifier><identifier>DOI: 10.5047/eps.2010.07.011</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Earth and Environmental Science ; Earth Sciences ; Geology ; Geophysics/Geodesy</subject><ispartof>Earth, planets, and space, 2010-10, Vol.62 (10), p.833-841</ispartof><rights>The Society of Geomagnetism and Earth, Planetary and Space Sciences, The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences; TERRAPUB 2010</rights><rights>The Society of Geomagnetism and Earth, Planetary and Space Sciences, The Seismological Society of Japan 2010</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a428t-eb9a3cf6f0dcb1428ce002119213f00ab6214bcb3ec41a46961ec78f6149ec393</citedby><cites>FETCH-LOGICAL-a428t-eb9a3cf6f0dcb1428ce002119213f00ab6214bcb3ec41a46961ec78f6149ec393</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.5047/eps.2010.07.011$$EPDF$$P50$$Gspringer$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://doi.org/10.5047/eps.2010.07.011$$EHTML$$P50$$Gspringer$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,27923,27924,41119,41487,42188,42556,51318,51575</link.rule.ids></links><search><creatorcontrib>Qamili, Enkelejda</creatorcontrib><creatorcontrib>De Santis, Angelo</creatorcontrib><creatorcontrib>Cianchini, Gianfranco</creatorcontrib><creatorcontrib>Duka, Bejo</creatorcontrib><creatorcontrib>Gaya-Piqué, Luis R.</creatorcontrib><creatorcontrib>Dominici, Guido</creatorcontrib><creatorcontrib>Hyka, Niko</creatorcontrib><title>Two geomagnetic regional models for Albania and south-east Italy from 1990 to 2010 with prediction to 2012 and comparison with IGRF-11</title><title>Earth, planets, and space</title><addtitle>Earth Planet Sp</addtitle><description>Here we present a revised geomagnetic reference model for the region comprising Albanian territory, southeast part of Italian Peninsula and Ionian Sea from 1990 to 2010 with prediction to 2012. This study is based on the datasets of magnetic measurements taken during different campaigns in Albania and Italy in the time of concern, together with a total intensity data set from the ∅rsted and CHAMP satellite missions. The model is designed to represent the Cartesian components,
X, Y, Z
and the total intensity
F
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X, Y, Z
and the total intensity
F
of the main geomagnetic field (and its secular variation SV) for the period of interest. To develop the model, we applied a Spherical Cap Harmonic Analysis (SCHA) of the geomagnetic potential over a 16° cap with most of the observations concentrated in the central 4° half-angle. The use of a larger cap than that containing the data was made to reduce the typical problems in SV modelling over small regions. Also a new technique, called “Radially Simplified Spherical Cap Harmonic Analysis” (RS-SCHA), was developed to improve the model especially in the radial variation of the geomagnetic field components. Both these models provide an optimal representation of the geomagnetic field in the considered region compared with the International Geomagnetic Reference Field model (IGRF-11) and can be used as reference models to reduce magnetic surveys undertaken in the area during the time of validity of the model, or to extrapolate the field till 2012.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.5047/eps.2010.07.011</doi><tpages>9</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Earth and Environmental Science Earth Sciences Geology Geophysics/Geodesy |
title | Two geomagnetic regional models for Albania and south-east Italy from 1990 to 2010 with prediction to 2012 and comparison with IGRF-11 |
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