Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/899
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dc.contributor.authorallKane, I.; Department of Geophysics, School of Geology, Aristotle University of Thessaloniki, Greeceen
dc.contributor.authorallStampolidis, A.; Department of Geophysics, School of Geology, Aristotle University of Thessaloniki, Greeceen
dc.contributor.authorallTsokas, N. G.; Department of Geophysics, School of Geology, Aristotle University of Thessaloniki, Greeceen
dc.contributor.authorallBushati, S.; Centre of Geophysical and Geochemical Exploration (CGGE), Tirana, Albaniaen
dc.contributor.authorallKondopoulou, D.; Department of Geophysics, School of Geology, Aristotle University of Thessaloniki, Greeceen
dc.contributor.authorallTsourlos, P.; Department of Geophysics, School of Geology, Aristotle University of Thessaloniki, Greeceen
dc.date.accessioned2006-02-22T13:38:26Zen
dc.date.available2006-02-22T13:38:26Zen
dc.date.issued2005en
dc.identifier.urihttp://hdl.handle.net/2122/899en
dc.description.abstractThe ground magnetic measurements in Albania were used for the compilation of the Total Magnetic Field (TMF) anomaly map of Albania. The magnetic data were processed and interpreted in order to study the structure of the ophiolitic belts of Albania. The ophiolites of Albania are placed at the Mirdita zone and are divided into two parallel alignments which are called the eastern and western ophiolitic belts. They are associated with strong potential field anomalies and their characteristics are considered crucial for a better understanding of the tectonic settings of Albania. The ground TMF data used in this study were acquired over various campaigns (1990-1994) and cover most of Albania's territory. The data were compiled to a map after reduction to the epoch 1990.4. The strongest magnetic anomalies in Albania appear along the known ophiolitic belts which trend NE-SW to the north and NW-SE to the south. Several processing steps were applied to the unified and gridded data in order to obtain information on the distribution of the magnetic sources. The magnetic sources were subsequently modeled using a 2.5D inversion technique. The magnetic properties of the ophiolites determined from laboratory measurements on rock samples, while their lateral extent was calculated from the processing of the magnetic data and used as constraints to the inversion procedure. The bottom of the ophiolitic belts is considered to be predominated by harzburgites. They exhibit lower magnetization than other rocks of the complex, i.e. gabbros, basalt. In fact gabbros are associated with the observed high frequency magnetic anomalies. The modeling results indicate that the thickness of the ophiolites is reduced from east to west. The eastern ophiolitic belt has a maximum thickness of approximately 12 km at its northern section (Kukesi and Lura massifs). The magnetic sources appear with relatively small thickness at the western ophiolitic belt. Boundaries of the eastern ophiolites are characterized by vertical contacts.en
dc.format.extent4030169 bytesen
dc.format.mimetypeapplication/pdfen
dc.language.isoEnglishen
dc.publisher.nameINGVen
dc.relation.ispartofAnnals of Geophysicsen
dc.relation.ispartofseries2/48 (2005)en
dc.subjectTotal Magnetic Fielden
dc.subjectophioltic belten
dc.subject2.5D modellingen
dc.titleThe structure of the ophiolitic beltin Albania inferred from geomagnetic anomaliesen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.subject.INGV04. Solid Earth::04.04. Geology::04.04.11. Instruments and techniquesen
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.04. Magnetic anomaliesen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorKane, I.en
dc.contributor.authorStampolidis, A.en
dc.contributor.authorTsokas, N. G.en
dc.contributor.authorBushati, S.en
dc.contributor.authorKondopoulou, D.en
dc.contributor.authorTsourlos, P.en
dc.contributor.departmentDepartment of Geophysics, School of Geology, Aristotle University of Thessaloniki, Greeceen
dc.contributor.departmentDepartment of Geophysics, School of Geology, Aristotle University of Thessaloniki, Greeceen
dc.contributor.departmentDepartment of Geophysics, School of Geology, Aristotle University of Thessaloniki, Greeceen
dc.contributor.departmentCentre of Geophysical and Geochemical Exploration (CGGE), Tirana, Albaniaen
dc.contributor.departmentDepartment of Geophysics, School of Geology, Aristotle University of Thessaloniki, Greeceen
dc.contributor.departmentDepartment of Geophysics, School of Geology, Aristotle University of Thessaloniki, Greeceen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptDepartment of Geophysics, School of Geology, Aristotle University of Thessaloniki, Greece-
crisitem.author.deptDepartment of Geophysics, School of Geology, Aristotle University of Thessaloniki, Greece-
crisitem.author.deptGeophysical Laboratory of Thessaloniki, Greece-
crisitem.author.deptCentre of Geophysical and Geochemical Exploration (CGGE), Tirana, Albania-
crisitem.author.deptDepartment of Geology, Aristotle University of Thessaloniki, Greece-
crisitem.author.deptDepartment of Geophysics, School of Geology, Aristotle University of Thessaloniki, Greece-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
Appears in Collections:Annals of Geophysics
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