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dc.contributor.authorAl-Damegh, Khaled
dc.date.accessioned2007-01-26T16:02:32Z
dc.date.available2007-01-26T16:02:32Z
dc.date.issued2004-05
dc.identifier.citationPh. D. Dissertation, Cornell University, May 2004en_US
dc.identifier.urihttps://hdl.handle.net/1813/5263
dc.descriptionCopyright 2003, Khaled Al-Damegh See also: http://atlas.geo.cornell.edu/SaudiArabia/publications/Al-Damegh%20Dissertation%202004.htmen_US
dc.description.abstractContinuous waveform recording from a newly established broadband seismic network in Saudi Arabia, in addition to data produced by other stations in the region, were used to map regional seismic wave propagation (Lg and Sn) and Pn attenuation. Moreover, crustal thickness in the Arabian plate was also estimated based on receiver function analysis. Zone blockage and inefficient Sn propagation is observed along and to the east of the Dead Sea fault system and in the northern portion of the Arabian plate (south of the Bitlis suture)., We observed Sn blockage across some segments of the Red Sea. These regions of high Sn attenuation have anomalously hot and possibly thin lithospheric mantle (i.e., mantle lid). Consistent with our Sn attenuation findings, we also observed low Qpn along the western portion of the Arabian plate and along the Dead Sea fault system. Our results imply the presence of a major anomalously hot and thinned lithosphere in these regions that may be caused by the extensive upper mantle anomaly that appears to span most of east Africa and western Arabia. These mapped zones of high attenuation closely coincide with an extensive Neogene and Quaternary volcanic activity. We found that the average crustal thickness of the Arabian shield is 39 km. The crust thins to about 23 km along the Red Sea coast and to about 25 km along the Gulf of Aqaba. We observed a dramatic change in crustal thickness between the topographic escarpment of the Arabian shield and the shorelines of the Red Sea. We compared our results in the Arabian shield to nine other Proterozoic and Archean shields that include reasonably well-determined Moho depths. We do not observe a significant difference between Proterozoic and Archean crustal thickness. Our observations show that the transition from oceanic to continental crust along the Red Sea margin occurs over a relatively short distance compared to a typical west Atlantic continental margin. We argue that the anomalous nature of the Red Sea margin may be one of the consequences of the presence of a mega plume that extends from the core-mantle boundary into the upper mantle beneath east Africa, the Red Sea, and the western portion of the Arabian plate. In addition, the site where the sea-floor spreading of the Red Sea occurred was a Proterozoic suture and a zone of weakness. These observations combined may explain the relatively abrupt breakup of the Arabian plate and the anomalous nature of the Red Sea margin.en_US
dc.format.extent6319691 bytes
dc.format.mimetypeapplication/pdf
dc.language.isoenen_US
dc.subjectArabian plateen_US
dc.subjectReceiver functionsen_US
dc.subjectSeismologyen_US
dc.subjectSeismic attenuationen_US
dc.subjectCrustal structureen_US
dc.subjectRed Seaen_US
dc.subjectSn wavesen_US
dc.subjectLg wavesen_US
dc.titleLithospheric Structure of the Arabian Plate and Surrounding Regionsen_US
dc.typedissertation or thesisen_US


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