首页 | 本学科首页   官方微博 | 高级检索  
     检索      


Volcanism and mantle–crust evolution: The Etna case
Institution:1. Department of Geology and Planetary Science, University of Pittsburgh, Pittsburgh, PA, USA;2. Laboratoire Magmas et Volcans, Université Blaise Pascal, Clermont-Ferrand, France;3. Planetary Science Institute, 1700 E. Ft. Lowell Rd., Suite 106, Tucson, AZ, USA;1. GEOPS, Univ. Paris-Sud, CNRS, Université Paris-Saclay, 91405 Orsay, France;2. Laboratoire Magmas et Volcans, Université Clermont Auvergne, CNRS, IRD, OPGC, F-63000 Clermont-Ferrand, France;3. Instituto Geofísico, Escuela Politécnica Nacional, Ap. 17-01-2759, Quito, Ecuador;4. Université de Bretagne Occidentale, Domaines Océaniques IUEM, 29280 Plouzané, France;5. Facultad de Geología, Universidad Central del Ecuador, Casilla 872 A, Quito, Ecuador;1. Laboratoire GéoSciences, Institut de Physique du Globe de Paris (IPGP), Sorbonne Paris-Cité, UMR 7154 CNRS Sciences Réunion, Université de La Réunion, F-97715 Saint-Denis, France;2. Observatoire Volcanologique du Piton de la Fournaise (OVPF), Institut de Physique du Globe de Paris (IPGP), Sorbonne Paris-Cité, UMR 7154 CNRS, Université Paris Diderot, Bourg Murat, France;3. Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Palermo, V. Ugo La Malfa 153, – 90146 Palermo, Italy;4. Institut de Physique du Globe de Paris (IPGP), Sorbonne Paris-Cité, UMR 7154 CNRS, Université Paris Diderot, F-75005 Paris, France;5. Ecole et Observatoire des Sciences de la Terre (EOST), 5 rue René Descartes, F-67084 Strasbourg, France
Abstract:Mount Etna is located in a particular region of convergence of African and Eurasian plates where intense post-collisional tectonics caused considerable uplift. However we present arguments supporting the hypothesis that volcanism and associated seismic activity would result from a local mantle uprise leading to a “horst”, probably linked to a deep-rooted hot spot. It ensued deformation and fracturing of the overlying crust with emission of aphyric tholeiitic basalts directly from their mantle source, and subsequent development of a “deep reservoir” (or complex of intrusions) at the top of a mantle diapir near 30 km depth. This is advocated by the appearance of porphyritic alkaline lavas whose mineral equilibria and differentiation processes are consistent with an 8–10 kbar pressure, and by the development of central volcanoes. The horst itself appears to have begun in the SW sector of the present volcanic area. Its uplift was greater westward, as seen from the trend of the terraces along the Simeto river, and became later obvious toward the SE. These differential movements produced fractures and faults which are to day evident in the southern area of Mt Etna. The growth of the horst then proceeded in a NE direction, following the regional tectonic lines and with a greater intensity along the side facing SE, crossed by the regional NNW–SSE line (Aeolian–Maltese escarpment).The seismicity and ground deformation registered over the last twenty years support the proposed model. Earthquakes are unfrequent in the lower southern and western areas of the volcano, whereas they are numerous and stronger to the north-east, in the summit area above 1600 m a.s.l., and in the eastern sector along the NW–SE faults and fractures. Finally, a digital elevation model recently published reveals the existence of two tectonic domains. The first one is associated with the horst and contains prevalently NE–SW oriented faults, whereas the second is mainly linked to regional tectonics with NNW–SSE and NW–SE faults and fractures.
Keywords:
本文献已被 ScienceDirect 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号