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Rupture area analysis of the Ecuador (Musine) Mw = 7.8 thrust earthquake on April 16, 2016, using GOCE derived gradients

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Geodesy and Geodynamics 2017年第1期8卷 49-58页

作者： Orlando Alvarez Andres Folguera Mario Gimenez lnstituto geofisico y sismologico lng Volponi Universidad Nacional de San Juan Argentina Consejo Nacional de Investigaciones Cientificas y Tecnicas Argentina indean-instituto de Estudios Andinos "Don Pablo Groeber" Departamento de Cs. Geologicas FCEN Universidad de Buenos Aires Argentina

The Ecuador Mw - 7.8 earthquake on April 16, 2016, ruptured a nearly 200 km long zone along the plate interface between Nazca and South American plates which is coincident with a seismic gap since 1942, when a Mw - 7.8 earthquake happened. This earthquake occurred at a margin characterized by moderately big to giant earthquakes such as the 1906 （Mw 8.8）. A heavily sedimented trench explains the abnormal lengths of the rupture zones in this system as inhibits the role of natural barriers on the propagation of rupture zones. High amount of sediment thickness is associated with tropical climates, high erosion rates and eastward Pacific dominant winds that provoke orographic rainfalls over the Pacific slope of the Ecuatorian Andes. Offshore sediment dispersion off the oceanic trench is controlled by a close arrangement of two aseismic ridges that hit the Costa Rico and South Ecuador margin respectively and a mid ocean ridge that separates the Cocos and Nazca plate trapping sediments. Gravity field and Ocean Circulation Explorer （GOCE） satellite data are used in this work to test the possible relationship between gravity signal and earthquake rupture structure as well as registered aftershock seismic activity. Reduced vertical gravity gradient shows a good correlation with rupture structure for certain degrees of the harmonic expansion and related depth of the causative mass; indicating, such as in other analyzed cases along the subduction margin, that fore-arc structure derived from density heterogeneities explains at a certain extent propagation of the rupture zones. In this analysis the rupture zone of the April 2016 Ecuador earthquake developed through a relatively low density zone of the fore-arc sliver. Finally, aftershock sequence nucleated around the area of maximum slips in the rupture zone, suggesting that heterogeneous density structure of the fore-arc determined from gravity data could be used in forecasting potential damaged zones associated with big rupture

关键词： Gravity field and Ocean Circulation Explorer(GOCE)Vertical gravity gradientEcuador earthquakeTrench sedimentsRupture zone

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Payenia Quaternary flood basalts(southern Mendoza, Argentina)：Geophysical constraints on their volume

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Geoscience Frontiers 2016年第5期7卷 775-782页

作者： Mauro G.Spagnuolo Darío L.Orts Mario Gimenez Andres Folguera Victor A.Ramos Instituto de Estudios Andinos Don Pablo Groeber (I DEAN) UBA-CONICET Argentina Instituto de Investigacion en Paleobiologia y Geologia Universidad Nacional de Rio Negro - CONICET Argentina Instituto geofisico y sismologico Ing. Volponi Universidad Nacional de San Juan. CONICET Argentina

The Quaternary volcanic province of Payenia is located in southern Mendoza and northern Neuquén provinces of Argentina and is characterized by a dominant basaltic composition. The volcanic province covers an area larger than 40,000 km2 and its origin and evolution has been the center of several *** this study we analyzed gravity data together with more accurate volcanic volumes calculations in order to investigate the subsurface structure of the Payenia volcanic province. The volume of material was calculated using digital elevation models and geographic information system（GIS） techniques to estimate the volume of material erupted and then, with those values, make an estimation of the intrusive material that could be located within the crust. The results of the calculations were compared with different 2D-sections constructed to model the gravity data and compare with the observed satellite gravity. After evaluating different models which have been generated to match both： the observed gravity data and the subsurface material calculated, we discuss those that best fit with observation. The results clearly indicate that the lithosphere is attenuated below the region.

关键词： Payenia Gravimetric model Plume Uplift Andes

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The subduction of the Copiapó aseismic ridge,is the causing of the formation of metallic minerals deposits in north of Chile and Argentina?

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Geodesy and Geodynamics 2019年第6期10卷 471-476页

作者： Mario Gimenez Gemma Acosta Orlando Alvarez Agustina Pesce Federico Lince Kinger Andres Folguera Instituto geofisico sismologico Volponi FCEFNUniversidad Nacional de San JuanCONICETRuta 12 Marguesado(Jardin de Los Poetas)RiνadaviaSanJuanArgentina IDEAN-CONICET Universidad de Buenos Aires Argentina

The results obtained in this work evince that the metallic mineral deposits located in the northern region of the Chilean-Pampean flat slab(in northern Chile and north-western Argentina),at approximately 27°30’S,would be related to the subduction of the Copiapo aseismic *** analysis of the gravity anomalies and vertical gravity gradient allows inferring a deflection and truncation of the main trend of the Andean structures at the extrapolated zone of the Copiapo ridge beneath South ***,the general NNE-trend of the Andean structures are rotated locally to an ENE-strike within the area of the Ojos del Salado-San Buena Ventura *** explain that this anomalous behavior of the gravity derived anomalies is related to the deformational effects imprinted by the ridge *** with a low subduction angle(y dehydration of the subducting *** addition,a higher degree of mantle melting could be produced by a thicker oceanic ***,we interpret that the processes associated to the subduction of the Copiapo aseismic ridge(emplaced on a thickened oceanic crust due to a local compensation of the seamounts)are the cause of formation and emplacement of big metallic mineral deposits in this region of Chile and Argentina.

关键词： Aseismic ridge Satellite gravity Ojos del Salado-San Buena Ventura lineament Metallic mineral deposits

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