993 resultados para Talude continental
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Preservation of ultrahigh-pressure (UHP) minerals formed at depths of 90–125 km require unusual conditions. Our subduction model involves underflow of a salient (250 ± 150 km wide, 90–125 km long) of continental crust embedded in cold, largely oceanic crust-capped lithosphere; loss of leading portions of the high-density oceanic lithosphere by slab break-off, as increasing volumes of microcontinental material enter the subduction zone; buoyancy-driven return toward midcrustal levels of a thin (2–15 km thick), low-density slice; finally, uplift, backfolding, normal faulting, and exposure of the UHP terrane. Sustained over ≈20 million years, rapid (≈5 mm/year) exhumation of the thin-aspect ratio UHP sialic sheet caught between cooler hanging-wall plate and refrigerating, downgoing lithosphere allows withdrawal of heat along both its upper and lower surfaces. The intracratonal position of most UHP complexes reflects consumption of an intervening ocean basin and introduction of a sialic promontory into the subduction zone. UHP metamorphic terranes consist chiefly of transformed, yet relatively low-density continental crust compared with displaced mantle material—otherwise such complexes could not return to shallow depths. Relatively rare metabasaltic, metagabbroic, and metacherty lithologies retain traces of phases characteristic of UHP conditions because they are massive, virtually impervious to fluids, and nearly anhydrous. In contrast, H2O-rich quartzofeldspathic, gneissose/schistose, more permeable metasedimentary and metagranitic units have backreacted thoroughly, so coesite and other UHP silicates are exceedingly rare. Because of the initial presence of biogenic carbon, and its especially sluggish transformation rate, UHP paragneisses contain the most abundantly preserved crustal diamonds.
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Acknowledgements This research was supported by NERC grants (NE/L001764/1, NE/M010953/1). We are grateful to J. Still and A. Sandison for technical support and to the gypsum mines and C. Brolley for access and sampling. Critical comments from Cristiana Ciobanu, Eric Gloaguen and Georges Calas are gratefully acknowledged. The authors have no conflicts of interest to declare
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Inclui bibliografia.
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Inclui bibliografia.
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La presente Tesis Doctoral lleva por t tulo Geodin amica del margen continental de Galicia: Estructura profunda y morfotect onica. Este estudio se aborda a partir de la integraci on de un gran volumen de nuevos datos geof sicos (gravim etricos, batim etricos y s smica de re exi on multicanal 2D y de ultra-alta resoluci on), procedentes de los proyectos ZEEE, ERGAP y BURATO4242. La nueva informaci on ha aportado constricciones muy relevantes sobre el origen, la estructura profunda y la complejidad siogr a ca del margen, as como sobre la caracterizaci on de la variaci on lateral de la transici on oc eano-continente. El margen continental de Galicia se clasi ca como un margen de rift pobre en magma. Este tipo de m argenes tienen dos rasgos comunes, que son: 1) Los pares de m argenes conjugados son asim etricos, teniendo uno de ellos una zona m as ancha de corteza extremadamente adelgazada, subrayada por un re ector s smico subhorizontal; 2) Entre la corteza continental adelgazada y la corteza oce anica normal, hay una zona de basamento compuesto por manto serpentinizado. La estructura del margen continental gallego es extremadamente compleja, re ejando la superposici on de varias etapas sucesivas de rift, y una etapa compresiva posterior que da como resultado la inversi on parcial del margen. Adem as, la proximidad de un punto triple de dorsal produce un cambio de orientaci on de las estructuras principales. Este margen continental ha sido ampliamente estudiado desde la d ecada de los '70. Sin embargo, la mayor parte de los estudios se han centrado en la parte occidental, existiendo una importante carencia de informaci on en los ancos norte y noroeste. Este hecho, junto con su gran complejidad estructural, ha provocado que no exista un modelo geodin amico previo que integre todos los procesos observados. Algunos aspectos, como son la transici on entre el margen oeste (extensivo) y el margen norte (compresivo), y la forma en que se produce su inversi on tect onica, apenas han sido abordados con anterioridad por la comunidad científica...
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This capstone reviews uses of the Continental Divide National Scenic Trail. Policies governing use of the trail appear to be ambiguous, especially regarding mountain bicycles. Mountain biking has grown since the trail was created, but is not fully addressed in existing or proposed policy. 382 people on five segments of the trail in Colorado were interviewed for this capstone. Mountain bikes, hiking, and motorized recreation were observed uses. User conflict, overcrowding, degraded recreation experiences, or user displacement was not reported. User satisfaction was high and most would return. Interviewees requested increased public involvement and recognition of user needs in setting policy. Trail degradation occurs, but is unassociated with any particular use. Recommendations for trail improvement and maintenance are presented.
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High resolution seismic profiles of the Alicante continental shelf have been studied identifying a seismic prism which top at about -20 m below today sea-level. The prism is covered by recent sediments and can be interpreted as formed during a short interval of stand-by in the general transgression after the last glacial maximum. The -20 m level have been compared with the holocene Mediterranean sea-level-curve to propose an age of about 8 ka BP coinciding with the «8.2 ka cooling event» that was an abrupt, widespread climate instability. The prism top is deeper in the northern seismic profiles thus indicating a more subsidence that the southern coastal shelf where an erosion surface with rocky shoals configure the sea bottom.
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Con el objetivo de ampliar los conocimientos en relación a los cambios recientes del nivel en la plataforma continental de Alicante se ha procedido al estudio de diferentes perfiles sísmicos de alta resolución. En el presente trabajo se ha identificado un prisma sedimentario cuyo techo se ubica alrededor de los 60 metros por debajo del nivel del mar actual. Comparando los resultados con la curva de variaciones del nivel del mar de los últimos 20 milenios, se puede confirmar que éste se formó durante un periodo en que el nivel del mar permaneció relativamente constante o disminuyó levemente entre el final del Bølling Warming y tras el evento frío Younger Dryas. Un total de tres unidades sísmicas (1, 2 y 3 de base a techo) se pueden diferenciar en el prisma. La subunidad 1, depositada entre el final del Bølling Warming y antes del Younger Dryas, indicando una mayor ralentización de la tasa de ascenso del nivel del mar. La subunidad 2, formada durante el evento frío Younger Dryas, reflejando un episodio de detención del nivel del mar alrededor de los 60 metros, seguido de una caída relativa mismo. La subunidad 3, formada tras este periodo frío y que se caracteriza por un incremento de la tasa de ascenso del nivel del mar.