298 resultados para Dunes côtières
Resumo:
Relict dune fields that are found as far south as 14° N in the modern-day African Sahel are testament to equatorward expansions of the Sahara desert during the Late Pleistocene. However, the discontinuous nature of dune records means that abrupt millennial-timescale climate events are not always resolved. High-resolution marine core studies have identified Heinrich stadials as the dustiest periods of the last glacial in West Africa although the spatial evolution of dust export on millennial timescales has so far not been investigated. We use the major-element composition of four high-resolution marine sediment cores to reconstruct the spatial extent of Saharan-dust versus river-sediment input to the continental margin from West Africa over the last 60 ka. This allows us to map the position of the sediment composition corresponding to the Sahara-Sahel boundary. Our records indicate that the Sahara-Sahel boundary reached its most southerly position (13° N) during Heinrich stadials and hence suggest that these were the periods when the sand dunes formed at 14° N on the continent. Heinrich stadials are associated with cold North Atlantic sea surface temperatures which appear to have triggered abrupt increases of aridity and wind strength in the Sahel. Our study illustrates the influence of the Atlantic meridional overturning circulation on the position of the Sahara-Sahel boundary and on global atmospheric dust loading.
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The Palestine Exploration Fund (PEF) Survey of Western Palestine (1871-1877) is highly praised for its accuracy and completeness; the first systematic analysis of its planimetric accuracy was published by Levin (2006). To study the potential of these 1:63,360 maps for a quantitative analysis of land cover changes over a period of time, Levin has compared them to 20th century topographic maps. The map registration error of the PEF maps was 74.4 m using 123 control points of trigonometrical stations and a 1st order polynomial. The median RMSE of all control and test points (n = 1104) was 153.6 m. Following the georeferencing of each of the 26 sheets of the PEF maps of the Survey of Western Palestine, a mosaicked file has been created. Care should be taken when analysing historical maps, as it cannot be assumed that their accuracy is consistent at different parts or for different features depicted on them.
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Flow transverse bedforms (ripples and dunes) are ubiquitous in rivers and coastal seas. Local hydrodynamics and transport conditions depend on the size and geometry of these bedforms, as they constitute roughness elements at the bed. Bedform influence on flow energy must be considered for the understanding of flow dynamics, and in the development and application of numerical models. Common estimations or predictors of form roughness (friction factors) are based mostly on data of steep bedforms (with angle-of-repose lee slopes), and described by highly simplified bedform dimensions (heights and lengths). However, natural bedforms often are not steep, and differ in form and hydraulic effect relative to idealised bedforms. Based on systematic numerical model experiments, this study shows how the hydraulic effect of bedforms depends on the flow structure behind bedforms, which is determined by the bedform lee side angle, aspect ratio and relative height. Simulations reveal that flow separation behind bedform crests and, thus, a hydraulic effect is induced at lee side angles steeper than 11 to 18° depending on relative height, and that a fully developed flow separation zone exists only over bedforms with a lee side angle steeper than 24°. Furthermore, the hydraulic effect of bedforms with varying lee side angle is evaluated and a reduction function to common friction factors is proposed. A function is also developed for the Nikuradse roughness (k s), and a new equation is proposed which directly relates k s to bedform relative height, aspect ratio and lee side angle.
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Continuous Wavelet Transform was applied to bed elevation profiles (BEP) and used in the study in order to recognise the spatial distribution of bedforms and discriminate between their hierarchical scales. In particular, the spatial distribution of the hierarchical scales is highlighted by averaging wavelet power spectra over different bands, and displayed as the wavelet variance of the BEP (see map). Four dune classes were defined, following Ashley (1990): small dunes (1-5 m), medium dunes (5-10 m), large dunes (10-100 m), and very large dunes (>100 m).
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Tel-Aviv: años 30. La situación en Europa comienza a ser insostenible y muchos arquitectos judíos huyen a Palestina donde importan y adecuan los modelos modernos, aprendidos en el viejo continente, de hacer arquitectura. La ciudad, nacida en 1909 sobre las dunas a las afueras de Jaffa, crece vertiginosamente y se convierte en un laboratorio moderno sobre el tapiz urbano planeado por Patrick Geddes en 1925. En este trabajo, los múltiples factores arquitectónicos, sociales, culturales e históricos que llevaron a Tel Aviv a convertirse en la ciudad del mundo con más concentración de arquitectura moderna se entrelazan entre sí para perfi lar una imagen global a través de recorridos no lineales de lo acontecido en Tel Aviv durante los años 30. PALABRAS CLAVE: Tel Aviv, Movimiento Moderno Tel-Aviv. 30s The situation in Europe is becoming unsustainable and many Jewish architects fl ee to Palestine where they import the modernist way of thinking and doing architecture from the old continent. The city, born in 1909 on the dunes outside Jaffa, grows rapidly and becomes a modern laboratory over the urban tapestry planned by Patrick Geddes in 1925. In this paper, multiple architectural, social, cultural and historical factors that led Tel Aviv to become the city of the world with the highest concentration of modern architecture overlap over each other to shape a global image through non-linear paths of what happened in Tel Aviv during the 30’s.
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Context. Debris discs are a consequence of the planet formation process and constitute the fingerprints of planetesimal systems. Their solar system counterparts are the asteroid and Edgeworth-Kuiper belts. Aims. The DUNES survey aims at detecting extra-solar analogues to the Edgeworth-Kuiper belt around solar-type stars, putting in this way the solar system into context. The survey allows us to address some questions related to the prevalence and properties of planetesimal systems. Methods. We used Herschel/PACS to observe a sample of nearby FGK stars. Data at 100 and 160 μm were obtained, complemented in some cases with observations at 70 μm, and at 250, 350 and 500 μm using SPIRE. The observing strategy was to integrate as deep as possible at 100 μm to detect the stellar photosphere. Results. Debris discs have been detected at a fractional luminosity level down to several times that of the Edgeworth-Kuiper belt. The incidence rate of discs around the DUNES stars is increased from a rate of ~12.1% ± 5% before Herschel to ~20.2% ± 2%. A significant fraction (~52%) of the discs are resolved, which represents an enormous step ahead from the previously known resolved discs. Some stars are associated with faint far-IR excesses attributed to a new class of cold discs. Although it cannot be excluded that these excesses are produced by coincidental alignment of background galaxies, statistical arguments suggest that at least some of them are true debris discs. Some discs display peculiar SEDs with spectral indexes in the 70–160 μm range steeper than the Rayleigh-Jeans one. An analysis of the debris disc parameters suggests that a decrease might exist of the mean black body radius from the F-type to the K-type stars. In addition, a weak trend is suggested for a correlation of disc sizes and an anticorrelation of disc temperatures with the stellar age.
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We present Herschel PACS 100 and 160 μm observations of the solar-type stars α Men, HD 88230 and HD 210277, which form part of the FGK stars sample of the Herschel open time key programme (OTKP) DUNES (DUst around NEarby Stars). Our observations show small infrared excesses at 160 μm for all three stars. HD 210277 also shows a small excess at 100 μm, while the 100 μm fluxes of α Men and HD 88230 agree with the stellar photospheric predictions. We attribute these infrared excesses to a new class of cold, faint debris discs. Both α Men and HD 88230 are spatially resolved in the PACS 160 μm images, while HD 210277 is point-like at that wavelength. The projected linear sizes of the extended emission lie in the range from ~115 to ≤ 250 AU. The estimated black body temperatures from the 100 and 160 μm fluxes are ≲22 K, and the fractional luminosity of the cold dust is L_dust/L_⋆ ~ 10^-6, close to the luminosity of the solar-system’s Kuiper belt. These debris discs are the coldest and faintest discs discovered so far around mature stars, so they cannot be explained easily invoking “classical” debris disc models.
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The study of the Upper Jurassic-Lower Cretaceous deposits (Higueruelas, Villar del Arzobispo and Aldea de Cortés Formations) of the South Iberian Basin (NW Valencia, Spain) reveals new stratigraphic and sedimentological data, which have significant implications on the stratigraphic framework, depositional environments and age of these units. Moreover, these new data encourage revising the previously proposed stratigraphic correlations between the studied units and those deposited in adjacent areas of the Iberian Basin. The Higueruelas Fm was deposited in a mid-inner carbonate platform where oncolitic bars migrated by the action of storms and where oncoid production progressively decreased towards the uppermost part of the unit. The overlying Villar del Arzobispo Fm has been traditionally interpreted as an inner platform-lagoon evolving into a tidal-flat. Here it is interpreted as an inner-carbonate platform affected by storms, where oolitic shoals protected a lagoon, which had siliciclastic inputs from the continent. The Aldea de Cortés Fm has been previously interpreted as a lagoon surrounded by tidal-flats and fluvial-deltaic plains. Here it is reinterpreted as a coastal wetland where siliciclastic muddy deposits interacted with shallow fresh to marine water bodies, aeolian dunes and continental siliciclastic inputs. The contact between the Higueruelas and Villar del Arzobispo Fms, classically defined as gradual, is interpreted here as gradual and rapid, because the transition between both units comprises few meters. More importantly, the contact between the Villar del Arzobispo and Aldea de Cortés Fms, previously considered as unconformable, is here interpreted as gradual. The presence of Alveosepta in the Villar del Arzobispo Fm suggests that at least part of this unit is Kimmeridgian, unlike the previously assigned Late Tithonian-Middle Berriasian age. Consequently, the underlying Higueruelas Fm, previously considered Tithonian, should not be younger than Kimmeridgian. Accordingly, sedimentation of the Aldea de Cortés Fm, previously considered Valanginian-Hauterivian, probably started during the Tithonian and it may be considered part of the regressive trend of the Late Jurassic-Early Cretaceous cycle. This is consistent with the dinosaur faunas, typically Jurassic, described in the Villar del Arzobispo and Aldea de Cortés Fms.
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El gasterópodo marino Patella ferruginea se encuentra incluido en los Catálogos Español y Andaluz de Especies Amenazadas en la categoría “En peligro de extinción”. En 2008 fue aprobada la Estrategia de Conservación Nacional de la especie que establece la realización de un seguimiento de la población cada cuatro años. En Andalucía se ha realizado en 2010 el seguimiento de la especie empleando dos tipos de metodología: los “Controles de crecimiento”, mediante marcaje de ejemplares, y los “Censos exhaustivos” en “Tramos” de costa, para intentar detectar todos los individuos presentes. En el censo de 2010 se han muestreado unos 21 km de costa en 34 localidades, un 5% del litoral andaluz con presencia de la especie, lo que constituye un esfuerzo considerable, pero asumible para el control periódico de la misma. La densidad media detectada es muy baja, de 0,048 ind./m. El mayor número de individuos se encuentra en Cádiz y la población mejor estructurada en la isla de Alborán. Se estima que el tamaño actual de la población en Andalucía ronda los 1.800 ejemplares, lo que constituye un aumento con respecto a inventarios anteriores. Sin embargo, el contingente es muy reducido para garantizar la supervivencia de la especie. La categoría de protección propuesta por el Libro Rojo de los Invertebrados de Andalucía, “En peligro crítico” (MORENO y ARROYO, 2008), debe considerarse, por lo tanto, la más adecuada para la lapa ferruginosa siguiendo los criterios de valoración de la UICN (2001).
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Se ha estudiado la composición de las poblaciones de crustáceos decápodos en los fondos detríticos circalitorales del Este y Sureste ibérico, con relación a sus diferentes facies, efectuándose diferentes análisis estadísticos sobre la composición y diversidad. La taxocenosis de crustáceos decápodos muestra elevados valores de abundancia, riqueza y diversidad en las localidades identificadas como fondos detríticos costeros de aspecto típico. Por último, algunos grupos de especies podrían ser utilizados para caracterizar las biocenosis típica de fondos detríticos costeros, tales como: Paguristes eremita, Ebalia edwardsi, E. deshayesi, Eurynome aspera, Galathea intermedia, Parthenope massena, y Anapagurus hyndmani; la biocenosis del detrítico costero enfangada: Ebalia tuberosa, Atelecyclus rotundatus, Ethusa mascarone, y Liocarcinus zariquieyi; y la biocenosis de arenas fangosas: Upogebia deltaura, Goneplax rhomboides.
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Se publican las noticias que ha arrojado la excavación en 2004 de unos muros situados en la denominada playa de El Moncayo. Los hallazgos se sitúan a unos 3 kilómetros al Sur del casco urbano de Guardamar del Segura; a unos 135 m. en dirección Norte está la Torre del Descargador (torre almenara de los siglos IV/X y V/XI), a unos 3,5 kilómetros se localiza El Castillo de Guardamar (de los siglos VIII a.C. al XIX) y, un poco más al Norte, a unos 4 kilómetros, en las proximidades de la desembocadura del Segura, los oratorios o rábitas de las dunas de Guardamar. Se dan a conocer los restos arquitectónicos y cerámicos aparecidos en la excavación del 2004 que se interpretan como de restos del recinto de una rábita o mezquitilla (cuando se excave más se verá si está aislada o hay más edificios similares), se presentan unos apuntes al hilo de la orientación de la rábita de El Moncayo y un estudio de la moneda andalusí hallada en la excavación de El Moncayo (datables entre en 429/1037-8 y 433/1041-2).
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A detailed taphonomic analysis was carried out on the lower Albian deposits of the Sierra Helada section (Alicante, Betic Cordillera, southeastern Spain). Ten taphonomic characters were studied and ten skeletal concentrations were defined on the basis of taphonomic features and the dominant taxa. Cluster analysis was performed on the dataset represented by the abundance of the taphonomic characters in each skeletal concentration. This enabled the definition of four different taphonomic categories: 1) skeletal concentrations characterized by the presence of fossils preserved in life position, 2) skeletal concentrations showing very little physical reworking, 3) skeletal concentrations related to high-energy background conditions, and 4) skeletal concentrations produced by medium- to high-energy events. Four taphofacies were defined on the basis of the main sedimentological features and the most representative skeletal concentrations. Taphofacies A represents the low energy outer platform, rich in skeletal concentrations with echinoids in life position and only slightly reworked. The second taphofacies (taphofacies B) is very rich in reworked echinoid tests and calcarenitic beds and records the transition to shallower areas, while taphofacies C shows abundant thick-bedded calcarenites and skeletal concentrations produced by sediment transport and rapid deposition. Finally, cross-bedded grainstone beds, which are rich in fine-grained fragmented, locally reoriented bioclasts (taphofacies D), record the existence of shifting sandy dunes in the shallow inner part of the platform.
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The Australian southern continental margin is the world’s largest site of cool-water carbonate deposition, and the Great Australian Bight is its largest sector. The Eyre Peninsula is fringed by coastal beaches with aeolianites and marks the eastern edge of the Great Australian Bight. Five shoreline transects of varying lengths spanned a 150km longitudinal distance and at each the intertidal, beach, dune and secondary dune environments were sampled, for a total of 18 samples. Sediments are a mixture of modern, relict, and Cenozoic carbonates, and quartz grains. Carbonate aeolianites on the western Eyre Peninsula are mostly composed of modern carbonate grains: predominantly molluscs (23-33%) and benthic foraminifera (10-26%), locally abundant coralline algae (3-28%), echinoids (2-22%), and bryozoans (2-14%). Cenozoic grain abundance ranges from 1-6% whereas relict grain abundance ranges from 0-17%. A southward increase in bryozoan particles correlates with a nutrient element abundance and decrease in temperature due to a large seasonal coastal upwelling system that drives 2-3 major upwelling events per year, bringing cold, nutrient rich, Sub-Antarctic Surface Water (<12°C) onto the shelf. In southern, mostly wind protected locations, the beach and dune sediment compositions are similar, indicating that wind energy has successfully carried all sediment components of the beach into the adjacent dunes. In northern, exposed locations, the composition is not the same everywhere, and trends indicate that relative wind energy has the ability to impact grain composition through preferential wind transport. Aeolianite composition is therefore a function of both upwelling and the degree of coastal exposure.
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As paisagens dunares são sistemas de elevado dinamismo, devido à proximidade do mar e à extrema mobilidade do substrato arenoso e prevê-se que venham a ser severamente afetadas pelas alterações ambientais globais. As dunas são depósitos de areia criados por processos eólicos e apresentam uma vegetação muito característica. Estes depósitos de areia em conjunto com a vegetação formam uma barreira essencial ao avanço do mar durante as marés altas de águas vivas e tempestades. Em Portugal, a degradação dos ecossistemas costeiros é muito preocupante. O problema das espécies exóticas invasoras agravou-se, aumentando a pressão sobre as plantas nativas. Embora este problema não seja o único motivo da degradação dos ecossistemas costeiros, este trabalho pretende divulgar as plantas dunares da zona costeira de Matosinhos, sensibilizar para a proteção e conservação das dunas e alertar para o facto de diversas plantas invasoras rapidamente colonizarem espaços abertos, pondo em causa e estabilidade dos ecossistemas costeiros. O conhecimento detalhado destes ecossistemas permitirá a aplicação de processos de vigilância e monitorização bem como o restauro ecológico de áreas dunares degradadas.
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Issued July 1977.