992 resultados para 7038-507


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An integrated instrument package for measuring and understanding the surface radiation budget of sea ice is presented, along with results from its first deployment. The setup simultaneously measures broadband fluxes of upwelling and downwelling terrestrial and solar radiation (four components separately), spectral fluxes of incident and reflected solar radiation, and supporting data such as air temperature and humidity, surface temperature, and location (GPS), in addition to photographing the sky and observed surface during each measurement. The instruments are mounted on a small sled, allowing measurements of the radiation budget to be made at many locations in the study area to see the effect of small-scale surface processes on the large-scale radiation budget. Such observations have many applications, from calibration and validation of remote sensing products to improving our understanding of surface processes that affect atmosphere-snow-ice interactions and drive feedbacks, ultimately leading to the potential to improve climate modelling of ice-covered regions of the ocean. The photographs, spectral data, and other observations allow for improved analysis of the broadband data. An example of this is shown by using the observations made during a partly cloudy day, which show erratic variations due to passing clouds, and creating a careful estimate of what the radiation budget along the observed line would have been under uniform sky conditions, clear or overcast. Other data from the setup's first deployment, in June 2011 on fast ice near Point Barrow, Alaska, are also shown; these illustrate the rapid changes of the radiation budget during a cold period that led to refreezing and new snow well into the melt season.

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The dataset contains the revised age models and foraminiferal records obtained for the Last Interglacial period in six marine sediment cores: - the Southern Ocean core MD02-2488 (age model, sea surface temperatures, benthic d18O and d13C for the period 136-108 ka), - the North Atlantic core MD95-2042 (age model, planktic d18O, benthic d18O and d13C for the period 135-110 ka), - the North Atlantic core ODP 980 (age model, planktic d18O, sea surface temperatures, seawater d18O, benthic d18O and d13C, ice-rafted detritus for the period 135-110 ka), - the North Atlantic core CH69-K09 (age model, planktic d18O, sea surface temperatures, seawater d18O, benthic d18O and d13C, ice-rafted detritus for the period 135-110 ka), - the Norwegian Sea core MD95-2010 (age model, percentage of Neogloboquadrina pachyderma sinistral, sea surface temperatures, benthic d18O, ice-rafted detritus for the period 134-110 ka), - the Labrador Sea core EW9302-JPC2 (age model, percentage of Neogloboquadrina pachyderma sinistral, sea surface temperatures, benthic d18O for the period 134-110 ka).

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Ocean Drilling Program (ODP) Sites 832 and 833 were drilled in the intra-arc North Aoba Basin of the New Hebrides Island Arc (Vanuatu). High volcanic influxes in the intra-arc basin sediment resulting from erosion of volcanic rocks from nearby islands and from volcanic activity are associated with characteristic magnetic signals. The high magnetic susceptibility in the sediment (varying on average from 0.005 to more than 0.03 SI) is one of the most characteristic physical properties of this sedimentary depositional environment because of the high concentration of magnetites in redeposited ash flows and in coarse-grained turbidites. Susceptibility data correlate well with the high resolution electrical resistivity logs recorded by the formation microscanner (FMS) tool. Unlike the standard geophysical logs, which have low vertical resolution and therefore smooth the record of the sedimentary process, the FMS and whole-core susceptibility data provide a clearer picture of turbiditic sediment deposition. Measurements of Curie temperatures and low-temperature susceptibility behavior indicate that the principal magnetic minerals in ash beds, silt, and volcanic sandstone are Ti-poor titanomagnetite, whereas Ti-rich titanomagnetites are found in the intrusive sills at the bottom of Site 833. Apart from an increase in the concentration of magnetite in the sandstone layer, acquisition of isothermal and anhysteretic remanences does not show significant differences between sandstone and clayey silts. The determination of the anisotropy of magnetic susceptibility (AMS) in more than 400 samples show that clayey siltstone have a magnetic anisotropy up to 15%, whereas the AMS is much reduced in sandstone layers. The magnetic susceptibility fabric is dominated by the foliation plane, which is coplanar to the bedding plane. Reorientations of the samples using characteristic remanent magnetizations indicate that the bedding planes dip about 10° toward the east, in agreement with results from FMS images. Basaltic sills drilled at Site 833 have high magnetic susceptibilities (0.05 to 0.1 SI) and strong remanent magnetizations. Magnetic field anomalies up to 50 µT were measured in the sills by the general purpose inclinometer tool (GPIT). The direction of the in-situ magnetic anomaly vectors, calculated from the GPIT, is oriented toward the southeast with shallow inclinations which suggests that the sill intruded during a reversed polarity period.

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Four samples of Nauru Basin basalts (Cores 94 to 109 of Hole 462A, sub-bottom depth 1077-1209 m) have 87Sr/86Sr ratios in the range 0.7037 to 0.7038, which is distinctly higher than the ratios of N-type MORB. The Rb contents of the samples are depleted in comparison with those of MORB and ocean-island basalts. These chemical and isotopic characteristics are identical to those of the basalts previously drilled during Leg 61 (Cores 75 to 90 of Hole 462A), and are explained in terms of inhomogeneity of the source region in the mantle or later alteration effects. Sr/Ca-Ba/Ca systematics of 15 samples from Cores 462A-94 to 462A-109 and 14 samples from Cores 462A-75 to 462A-90 suggest that the Nauru Basin basalts are derived from a mantle peridotite by 20 to 30% partial melting with subsequent Plagioclase crystallization.

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Se presentarán los resultados de un estudio denominado "Consumo de sustancias psicoactivas en estudiantes de la Universidad Nacional de San Luis 2009". Investigaciones anteriores (OAD, 2006) evidencian el consumo de sustancias psicoactivas en estudiantes universitarios, mostrando que la institución universitaria no se encuentra exenta de esta problemática. El estudio indagó la presencia de comportamientos de consumo de sustancias psicoactivas, la modalidad de presentación del fenómeno y las dificultades de los estudiantes para la consecución de sus estudios universitarios. Los resultados aportan información para el desarrollo de estrategias de prevención del consumo de sustancias psicoactivas en esta comunidad universitaria. Se siguió un diseño de tipo exploratorio descriptivo. La muestra, no aleatoria, estuvo conformada por 507 estudiantes de las diversas facultades y carreras de la UNSL. Para la recolección de datos se utilizó un 'Cuestionario autoadministrado' (Vavassori, D., 2003), anónimo y voluntario. Este instrumento indagó acerca de los datos que permitieron caracterizar sociodemográficamente a la muestra, sobre la situación académica de los sujetos, y acerca de la presentación de la conducta de consumo de una o varias sustancias psicoactivas. Los resultados dejan en evidencia que de la totalidad de la muestra (507 estudiantes) consumen algún tipo de sustancia tóxica 395 sujetos (77,9) Discriminados por el tipo de sustancia consumen alcohol el 70,2de los estudiantes, tabaco el 28,8, medicamentos el 14,6y sustancias ilegales el 9,9. Respecto a los datos en función de las variables sexo y edad de los sujetos, se observó que son los varones quienes más consumen sustancias psicoactivas legales, mientras que las mujeres consumen más sustancias ilegales en comparación con los primeros. El uso de alcohol es mayor en el grupo que tienen entre 19 y 26 años (72,9), el uso de tabaco tuvo una alta prevalencia en el grupo de 31 a 34 años; el uso de medicamentos en el grupo de sujetos que tienen más de 35 años (44,4); el mayor consumo de sustancias ilegales se observó en el grupo que tiene entre 19 y 22 años. Se observó un importante porcentaje de estudiantes que consumen alcohol durante los fines de semana El consumo de alcohol se asocia con el alivio de estados de malestar y tensión. El hecho que una gran cantidad de estudiantes consuman alcohol durante el fin de semana, se presentacomo un aspecto que podría llegar a considerarse un abuso de esta sustancia psicoactiva en la medida en que este consumo se regularice. Los resultados muestran que lasustancia psicoactiva ilegal de mayor consumo es la marihuana, en menor medida la ingesta de cocaína. El consumo de estas drogas adquiere características recreativas, en función de la frecuencia, modalidad y lugar de consumo. La mitad de los sujetos que usan sustancias ilegales no ha cursado deforma regular su carrera universitaria, tienen dificultades para rendir exámenes finales y no están satisfechos con su rendimiento académico. Se concluye que hay un grupo pequeño de estudiantes en situación de riesgo respecto al consumo y una serie de factores de riesgo que podrían incidir en el consumo de sustancias (personales, familiares y sociales), sobre los cuales debería focalizarse toda acción preventiva primaria. Es preciso reflexionar sobre el papel que debe cumplir la UNSL, como institución formadora de profesionales, en el desarrollo de políticas y acciones de prevención primaria. Los resultados de este estudio aportan la información necesaria para un diagnóstico situacional sobre el consumo de sustancias piscoactivas, punto de partida primordial para diseñar, planificar y ejecutar en conjunto acciones preventivas dirigidas a esta comunidad universitaria

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Strontium- and oxygen-isotopic measurements of samples recovered from the Trans-Atlantic Geotraverse (TAG) hydrothermal mound during Leg 158 of the Ocean Drilling Program provide important constraints on the nature of fluid-rock interactions during basalt alteration and mineralization within an active hydrothermal deposit. Fresh Mid-Ocean Ridge Basalt (MORB), with a 87Sr/86Sr of 0.7026, from the basement beneath the TAG mound was altered at both low and high temperatures by seawater and altered at high temperature by near end-member black smoker fluids. Pillow breccias occurring beneath the margins of the mound are locally recrystallized to chlorite by interaction with large volumes of conductively heated seawater (>200°C). The development of a silicified, sulfide-mineralized stockwork within the basaltic basement follows a simple paragenetic sequence of chloritization followed by mineralization and the development of a quartz+pyrite+paragonite stockwork cut by quartz-pyrite veins. Initial alteration involved the development of chloritic alteration halos around basalt clasts by reaction with a Mg-bearing mixture of upwelling, high-temperature (>300°C), black smoker-type fluid with a minor (<10%) proportion of seawater. Continued high-temperature (>300°C) interaction between the wallrock and these Mg-bearing fluids results in the complete recrystallization of the wallrock to chlorite+quartz+pyrite. The quartz+pyrite+paragonite assemblage replaces the chloritized basalts, and developed by reaction at 250-360°C with end-member hydrothermal fluids having 87Sr/86Sr ~0.7038, similar to present-day vent fluids. The uniformity of the 87Sr/86Sr ratios of hydrothermal assemblages throughout the mound and stockwork requires that the 87Sr/86Sr ratio of end-member hydrothermal fluids has remained relatively constant for a time period longer than that required to change the interior thermal structure and plumbing network of the mound and underlying stockwork. Precipitation of anhydrite in breccias and as late-stage veins throughout most of the mound and stockwork, down to at least 125 mbsf, records extensive entrainment of seawater into the hydrothermal deposit. 87Sr/86Sr ratios indicate that most of the anhydrite formed from ~2:1 mixture of seawater and black smoker fluids (65%±15% seawater). Oxygen-isotopic compositions imply that anhydrite precipitated at temperatures between 147°C and 270°C and require that seawater was conductively heated to between 100°C and 180°C before mixing and precipitation occurred. Anhydrite from the TAG mound has a Sr-Ca partition coefficient Kd ~0.60±0.28 (2 sigma). This value is in agreement with the range of experimentally determined partition coefficients (Kd ~0.27-0.73) and is similar to those calculated for anhydrite from active black smoker chimneys from 21°N on the East Pacific Rise. The d18O (for SO4) of TAG anhydrite brackets the value of seawater sulfate oxygen (~9.5?). Dissolution of anhydrite back into the oceans during episodes of hydrothermal quiescence provides a mechanism of buffering seawater sulfate oxygen to an isotopically light composition, in addition to the precipitation and dissolution of anhydrite within the oceanic basement during hydrothermal recharge at the mid-ocean ridges.

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