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51.
Eleonora S. Carol Eduardo Emilio Kruse Jorge L. Pousa 《Environmental Earth Sciences》2010,60(4):749-756
Although not well known, the eco-hydrological functions of deep aquifers (those having no contact with surface hydrological
events) play an important role in the hydrological regime because they can affect the type of habitats, the availability of
water and nutrients and the salinity of the medium, among other environmental features. This work aims at characterizing the
deep Tertiary hydrogeological units of the Salado sedimentary basin in the Province of Buenos Aires, Argentina, at a regional
scale, and to determine their environmental importance in the hydrological cycle. The geological characterization of the study
area is based on the drilling profiles from oil exploration wells bored by different oil companies between 1948 and 1994,
and also from the existing literature. The conclusion is that water exchange between quaternary surface aquifers in contact
with atmospheric events and deep tertiary aquifers is one of the main processes that keep the hydrologic balance of the region.
Not only is this crucial for the conservation of the numerous and well-developed ecosystems in the basin wetlands, but also
significant for the agricultural and cattle-raising activities of the region. 相似文献
52.
Owing to gravitational instability, an initially Gaussian density field develops non-Gaussian features as the Universe evolves. The most prominent non-Gaussian features are massive haloes, visible as clusters of galaxies. The distortion of high-redshift galaxy images because of the tidal gravitational field of the large-scale matter distribution, called cosmic shear, can be used to investigate the statistical properties of the large‐scale structure (LSS) . In particular, non-Gaussian properties of the LSS will lead to a non-Gaussian distribution of cosmic-shear statistic. The aperture mass ( M ap ) statistics, recently introduced as a measure for cosmic shear, is particularly well suited for measuring these non-Gaussian properties. In this paper we calculate the highly non-Gaussian tail of the aperture mass probability distribution, assuming Press–Schechter theory for the halo abundance and the 'universal' density profile of haloes as obtained from numerical simulations. We find that for values of M ap much larger than its dispersion, this probability distribution is closely approximated by an exponential, rather than a Gaussian. We determine the amplitude and shape of this exponential for various cosmological models and aperture sizes, and show that wide-field imaging surveys can be used to distinguish between some of the currently most popular cosmogonies. Our study here is complementary to earlier cosmic-shear investigations, which focused more on two- and three-point statistical properties. 相似文献
53.
Zou Yilin Stock Alexia Davidson Rachel Nozick Linda Trainor Joseph Kruse Jamie 《Natural Hazards》2020,104(1):201-224
Natural Hazards - Understanding how homeowners make protective action decisions is important for designing policies and programs to encourage those actions and community resilience as a whole. This... 相似文献
54.
E‐mobility has been gaining importance in recent years in Germany, with the National Platform for E‐mobility infrastructure in Germany is expected to change fast, therefore many charging stations will appear. These need to be managed, and the aim of this work is to explore how web applications could best support productivity and user experience in this context. We compared a text‐form‐based approach to a map‐based approach for the addition and update of locations and chargepoints. We found that the map‐based approach yields better learning effects and offers a better compromise between pragmatic and hedonic properties. The results are useful for a better understanding of the impact of interactive maps on work and user experience in the e‐mobility domain and beyond. 相似文献