Modeling aquifer�Criver interactions under the influence of groundwater abstraction in the Mancha Oriental System (SE Spain)     

David Sanz  Santiago Casta?o  Eduardo Cassiraga  Andr��s Sahuquillo  Juan Jos�� G��mez-Alday  Salvador Pe?a  Alfonso Calera 《Hydrogeology Journal》2011,19(2):475-487

The Mancha Oriental System (MOS, 7,260?km²) is one of the largest aquifers within Spain, and is encompassed by the Jucar River Basin. Over the past 30?years, socioeconomic development within the region has been largely due to intensive use of groundwater resources for irrigating crops (1,000?km²). Groundwater pumping (406 million m³/year) has provoked a steady drop in the groundwater level and a reduction of MOS discharge to the Jucar River. The study aims to characterize the river?Caquifer relationship, to determine the influence that groundwater abstraction has on the river discharge. This research has advanced a three-dimensional large-scale numerical groundwater-flow model (MODFLOW 2000) in order to spatially and temporally evaluate, quantify and predict the river?Caquifer interactions that are influenced by groundwater abstraction in MOS. It is demonstrated that although groundwater abstraction increased considerably from the early 1980s to 2000, the depletion of water stored in the aquifer was lower than might be expected. This is mainly due to aquifer recharge from the Jucar River, induced by groundwater abstraction. The area of disconnection between the river and the water table (i.e. where groundwater head is lower than the riverbed) is found to have spread 20?km downstream from its position before pumping started.  相似文献   

Preface to John W. Morse Special Issue of Aquatic Geochemistry     

Fred T. Mackenzie  Alfonso Mucci  George W. Luther III 《Aquatic Geochemistry》2011,17(4-5):307-310

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Magnetic classification of stony meteorites: 1. Ordinary chondrites     

Pierre ROCHETTE  Leonardo SAGNOTTI  Michle BOUROT‐DENISE  Guy CONSOLMAGNO  Luigi FOLCO  Jrme GATTACCECA  Maria Luisa OSETE  Lauri PESONEN 《Meteoritics & planetary science》2003,38(2):251-268

Abstract— We present a database of magnetic susceptibility measurements on 971 ordinary chondrites. It demonstrates that this parameter can be successfully used to characterize and classify ordinary chondrite meteorites. In ordinary chondrites, this rapid and non‐destructive measurement essentially determines the amount of metal in the sample, which occurs in a very narrow range for each chondrite class (though terrestrial weathering can result in a variable decrease in susceptibility, especially in finds). This technique is particularly useful not only for a rapid classification of new meteorites, but also as a check against curation errors in large collections (i.e., unweathered meteorites, the measured susceptibility of which lies outside the expected range, may well be misclassified or misidentified samples). Magnetic remanence, related to magnetic field measurements around asteroids, is also discussed.  相似文献   

Strike-slip faults parallel to crustal spreading axes: data from Iceland and the Afar Depression     

Pietro Passerini  Marta Marcucci  Giovanni Sguazzoni  Leonardo Zan  Abdourahman Omar Haga 《地学学报》1991,3(6):607-618

Slickenside studies in regions of crustal spreading such as Iceland and the Afar Depression, East Africa, reveal that a significant number of faults parallel and close to rift axes are strike-slip rather than normal. Therefore, the pattern of brittle deformation in these regions does not conform to the classic two-dimensional schemes of oceanic tectonics and pre-oceanic rifting. Dip-slip and strike-slip faulting presumably alternated along or in the vicinity of spreading axes, indicate a varying stress field and a combination of transverse and longitudinal movements. In Iceland, strike-slip faults parallel to rifts are observed both west and east of the rift system as well as in a median area between overlapping rifts; the mechanisms proposed for their origin include accommodation of oblique convergence or divergence of crustal sections due to variations of spreading directions along axis and the interaction of overlapping rifts. In the Afar Depression this kind of fault is recorded west of the rift of Asal and can be imputed to reflect an interaction among rifts in the vicinity of the Afar triple junction. Rift-parallel strike-slip faults cannot however be assumed to be a feature of all crustal spreading axes due to the peculiarity of the examined regions: both of them are hot-spot areas and the Afar Depression lies at a triple junction.  相似文献   

Waiting Time Distribution of Emissions in Complex Coronal Mass Ejections     

Adolfo L. Méndez Berhondo  Ramón E. Rodríguez Taboada  Liliana Alfonso Larralde 《Astrophysics and Space Science》2006,302(1-4):213-216

The waiting time distribution of emissions in Coronal Mass Ejections (CMEs) with several emissions is examined. We define the waiting time as the time interval between the commencement of an emission and the commencement of the next emission considered as parts of a unique CME. The distribution seems to follow a power-law. Two classes of CMEs several emissions are considered: “close” and “separate” depending on angular distance between emissions.  相似文献   

Near-IR Integral Field Spectroscopy of High-z Galaxies     

Andrew Bunker  Annette Ferguson  Rachel Johnson  Richard McMahon  Ian Parry  Max Pettini  Alfonso Aragón-Salamanca  Rachel Somerville  Nicole Vogt 《Astrophysics and Space Science》2002,281(1-2):529-529

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On gravitational instability of the interstellar gas     

Bruno Bertotti  Alfonso Cavaliere 《Astrophysics and Space Science》1969,5(1):78-91

In the galaxy, Jeans' critical length for the interstellar gas is appreciably smaller than the critical length for the stars, a necessary condition for the gravitational instability of the former to have a local character. An accurate discussion of the orders of magnitude involved leads to the establishment of a well defined limiting procedure and to simplified equations in which the effect of stars occurs only through the equilibrium, but disappears from the perturbations. The equations are spatially local, but their coefficients are time-dependent, in that they describe the evolution of a small wave packet dragged along by the supersonic gas motion. They have been solved in several interesting cases by the introduction of an effective, time-dependent wave vector, which describes the deformation of a wave profile due to the velocity gradients. The ordinary Jeans' instability is recovered only when the velocity gradient is a skew tensor; otherwise we find a stabilizing effect in accelerated and sheared flows, a destabilizing effect in a decelerated flow. Possible connections of this model with the observed turbulent structure of the interstellar gas are discussed.  相似文献   

The density of Red Sea brines     

Frank J. Millero  Alfonso Mucci  James Zullig  Peter Chetirkin 《Marine Chemistry》1982,11(5):463-475

The densities of artificial and real Red Sea brines have been measured at 25°C with a vibrating tube densimeter. Measurements were also made on mixtures of Red Sea brines with seawater and pure water. The results have been used to characterize the density—composition relations of waters across the interface of brine and average Red Sea waters. The results for the real and artificial brines are in reasonable agreement.The composition of the brines and mixtures with seawater have been characterized by conductivity measurements of weight diluted samples. The conductivity salinities were found to be conservative to within $\text{±0.07‰}$ for the mixtures.The densities of brines and mixtures of brines and seawater were estimated from apparent molal volume data using Young's rule. The calculated densities for all of the solutions were found to be in good agreement with the measured values, demonstrating the applicability of Young's rule to concentrated natural waters.  相似文献   

Diffuse Baryons in Cosmic Structures     

Alfonso Cavaliere 《Astrophysics and Space Science》2004,294(1-2):109-124

I review the processes that govern the amount and the thermal state of the hot plasma pervading clusters and groups of galaxies: the gravitational heating driven by the DM merging histories, the radiative cooling of baryons, and the energy fed back by SNe and by AGNs or quasars. I argue that the X-ray emissions and the entropy levels now observed from clusters to groups require the AGNs to contribute substantially to preheat the gas before it falls into clusters, and the quasars to blow some plasma out of groups and galaxies.  相似文献   

Undrained instability detection under general stress conditions     

Leguizamón-Barreto  Luis C.  Ramos-Cañón  Alfonso M.  Andrade  José E. 《Acta Geotechnica》2021,16(10):3041-3059

Acta Geotechnica - This work proposes a criterion for the detection of undrained instability under multiaxial stress conditions at elemental level. To do so, it develops the application of the...  相似文献