Hydrological and erosional response to natural rainfall in a semi‐arid area of south‐east Spain     

M. Martinez‐Mena  V. Castillo  J. Albaladejo 《水文研究》2001,15(4):557-571

A better knowledge of soil erosion by water is essential for planning effective soil and water conservation practices in semi‐arid Mediterranean environments. The special climatic and hydrological characteristics of these areas, however, make accurate soil loss predictions difficult, particularly in the absence of minimal data. Two zero‐order experimental microcatchments (328–759 m²), representative of an extensive semi‐arid watershed with a high potential erosion risk in the south‐east of Spain, were selected and monitored for 3 years (1991–93) in order to provide information on the hydrological and erosional response. A pluviogram and hydrograph recorded data at 1‐min intervals during each storm, after which the soil loss was collected and the particle size of the sediment was analysed. Runoff coefficients of about 9% and soil losses of between 84·83 and 298·9 g m^?2 year^?1 were observed in the area. Rapid response times (geometric mean values lower than 2 h) and low runoff thresholds (mean values between 3·5 to 5·9 mm) were the norm in the experimental areas. A rain intensity of over 15 mm h^?1 was considered as ‘erosive rainfall’ in these areas because of the total soil loss and the transport capacity of the overland flow. Differences in pore‐size distribution explained the different hydrological responses observed between areas. The erosional response was more complex and basically seemed to be determined by soil aggregate stability and topographical properties. A greater proportion of finer particles in the eroded material than in the soil matrix indicated selective erosion and the transport of finer material. Copyright © 2001 John Wiley & Sons, Ltd.  相似文献   

Contrasting conditions preceding MIS3 and MIS2 Heinrich events   总被引：2，自引：0，他引：2  

Elsa Jullien  Francis E. Grousset  Sidney R. Hemming  Victoria L. Peck  Ian R. Hall  Cdric Jeantet  Isabelle Billy 《Global and Planetary Change》2006,54(3-4):225-238

This paper presents an integrated multi-tracer study performed on piston cores recovered in the glacial ice-rafted detritus belt, stretching from Newfoundland to the Irish margin across the North Atlantic (40–55°N), in order to compare in detail the internal structure of each Heinrich event (HE). These tracers are IRD counts (quartz, dolomite, volcanic grains), their Nd isotopic composition and Ar–Ar datings of individual hornblende grains. A focus on the detailed structure of HE confirms that all intervals of massive sediment flux, specifically Heinrich layers HL1-to-5 (HLs), were dominated by North American, Laurentide ice-sheet surges from Hudson Strait, that are evident as far east as the Bay of Biscay (European margin). The sequences of events leading up to the HLs, however, present significant dissimilarities. One important difference is that HL2 and HL1 were preceded by “precursor events” (increases in the number of lithic grains per gram from non-Laurentide sediment sources). Sediment debris derived from near-simultaneous iceberg releases originating from the European ice-sheet are only detectable close to the European margin. In contrast there are no comparable precursor events before HL5 and HL4. This observation implies that precursor events are unlikely to be mechanistically linked to the triggering of HEs. The similarity of the HLs, against contrasting background conditions, is a significant observation that should add constraints to their origin.  相似文献   

A photometric and spectroscopic study of the hottest pulsating extreme helium star, V2076 Oph (HD 160641)     

D. J. Wright  A. E. Lynas-Gray  D. Kilkenny  P. L. Cottrell  R. R. Shobbrook  C. Koen  F. W. van Wyk  P. M. Kilmartin  P. Martinez  A. C. Gilmore 《Monthly notices of the Royal Astronomical Society》2006,369(4):2049-2058

We present results from a three-site photometric and high-resolution spectroscopic campaign on the hottest known extreme helium star V2076 Oph (HD 160641). A core programme of intensive observations covered two weeks and a much lower sampling rate extended over another two months. Despite the fact that the data seem to indicate periodicity near half a day (though the light curves are clearly not formed by a single periodicity), conventional Fourier analysis of the data fails to reveal coherent frequencies. Furthermore, we are unable to recover frequencies which were apparently clear in an earlier campaign on the star. Evidence of monotonic pulsation amplitude changes is seen at the higher frequencies from a wavelet analysis, but more data are needed before this study can be extended to lower frequencies. The application of linear stochastic differential equation (LSDE) methods indicates that the observed light variations could be a result of random variations giving the appearance of intermittent periodicity. High-resolution spectroscopic observations were obtained during the campaign and additional observations were made three years later. Complex line profile variations were observed. It is proposed that the different behaviour of the emission line studied may indicate it is associated with a stellar wind or resident circumstellar material. The frequencies that are extracted from the velocity data do not conform to those identified in the current or previous photometric campaigns.  相似文献   

Temporal Variations of Perturbed Elliptic Elements: A Semi-Analytical Approach     

F.J. Marco  J.A. Lopez  M.J. Martinez 《Celestial Mechanics and Dynamical Astronomy》1997,68(2):193-198

The classical treatment of implied differences on the orbital ellipticelements from the errors involved at an initial epoch is not possible toapply if we consider a long interval of integration, because there is atemporal variation for all the partial derivatives of the elements withrespect to all the variations in the initial ones. We propose asemi-analytical method to compute these partial derivatives by solving a setof initial value problems which are obtained from the planetary Lagrangeequations and their partial derivatives with respect to all the variationsin the initial elements.  相似文献   

Evaluation of sulfate reduction at experimentally induced mixing interfaces using small-scale push–pull tests in an aquifer–wetland system     

Tara A. Kneeshaw  Jennifer T. McGuire  Erik W. Smith  Isabelle M. Cozzarelli 《Applied Geochemistry》2007,22(12):2618-2629

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Centimeter-scale characterization of biogeochemical gradients at a wetland–aquifer interface using capillary electrophoresis     

Susan Bez-Cazull  Jennifer T. McGuire  Isabelle M. Cozzarelli  Anne Raymond  Lisa Welsh 《Applied Geochemistry》2007,22(12):2664-2683

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Description of a very dense meteorite collection area in western Atacama: Insight into the long‐term composition of the meteorite flux to Earth          下载免费PDF全文

Aurore Hutzler  Jérôme Gattacceca  Pierre Rochette  Régis Braucher  Bertrand Carro  Eric J. Christensen  Cécile Cournede  Matthieu Gounelle  Nejia Laridhi Ouazaa  Rodrigo Martinez  Millarca Valenzuela  Michael Warner  Didier Bourles 《Meteoritics & planetary science》2016,51(3):468-482

We describe the geological, morphological, and climatic settings of two new meteorite collections from Atacama (Chile). The “El Médano collection” was recovered by systematic on‐foot search in El Médano and Caleta el Cobre dense collection areas and is composed of 213 meteorites before pairing, 142 after pairing. The “private collection” has been recovered by car by three private hunters and consists of 213 meteorites. Similar to other hot desert finds, and contrary to the falls and Antarctica finds, both collections show an overabundance of H chondrites. A recovery density can be calculated only for the El Médano collection and gives 251 and 168 meteorites larger than 10 g km^?2, before and after pairing, respectively. It is by far the densest collection area described in hot deserts. The Atacama Desert is known to have been hyperarid for a long period of time and, based on cosmic‐ray exposure ages on the order of 1–10 Ma, to have been stable over a period of time of several million years. Such a high meteorite concentration might be explained invoking either a yet unclear concentration mechanism (possibly related to downslope creeping) or a previously underestimated meteorite flux in previous studies or an average terrestrial age over 2 Myr. This last hypothesis is supported by the high weathering grade of meteorites and by the common terrestrial fragmentation (with fragments scattered over a few meters) of recovered meteorites.  相似文献   

Estimating Sensible and Latent Heat Fluxes over an Inland Water Body Using Optical and Microwave Scintillometers     

Pierre  Adrien  Isabelle  Pierre-Erik  Nadeau  Daniel F.  Thiboult  Antoine  Perelet  Alexei  Rousseau  Alain N.  Anctil  François  Deschamps  Jaril 《Boundary-Layer Meteorology》2022,185(2):277-308

Boundary-Layer Meteorology - Observations of turbulent heat fluxes over inland water bodies are scarce despite being critical to adequate lake parametrization for numerical weather forecast and...  相似文献   

Automatic road change detection and GIS updating from high spatial remotely-sensed imagery     

Zhang Qiaoping  Isabelle Couloigner 《地球空间信息科学学报》2013,16(2):89-95

This paper presents a framework for road network change detection in order to update the Canadian National Topographic DataBase (NTDB). The methodology has been developed on the basis of road extraction from IRS-pan images (with a 5.8 m spatial resolution) by using a wavelet approach. The feature matching and conflation techniques are used to road change detection and updating. Elementary experiments have showed that the proposed framework could be used for developing an operational road database updating system.  相似文献   

Validation and calibration of solar radiation equations for estimating daily reference evapotranspiration at cool semi-arid and arid locations     

Hossein Tabari  Parisa Hosseinzadehtalaei  Patrick Willems  Christopher Martinez 《水文科学杂志》2013,58(3):610-619

ABSTRACT

In this work, the applicability of 12 solar radiation (R_S) estimation models and their impacts on daily reference evapotranspiration (ET_o) estimates using the Penman‐Monteith FAO-56 (PMF-56) method were tested under cool arid and semi-arid conditions in Iran. The results indicated that the average increase in accuracy of the ET_o estimates by the calibrated R_S models, quantified by the decrease in RMSE, was 2.8% and 6.4% for semi-arid and arid climates, respectively. Mean daily deviations in the estimated ET_o by the calibrated R_S equations in semi-arid climates varied from ?0.283?mm/d^-1 for the Glover‐McCulloch model to 0.080?mm/d for the El-Sebaii model, with an average of ?0.109?mm/d^-1, and in arid climates, they ranged from ?0.522?mm/d^-1 for the Samani model to 0.668?mm/d for the El-Sebaii model, with an average of 0.125?mm/d^-1.