Special Issue on Environmental Geostatistics     

J. Jaime Gómez-Hernández  Celine Scheidt 《Mathematical Geosciences》2013,45(5):507-509

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Predictability of currents on a mesotidal estuary (Ria de Vigo, NW Iberia)     

Pablo Cerralbo  Manel Grifoll  Manuel Espino  Jaime López 《Ocean Dynamics》2013,63(2-3):131-141

In this contribution, the implementation, validation and sensitivity analysis of an operational forecasting system (three-dimensional hydrostatic model) in the Ría de Vigo is presented. A set of sensitivity tests for different atmospheric and hydrodynamic typical periods was performed. The goal is to determine the relative importance of forcing mechanisms in order to evaluate the source of errors in predictions. Previously, validations for three periods of about 15 days were compared with measured data. Sea-level evolution reveals low errors and correlation values close to 1. Surface velocities were compared with high-frequency radar and horizontal Acoustic Doppler Current Profiler data, showing acceptable results on radar area, where tidal and wind circulation patterns are well reproduced by the model. Conductivity, temperature, and depth profiles were used to validate simulated temperature and salinity. While modelled temperature profiles show good agreement with measured profiles, eventual errors are detected on salinity. The sensitivity analysis took three variables into account: sea level, currents at open boundary conditions, and winds (two different configurations). The results show that the most important source of errors on simulated surface currents is wind. Errors on open boundary conditions seem to be limited on the outermost part of the Ría. Although the results presented mainly focus on the Ría de Vigo, the method and conclusions may be applied to other mesotidal estuaries. Moreover, this work will allow a more effective operational system focused on coastal management to be performed.  相似文献   

Magnetic characterization of Cretaceous‐Tertiary boundary sediments     

Víctor Villasante‐Marcos  Francisca MartÍNez‐Ruiz  María Luisa Osete  Jaime Urrutia‐Fucugauchi 《Meteoritics & planetary science》2007,42(9):1505-1527

Abstract— Rock magnetic properties across several K‐T boundary sections have been investigated to reveal any possible magnetic signature associated with the remains of the impact event at the end of the Cretaceous. Studied sections' locations vary in distance to the Chicxulub structure from distal (Agost and Caravaca, Spain), through closer (ODP Hole 1049A, Blake Nose, North Atlantic), to proximal (El Mimbral and La Lajilla, Mexico). A clear magnetic signature is associated with the fireball layer in the most distal sections, consisting of a sharp increase in susceptibility and saturation isothermal remanent magnetization (SIRM), and a decrease in remanence coercivity. Magnetic properties in these sections point to a distinctive ferrimagnetic phase, probably corresponding to the reported Mg‐ and Ni‐rich, highly oxidized spinels of meteoritic origin. At closer and proximal sections magnetic properties are different. Although there is an increase in susceptibility and SIRM associated with a rusty layer placed on top of the siliciclastic deposit in proximal sections, and with a similar limonitic layer on top of the spherule bed that defines the boundary at Blake Nose, the magnetic properties indicate a mixture of iron oxyhydroxides dominated by fine‐grained goethite. Based on previous geochemical studies at Blake Nose and new geochemical and PGE abundance measurements performed in this work at El Mimbral, this goethite‐rich layer can be interpreted as an effect of diagenetic remobilization and precipitation of Fe. There is not enough evidence to assert that this Fe concentration layer at proximal sections is directly related to deposition of fine meteoritic material. Magnetic, geochemical, and iridium data reject it as a primary meteoritic phase.  相似文献   

Magnetostratigraphy of the impact breccias and post‐impact carbonates from borehole Yaxcopoil‐1, Chicxulub impact crater,Yucatán,Mexico     

Mario Rebolledo‐Vieyra  Jaime Urrutia‐Fucugauchi 《Meteoritics & planetary science》2004,39(6):821-829

Abstract— We report the magnetostratigraphy of the sedimentary sequence between the impact breccias and the post‐impact carbonate sequence conducted on samples recovered by Yaxcopoil‐1 (Yax‐1). Samples of impact breccias show reverse polarities that span up to ～56 cm into the post‐impact carbonate lithologies. We correlate these breccias to those of PEMEX boreholes Yucatán‐6 and Chicxulub‐1, from which we tied our magnetostratigraphy to the radiometric age from a melt sample from the Yucatán‐6 borehole. Thin section analyses of the carbonate samples showed a significant amount of dark minerals and glass shards that we identified as the magnetic carriers; therefore, we propose that the mechanism of magnetic acquisition within the carbonate rocks for the interval studied is detrital remanent magnetism (DRM). With these samples, we constructed the scale of geomagnetic polarities where we find two polarities within the sequence, a reverse polarity event within the impact breccias and the base of the post‐impact carbonate sequence (up to 794.07 m), and a normal polarity event in the last ～20 cm of the interval studied. The polarities recorded in the sequence analyzed are interpreted to span from chron 29r to 29n, and we propose that the reverse polarity event lies within the 29r chron. The magnetostratigraphy of the sequence studied shows that the horizon at 794.11 m deep, interpreted as the K/T boundary, lies within the geomagnetic chron 29r, which contains the K/T boundary.  相似文献   

Teaching Numerical Groundwater Flow Modeling with Spreadsheets     

Gómez-Hernández  J. Jaime 《Mathematical Geosciences》2022,54(6):1121-1138

Mathematical Geosciences - The use of spreadsheets for numerical groundwater flow modeling is not a novelty; however, its potential in the classroom has not been emphasized enough. This Teachers...  相似文献   

Buried impact basins,the evolution of planetary surfaces and the Chicxulub multi‐ring crater     

Jaime Urrutia‐Fucugauchi  Ligia Perez‐Cruz 《Geology Today》2011,27(6):220-225

Impact craters are distinctive landforms on Moon, Mars, Venus and other bodies of the Solar System. In contrast, the Earth has few craters, due to the dynamic nature of the planet, where craters and other geological structures are destroyed, modified or covered. Planetary missions have also shown that in other worlds where craters are numerous and well preserved, the crater record has been modified, through the identification of buried structures. Studies of the concealed crater record have major implications for the crater‐size frequency distribution and crater‐counting chronologies. On Earth, Chicxulub is an example of a large multi‐ring buried basin. Its study provides clues for the investigation other planetary surfaces. In addition, geophysical surveys have unravelled its deep 3‐D structure, providing data and constraints for new planetary missions.  相似文献   

New evidence of sea‐level lowstands and paleoenvironment during MIS 6 and 4 in the Cantabrian coastal karst: the Cobiheru cave (North Iberia)          下载免费PDF全文

Daniel Ballesteros  Laura Rodríguez‐Rodríguez  Saúl González‐Lemos  Santiago Giralt  Diego Jaime Álvarez‐Lao  Luna Adrados  Montserrat Jiménez‐Sánchez 《地球表面变化过程与地形》2017,42(11):1704-1716

The geomorphological evolution of the Cobiheru Cave shows the influence of the non‐carbonate coastal mountain ranges on coastal karst evolution, as well as the temporal distribution of the cold‐adapted fauna sites in the Cantabrian Coast. Geomorphological observation and uranium/thorium (U/Th) dating lead to the construction of an evolution model. The model comprises two episodes of cave deposition occurring at c. 60–70 and 130–150 ka, linked to cold climate conditions, global sea‐level lowstands and the erosion of alluvial fans that covered the karst. Moreover, the comparison between the Cobiheru record and some raised beaches identified in previous studies sets the beginning of the sea‐level lowering in the Cantabrian Sea during the marine isotope stages (MIS) 5–4 transition. Two palaeoenvironments are inferred based on finding Equus ferus and Elona quimperiana. A wet deciduous forest would have developed on the emerged marine terrace of the Cobiheru Cave since at least the Middle Pleistocene, and an open landscape with scarce vegetation would have been present at c. 65 ka. The erosional event identified in the Cobiheru Cave helps to understand the temporal distribution of cold‐adapted mammals located in the Asturias region. The probable sites of cold‐adapted fauna developed in caves and alluvial fans would have disappeared after 65 ka. Therefore, palaeontological and palaeoclimate research based on cold‐adapted mammals suggests the occurrence of an hiatus in the palaeontological record prior to 50 ka. Copyright © 2017 John Wiley & Sons, Ltd.  相似文献   

Measurement and modelling evaporation for irrigated crops in north-west Mexico     

Jaime Garatuza-Payan  W. James Shuttleworth  David Encinas  David D. McNeil  John B. Stewart  Henk deBruin  Christopher Watts 《水文研究》1998,12(9):1397-1418

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Multi-platform model assessment in the Western Mediterranean Sea: impact of downscaling on the surface circulation and mesoscale activity     

Aguiar  Eva  Mourre  Baptiste  Juza  Mélanie  Reyes  Emma  Hernández-Lasheras  Jaime  Cutolo  Eugenio  Mason  Evan  Tintoré  Joaquín 《Ocean Dynamics》2020,70(2):273-288

Ocean Dynamics - In numerical ocean modeling, dynamical downscaling is the approach consisting in generating high-resolution regional simulations exploiting the information from coarser resolution...  相似文献   

Robert N. Farvolden − Pioneering contributions in Mexican hydrogeology     

Alejandra Cortes  Jaime Durazo 《Hydrogeology Journal》2000,8(2):251-253

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