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61.
Marcelo A. Lomeli-Banda Jorge Ramírez-Hernández Jesús Eliana Rodríguez-Burgueño Carlos Salazar-Briones 《水文研究》2021,35(2):e14013
Water agreements between Mexico and the United States have been crucial to preserving and restoring the Colorado River Delta's wetlands. Nowadays, increased water demand and climate change in the Colorado River Basin could threaten the conservation of the Ciénega de Santa Clara, a 4709 ha coastal wetland at the Sonoran Desert's edge. The international Ramsar convention recognizes the Ciénega de Santa Clara ecosystem for providing vital ecological services, including habitat for endemic, endangered, and migratory species. The hydrology of this wetland has not been completely understood since the 2010–2011 trial run of the Yuma Desalting Plant. Therefore, this study was conducted to identify and quantify the hydrological elements essential for the conservation of this wetland, under three scenarios: (a) normal inflow conditions of the water source – the Wellton-Mohawk canal; (b) inflow reductions, and; (c) an increase of temperature due to global warming. Water and mass balances estimates were conducted every month during 2014–2015; in situ measurements of inflows were carried out on Southern International Boundary in Wellton-Mohawk canal, the Riíto Drain, groundwater, and precipitation: evapotranspiration outputs were estimated using local weather stations and Penman-Monteith formulations. Temperature increases were based on the Intergovernmental Panel on Climate Change projections for the next 100 years. Results showed disconnection in the surface flow of water from the wetland to the adjacent Gulf of California. This behaviour was observed mainly in the summer months in the three scenarios. The disconnections reduced the wetland area and water storage. The hydrological functionality of the Ciénega de Santa Clara wetland depends on the water supply from the Wellton-Mohawk canal, with a minimum continuous discharge of 5.10 m3 s−1 during the summer months. 相似文献
62.
63.
Francisco Jos�� Lobo Francisco Javier Hern��ndez-Molina Fernando Bohoyo Jes��s Galindo-Zald��var Andr��s Maldonado Yasmina Martos Jos�� Rodr��guez-Fern��ndez Luis Somoza Juan Tom��s V��zquez 《Geo-Marine Letters》2011,31(5-6):451-464
Multibeam echosounder data and TOPAS seismic reflection profiles collected during the AntPac 1997, Scan 2004, and Scan 2008 cruises aboard the RV Hespérides reveal a host of surficial geomorphological features as yet poorly investigated in the Scan Basin, south-central Scotia Sea. This area represents one of the deep gateways between the Weddell Sea and the Scotia Sea, since it enables the northward flow of a branch of the Weddell Sea Deep Water (WSDW). Analysis of the data identifies numerous elongated depressions interpreted as furrows in the southernmost sector of the basin. These furrows show two main trends, i.e., either N?CNNW parallel to, or NE oblique to regional bathymetric contours. These trends plausibly reflect a tectonic influence on the bottom-flow distribution, conditioned by a set of recent, conjugate strike-slip faults that developed on the seafloor under dominant NNE?CSSW compression and orthogonal extension. The furrows exhibit distinct geomorphological patterns at either side of the basin, which can be related to west?Ceast asymmetry in the WSDW flow direction. Consistent with existing knowledge of regional WSDW dynamics, northward WSDW overflows would be channeled along the western part of the basin at higher bottom-current velocities, thereby generating more erosional-type furrows that are straighter, more elongated, and have more abrupt sidewalls than their eastern counterparts. In contrast, weaker southward WSDW would flow along the eastern part of the basin, resulting in more depositional-type furrows that are more curved, less elongated, and have gentler sidewalls. 相似文献
64.
Agricultural risk management policies under climate uncertainty 总被引:1,自引:0,他引:1
Jesús Antón Andrea Cattaneo Shingo Kimura Jussi Lankoski 《Global Environmental Change》2013,23(6):1726-1736
Climate change is forecasted to increase the variability of weather conditions and the frequency of extreme events. Due to potential adverse impacts on crop yields it will have implications for demand of agricultural risk management instruments and farmers’ adaptation strategies. Evidence on climate change impacts on crop yield variability and estimates of production risk from farm surveys in Australia, Canada and Spain, are used to analyse the policy choice between three different types of insurance (individual, area-yield and weather index) and ex post payments. The results are found to be subject to strong uncertainties and depend on the risk profile of different farmers and locations; the paper provides several insights on how to analyse these complexities. In general, area yield performs best more often across our countries and scenarios, in particular for the baseline and marginal climate change (without increases in extreme events). However, area yield can be very expensive if farmers have limited information on how climate change affects yields (misalignment in expectations), and particularly so under extreme climate change scenarios. In these more challenging cases, ex post payments perform well to increase low incomes when the risk is systemic like in Australia; Weather index performs well to reduce the welfare costs of risks when the correlation between yields and index is increased by the extreme events. The paper also analyses the robustness of different instruments in the face of limited knowledge of the probabilities of different climate change scenarios; highlighting that this added layer of uncertainty could be overcome to provide sound policy advice under uncertainties introduced by climate change. The role of providing information to farmers on impacts of climate change emerges as a crucial result of this paper as indicated by the significantly higher budgetary expenditures occurring across all instruments when farmers’ expectations are misaligned relative to actual impacts of climate change. 相似文献
65.
Isabel Márquez Josefa Masegosa Mariano Moles Jesús Varela Daniella Bettoni Giusseppe Galletta 《Astrophysics and Space Science》2003,284(2):711-714
We present the study of long slit spectra in the region ofHα emission line of a sample of 111 spiral galaxies with recognizable
and well defined spiral morphology and with a well determined environmental status, ranging from isolation to non-disruptive
interaction with satellites or companions. The form and properties of the rotation curves (RC) are considered as a function
of the isolation degree, morphological type, t, and luminosity. The line ratios are used to estimate the metallicity of all
the detected HII regions, thus producing a composite metallicity profile for different types of spirals. We have found that
isolated galaxies (ISO) tend to be of later types and lower luminosity than the interacting galaxies (INT). The outer parts
of the RC of ISO tend to be flatter than in INT, but they show similar relations between global parameters. The scatter of
the Tully-Fisher (TF) relation defined by ISO is significantly lower than that of INT. The [NII]/Hα ratios, used as a metallicity
indicator, show a clear trend between Z and t, with earlier spirals showing higher ratios; this trend is tighter when instead
of t the gradient of the inner RC, G, is used; no trend is found with the change in interaction status. The Z-gradient of
the disks depends on the type, being almost flat for early spirals, and increasing for later types. The [NII]/Hα ratios measured
for disk HII regions of INT are higher than for normal/ISO objects, even if all the galaxy families present similar distributions
of Hα Equivalent Width.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
66.
Pedro Corona-Chávez María del Sol Hernández-Bernal Pietro Vignola Rufino Lozano-Santacruz Juan Julio Morales-Contreras Margarita Reyes-Salas Jesús Solé-Viñas José F. Molina 《Chemie der Erde / Geochemistry》2018,78(2):248-253
We present the results of physical properties, petrography, bulk chemistry, mineral compositions, phase relations modelling and Noble gases study of the meteorite El Pozo. The petrography and mineral compositions indicate that the meteorite is an L5 chondrite with a low shock stage of S2-S3. Heterogenous weathering was preferentially along shock structures. Thermobarometric calculations indicate thermal equilibrium conditions between 768?°C and 925?°C at ~4 to 6?kb, which are substantially consistent with the petrological metamorphism type 5. A pseudosection phase diagram is relatively consistent with the mineral assemblage observed and PT conditions calculated. Temperature vs. fO2 diagram shows that plagioclase compositional stability is very sensitive to Tschermack substitution in orthopyroxene, clinopyroxene and XAn plagioclase during the high temperature metamorphic process. Based on noble gases He, Ne, Ar and K contents a cosmogenic exposure age CRE of 1.9?Myr was calculated. The 21Ne would be totally cosmogenic, with no primordial Ne. The 21Ne/22Ne value (0.97) is higher than solar value. According to the cosmogenic Ne content, we argue that El Pozo chondrite originally had a pre-atmospheric mass of 9–10?kg, which would have been produced by a later collision after the recognized collision of the L-chondrite parent body ~470?Ma ago. 相似文献
67.
Orenday-Tapia Edith Estefanía Pacheco-Martínez Jesús Padilla-Ceniceros Raudel López-Doncel Rubén Alfonso 《Environmental Earth Sciences》2018,77(7):286
The necessity of conserving and preserving the heritage is nowadays a developing study line for several researchers. From a civil engineering perspective, one of the most important issues for the conservation of historical buildings is to ensure the structural stability. For this purpose, it is necessary to determine the mechanical properties of the ancient construction materials. However, these structures cannot be evaluated by destructive tests due to politics and restrictions for preserving the heritage built. As a consequence, new methods that do not put in risk the integrity of the materials and the structure are becoming useful tools for researchers who work on structural engineering of heritage buildings. This paper presents a nondestructive method (NDM) that has been used to characterize the mechanical properties of different constructive systems of the San Antonio de Padua Temple, which is a religious icon in Aguascalientes, Mexico. This method includes the measuring of seismic waves’ travel time in order to obtain shear and compressional velocity waves. Results show that with this method mechanical properties of masonry can be obtained such as Young’s modulus, Poisson ratio and bulk density, which are needed for the structural analysis using numerical simulation models. 相似文献
68.
The partial pressure of CO2 (pCO2) and concentration of dissolved CH4 in surface waters have been studied in three coastal systems connected to Cadiz Bay (southwestern coast of Spain) over different time scales. The concentration of CH4 varied from 1 to 4200 nmol kg?1 (192.1 ± 463.6 nmol kg?1) and the saturation percent from 19 to 159,577% (6645 ± 16,921%), and pCO2 from 315 to 3240 μatm (841.9 ± 466.3 μatm), with saturation percent values varying between 72 and 981% (220 ± 133%). The seasonal variation of pCO2 mainly depends on the temperature. On the contrary, the annual distribution of dissolved CH4 is associated with the precipitation regime. In addition, pCO2 and dissolved CH4 showed spatial variation. pCO2 increased toward the inner part of the systems, with the proximity to the discharge points from human activities. Dissolved CH4 is influenced by both anthropogenic inputs and natural processes such as benthic supply and exchange with the adjacent salt marshes. pCO2 and dissolved CH4 also varied with the tides: The highest concentrations were measured during the ebb, which suggests that the systems export CO2 and CH4 to the Bay and adjacent Atlantic Ocean. 相似文献
69.
Georgios Etsias Gerard A. Hamill Jesús F. Águila Eric M. Benner Mark C. McDonnell Ashraf A. Ahmed Raymond Flynn 《水文研究》2021,35(4):e14120
Laboratory experiments and numerical simulations were utilized in this study to assess the impact of aquifer stratification on saltwater intrusion. Three homogeneous and six layered aquifers were investigated. Image processing algorithms facilitated the precise calculation of saltwater wedge toe length, width of the mixing zone, and angle of intrusion. It was concluded that the length of intrusion in stratified aquifers is predominantly a function of permeability contrast, total aquifer transmissivity and the number of heterogeneous layers, being positively correlated to all three. When a lower permeability layer overlays or underlays more permeable zones its mixing zone widens, while it becomes thinner for the higher permeability strata. The change in the width of the mixing zone (WMZ) is positively correlated to permeability contrast, while it applies to all strata irrespectively of their relative vertical position in the aquifer. Variations in the applied hydraulic head causes the transient widening of WMZ. These peak WMZ values are larger during saltwater retreat and are negatively correlated to the layer's permeability and distance from the aquifer's bottom. Moreover, steeper angles of intrusion are observed in cases where low permeability layers overlay more permeable strata, and milder ones in the inverse aquifer setups. The presence of a low permeability upper layer results in the confinement of the saltwater wedge in the lower part of the stratified aquifer. This occurs until a critical hydraulic head difference is applied to the system. This hydraulic gradient value was found to be a function of layer width and permeability contrast alike. 相似文献
70.
Jesús Arturo Robles-Gutiérrez Ernesto Lacomba Zamora Jesús Martiniano Arturo Robles-Domínguez Cinna Lomnitz María Eugenia Robles-Gutiérrez 《Geofísica Internacional》2013,52(2):153-157
Experimental data in fluids suggest that nonadditive electromagnetic forces between 3 or more molecules account for the existence of critical points, triple states and phase transitions (Robles-Domínguez et al., 2007; Robles-Gutiérrez et al., 2010). Similar nonadditive forces between 3 or more molecules in the gravitational field incorporated into Newton’s universal gravitational law may also explain the existence of dark matter. 相似文献