Ephemeral stream chemistry below the elevation of near‐zero net infiltration          下载免费PDF全文

Omar M. Al‐Qudah  Arturo Woocay  John C. Walton 《水文研究》2015,29(10):2385-2401

Stormwater along ephemeral arroyos and areal infiltration in nearby boreholes were studied in the Amargosa Desert Region of Southern Nevada, USA. Chemical composition of ephemeral stream runoff was measured at elevations below where areal infiltration generally occurs in arid environments using lysimeters designed for this study. Borehole cuttings from several wells were evaluated in terms of chloride migration. Analysis of the borehole data indicates that net areal infiltration has been insignificant for the past 10 000+ years. This is associated with an environment where chloride and other soluble salts accumulate in shallow sediments and potentially in runoff waters. Measured storm events during the 4‐year study period were small and localized but sufficient to produce surface runoff, at least near the lysimeters. Composition of storm runoff captured by the lysimeters was found to be a combination of the water chemistry types found in precipitation and from leaching tests of near‐surface sediments. All major cations and bicarbonate increased relative to chloride when precipitation interacted with sediments to form ephemeral stream runoff. The changes were consistent with calculated saturation indices. Despite the long‐term accumulation of chloride in soils and deep sediments caused by complete evapotranspiration of infiltrating precipitation, runoff waters were characterized by low chloride and total dissolved solids. This study presents a limitation of the chloride mass‐balance method, as chloride and water migration were disassociated from each other in the study area. Copyright © 2014 John Wiley & Sons, Ltd.  相似文献   

The Local Group Census: searching for planetary nebulae in IC 1613, WLM and GR8     

L. Magrini  R. L. M. Corradi  R. Greimel  P. Leisy  A. Mampaso  M. Perinotto  J. R. Walsh  N. A. Walton  A. A. Zijlstra  D. Minniti  M. Mora 《Monthly notices of the Royal Astronomical Society》2005,361(2):517-524

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The quality factor of oscillating bubbles as an indication of gas content with particular reference to methane     

Walton  A.J. Gunn  M.G. Reynolds  G.T. 《Oceanic Engineering, IEEE Journal of》2005,30(4):924-926

There has been much interest in detecting the presence of methane gas in the ocean. Although methane exists predominantly as methane hydrate (a buoyant compound) in the deep ocean, recent computer simulations and anecdotal evidence have reported that these hydrates will decompose to produce methane bubbles in shallower waters. This paper describes how the quality factor Q of oscillating bubbles can be used to distinguish methane bubbles (Q=24) from the air bubbles (Q=34) which are ubiquitous near the ocean surface. Values of Q are reported for bubbles in water at atmospheric pressure containing air, carbon dioxide, argon, helium, methane and butane. Possible acoustic techniques for detecting and sizing methane bubbles in the ocean are discussed briefly.  相似文献   

Shoreline change at an infinite jetty for wave time series     

Todd L. Walton Jr.  Robert G. Dean 《Continental Shelf Research》2011,31(14):1474-1480

Future shoreline changes on a sandy beach with a structure such as a jetty or groin can be estimated when wave time series is known (i.e. sequence of wave height, period, and direction). This paper presents an extension of an existing solution (Pelnard-Considere, 1956) for the linearized partial differential equation for shoreline change at an infinite jetty where waves are time varying and when the angle of the shoreline is small with respect to the waves breaking at the shoreline. The novel solution provided in this paper allows the previous constant wave condition solution to be extended to the case where wave properties (i.e. wave direction, wave height, and wave period) are time varying. Example usage of the method presented shows that shorelines may be of different final plan form shape for time varying wave conditions even though the sediment transport along adjacent beaches is not spatially varying (i.e. spatially constant) from time step to time step. Although this difference in shape may have been known previously using numerical models, it could not be proved analytically. Reversals of wave height, period, and direction time series are shown to provide different final shoreline shapes even though the time series consists of the same waves although in different ordered time. The solution provided will allow one line numerical shoreline models to be tested using an analytic solution.  相似文献   

The journal of 'ground water': in the beginning     

Walton WC 《Ground water》2003,41(1):100-101

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Secondary Effects of Soil Venting and Potential Low-Cost Enhancements     

John C. Walton  Charles B. Anker 《Ground Water Monitoring & Remediation》1996,16(3):91-97

Soil venting, in addition to removing volatile organic compounds, has secondary effects on soil temprature and moisture content. A simple enthalpy balance model is used to illustrate the maganitude and direction of temperature and moisture content changes in the soil during ordinary venting and with several potential modifications to venting. Because of the importance of latent heat of vaporization, injection of warm, dry air into the substance is generally ineffective in heating the soil. In contrast, injection of humidified, slightly heated air is found to result in significant soil warming even at low flow rates. Soil warming is thought to be an important mechanism for enhancing remediation, particularly in the final or tail stage of cleanup where concentrations slowly decline wiht time. A variety of soil venting alternatives are simulated at hypothetical sites in Chicago, Illinois, and Tucson, Arizona, including simple humidification, humidification with solar heating, and venting under positive pressure. All there methods result in higher final soil temperatures than the control case of normal soil venting. Humidification of the input air at the rates applied does not result in significant change in average soil moisture content or saturation of the soil wtih water.  相似文献   

Comprehensive Analysis of Water-Table Aquifer Test Data     

William C. Walton 《Ground water》1978,16(5):311-317

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Effects of temperature and pressure on frost heaving     

E. Penner  T. Walton 《Engineering Geology》1979,13(1-4):29-39

Concerning the influence of overburden pressure on the relation between rate of heave and cold-side temperature, studies show that the heave rate for various overburden pressures tends to converge as the cold-side temperature is lowered, and the maximum rates of ice accumulation at low pressures occur at temperatures closer to 0°C than do those at high pressures. Evidence is also presented that aheaving zone is involved in frost action rather than a freezing plane. This zone extends over an increasingly greater temperature range and distance as the overburden pressure is increased. Using the concept of a heaving zone leads to a method for calculating the heave-decrease curve. The period of heave decrease is marked by a rapidly increasing ice segregation ratio and a reduced frostpenetration rate.  相似文献   

Inert gases in a terra sample: measurements in six grain-size fractions and two single particles from Luna 20     

D Heymann  S Lakatos  J.R Walton 《Geochimica et cosmochimica acta》1973,37(4):875-885

The inert gases have been measured in six size fractions covering the range below 500 μm, in a single feldspathic fragment weighing 523 μg, and in an agglutinate particle weighing 465 μg. The two size fractions between 125 and 250 μm as well as 250 and 500 μm were separated into magnetic and non-magnetic portions, which were measured separately. Like the Apollo and Luna 16 fines, the terra fines represented by Luna 20 are very rich in trapped solar-wind gases, but they contain relatively less He⁴ and Ne²⁰, which is revealed by their average $\text{He}{}^4\text{Ne}{}^{20}$ ratio of 35 and $\text{Ne}{}^{20}\text{Ar}{}^{36}$ ratio of 2.9. Obviously the terra materials are less retentive for solar-wind He and Ne than typical mare fines such as 10084. Whether this is due to the relatively small TiO₂ or the relatively large plagioclase content of the former is not resolved. ($\text{Ar}{}^{36}\text{Kr}{}^{84}\text{)}{}_{\mathrm{trapped}}$ and ($\text{Ar}{}^{36}\text{Xe}{}^{132}\text{)}{}_{\mathrm{trapped}}$ ratios are relatively large; the average values are 2800 and 14400, respectively. The apparent Ne²¹ radiation ages of all the size fractions are in the range 209–286 × 10⁶ yr; the average is 260 × 10⁶ yr. This is in the range of values known for the Apollo and Luna 16 fines. The feldspathic fragment has a much greater apparent Ne_c²¹ age of 780 × 10⁶ yr. The Ar⁴⁰-Ar³⁶ systematic reveals the presence of two Ar⁴⁰ components, because Ar⁴⁰ = (1.41 ± 0.076)Ar³⁶ + (0.490 ± 0.130) × 10^?4 (cm³ STP/g). The $\text{Ar}{}^{40}\text{Ar}{}^{36}$ slope of 1.41 is not inconsistent with an origin of the sample from a relatively old terra region.  相似文献   

Hydrogeologic Aspects of the International Hydrological Decade     

W. C. Walton Member NWWA 《Ground water》1966,4(4):36-47

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