On the frequency contents of local events: source or path effect?

Local events which occurred in the Timanfaya volcanic field are analysed and their spectral contents are interpreted as being due to the effect of a finely layered medium with large impedance contrast, the presence of which is well known from well-logging data. By considering the layered medium as a filter, its spectral response (amplitude and phase) is computed from different randomly generated values of its parameters (total thickness, mean thickness of the individual layers and impedance contrast), showing that this stratigraphic filter acts as a low-pass filter. This effect can be correctly modelled by means of an exponential correlation function. However, in some cases resonant peaks appear in the spectrum superimposed on the low-pass filter effect, which can only be attributed to resonant scattering. An analysis of the phase and group delay associated with the amplitudes is made and strongly suggests that it is necessary to incorporate the theory of resonant scattering for the retrieval of medium properties. From the point of view of the amplitudes, the superposition of both effects, low-pass filter and resonant peaks, allows us to reproduce the gross features that are usually attributed to source effects. The need for a careful analysis of the local site response previous to any interpretation of the spectral features in terms of source characteristics is thus emphasized.     

塔克拉玛干沙漠的形成时代及发展过程

对塔克拉玛干沙漠腹地的近期研究表明，塔里木盆地虽早在白垩纪晚期已出现明显的干旱环境，但具有现代干旱特征的环境始于第三纪末，形成于第四纪初。盆地内部沙漠环境形成中更新世或其晚期。沙漠在晚更新世晚期和全新世中晚期大模型向西、西南地区和东部发展。     

Seismic codas on the Earth and the Moon: a comparison

The phenomenon of the seismic coda, which is composed of seismic energy delayed by scattering, is seen on both the Earth and the Moon. On the Moon the scattered coda is very large relative to body wave arrivals with a delay of the time of maximum energy, whereas on Earth scattered codas are relatively small and show no delay of the energy maximum. In both cases the form of the coda is controlled by three distance scales, the mean free path L, which is the average distance seismic energy travels before it is scattered, the attenuation distance $\text{x1}$, which is the average distance seismic energy travels before it is attenuated, and the source-receiver distance R. Two coda models are discussed based on these parameters; a strong scattering (diffusion) model, and a weak scattering (single scattering) model. A discussion of the diffusion scattering model indicates that if $\text{x1/L ? 1}$, diffusion scattering is an appropriate model, but if $\text{x1/L ? 1}$, single scattering is the appropriate model, within the appropriate range of R. A survey of the literature indicates that for the frequency range 0.5–10 Hz, diffusion scattering is important in lunar codas, but for the frequency range 1–25 Hz single scattering is important in terrestrial codas. Another important effect of attenuation is the elimination of scattering paths much longer than $\text{x1}$. On the Moon, this means that seismic energy in the coda can only propagate directly in the near-surface strong scattering zone between surface sources and the seismometer for source-seismometer separations of the order of $\text{(x1L)}{}^{\mathrm{<mtext>1</mtext><mtext>2</mtext>}}$; otherwise, scattering is limited to regions near the source and the receiver. On Earth, this effect probably prevents multiple scattering.     

Effects of water-soluble fractions of crude oil and dispersants on nitrate generation by sandy beach microfauna

Effects on sandy beach microfauna of soluble pollutants, such as might be associated with an oil spill, were investigated in terms of nitrate generation. Nitrate generation by the microfauna in small sand columns in the laboratory was severely inhibited by water-soluble fractions of crude oil, dispersant and oil/dispersant mixtures in order of increasing effects. Short-term effects of such pollutants on nutrient regeneration by exposed sandy beaches are discussed.     

MELIMEX,an experimental heavy metal pollution study: Effects of increased heavy metal loads on phytoplankton communities

Long-term impacts of increased metal loading (Hg, Cu, Cd, Zn and Pb) on phytoplankton communities of large limno-corrals (diameter 12 m, depth 10 m) were studied. Increased metal concentrations initially lowered phytoplankton biomass, as well as species number and photosynthetic activity of phytoplankton. They caused changes in metal speciation and shifts in phytoplankton community structure, favoring less susceptible species. Although adaptation was not sufficient to completely prevent the metal-induced depression of photosynthesis, due to depressed zooplankton grazing, at the end of the experiment even higher phytoplankton densities were observed in the metal-loaded corrals than in the control.     

Geochemistry of Karroo dolerite sills in the Calvinia district,Western Cape Province,South Africa

Two Karroo dolerite sills display chemical and mineralogical variation compatible with cumulus enrichment. The Blaauwkrans sill is an olivine tholeiite and contains a central zone slightly enriched in olivine, plagioclase and clinopyroxene. The thicker Hangnest sill is a quartz tholeiite and shows evidence of crystal settling and has a lower zone enriched in cumulus orthopyroxene and plagioclase.The two sills differ quite markedly in their trace element compositions, with the Hangnest magma enriched by a factor of two in LIL elements (Rb, Ba, Nb, Zr, Y) relative to the Blaauwkrans magma. The Hangnest magma contained extremely low Ni contents (3–5 ppm), whereas the Blaauwkrans magma contained higher but more normal Ni (100–110ppm). Such contrasting trace element compositions preclude any simple genetic relationship between the two Karroo magmas but they may be related either through a common parent or are derivatives from separate parental magmas.South African Contribution No. 24 to the International Geodynamics Project     

Tracing the anthropogenic lead sources in coastal sediments of SE-pacific (36 degrees Lat. S) using stable lead isotopes

This study evaluates the main sources of antropogenic Pb in one of the most industrialized centers of the southern Chilean coast (36 degrees S). Stable lead isotopes ((206)Pb/(207)Pb, (208)Pb/(207)Pb) were used to trace main Pb sources to coastal sediments, considering the suspended particulate matter (SPM) from marine (traps), continental (rivers) and industrial effluents, sediments and leaded gasoline samples. The atmospheric input was evaluated through natural collectors; i.e. Raqui-Tubul salt marsh. Results show that marine samples lie on a trend between industrial effluents ( approximately 1.16, 2.44) and natural sources (1.20, 2.50), not related to gasoline consumption. Salt marsh sediments show comparable isotopic composition to marine samples, suggesting the importance of the atmospheric input in the coastal sediments, not related to the leaded gasoline composition either. The continental input (1.18, 2.48) is highly influenced by precipitation, being difficult to separate both sources (atmosphere and continental runoff), showing also similar isotopic ratio to marine sediments. The signal of industrial emissions is masked with the introduction of Pb with higher isotopic ratios, compared to the values observed in the material collected from traps (SPM approximately 1.19, 2.48). The contribution of more radiogenic Pb by the upwelling is suggested.     

Evaluation of groundwater availability and sustainable extraction rate for the Upper Santiago Valley Aquifer,Chile

The use of groundwater as water supply has increased dramatically in Santiago, Chile, during the last decades, and there is a need for accurately estimating the actual groundwater supply capacity in the upper Santiago Valley aquifer. The behavior of this aquifer was studied in order to determine the availability of water and the long-range sustainable extraction rate.Water-table depths were simulated using a numerical model with information on recharge from the last 48 years under different extraction policies. With this series of groundwater level data, groundwater level probability distribution functions were determined and extraction statistics were estimated by fitting time series models and by using the crossing theory. With this information, it has been possible to calculate the risk of being unable to supply groundwater demand because the results verify that only 67% of the water rights granted are able to be extracted on a sustained basis with a 90% exceedance probability. Furthermore, the results obtained demonstrate that the method is adequate for determining exceedance probabilities of groundwater flow.

---

Resumen El uso de las aguas subterráneas como fuente de abastecimiento se ha incrementado enormemente en Santiago de Chile durante las últimas décadas, por lo que se necesita estimar de forma adecuada la capacidad actual de suministro del acuífero superior del Valle de Santiago. Se ha estudiado el comportamiento de este acuífero para determinar la disponibilidad de recursos y la tasa de extracción sustentable a largo plazo.Se ha simulado los niveles freáticos del acuífero utilizando un modelo numérico con información de la recarga en los últimos 48 años bajo diferentes regímenes de extracción. Con esta serie de datos de los niveles en el acuífero, se ha determinado la distribución de probabilidad de los niveles de las aguas subterráneas y se ha estimado las estadísticas de las extracciones mediante el ajuste de modelos de series temporales y la teoría de cruce. Con esta información, se ha podido calcular el riego de no satisfacer la demanda de abastecimiento, puesto que los resultados verifican que sólo se podría extraer el 67% de las concesiones de agua existentes de manera sustentable con un 90% de probabilidad de excedencia. Aún más, los resultados obtenidos demuestran que el método es adecuado para determinar las probabilidades de excedencia del flujo de las aguas subterráneas.

---

Resumé Lutilisation de leau souterraine pour leau potable sest considérablement accrue à Santiago (Chili) au cours des derniers lustres; cest pourquoi il est maintenant nécessaire destimer avec précision la capacité réelle dalimentation de la nappe de laquifère supérieur de la vallée de Santiago. Le fonctionnement de cet aquifère a été étudié afin de déterminer la disponibilité en eau et le taux dextraction durable à long terme.Les niveaux de la nappe ont été simulés avec un modèle numérique à partir dinformation sur la recharge au cours des 48 dernières années pour différentes politiques dextraction. A partir de cette série de données piézométriques, des fonctions de distribution de probabilité des niveaux de la nappe ont été déterminées et des statistiques dextraction ont été estimées par ajustement de modèles de séries chronologiques en utilisant la théorie du croisement. Avec ces informations, il a été possible de calculer le risque de ne pas pouvoir satisfaire la demande deau souterraine, puisque les résultats vérifient que seulement 67% des droits deau attribués peuvent être extraits sur une base durable avec une probabilité de dépassement de 90%. En outre, les résultats obtenus démontrent que la méthode est adaptée à la détermination des probabilités de dépassement de lécoulement souterrain.

     

雷暴云不同空间电荷结构数值模拟研究

利用一个三维时变双参数动力电耦合模式对决定雷暴云空间电荷结构的三个初始场：反转温度、中心最大扰动位温和扰动区域进行模拟对比研究。结果表明,选取不同的参数值,雷暴云电结构有很大差异,从而解释了在不同地区、季节、强度的雷暴云中所观测到得不同的空间电荷结构的原因。