EDAPHIC PROPERTIES AND FOLIAR ELEMENTAL CONCENTRATIONS FROM SAND PINE (PINUS CLAUSA) POPULATIONS THROUGHOUT FLORIDA

Soil physical and chemical properties, plus foliar elemental concentrations, are reported for surface (5–10 cm) and subsurface (35–40 cm) soil and foliar tissue samples from 20 sand pine (Pinus clausa) populations, 9 from the Choctawhatchee variety on the Florida panhandle and 11 from the Ocala variety on the Florida peninsula. Sand pine occurred exclusively on sandy soils, with mean sand content >97%. Soils generally were low in organic carbon and soil elemental concentrations. Both K and P were below analytic detection limits, whereas Ca and Mg were present at only modest levels. Only soil Al and Fe were relatively abundant. Foliar elemental concentrations indicated pronounced bioconcentration of nutrients by sand pine. Macronutrients (Ca, K, Mg, and P) approached or exceeded levels typical of other southern pine species. Some contrasts in edaphic and foliar tissue properties were apparent between varieties, but contrasts were more pronounced between groups of populations based on both soil color (yellow-sand group) and variety (Choctawhatchee white-sand and Ocala white-sand groups). The yellow-sand group, dominated by inland Choctawhatchee sites on sediments of mixed marine/fluvial origin, possessed less well sorted sand grains, higher clay content, lower pH, and higher levels of soil Al and Fe. The Choctawhatchee white-sand group consisted primarily of coastal dune sites, with well-sorted sands that reflect an eolian substrate. The Ocala white-sand group ranged primarily along the interior sand ridges of central Florida and was intermediate in sedimentological character. Foliar elemental concentrations did not reflect soil elemental patterns. Whereas Ocala samples were significantly higher in P and Mg, Choctawhatchee samples were higher in K, and there were no signficant varietal differences in foliar Ca. [Key words: sand pine, soil elemental concentrations, foliar elemental concentrations, Florida.]     

Effects of chemical dispersants and mineral fines on crude oil dispersion in a wave tank under breaking waves

The interaction of chemical dispersants and suspended sediments with crude oil influences the fate and transport of oil spills in coastal waters. A wave tank study was conducted to investigate the effects of chemical dispersants and mineral fines on the dispersion of oil and the formation of oil-mineral-aggregates (OMAs) in natural seawater. Results of ultraviolet spectrofluorometry and gas chromatography flame ionized detection analysis indicated that dispersants and mineral fines, alone and in combination, enhanced the dispersion of oil into the water column. Measurements taken with a laser in situ scattering and transmissometer (LISST-100X) showed that the presence of mineral fines increased the total concentration of the suspended particles from 4 to 10microl l(-1), whereas the presence of dispersants decreased the particle size (mass mean diameter) of OMAs from 50 to 10microm. Observation with an epifluorescence microscope indicated that the presence of dispersants, mineral fines, or both in combination significantly increased the number of particles dispersed into the water.     

Provenance of the HP–HT subducted margin in the Variscan belt (Cabo Ortegal Complex,NW Iberian Massif)

The Variscan Upper Allochthon is a continental‐affinity terrane that recorded a Cambrian–Ediacaran magmatic arc generation, a subsequent transition to a passive margin, and a collision‐related high‐P metamorphism during the Devonian–Carboniferous amalgamation of Pangea. The objective of this article is to decipher which continental margin subducted in the Devonian high‐P–high‐T (HP–HT) event. To do so, a provenance study is presented using combined U–Pb (n = 613) and Lu–Hf (n = 463) isotopic LA–ICP–MS zircon analyses and Sm–Nd whole–rock (n = 5) determinations. These analyses have been performed on five samples of the Banded Gneisses (Cabo Ortegal Complex, NW Iberia), which forms a part of the HP–HT bottom member of the Upper Allochthon. Palaeozoic–Neoproterozoic zircon ages (34.7%) have a maximum abundance at 522–512 Ma, peaks at 575, 561, 545 Ma and minor abundance peaks between 780 and 590 Ma, and show from their Lu–Hf compositions a volcanic arc mixing pattern. This arc was probably related to the Cadomian arc system. The Mesoproterozoic population is scarce and scattered (2.8%), and due to its Lu–Hf pattern, it is proposed that this population is also West Africa Craton derived. The Paleoproterozoic population (39.6%) is concentrated at 2.07 Ga and it is linked to the Eburnean Orogeny, where depleted mantle derived magmas intruded an Archean craton margin. This craton is represented by the Archean population (22.8%), which is grouped at 3.0, 2.68‐2.61 and 2.52‐2.48 Ga, and shows long‐term reworking processes and at least two juvenile magma intrusions. These data show that the Variscan Upper Allochthon has a West African provenance and therefore, it strongly suggests that the NW Iberian allochthonous complexes and their correlative European terranes are also West Africa derived. These results allow us to finally clarify that the first high‐P event, recorded during the eo‐Variscan amalgamation of Pangea, was attained by the subduction of the margin of Gondwana under Laurussia.     

Alpine climate during the Holocene: a comparison between records of glaciers,lake sediments and solar activity

The European Alps are very sensitive and vulnerable to climate change. Recent improvements in Alpine glacier length records and climate reconstructions from annually laminated sediments of Alpine Lake Silvaplana give the opportunity to investigate the relationship between these two data sets of Alpine climate. Two different time frames are considered: the last 500–1000 years as well as the last 7400 years. First, we found good agreement between the two different climate archives during the past millennium: mass accumulation rates and biogenic silica concentration are largely in phase with the glacier length changes of Mer de Glace and Unterer Grindelwaldgletscher, and with the records of glacier length of Grosser Aletschgletscher and Gornergletscher. Secondly, the records are compared with temporally highly resolved data of solar activity. The Sun has had a major impact on the Alpine climate variations in the long term, i.e. several centuries to millennia. Solar activity varies with the Hallstatt periodicity of about 2000 years. Hallstatt minima are identified around 500, 2500 and 5000 a. Around these times grand solar minima (such as the Maunder Minimum) occurred in clusters coinciding with colder Alpine climate expressed by glacier advances. During the Hallstatt maxima around 0, 2000 and 4500 a, the Alpine glaciers generally retreated, indicating a warmer climate. This is supported by archaeological findings at Schnidejoch, a transalpine pass in Switzerland that was only accessible when glaciers had retreated. On shorter timescales, however, the influence of the Sun cannot be as easily detected in Alpine climate change, indicating that in addition to solar forcing, volcanic influence and internal climate variations have played an important role. Copyright © 2011 John Wiley & Sons, Ltd.     

From ambient noise recordings to site effect assessment: The case study of Barcelona microzonation

As local site effects have a drastic influence on seismic hazard, it is a major issue to characterize them in vulnerable areas such as highly urbanized zones, like Barcelona city. The aim of this work is to improve the knowledge of geophysical characteristics of Barcelona in the perspective of a seismic microzonation that takes into account site effect. The first step was to gather the existing data from geological, geotechnical, geophysical, and seismological investigations, bringing us to keep the four zones proposed by previous work as a base of zonation. The second step was to characterize each zone by time-averaged shear-wave velocity and fundamental resonance frequency, with ambient noise techniques over 17 sites, providing new knowledge about the soil of Barcelona. The third step was to propose an amplification function between an average soil for each zone and a standard reference rock site, using empirically based propositions and to compare them to previous numerical approaches.     

基于井下摆天然地震数据测量首都圈近地表波速结构

收集了首都圈数字化地震遥测台网58个井下摆2003-2008年记录的102次M≥3.0地震的数据.通过鉴别直达波及对应地表反射波的波形,发现两者到时差与震中矩和方位角无关.基于斯涅尔定律,分析获得了这些台站上方厚约300 m浅地表土层P波和S波平均速度结构以及波速比.结果表明,首都圈区域近地表P波和S波平均速度分别约为...     

Oxygen stable isotope fractionation behavior of cerussite and hydrocerussite: New results and reconciliation of the recent literature

Recent empirical and theoretical calculations of the temperature-dependant oxygen stable isotope fractionation behavior of cerussite have highlighted potential problems with earlier work on this topic. The synthetic cerussite which was used earlier by the lead author to determine fractionation factors was re-examined using energy dispersive X-ray analysis, and found to be internally contaminated with inclusions of the phase hydrocerussite at levels of 5-10% by volume. The volume of hydrocerussite present within the samples is not sufficient to explain the entire discrepancy between this work and the empirical and theoretical calculations made earlier by the second author of this paper. Regardless of the exact causes of experimental failure or kinetic effects, the hydrocerussite contamination and the difficulty of demonstrating that these experiments reached isotopic equilibrium suggest that the use of cerussite oxygen isotope fractionation factors determined by slow precipitation experiments be discontinued in favor of the empirically calibrated fractionation factor 1000 ln α_{cerussite-water} = 2.29(10⁶/T²) − 3.56. In addition, we have determined that the oxygen isotope fractionation factor between hydrocerussite and water at 20 °C is 1.0232.     

一种改进的极大验后估计序列超分辨率重建算法

提出一种基于极大验后估计(MAP)超分辨率重建算法的新的改进算法.该算法将MAP算法或其他超分辨率重建算法所获得的高分辨率影像引入到MAP算法中,主要思想是基于所求取的分辨率应该与理想的高分辨率影像最大相关的原理.最后采取基于灰度的四参数仿射变换模型的配准算法,采用共轭梯度算法来迭代求解超分辨率重建方程.仿真试验证明,...     

赤水地区下三叠统嘉陵江组嘉二1——嘉一段有利储层研究

贵州省赤水地区下三叠统嘉陵江组的沉积相属于陆表海碳酸盐台地沉积,嘉二1-嘉一层段储层岩性主要为颗粒灰岩、粉晶白云岩.有利储层为裂缝-孔隙型,并具有低孔、低渗的特点,有利储产层的发育须要构造裂缝的连通.宝元构造为嘉二1～嘉一有利储层发育的最有利区,旺隆构造为嘉二1～嘉一有利储层发育的次有利区,太和构造为嘉二1～嘉一有利储层发育的差有利区.     

自动气象站监测运行能力可靠性评估

自动气象站运行能力的评估,其实质就是对自动气象站可靠性的评估,其目的在于指导自动气象站保障维护体系的建立和健全.借鉴大气透明度定义探讨自动气象站可靠性,解释产品可靠性指数分布的物理意义.根据模型统计分析在修改采集器设计、增加状态检测电路后自动气象站的运行能力(平均无故障时间),计算出实验考核指标.通过试验获得试验产品的平均无故障时间和置信度0.95下的最小无故障时间,并对将投入业务使用的双套站和三套站系统,在平均无故障时间和平均维修周期上做了相关讨论,为科学决策提供相关技术支持.