尾矿坝稳定性的可靠度分析   总被引：12，自引：2，他引：10  

张超  杨春和  徐卫亚 《岩土力学》2004,25(11):1706-1711

以极限平衡理论和传统的安全系数方法为基础,将可靠度理论引入尾矿坝稳定性分析中。通过敏感性分析和可靠度计算分析发现,尾矿材料的内摩擦角的变异性将显著地影响尾矿坝稳定性分析的可靠指标,重度的变异性对可靠指标的影响大于粘聚力的变异性的影响。简述了尾矿坝稳定性分析中利用可靠度理论的重要性,并建议在尾矿坝的可靠度分析中,将尾矿材料的抗剪强度指标c, 和重度 作为基本随机变量。  相似文献   

生物结皮恢复过程中土壤生态因子分异特征   总被引：19，自引：14，他引：5  

吴楠  张元明  张静  王红玲  聂华丽  陈荣毅 《中国沙漠》2007,27(3):397-404

对新疆古尔班通古特沙漠生物结皮恢复过程中土壤因子的动态变化进行关联性测度、方差分析、相关性分析相结合的定量研究,着重分析结皮恢复年限对土壤微生物数量、养分、盐分、土壤酶的影响,有机质与土壤盐分、pH值、土壤酶的线性关系及土壤生态因子间的相关性。结果表明：相对于土层深度,有机养分、土壤酶等生态因子与生物结皮恢复年限的联系更加紧密。结皮恢复年限对全P、全K、有机质、脲酶、真菌的影响极显著（P<0.01）;对速效P、速效K、全N、总盐、中性碱性磷酸酶、蛋白酶的影响显著(P<0.05)。随结皮恢复年限的增加,结皮层和结皮以下土层中有机养分、土壤酶均有不同程度的增加,逐步具备较高的生物学活性,沙土性状变化较快,渐渐形成抗风蚀、抗干扰能力较强的地衣苔藓结皮。结皮恢复过程中pH值与有机质呈显著线性负相关（R2＝0.701,P<0.05）,土壤盐分与有机质存在线性正相关（R2＝0.653）,但显著性不强（P>0.05）。电导率、脲酶、碱性磷酸酶、中性磷酸酶、蛋白酶与有机质存在极为显著的线性正相关（R2分别为0.888、0.993、0.958、0.948、0.911,P<0.01）,土壤生态因子的协调发展和紧密配合促进了生物结皮的恢复。  相似文献   

连续变量的自适应局部空间同位模式挖掘算法     

范协裕  陈瀚阅  刑世和 《地球信息科学学报》2016,18(7):902-909

目前,局部空间同位模式挖掘方法存在需要预设定邻域范围、挖掘的结果无统计显著性意义而难以对结论进行科学地判定等问题,如当前常用的\begin{array}{c}K\end{array}近邻方法难以确定合适的搜索圆半径,而固定距离法由于空间数据集的多尺度特性,距离阈值的设定对结果的影响较大。因此,针对连续变量的空间采样点数据集,本文提出了一种自适应局部空间同位模式挖掘算法。首先,定义了连续变量的空间同位模式兴趣度函数、模式指示器函数及Voronoi邻域,并通过构建Voronoi邻域矩阵避免了预设定邻域阈值的问题,最后采用\begin{array}{c}{G_i}^{*}\end{array}统计量进行局部空间同位模式及其区域的发现,使挖掘的结果具有统计显著性意义,进而帮助专家对挖掘结果做出更科学的判定。通过使用真实的连接了烟草适应性评价结果的耕地地力样点调查数据和水污染数据,对开发的算法进行测试。实验结果表明,算法无需预设邻域范围,可查找同区域内的不同空间同位模式。实验所发现的局部空间同位模式发现了实验数据研究区域存在的特有现象,对耕地地力调查工作具有实际的指导作用。  相似文献   

A protocol for classifying ecologically relevant marine zones,a statistical approach     

Els Verfaillie  Steven Degraer  Kristien Schelfaut  Wouter Willems  Vera Van Lancker 《Estuarine, Coastal and Shelf Science》2009

Mapping ecologically relevant zones in the marine environment has become increasingly important. Biological data are however often scarce and alternatives are being sought in optimal classifications of abiotic variables. The concept of ‘marine landscapes’ is based on a hierarchical classification of geological, hydrographic and other physical data. This approach is however subject to many assumptions and subjective decisions.  相似文献   

Inter-season and interannual variations in fish and macrocrustacean community structure on a eastern English Channel sandy beach: Influence of environmental factors     

Jonathan Selleslagh  Rachid Amara 《Estuarine, Coastal and Shelf Science》2008,77(4):721-730

The intertidal zone of an exposed sandy beach on the French coast of the English Channel was sampled with a 1.5 m beam-trawl over five years (2000 and 2003–2006) at weekly intervals. The fish and macrocrustacean catches were analysed to determine the inter-season and interannual variation in community structure and relate these variations to changes in the major environmental variables. Only six species (plaice Pleuronectes platessa, common goby Pomatoschistus microps, sprat Sprattus sprattus, sand eel Ammodytes tobianus, brown shrimp Crangon crangon and shore crab Carcinus maenas) from the 27 species captured can be considered as dominant species of the intertidal zone, and they accounted for >90% of total numbers. Most individuals caught were young-of-the-year or juvenile. Analysis of similarities (ANOSIM) and similarities percentage (SIMPER) indicated that inter-season variability of community structure (mean average similarity = 47%) was more pronounced than interannual variability (mean average similarity = 65%). Canonical correspondence analysis (CCA) indicates that a substantial component (32.2%) of the measured inter-season variation in community structure can be explained by environmental factors (mainly water temperature). The main inter-season changes in the abundance and community structure were due to the variation of the six key species and reflect the different times of their recruitment. During the five years of the study, the structure of the fish and macrocrustacean spring community persisted from year to year, with the dominant species reappearing consistently even though their abundances fluctuated from year to year. This interannual variation probably reflects variable recruitment success influenced by physico-chemical conditions. In spite of the considerable interannual variation (40 times) in the spring bloom of the prymnesiophyte alga Phaeocystis globosa we found no effect of this bloom on either fish and macrocrustacean species densities or diversity index.  相似文献   

Surface sediment diatoms from the western Pacific marginal seas and their correlation to environmental variables     

黄玥  蒋辉  Svante Bjrck  李铁刚  吕厚远  冉莉华 《中国海洋湖沼学报》2009,27(3):674-682

Diatom data of 192 surface sediment samples from the marginal seas in the western Pacific together with modern summer and winter sea surface temperature and salinity data were analyzed.The results of canonical correspondence analysis show that summer sea-surface salinity(SSS) is highly positively correlated with winter SSS and so is summer sea-surface temperature(SST) with winter SST.The correlations between SSSs and SSTs are less positively correlated,which may be due to interactions of regional current pa...  相似文献   

White dwarf + red dwarf binary systems and the period gap of cataclysmic variables     

N. F. Vojkhanskaja 《Astrophysics》2007,50(3):351-361

Cataclysmic variables (CV) and pre-cataclysmic binaries (PCB) are discussed. The main difference between them (accretion or its absence) is shown to be a consequence of the evolutionary process and the properties of their progenitors. Both types of system have a bimodal distribution of their periods, but the extrema are in counterphase. Luminosity-effective temperature diagrams for the primary components are used to show that both systems have approximately the same age, which conflicts with the notion of PCBs as precursors of CVs. Calculations of the maximum distance between components for which the system remains stable show that CVs have passed this limit, while PCBs maintain their stability during this evolution. It is suggested that, after ejecting a common shell, future CVs immediately become semi-detached systems. It this is so, then there must be cataclysmic variables which are the central stars of planetary nebulae. __________ Translated from Astrofizika, Vol. 50, No. 3, pp. 427–439 (August 2007).  相似文献   

Outbursts of EX Hydrae revisited     

N. Mhlahlo  D. A. H. Buckley  V. S. Dhillon  S. B. Potter  B. Warner  P. A. Woudt 《Monthly notices of the Royal Astronomical Society》2007,380(1):353-364

  相似文献   

The space density of cataclysmic variables: constraints from the ROSAT North Ecliptic Pole survey     

M. L. Pretorius  C. Knigge  D. O'Donoghue  J. P. Henry  I. M. Gioia  C. R. Mullis 《Monthly notices of the Royal Astronomical Society》2007,382(3):1279-1288

We use the ROSAT North Ecliptic Pole (NEP) survey to construct a small, but purely X-ray flux-limited sample of cataclysmic variable stars (CVs). The sample includes only four systems, two of which (RX J1715.6+6856 and RX J1831.7+6511) are new discoveries. We present time-resolved spectroscopy of the new CVs and measure orbital periods of 1.64 ± 0.02 and 4.01 ± 0.03 h for RX J1715.6+6856 and RX J1831.7+6511, respectively. We also estimate distances for all the CVs in our sample, based mainly on their apparent brightness in the infrared. The space density of the CV population represented by our small sample is  1.1^+2.3_−0.7× 10⁻⁵ pc⁻³  . We can also place upper limits on the space density of any subpopulation of CVs too faint to be included in the NEP survey. In particular, we show that if the overall space density of CVs is as high as  2 × 10⁻⁴ pc⁻³  (as has been predicted theoretically), the vast majority of CVs must be fainter than   L _X≃ 2 × 10²⁹ erg s⁻¹  .  相似文献   

The population of AM CVn stars from the Sloan Digital Sky Survey     

G. H. A. Roelofs  G. Nelemans  P. J. Groot 《Monthly notices of the Royal Astronomical Society》2007,382(2):685-692

The AM Canum Venaticorum (AM CVn) stars are rare interacting white dwarf binaries, whose formation and evolution are still poorly known. The Sloan Digital Sky Survey provides, for the first time, a sample of six AM CVn stars (out of a total population of 18) that are sufficiently homogeneous that we can start to study the population in some detail.
We use the Sloan sample to 'calibrate' theoretical population synthesis models for the space density of AM CVn stars. We consider optimistic and pessimistic models for different theoretical formation channels, which yield predictions for the local space density that are more than two orders of magnitude apart. When calibrated with the observations, all models give a local space density  ρ₀= 1–3 × 10⁻⁶ pc⁻³  , which is lower than expected.
We discuss the implications for the formation of AM CVn stars, and conclude that at least one of the dominant formation channels (the double-degenerate channel) has to be suppressed relative to the optimistic models. In the framework of the current models this suggests that the mass transfer between white dwarfs usually cannot be stabilized. We furthermore discuss evolutionary effects that have so far not been considered in population synthesis models, but which could be of influence for the observed population. We finish by remarking that, with our lower space density, the expected number of Galactic AM CVn stars resolvable by gravitational-wave detectors like the Laser Interferometer Space Antenna ( LISA ) should be lowered from current estimates, to about 1000 for a mission duration of 1 yr.  相似文献