Storm surges in the northern part of the Sea of Japan

All the available historic records of sea level and appropriate weather charts have been used to study storm surges in the northern part of the Sea of Japan. The generation of surges in this area was investigated by means of a two-dimensional numerical model. Computed sea levels were compared with hourly observed residual sea levels in De-Kastri. The agreement between computed and observed storm surges is quite satisfactory. The relative importance of various meteorological parameters and bottom topography in formation of the strong storm surge on 20–21 September 1975 was studied numerically.     

筋土界面特性宏细观分析试验仪器研制与应用

为了更全面地分析筋土界面相互作用特性,改制了一台可视加筋土界面特性宏细观分析的试验仪器,可开展不同土工合成材料与填料的直剪和拉拔试验;该仪器改进了试验箱的尺寸,可方便两种试验的对比分析,增加了图像摄录系统,可进行试验过程的细观分析。使用新研制仪器分别进行了土工合成材料（土工格栅和土工布）加筋尾矿砂的直剪和拉拔试验,试验结果表明:两种试验条件下,土工格栅与尾矿的界面参数（似黏聚力和似摩擦角）及似摩擦系数均比土工布与尾矿的界面参数和似摩擦系数大;直剪试验下筋材网孔的有无对筋-尾矿界面参数均有较大影响,拉拔试验下筋材网孔有无对筋-尾矿界面参数似黏聚力的影响较为显著,对似摩擦角的影响较小。随着宏观变量法向应力的增加,细观参数孔隙率减小,平均接触数增加,反映在宏观上的现象就是填料颗粒被压密,筋材需要克服的阻力增大。该试验仪器能够较好地分析筋土界面宏细观特性,获得关键技术指标以用于加筋结构的设计。      

考虑结构性的原状黄土应力-应变关系的探讨

土体的结构是其强度、变形的内在决定因素,黄土的结构性由黄土颗粒之间的联结结构强度和摩擦结构强度所决定。由此,提出了黄土静力结构性参数即联结结构静力强度势参数m? 1、摩擦结构静力强度势参数m? 2以及结构静力强度势参数m? 。这些结构性参数具有明确的物理意义,既能反映黄土的综合结构性,又能分别反映黄土联结结构性和摩擦结构性。分析了静三轴应力条件下黄土的应力-应变特性以及黄土静力结构性参数的变化规律,建立了考虑黄土结构性的原状黄土应力-应变关系式,从而可以由结构性最弱的饱和重塑黄土的应力-应变曲线,通过结构参数模拟得到考虑结构性的原状黄土的应力-应变关系曲线。利用考虑结构性的原状黄土应力-应变关系式可整理计算出原状黄土的强度指标c、初始切线模量Ei、破坏比Rf、应力水平S以及切线弹性模量Et等参数,可应用于静荷载作用下黄土应力-应变有限元分析计算。     

环境磁学研究现状和进展

环境磁学是八十年代逐步发展起来的具有学科交叉特点的边缘学科。它主要应用岩石和矿磁学研究磁性颗粒的搬运、沉积以及转化受大气圈、水圈和岩石圈环境变化影响的过程。近年来，环境磁学已提供了大量有关全球变化过程以及人类活动对环境影响等重要资料，其研究范畴迅速扩展，已成为当今地学的前沿学科之一。     

Long-term Changes in the Saline Lake Qarun(Egypt)

正1 Introduction There is now ample evidence of the impacts of the recent climate change and anthropogenic activities on different saline lake ecosystems.All over the world salt lakes are threatened by climate change,water diversions upstream for agricultural purposes,watershed changes,introduction of aliens,etc.that result in catastrophic     

基于GPS基准站网的GPS测量

采用基于GPS基准网的GPS测量可以提高GPS测量的可靠性和准确性 ,可以消除和减小GPS测量观测值中与时间和空间相关的大气误差和轨道误差的影响 ,使中、长距离快速静态定位和RTK动态定位成为现实 ,还具有可直接得到WGS84Z坐标等优点。本文介绍基于GPS基准站网的GPS测量 ,简要地论述GPS虚拟参考站法VRS和区域改正数法FKP的原理、方法和特点 ,以及目前实施中存在的一些问题     

利用父母本微卫星标记估计大菱鲆(Scophthalmus maximus L.)幼鱼生长性状的遗传参数

The estimation of genetic parameters has played an important role in animal selective breeding for growth traits.Recently studies show that molecular markers can be incorporated into genetic evaluations. In order to improve the performance of an incomplete pedigree(i.e, only parents are known) in the genetic evaluations, 12 microsatellite markers have been applied in the estimation of the genetic parameters for body weight in a farmed population(n=1 890) of juvenile turbot(Scophthalmus maximus L.). A new relatedness called parental molecular relatedness(PMR) is estimated based on results of genotyping of 48 parents(31 males, 17 females) with microsatellites markers. The feasibility of PMR in estimation of genetic parameters is verified by comparison with pedigree related(PR) which is obtained from a complete pedigree. The results demonstrate that a high correlation(0.872) between them is found. Heritabilities are estimated using the PMR(0.52±0.13) and PR(0.55±0.22) with the same animal model. A cross-validation shows that the predictive abilities of models using the PMR and the PR are identical(0.81). From that, a conclusion can be made that PMR and PR predicted genetic values equally well in a population of juvenile turbot. Therefore PMR can be applied as an alternative of the PR when only parents are known. However, for a better performance, more markers and more families should be included in a further study.     

强夯法加固地基在青岛海关H986工程中的应用

重点介绍了在青岛海关Ｈ９８６工程中,对滨海浅滩近期回填的杂填土地基的强夯方法,并对施工中的一些问题予以分析,给出了处理办法。     

Estimates of AGN Black Hole Mass and Minimum Variability Timescale

Black hole mass is one of the fundamental physical parameters of active galactic nuclei (AGNs), for which many methods of estimation have been proposed. One set of methods assumes that the broad-line region (BLR) is gravitationally bound by the central black hole potential, so the black hole mass can be estimated from the orbital radius and the Doppler velocity. Another set of methods assumes the observed variability timescale is determined by the orbital timescale near the innermost stable orbit around the Schwarzschild black hole or the Kerr black hole, or by the characteristic timescale of the accretion disk. We collect a sample of 21 AGNs, for which the minimum variability timescales have been obtained and their black hole masses (Mσ) have been well estimated from the stellar velocity dispersion or the BLR size-luminosity relation. Using the minimum variability timescales we estimated the black hole masses for 21 objects by the three different methods, the results are denoted by Ms, Mk and Md, respectively. We compared each of them with Mσindividually and found that: (1) using the minimum variability timescale with the Kerr black hole theory leads to small differences between Mσand Mk, none exceeding one order of magnitude, and the mean difference between them is about 0.53 dex; (2) using the minimum variability timescale with the Schwarzschild black hole theory leads to somewhat larger difference between Mσand Ms: larger than one order of magnitude for 6 of the 21 sources, and the mean difference is 0.74 dex; (3) using the minimum variability timescale with the accretion disk theory leads to much larger differences between Mσand Md, for 13 of the 21 sources the differences are larger than two orders of magnitude; and the mean difference is as high as about 2.01 dex.