钢筋混凝土柱的破坏与能量吸收

本文根据作者所做钢筋混凝土柱的低周疲劳试验,就钢筋混凝土柱的破坏与其能量吸收之间的关系进行了分析。     

天目山龙王庙地区晚更新世沉积环境研究

本文对天目山龙王庙地剖面样品的测试分析,得出以下结论：１．古地磁揭示,该剖面主要属布容正极性世,地层年代属于Ｑ３－Ｑ。４     

考虑回水顶托影响的水位预报研究

将有回水顶托影响的河段视为多输入-单输出系统,把水位过程视为时间序列,用时间序列分析最优控制理论,建立了可考虑回水顶托影响的水位过程预报模型。提出了在棱柱形河道情况下,以时段水位涨差作变量时,模型中各参数应满足的物理性约束条件;较好地解决了长江荆江河段中受回水顶托影响的石首站的水位过程预报问题,为水位过程预报提供了一条不同于水文学途径和水力学途径的建模途径。     

潜在腾发量的随机过程特性探讨—— 一个实例研究

利用中国科学院禹城试验站的系列气象观测资料计算了逐日潜在腾发量(ETP).将日潜在腾发量系列分解为均值项和随机项两个部分,利用标准差对随机项进行了标准化处理.而后着重研究了标准化以后的随机序列的随机过程特征.首先,建立了该系列的离散的时间序列模型,然后在此基础上建立了相应的连续参数的随机模型,取得了该序列的理论概率分布密度和稳态概率分布密度,并得到了观测结果的验证,同时,还得到了该序列的自相关函数和谱密度函数的解析表达式,从而比较全面地分析了腾发量系列的随机过程特性.     

应用数字滤波消除潮位短周期波动对确定海平面变化趋势的影响

由一元线性回归分析的正则方程计算表明,在验潮记录较短的客观条件下,验潮序列中的周期波动对确定海平面变化趋势的影响是显着的.着重讨论采用数字滤波方法消除周期小于4年的短周期波动对确定海平面变化趋势的影响,并设计了最平滤波器,其通带截止频率对应的周期为4年,即应用最平滤波器对月均验潮序列进行低通滤波,基本上可消除周期小于4年的短周期波动对确定海平面变化趋势的影响.     

商洛地区金属矿产成矿系列刍议

本文以赋矿岩石建造及成矿作用为依据,将商洛地区主要金属矿产分为三个系列,24个亚系列,指出不同成矿系列相互迭加,构成各具特色的成矿带。     

热电离质谱铀系法测定碳酸盐标样

用高精度热电离质谱（ＴＩＭＳ）铀系法测定碳酸盐标样的年龄,测定结果与α谱仪铀系法进行比较,铀含量和年龄值均吻合。方法对Ｕ的回收率可达９５％,Ｔｈ为９２％。ＴＩＭＳ铀系法具有样品用量少、测试时间短、精度高的优点。     

Charts for probabilistic design of strip footings in cohesionless soils

Design charts that enable quick determination of the probability distribution parameters related to the ultimate bearing capacity of shallow foundations resting on (c = 0) soils are developed. These charts are intended to assist foundation designers and analysts in studying the reliability of structures as related to the capacity of the foundation system. The approach presented herein provides a more reliable alternative to foundation design and analysis than the current conventional design procedure which employs the assumption of an appropriate factor-of-safety. © Rapid Science Ltd. 1998     

Analysis of groundwater discharge with a lumped-parameter model, using a case study from Tajikistan

 A lumped-parameter model of groundwater balance is proposed that permits an estimate of discharge variability in comparison with the variability of recharge, by taking into account the influence of aquifer parameters. Recharge–discharge relationships are analysed with the model for cases of deterministic and stochastic recharge time-series variations. The model is applied to study the temporal variability of groundwater discharge in a river valley in the territory of Tajikistan, an independent republic in Central Asia. Received, April 1996 Revised, August 1997 Accepted, March 1998     

Asteroid Mean Elements: Higher Order and Iterative Theories

Mean orbital elements are obtained from osculating ones by removing the short periodic perturbations. Large catalogues of asteroid mean elements need to be computed, as a first step in the computation of proper elements, used to study asteroid families. The algorithms for this purpose available so far are only accurate to first order in the masses of the perturbing planet; the mean elements have satisfactory accuracy for most of the asteroid belt, but degraded accuracy in the neighbourhoods of the main mean motion resonances, especially the 2:1. We investigate a number of algorithms capable of improving this approximation; they belong to the two classes of Breiter-type methods and iterative methods. The former are obtained by applying some higher order numerical integration scheme, such as Runge–Kutta, to the differential equation whose solution is a transformation removing the fast angular variables from the equations; they can be used to compute a full second order theory, however, only if the full second order determining function is explicitly computed, and this is computationally too cumbersome for a complicated problem such as the N-body. The latter are fixed point iterative schemes, with the first order theory as an iteration step, used to compute the inverse map from mean to osculating elements; formally the method is first order, but because they implement a fixed frequency perturbation theory, they are more accurate than conventional single iteration methods; a similar method is already in use in our computation of proper from mean elements. Many of these methods are tested on a sample of asteroid orbits taken from the Themis family, up to the edge of the 2:1 resonance, and the dispersion of the values of the computed mean semimajor axis over 100 000 years is used as quality control. The results of these tests indicate that the iterative methods are superior, in this specific application, to the Breiter methods, in accuracy and reliability. This is understood as the result of the cancellations occurring between second order perturbation terms: the incomplete second order theory, resulting from the use of a Breiter method with the first order determining function only, can be less accurate than complete, fixed frequency theories of the first order. We have therefore computed new catalogues of asteroid mean and proper elements, incorporating an iterative algorithm in both steps (osculating to mean and mean to proper elements). This new data set, significantly more reliable even in the previously degraded regions of Themis and Cybele, is in the public domain. This revised version was published online in July 2006 with corrections to the Cover Date.