近10年北京经济职能的发展变化

利用北京1992年、1997年和2002年投入产出表信息,根据净输出判断城市基本部门,采用主成分-因子分析等方法辨识产业群,借此分析了北京近10年间的经济功能变化。电子和信息产业群、医药产业群是北京第三功能优势和科技优势与第二产业的结合而发展的基本部门群。造纸及文教用品、家具制造业与高级服务业也形成了一个关联较密切的产业群。资源环境条件对北京的产业发展产生了一定的约束,但钢铁和机械工业群与石油加工和化学工业群中核心产业的发展却出现了相反的趋势,后者利用已有基础和相对有利的微观区位获得了明显的发展。本文尝试性地提出了“基本部门群”的概念,即核心产业为城市基本部门的产业群。     

地下水降深的未确知风险分析

地下水资源系统具有未确知性特征。在定义水文地质未确知参数的基础上,运用未确知数学理论建立了地下水位下降量预测的未确知数学模型。根据该模型不仅可以得到地下水位下降量的可能取值区间,也能够得到相应区间的主观可信度分布。通过将地下水位下降量超过某一给定限值定义为未确知事件,又建立了度量这一事件发生可能性的未确知可靠性计算模型。实例研究表明,所建模型对地下水降深风险的可靠性分析具有很好的适用性,研究成果有效地弥补了以往确定性模型的不足。     

基于缓解沙漠高速公路风沙危害的路基参数优化——以榆靖高速公路为例

在沙漠地区修筑高速公路时,风沙对公路路基的危害是公路安全和运营的最大影响因子之一。为了寻求最适合沙漠地区高速公路风沙危害最经济的理论路基断面形式,通过对榆（林）靖（边）沙漠高速公路各种路基实测数据应用数学模型进行定量分析,查明了影响路基沙害程度的主要参数,提出了减少路基沙害程度的设计理念,并对不同路基形式的沙害程度进行了比较,给出了路基沙害程度较小的路基断面形式及参数值。研究成果对今后在沙漠地区修筑高速公路设计及施工具有一定的指导意义。     

The value of the superstring tension and dark matter

We start from our extended scenario for the formation of astronomical objects from fragmenting macroscopic superstrings, and we combine it with our view of an “orderly” fragmentation applied to the formation of black holes (Brosche, Lentes & Tassie 2003), now to the whole objects: the radial order of the matter should be preserved. Then we have to adapt the value of the superstring tension derived from the observed ratios of κ = (angular momentum)/(mass squared). If we calculate potential energies on the basis of a fragmentation until baryonic elementary particles, it turns out that the changed string tension explains as well the mechanical state of observed astronomical objects (without large energy loss on the way from the parent string parts) as also the fraction of bound to unbound matter (about 1:10). The implied superstring tension is about μ = (1/3000) c ²/G . This corresponds to a string tension of 4 × 10⁴⁰ Newton. (© 2006 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

New observations,photometric study and preliminary elements of the W UMa system DF CVn

CCD (V) light curve of the EW‐type eclipsing variable DF CVn was obtained during seven nights in April–May, 2004. With our data we were able to determine 4 new times of minimum light. The light curve appears to exhibit a typical O'Connell effect, with Maximum I brighter than Maximum II by 0.013 mag. in V. TwoWilson‐Devinney (WD) code working sessions, using the V light curve, were done with and without spots. The analysis of the results shows that the best fit was obtained with the spotted solution and indicates contact geometry. The photometric mass ratio of the system is found to be q = 0.347 and its inclination i = 72°, the primary minimum shows a transit. The star may be classified as an A‐type W Uma system. Assuming a reasonable value for the mass of the primary component an estimate of the absolute elements of DF CVn has been made, with the assumption that the primary has a mass corresponding to its spectral type according to Straizys and Kuriliene (1981). (© 2005 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Assessment of generation temperatures of crude oils

Biological marker maturity parameters were used to estimate the minimum HC generation temperatures of crude oils from Eastern Hungary. More than 50 oils and oil shows were analysed. Molecular- and homologous-ratios of biological marker compounds (triterpanes, steranes, mono- and triaromatic steroid hydrocarbons) were used as maturation parameters. The oils have at least five maturity stages, i.e. they have been generated under different thermal conditions. The highest reservoir temperature in each group was chosen as the best estimate of the groups' temperature just below the generation temperature, i.e. reservoirs of the group might be expected to be at shallower depths (lower temperatures) than those of the generation zone due to vertical migration into pools. For each maturation level, a threshold temperature range for genesis was inferred from reservoir temperatures; they are from 130–135°C for the least mature oils to 210–215°C for the most mature oils. In the least mature oils cracking was not observed, hence carbon–carbon cracking reactions had not taken place during their genesis. The most mature oils are intensively cracked oils; they are almost condensates. Two major genetic groups (families) of oils were found in the area. Both are present in each maturation level. The effects of migration were checked, and no influence on maturation was found. A number of the oils are in overpressured reservoirs within, or just above, the zone of the present-day active oil generation, hence the present-day temperatures of the pools must have been maximum temperatures. Contrary to the traditionally accepted temperature range for petroleum generation–maturation reactions (50–150°C), there is strong evidence from this study that the onset of oil generation requires temperatures higher than 130°C and is still proceeding above 215°C.     

WGMD—1型高密度电阻率测量系统比值参数软件的开发与应用

高密度电阻率法测量中的比值视参数是近几年发展起来的高密度电阻率处理与解释参数,它们具有更好的横向、纵向分辨率以及抑制干扰等作用,介绍了适合于ＷＧＭＤ－１型高密度电阻率法测量系统的幽会参数软件的编制及其在工程勘测中的应用实例,实践证明,这是一组质量高,误差小,方便实用的组合参数,可广泛的用于工程勘测中。     

采油生产设备动力特性试验研究

本文通过脉动试验识别了采油生产设备的模态参数。     

调质阻尼器地震反应控制应用研究

本文在结构地震反应时程分析基础上,研究调质阻尼器控制地震反应的最优参数设计方法,分析了多自由度体系的阻尼器设计以及调质阻尼器控制的失调效应．并用算例验证了该设计方法用于地震反应控制的可行性。