Evolution of peaks in weakly non-linear density field and dark halo profiles

Using the two-point Edgeworth series up to second order in the linear rms density fluctuation we construct the weakly non-linear conditional probability distribution function for the density field around an overdense region. This requires calculating the two-point analogues of the skewness parameter S ₃. We test the dependence of the two-point skewness on distance from the peak for scale-free power spectra and Gaussian smoothing. The statistical features of such a conditional distribution are given as the values obtained within linear theory corrected by the terms that arise as a result of weakly non-linear evolution. The expected density around the peak is found to be always below the linear prediction while its dispersion is always larger than in the linear case. For large enough overdensities the weakly non-linear corrections can be more significant than the peak constraint introduced by Bardeen et al. We apply these results to the spherical model of collapse as developed by Hoffman & Shaham and find that in general the effect of weakly non-linear interactions is to decrease the scale from which a peak gathers mass and therefore also the mass itself. In the case of an open universe this results in steepening of the final profile of the virialized proto-object.     

Search for groups of extragalactic radio sources

We explore the possibility of searching for groups of radio sources from the FIRST catalog on angular scales 1′–5′. We developed an efficient method of searching for such groups that takes into account the need for combining the components of extended sources represented in the catalog by separate objects. We found 31 groups of radio sources with angular sizes <5′ that contain no fewer than five sources with flux densities ≥3 mJy. This number is at least triple the expected number of such groups for a random Poisson distribution of radio sources in the sky. The prospects for using groups of radio sources to detect and study distant systems of galaxies are discussed.     

新型土体固化剂加固海底淤泥力学特性研究

海底淤泥具有特殊的土性特点,其固化研究尚处于起步阶段。GS固化剂是一种以工业固废为主要原料的适用于软土加固的绿色固化材料。本文开展了GS固化剂加固海底淤泥的应用研究。以香港某工程海底淤泥为加固对象,对比分析了GS固化剂和水泥的掺量、龄期对固化土无侧限抗压强度的影响。研究结果表明,相比于普通水泥,GS固化土的早期强度更高、强度增长更快,强度提高比在2.03~2.91。同时,建立了回归模型,提出了GS固化剂加固海底淤泥的强度预测方法。研究成果有助于指导工业固废的资源化处置和建筑行业绿色发展。     

陕北油气田开发中水资源综合利用

通过对陕北工业用水短缺、大量污水无序排放的调查。研究了造成陕北严重缺水的原因，发现化工废水难以净化后供人们生活使用。但通过去重金属离子后可用于油田注水开发。炼油厂废水与油田产出水按不同比例混合处理后，根据不同油田储层物性进行回注采油。结果表明，处理后的污水适应于不同地质特征的产层。这即解决陕北特低渗油层注水的水敏性问题，同时也使大量污水得到充分利用，具有明显的经济效益和社会效益。     

论中国西部的经济开发

本文多方面系统地分析了中国西部地区的经济态势,从生产总值、产业结构(第一产业、工业、矿产、能源,第三产业等)以及生态环境等,论述西部的经济开发。     

产业集聚与城镇空间格局的耦合关系及时空演化——以长三角区域为例

产业集聚与城镇空间格局的变动之间存在着密切的联系。针对两者之间的耦合关系及时空演化问题,构建区域产业集聚与城镇空间格局演化综合评价指标,并利用1990—2016年长三角区域16个城市的统计数据,基于面板回归模型和空间重心模型探究两系统之间演化的互动作用关系和时空演化。结果表明：长三角区域的产业集聚与城镇空间格局间存在较显著的耦合关系;长三角区域各市区的耦合协调度及空间匹配度均稳步提升,但长三角区域耦合协调发展程度不够均衡,长三角南部的耦合协调的发展程度稍弱于长三角区域北部的发展;在近几十年的发展中,长三角北部地区逐渐形成以上海-南京为轴线的耦合协调发展区域,整个长三角区域的耦合协调则呈现“Z”字形特征。