卫星测高混合边值问题的球谐级数解法

研究了球界面下卫星测高问题的解法,利用有限逼近方法得到了下列结论：若陆地部分是球冠,则卫星测高问题的解可以转换成关于球谐级数位系数的线性方程组,并且位系数的阶和次是以分离形式出现的,从而确保该解法具有实用意义. 利用重力场360阶模型进行模拟计算的结果表明：该解法得到的位系数的相对精度达到了10－１１. 同时证明了常用的Stokes问题、Dirichlet问题、Neumann问题可以看成卫星测高问题的特殊情况.     

低地应力区地下洞室开挖围岩剪应力静态数值模拟研究

本文以西北某市大型水利地下洞室工程为例,采用弹塑性二维有限元法对低地应力区洞室开挖后围岩剪应力分布与围岩变形破坏进行了数值模拟,总结出了低地应力区地下洞室开挖后围岩剪应力大小、分布规律与围岩变形破坏的关系.该项研究它将有利于进一步研究低地应力区地下洞室开挖后围岩稳定性,同时对保障地下洞室工程的圆满进行具有重要的理论价值和现实意义.     

现代地球化学的理论思维结构

地球科学和地球化学的进展,不但加深和扩大了对地球的认识和理论成果,同时也总结提炼出了全新的科学思维方法。复杂性理论和系统思维是科学认识论的一次飞跃。现代地球化学建立了较完整的理论和方法体系,给地质科学认知地球提供了依据和支撑。作者论证了系统思维和逻辑演绎法相结合的思维方式,是研究和认识地球复杂巨系统以及推动地球科学理论创新的指导思想,并提出了运用现代地球化学理论构架和方法体系,综合地球科学系统思维与逻辑思维相结合方向的地球化学认知模型,为深入研究地球物质能量系统的行为和解决人类面临的资源、环境和灾害问题提供新的思路。     

Environmental isotopic and hydrochemical study of groundwater in the Ejina Basin,northwest China

The study investigates the groundwater evolution and its residence time in the Ejina Basin, northwest China according to isotope and hydrochemical analyses results. The groundwater chemistry is mainly controlled by the dissolution of halite, Glauber’s salt, gypsum, dolomite and calcite, also influenced by other processes such as evaporation, ion exchange, and deposition. Based on tritium content in atmospheric precipitation and by adopting a model with exponential time distribution function, the mean residence time of the unconfined aquifer groundwater with fairly high tritium activities (21–49 TU) is evaluated. The results show that these groundwaters have low residence time (5–120 years) and are renewable. In contrast, the deep confined groundwaters are tritium-free and radiocarbon values range from 18.3 to 26.7 pmc. According to the most commonly used ¹⁴C correction models, the radiocarbon groundwater ages were calculated which yield ages of approximately 4,087–9,364 years BP. Isotopic signatures indicate formation of deep confined groundwaters in a colder and wetter climate during the late Pleistocene and Holocene. It is suggested that long-term, rational water usage guide should be set up for the Heihe River Basin as a whole to permit a considerable discharge to the Ejina Basin.     

寒区有隔热层的圆形隧道温度场解析解

在多年冻土地区修建隧道,会影响到多年冻土的热稳定性,目前一般采用在隧道衬砌中设置隔热层的方法来防止冻土嗣岩融化.根据隧道现场实测的气温资料,考虑正弦曲线规律变化的对流换热边界条件,建立了一次衬砌、隔热层、二次衬砌及围岩4层结构的圆形隧道热传导方程.运用微分方程求解方法和贝塞尔特征函数的正交和展开定理,对4个热传导方程进行了求解,得到隧道一次衬砌、隔热层、二次衬砌及同岩4层结构温度场的解析解,将计算结果与现场实测结果进行比较,吻合良好.计算结果还表明,在衬砌中铺设厚5 cm、导热系数为0.03 W·m-1·℃-1的隔热层可以保证风火山隧道围岩不发生季节性融化.该解析解可用于验证其它数值方法的计算结果,也便于工程设计人员和施工人员对同类寒区隧道进行温度场的计算,因而具有一定的工程应用价值.     

冻土工程与环境研究的新进展——第八届国际冻土工程会议回顾

2009年10月在西安召开第八届国际冻土工程会议, 就冻土地区工程设计与建设、季节冻土区工程冻害防治、冻土物理力学特性、 模型发展及其应用、寒区气候、环境及冷生变化、多年冻土水文学、寒区水资源和土地应用等主要议题进行了广泛交流, 报告了近年来冻土工程与环境研究方面的一些新进展. 从冻土工程设计、施工和评价、普通冻土研究、冻土的物理力学性质、冻土模型发展及应用、 气候变化及冰冻圈环境等方面对该次会议交流的成果进行了总结. 与会研究者认为今后的研究一方面要加强理论研究、工程措施机理研究;另一方面要加强寒区环境对气候变化的响应及反馈、以及环境变化与冻土工程措施之间的相互作用研究.     

云南省东川铜矿区主要地质灾害与致损机制防控

云南省东川铜矿区因位于乌蒙山系侵蚀区和现代活动构造区,由于特殊的地形地貌、水文地质、新构造运动、植被、地层岩性和矿山开发等多因素耦合,东川铜矿区成为矿区地质灾害多发地区之一,这些诱发基本因素是矿山受损生态系统的致损机制。东川铜矿区开采历史较悠久且属于我国典型老矿山之一,由于长期的矿山开采和人类活动的影响,与本区特殊自然因素耦合等,一系列矿山地质灾害接踵而来,主要包括崩塌、滑坡、泥石流、地面塌陷、地裂缝、矿坑突水等,预防和治理矿山受损生态系统成为当前和今后首要难题之一。     

Studying the formation of massive stars with VLT/X‐shooter

The birth process and (early) evolution of massive stars is still poorly understood. Massive stars are rare, their birthplaces are hidden from view and their formation timescale is short. So far, our physical knowledge of these young massive stars has been derived from near‐IR imaging and spectroscopy, revealing populations of young OB‐type stars, some still surrounded by a (remnant?) accretion disk, others apparently “normal” main sequence stars powering H II regions. The most important spectral features of OB‐type stars are, however, located in the UV and optical range. With VLT/X‐shooter it is possible to extend the spectral coverage of these young massive stars into the optical range, to better determine their photospheric properties, to study the onset of the stellar wind, and to characterize the physical structure of the circumstellar disk (© 2011 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

X‐shooting Herbig Ae/Be stars: Accretion probed by near‐infrared He I emission

The Herbig Ae/Be stars are intermediate mass pre‐main sequence stars that bridge the gap between the low mass T Tauri stars and the Massive Young Stellar Objects. In this mass range, the acting star forming mechanism switches from magnetically controlled accretion to an as yet unknown mechanism, but which is likely to be direct disk accretion onto the star. We observed a large sample of Herbig Ae/Be stars with X‐shooter to address this issue from a multi‐wavelength perspective. It is the largest such study to date, not only because of the number of objects involved, but also because of the large wavelength coverage from the blue to the near‐infrared. This allows many accretion diagnostics to be studied simultaneously. By correlating the various properties with mass, temperature and age, we aim to determine where and whether the magnetically controlled mass accretion mechanism halts and the proposed direct disk accretion takes over. Here, we will give an overview of the background, present some observations and discuss our initial results. We will introduce a new accretion diagnostic for the research of Herbig Ae/Be stars, the HeI 1.083 μm line (© 2011 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

基于GRACE卫星测量得到的中国及其周边地区陆地水量变化

GRACE卫星成功开辟了空间大地测量对地观测的新途径。利用GRACE卫星得到的时变地球重力资料,分析估计了中国及其周边地区陆地水量的变化趋势,较为清晰地揭示了该地区季节性变化特征。进一步采用13点滑动平均的方法扣除了季节性变化,提取了4个特征区域(喜马拉雅南部,新疆与西藏及其周边的亚洲高山区域,中国华北、东北地区和中国南部地区)的陆地水量变化特征信息,这4个区域陆地水量的变化趋势分别为-12.7±0.7、-60.4±2.7、-12.5±0.5和6.6±0.9 km³/a。其中：喜马拉雅南部和亚洲高山区域陆地水量呈现明显的衰减趋势,与Matsuo和Heki模拟冰川质量损失源得到的结果较为一致;但近10年来亚洲高山区域西北部冰川加速融化趋势并不明显。中国华北、东北地区和南部地区水量变化比较复杂,具不稳定的变化趋势。