改进地电化学方法在矿区勘查中的试验与应用

CHIM法自提出以来,主要应用于矿产勘查的详查及异常查证阶段,其原因主要是CHIM法设备笨重、成本高、工作效率低,不适合大规模生产的需求。通过实验研究,对地电提取方法技术进行了改进——低电压“偶极子”供电方式下的CHIM。该改进方法在广西横县泰富金矿得到了较好的应用效果,在新疆金窝子-210金矿区以500m×500m 的网度进行了普查阶段的实验研究,也取得了应有的效果,表明地电提取方法不仅适用于矿产勘查的详查及异常查证阶段,而且可有效地应用于普查阶段。     

松辽盆地北部姚家组沉积特征及铀成矿条件

从基础地质条件出发,全面分析了松辽盆地北部姚家组铀成矿条件,认为该组广泛发育河流、三角洲相带,为铀成矿流体提供了疏导通道和储存空间.环绕盆地西、北、东缘的3条富铀花岗岩山脉,是良好的铀源.受燕山运动和喜马拉雅运动的影响,在挤压应力体制下形成的构造剥蚀天窗附近,是铀富集的有利区域.盆地水文地质条件较好,具备渗入型自流水盆地特征.姚家组沉积时,主要为干旱、半干旱或温热的古气候环境,有利于地层中铀的预富集或同生沉积成矿.     

The importance of interactions for mass loss from satellite galaxies in cold dark matter haloes

We investigate the importance of interactions between dark matter substructures for the mass loss they suffer whilst orbiting within a sample of high-resolution galaxy cluster mass cold dark matter (CDM) haloes formed in cosmological N -body simulations. We have defined a quantitative measure that gauges the degree to which interactions are responsible for mass loss from substructures. This measure indicates that interactions are more prominent in younger systems when compared to older more relaxed systems. We show that this is due to the increased number of encounters a satellite experiences and a higher mass fraction in satellites. This is in spite of the uniformity in the distributions of relative distances and velocities of encounters between substructures within the different host systems in our sample.
Using a simple model to relate the net force felt by a single satellite to the mass loss it suffers, we show that interactions with other satellites account for ∼30 per cent of the total mass loss experienced over its lifetime. The relation between the age of the host and the importance of interactions increases the scatter about this mean value from ∼25 per cent for the oldest to ∼45 per cent for the youngest system we have studied. We conclude that satellite interactions play a vital role in the evolution of substructure in dark matter haloes and that a significant fraction of the tidally stripped material can be attributed to these interactions.     

A Two—Temperature Supernova Fallback Disk Model for Anomalous X—ray Pulsars

We present a case study of the relevance of the radially pulsational instability of a two-temperature accretion disk around a neutron star to anomalous X-ray pulsars (AXPs). Our estimates are based on the approximation that such a neutron star disk with mass in the range of 10^-6-10^-5M⊙ is formed by supernova fallback. We derive several peculiar properties of the accretion disk instability: a narrow interval of X-ray pulse periods; lower X-ray luminosities; a period derivative and an evolution time scale. All these results are in good agreement with the observations of the AXPs.     

中国东北地区夏季旱涝的大气环流异常特征

利用东北地区均匀分布的69个测站35年(1961～1995年)夏季月平均降水资料和NCEP/NCAR 1958～1997年月平均再分析资料,对我国东北地区夏季旱涝发生的大气环流异常特征及其差异进行了诊断分析研究.结果表明,东北地区旱涝年夏季,高纬和极区大气环流特征、东北亚异常长波槽脊的分布和活跃程度、东亚大槽和西太平洋副热带高压的位置和强度等均有十分明显的差别.不仅如此,该区域夏季降水异常还显著地受到亚洲季风诸系统的影响,包括南亚季风,也包括南海季风和副热带季风,并且高空西风急流的位置和强度也有明显变化.涡度、散度、垂直速度和水汽含量等物理量特征在旱涝年不仅有截然相反的分布,而且还表现出与低纬地区存在着不同的联系方式.位于菲律宾以东洋面上行星尺度的高层辐散和低层辐合也有一定不同,并且受热带地区大气加热强度变化的影响,东北地区所在经度上的经圈环流在旱涝年也发生了明显变化,从而对该区域降水异常产生影响.     

相控阵馈源MVDR波束合成器缓解RFI仿真

相控阵馈源(Phased array feeds, PAFs)接收机作为下一代微波接收机,为大口径射电天文望远镜的射电干扰(Radio Frequency Interference, RFI)缓解工作带来了新的解决方法. PAFs接收机对射电望远镜焦平面的电磁波进行空域采样,返回时域阵列信号,使用最小方差无失真响应(Minimum Variance Distortionless Response, MVDR)波束合成器可以自适应地识别RFI的方向,同时抑制RFI在输出信号中的功率,从而达到提升射电望远镜灵敏度的效果.仿真结果表明MVDR波束合成器对有源高能量的射电干扰有很强的识别能力和一定程度的缓解能力,同时,该波束合成器对各阵元信道中加性噪声累积引起的无源干扰有很强的抑制能力,因此, PAFs接收机的MVDR波束合成器可以增强日益复杂电磁波环境下射电望远镜的抗干扰能力.     

Three dimensional numerical simulation of residential building on shrink–swell soils in response to climatic conditions

Shrink–swell soils can cause distresses in buildings, and every year, the economic loss associated with this problem is huge. This paper presents a comprehensive system for simulating the soil–foundation–building system and its response to daily weather conditions. Weather data include rainfall, solar radiation, air temperature, relative humidity, and wind speed, all of which are readily available from a local weather station or the Internet. These data are used to determine simulation flux boundary conditions. Different methods are proposed to simulate different boundary conditions: bare soil, trees, and vegetation. A coupled hydro‐mechanical stress analysis is used to simulate the volume change of shrink–swell soils due to both mechanical stress and water content variations. Coupled hydro‐mechanical stress‐jointed elements are used to simulate the interaction between the soil and the slab, and general shell elements are used to simulate structural behavior. All the models are combined into one finite element program to predict the entire system's behavior. This paper first described the theory for the simulations. A site in Arlington, Texas, is then selected to demonstrate the application of the proposed system. Simulation results are shown, and a comparison between measured and predicted movements for four footings in Arlington, Texas, over a 2‐year period is presented. Finally, a three‐dimensional simulation is made for a virtual residential building on shrink–swell soils to identify the influence of various factors. Copyright © 2015 John Wiley & Sons, Ltd.