三峡库区马家屋场-后坪滑坡成因及稳定性分析

详细介绍了三峡库区马家屋场-后坪滑坡体的特征，收集了大量软弱结构面资料，研究了各软弱结构面的组合关系，运用优势面理论，合理解释了该滑坡体的成因。采用剩余推力法，对滑坡体在各种不同工况下的稳定性作了科学分析，并对滑坡体在三蛱水库蓄水以后的稳定性作了合理预测，结果表明，滑坡体在目前状态下基本稳定，三峡水库蓄水以后，将对滑坡体稳定性产生较大影响，极有可能导致滑坡体失稳。     

Gravitational Mesoscopic Constraints in Cosmological Dark Matter Halos

We present an analysis of the behaviour of the ‘coarse-grained’ (‘mesoscopic’) rank partitioning of the mean energy of collections of particles composing virialized dark matter halos in a Λ-CDM cosmological simulation. We find evidence that rank preservation depends on halo mass, in the sense that more massive halos show more rank preservation than less massive ones. We find that the most massive halos obey Arnold’s theorem (on the ordering of the characteristic frequencies of the system) more frequently than less massive halos. This method may be useful to evaluate the coarse-graining level (minimum number of particles per energy cell) necessary to reasonably measure signatures of ‘mesoscopic’ rank orderings in a gravitational system.     

Cost Effective Frequency Ranges For Multi-Beam Dishes, Cylinders, Aperture Arrays, and Hybrids

Five out of six Square Kilometre Array (SKA) science programs need extensive surveys at frequencies below 1.4 GHz and only four need high-frequency observations. The latter ones drive to expensive high surface accuracy collecting area, while the former ask for multi-beam receiver systems and extensive post correlation processing. In this paper, we analyze the system cost of a SKA when the field-of-view (Fov) is extended from 1 deg² at 1.4 GHz to 200 deg² at 0.7 GHz for three different antenna concepts. We start our analysis by discussing the fundamental limitations and cost issues of wide-band focal plane arrays (FPA) in dishes and cylinders and of wide-band receptors in aperture arrays. We will show that a hybrid SKA in three different antenna technologies will give the highest effective sensitivity for all six key science programs.     

Cosmic and Galactic neutrino backgrounds from thermonuclear sources

We estimate energy spectra and fluxes at the Earth’s surface of the cosmic and Galactic neutrino backgrounds produced by thermonuclear reactions in stars. The extra-galactic component is obtained by combining the most recent estimates of the cosmic star formation history and the stellar initial mass function with accurate theoretical predictions of the neutrino yields all over the thermonuclear lifetime of stars of different masses. Models of the structure and evolution of the Milky Way are used to derive maps of the expected flux generated by Galactic sources as a function of sky direction. The predicted neutrino backgrounds depend only slightly on model parameters. In the relevant 50 keV–10 MeV window, the total flux of cosmic neutrinos ranges between 20 and 65 cm⁻² s⁻¹. Neutrinos reaching the Earth today have been typically emitted at redshift z2. Their energy spectrum peaks at E0.1–0.3 MeV. The energy and entropy densities of the cosmic background are negligible with respect to the thermal contribution of relic neutrinos originated in the early universe. In every sky direction, the cosmic background is outnumbered by the Galactic one, whose integrated flux amounts to 300–1000 cm⁻² s⁻¹. The emission from stars in the Galactic disk contributes more than 95% of the signal.     

Study on engineering geological stability of rock mass at Shanmen silver deposit

The natural balance conditions will be disturbed and produce a series of problems when mineral deposit has mined.This paper has researched the engineering rock masses have been researched in this study,structural planes,the distribution characteristics of tectonic geological factors and the stability of engineering structures according to the theory and research methods of rock mechanics,it will provide the engineering geological evidence for mining area exploited,meanwhile pledge the safety production.Shanmen silver deposit is a large epithermal deposit,it is controlled by NE to NNE strike faults.The stability of rock mass is acted on the tectonic movement and hot metalliferous brine in long-term.Especially,strength of rock mass becomes softened,muddy and loosed under the action of water,so the lower stability of rock mass is,the easier it can take place for harm of disaster threatening production safe of mining.For this reason,it is very important that drawing up a plan to lower harm for mine and protect.     

平面特征的多站地面激光雷达点云配准

为了进一步研究建筑物密集区域多站地面激光雷达(LiDAR)点云数据的配准问题,该文提出一种基于平面特征的地面LiDAR数据配准方法:对点云数据进行分割获取平面信息;人工选择典型的平面,对相应的点云数据进行平面拟合,得到相应法向量;利用罗德里格矩阵的性质,建立三维激光扫描数据配准模型。实验结果表明,该方法的配准精度较高、计算速度快,可以取得较好的点云配准效果。     

区域网平面平差超控外推定位技术验证

以资源三号卫星影像数据为例,基于RPC模型提出利用SRTM辅助的卫星影像区域网平面平差的方法进行超长距离控制外推,来提高无控地区的影像几何定位精度。试验表明,影像原始RPC直接定位精度含有明显的系统误差。在起算影像区域内布设一个控制点进行区域网平面平差,沿轨外推11景(491.62 km)、垂轨外推6景(282.36 km)后,相比原始影像13.335 m的平均定位精度,其外推区域影像的几何定位精度可优于7.5 m,无控区域的整体定位精度有明显提升,验证了该方法的有效性。     

数字地貌晕渲的特征增强方法研究

小比例尺DEM制作的晕渲图地形破碎,含有大量的干扰细节,不利于从宏观上把握地形的骨架。为了增强数字地貌晕渲图中的地形特征,本文利用滤波和平面曲率相组合的DEM化简方法来描述山谷和山脊区域。分别针对盆地、平原和山地三种地貌类型,采用90 m、100 m和110 m三种分辨率的DEM数据进行实验,研究发现,这三种地貌类型最佳的山脊夸张系数都为1.3,相应的山谷深化系数分别为0.4、0.6和0.8;而三种分辨率情况下山地的最佳山谷深化系数都为0.8,且山脊的夸张系数都为1.3。     

埋深对地铁车站地震反应的影响分析

关于埋深对地下结构地震反应的影响的研究对象多见于地下隧道,对地铁车站地震反应受埋深影响变化规律缺乏深入研究。本文基于ANSYS有限元软件,采用改进的简化方法建立三种不同埋深的地铁车站结构有限元模型,以两种基岩波的水平向和竖向地震动作为激励,求解各模型中地铁车站结构重要部位的地震反应。分析不同埋深时地铁车站结构惯性作用、侧面土体和上部土体三个因素对地铁车站地震反应的影响情况。分析结果表明:在双向地震作用下,地铁车站侧壁弯矩、剪力、轴力和中柱轴力随埋深的增加而增加,中柱剪力和弯矩随埋深增加而减少。埋深越深,侧面土体对地铁车站地震反应影响越大;上部土体使中柱轴力不断增加;结构自身的惯性作用对其地震反应的贡献逐渐减小。     

组构对自然休止角影响的试验研究

利用自制的模型试验装置,通过在不同方位沉积散体颗粒生成堆积体,研究不同沉积组构特征对自然休止角的影响,以及通过在母堆积体底部设置漏孔以生成子堆积体,研究堆积体内部结构对自然休止角的影响。研究发现,母堆积体休止角? 和子堆积体休止角? 随着沉积面倾角? 的增大（0° → 90°）呈现先减小后增大的趋势,子堆积体休止角? 则先增大后减小,且最小和最大值的分布区间正好互余,分别为? = 30°～45°和? = 45°～60°。当漏孔位置从左至右靠近母堆坡脚时,? 先增大后减小,? 则单调增大。基于模型的分析和推导,发现当沉积面与潜在滑动面越接近平行,休止角越小,越偏离,休止角则越大,并从细观上合理解释了?、? 和? 在特殊角度区间出现最大或最小值的原因。最后,提出了散粒堆积体的扰动分区模型,并以此为基础阐释了漏孔位置（堆积体内部结构）对休止角? 和? 的影响机制。