基于耦合场分割算法的ANSYS二次开发及其应用   总被引：2，自引：0，他引：2  

周健  孔戈  张刚  秦天 《地震工程与工程振动》2006,26(2):73-79

耦合场分割算法是当前研究的热点之一。本文首先对比研究了瞬态热传导方程和孔压增长消散方程,提出了一种适用于ANSYS二次开发的分割算法,并对2种不同的预测值计算模式对计算稳定性的影响进行了分析。然后,据之对ANSYS温度—结构耦合场模块进行了开发,形成了岩土工程有效应力计算模块。数值实验表明,这种方法具有较高的计算精度和良好的计算稳定性,并且能够充分利用现有程序资源,具有较高的工程应用价值。  相似文献   

青藏铁路沿线不同类型挡沙墙阻沙率     

杨印海  薛春晓  石龙  李凯崇  孔令伟  张芳 《中国沙漠》2020,40(1):173-178

基于风洞试验对青藏铁路沿线不同类型防沙措施防沙效果进行模拟研究,探讨了不同类型挡沙墙的防沙效果。结果表明：挂板式、轨枕式和箱式挡沙墙输沙率随高度基本呈递增缓变型趋势,最大输沙率低于20%;铃铛式和高立式聚乙烯（PE）网挡沙墙随高度呈递减陡降型趋势,距地表6~8 cm处为转折点,转折点以上输沙率随高度增大急剧减小,转折点以下输沙率随高度变化较为平缓,最大输沙率低于50%。随着风速的增大,各挡沙墙的阻沙率呈递减趋势：挂板式和轨枕式挡沙墙对风速的敏感性最弱,整体阻沙效果较优,可大范围推广;箱式挡沙墙对风速的敏感性较弱,建议在风速18 m·s^-1以下的地区使用;PE网挡沙墙防沙效果对风速的敏感性最强,建议在风速10 m·s^-1以下的地区使用。  相似文献   

利用背景噪声层析成像方法反演新疆天山及邻区S波速度结构     

孔祥艳  吴建平  刘靖 《中国地震》2021,37(1):43-58

利用新疆地震台网52个固定台站和天山地区新布设的11个流动台为期1年的观测数据,采用背景噪声层析成像方法获得了天山及邻区(41°～48°N,79°～91°E)10～50s的瑞利面波相速度分布图像,使用基于贝叶斯的马尔科夫链蒙特卡洛(MCMC)方法反演得到研究区地壳上地幔S波速度结构.研究结果表明,准噶尔盆地沉积盖层南深...  相似文献   

基于时间序列遥感数据的嵯岗国家沙化土地封禁保护成效评估     

田海静  孙涛  刘旭升  孔祥吉 《中国沙漠》2019,39(3):155-162

2013年中国启动实施了内蒙古自治区新巴尔虎左旗嵯岗国家沙化土地封禁保护区试点。本研究利用2001-2017年生长季NDVI数据分析了嵯岗封禁保护区及周边区域植被长势时空演变特征,分析了多年的生长季降水量和历年旱情,之后利用植被降水利用效率和NDVI残差趋势分析对保护成效进行了评估。结果表明:(1)封禁项目实施之前,封禁区内外植被长势变化趋势基本一致,而在项目实施后的2016、2017年,封禁区内NDVI距平明显高于封禁区外;(2)降水为影响该区域植被长势的主导气候因素,在封禁实施后的2015-2017年该区域连续3 a干旱,极大地限制了区域植被生长;(3)封禁区内植被降水利用效率和NDVI残差均呈现明显的增加趋势,而封禁区外变化不明显,说明封禁提升了植被的自我修复能力;(4)嵯岗封禁保护区由3个地块组成,其中嵯岗林场封禁效果比牧场八队和牧场十一队明显。国家沙化土地封禁保护措施有效促进了植被自我修复,提高了沙漠生态系统应对气候变化的能力。  相似文献   

Low-mass and high-mass supermassive black holes in radio-loud AGNs are spun-up in different evolution paths     

Jing Wang  Min-Zhi Kong  Shun-Fang Liu  Da-Wei Xu  Qiang Zhang  Jian-Yan Wei 《天文和天体物理学研究(英文版)》2019,(10)

How supermassive black holes(SMBHs) are spun-up is a key issue in modern astrophysics. As an extension to the study in Wang et al., here we address the issue by comparing the host galaxy properties of nearby(z 0.05) radio-selected Seyfert 2 galaxies. With the two-dimensional bulge+disk decompositions for the SDSS r-band images, we identify a dichotomy in various host galaxy properties for radio-loud SMBHs. By assuming that radio emission from the jet reflects a high SMBH spin, which stems from the well-known Blandford-Znajek mechanism of jet production, high-mass SMBHs(i.e., MBH 107.9 M⊙)have a preference for being spun-up in classical bulges, and low-mass SMBHs(i.e., MBH = 106-107 M⊙)in pseudo-bulges. This dichotomy suggests and confirms that high-mass and low-mass SMBHs are spun-up in different ways, i.e., a major "dry" merger and a secular evolution respectively.  相似文献   

Spatial optimization of rural settlement relocation by incorporating inter‐village social connections under future policy scenarios     

Dianfeng Liu  Xuesong Kong  Boyuan Zhou  Yasi Tian  Yaolin Liu  Hua Wang 《Transactions in GIS》2019,23(4):688-704

Social connections between villages can represent farmers’ interests and thus benefit participatory rural relocation planning. With rural development, however, these connections will change and may weaken the adaptation of relocation plans to future rural systems. As yet, most studies still use empirical social connections to guide relocation planning, while a few have incorporated predicted connections in the context of rural development into relocation decisions. Meanwhile, spatial optimization approaches have seldom been adopted to solve this geographical decision issue. Accordingly, our study proposes a novel spatial relocation framework that incorporates changed inter‐village social connections under future rural development scenarios. Empirical inter‐village connections and their policy‐induced changes in central China were explored using social network analysis. An integration of particle swarm optimization and geographic information systems was adopted to identify the relocation solutions with maximum inter‐village connections and maximum spatial land use compactness, and to examine how connection changes under different policy scenarios influenced relocation outcomes. The results demonstrate the significance of incorporating policy‐induced social connections into relocation plans, and most importantly, show the negative relations between changed social connections and the migration distance/direction of relocated settlements. Our study is expected to improve the adaptation of relocation plans to future rural development.  相似文献   

Analysis of types and changes of village-level economy in rural Gongyi city,Henan Province since 1990   总被引：1，自引：1，他引：0  

Jiajun Qiao  Yunfeng Kong  Xiaojian Li 《中国地理科学(英文版)》2008,18(2):101-108

Based on the research on the rural living standard in China in terms of annual net income per capita, we define six types of village-level economy, i.e. ＂to be extremely poor＂, ＂to make a basic living＂, ＂to dress warmly and eat one＇s fill＂, ＂to try to enrich （to disengage poverty）＂, ＂to be well-off＂ and ＂to be affluent＂. The data of average annual net income of all the 292 villages between 1990 and 2004 in rural Gongyi City, Henan Province were collected, verified and classified. By using standard deviation, coefficient of variation and regression analysis, it is found that the Gongyi＇s rural economy has boosted up remarkably from the relative-poverty and absolute-poverty stages in 1990 to the well-off in 2004. However, the absolute differences between villages present a trend of enlargement, while the relative differences fluctuating. On the other hand, spatial analysis of village-level economy shows that most villages with relatively high economic development level were located along national expressway and most villages with absolute-poverty lay in remote mountainous areas in 1990. Since the 1990s, the rapid urbanization and industrialization have had strongly positive effects on rural economic growth. Initial economic foundation, natural resources and traditional techniques also contribute to village economy. From the perspective of geography, villages with location advantages, such as near urban center or industrial parks, have more chances for their economic development and the ＂core-periphery＂ economic structure has been presented in the process of rural development.  相似文献   

Local Oceanic Vertical Deflection Determination with Gravity Data Along a Profile     

Jianbo Wang  Xin Liu  Yi Shen  Qiaoli Kong 《Marine Geodesy》2018,41(1):24-43

Deflections of the vertical (DOVs) over oceans cannot be directly measured, which restricts their applications. A local covariance function of anomalous potential is put forward in this paper in conjunction with the least-squares collocation (LSC) method to compute the oceanic DOVs utilization of oceanic gravity data along a profile. The covariance functions of gravity field quantities have been derived directly as functions of x, y and z without the need to introduce coordinate transformations corresponding to along- or cross-profile components. In the proposed methodology, gravity data along a profile were used to calculate the residual gravity anomaly using the remove-compute-restore technique. The residual gravity anomaly was used to calculate the parameters of the proposed covariance function of the local anomalous gravity field, which was used in the LSC to compute the residual DOVs along the profile. The residual DOVs added model DOVs to recover the DOVs along the profile. The results of a simulation experiment prove that the proposed methodology is feasible and effective.  相似文献   

A model of Saturn inferred from its measured gravitational field     

Dali Kong  Keke Zhang  Gerald Schubert  John D.Anderson 《天文和天体物理学研究(英文版)》2018,(4)

We present an interior model of Saturn with an ice-rock core,a metallic region,an outer molecular envelope and a thin transition layer between the metallic and molecular regions.The shape of Saturn’s 1 bar surface is irregular and determined fully self-consistently by the required equilibrium condition.While the ice-rock core is assumed to have a uniform density,three different equations of state are adopted for the metallic,molecular and transition regions.The Saturnian model is constrained by its known mass,its known equatorial and polar radii,and its known zonal gravitational coefficients,J_(2n),n=1,2,3.The model produces an ice-rock core with equatorial radius 0.203 R_S,where R_S is the equatorial radius of Saturn at the 1-bar pressure surface;the core densityρ_c=10388.1 kgm~(3)corresponding to 13.06 Earth masses;and an analytical expression describing the Saturnian irregular shape of the 1-bar pressure level.The model also predicts the values of the higher-order gravitational coefficients,J_8,J_10 and J_12,for the hydrostatic Saturn and suggests that Saturn’s convective dynamo operates in the metallic region approximately defined by 0.2 R_Sre0.7 R_S,where r_e denotes the equatorial radial distance from the Saturnian center of figure.  相似文献   

EUV and Magnetic Activities Associated with Type-I Solar Radio Bursts   总被引：1，自引：0，他引：1  

C. Y. Li  Y. Chen  B. Wang  G. P. Ruan  S. W. Feng  G. H. Du  X. L. Kong 《Solar physics》2017,292(6):82

Type-I bursts (i.e. noise storms) are the earliest-known type of solar radio emission at the meter wavelength. They are believed to be excited by non-thermal energetic electrons accelerated in the corona. The underlying dynamic process and exact emission mechanism still remain unresolved. Here, with a combined analysis of extreme ultraviolet (EUV), radio and photospheric magnetic field data of unprecedented quality recorded during a type-I storm on 30 July 2011, we identify a good correlation between the radio bursts and the co-spatial EUV and magnetic activities. The EUV activities manifest themselves as three major brightening stripes above a region adjacent to a compact sunspot, while the magnetic field there presents multiple moving magnetic features (MMFs) with persistent coalescence or cancelation and a morphologically similar three-part distribution. We find that the type-I intensities are correlated with those of the EUV emissions at various wavelengths with a correlation coefficient of 0.7?–?0.8. In addition, in the region between the brightening EUV stripes and the radio sources there appear consistent dynamic motions with a series of bi-directional flows, suggesting ongoing small-scale reconnection there. Mainly based on the induced connection between the magnetic motion at the photosphere and the EUV and radio activities in the corona, we suggest that the observed type-I noise storms and the EUV brightening activities are the consequence of small-scale magnetic reconnection driven by MMFs. This is in support of the original proposal made by Bentley et al. (Solar Phys. 193, 227, 2000).  相似文献