Paleoproterozoic accretion in the Northeast Siberian craton: Isotopic dating of the Anabar collision system   总被引：1，自引：0，他引：1  

O. M. Rosen  L. K. Levskii  D. Z. Zhuravlev  A. Ya. Rotman  Z. V. Spetsius  A. F. Makeev  N. N. Zinchuk  A. V. Manakov  V. P. Serenko 《Stratigraphy and Geological Correlation》2006,14(6):581-601

Geochronological database considered in the work and characterizing the Anabar collision system in the Northeast Siberian craton includes coordinated results of Sm-Nd and Rb-Sr dating of samples from crustal xenoliths in kimberlites, deep drill holes, and bedrock outcrops. As is inferred, collision developed in three stages dated at 2200–2100, 1940–1760, and 1710–1630 Ma. The age of 2000–1960 Ma is established for substratum of mafic rocks, which probably originated during the lower crust interaction with asthenosphere due to the local collapse of the collision prism. Comparison of Sm-Nd and Rb-Sr isochron dates shows that the system cooling from ≈700 to ≈300°C lasted approximately 300 m.y. with a substantial lag relative to collision metamorphism and granite formation. It is assumed that accretion of the Siberian craton resulted in formation of a giant collision mountainous structure of the Himalayan type that was eroded by 1.65 Ga ago, when accumulation of gently dipping Meso-to Neoproterozoic (Riphean) platform cover commenced.  相似文献   

论信息时代的城市发展     

金江军  潘懋  承继成 《国土资源信息化》2005,20(2):2-5,41

城市信息化是中国城市发展的新主题与新动力,是解决目前我国城市发展中诸多难题的重要途径。本文首先对比了数字城市和信息城市,然后指出了建设信息城市的迫切性和重要性,最后提出了城市信息科学的学科范畴。  相似文献   

地下导线随盾构推进逐段接测中的可靠性检验     

高俊强  潘庆林 《现代测绘》2005,28(1):17-19

盾构法施工的要点是需要在井下布设高精度的控制支导线，当我们根据盾构推进进度对导线接测时，由于观测条件、观测方法、观测仪器基本相同，但观测、的成果往往会存在一定的差异，有时我们无法直接判断成果的正确与否，此时，采用测量平差中的统计检验的方法来分析这些观测数据，可以取得比较满意的结果。  相似文献   

利用DXF文件进行测量数据辅助处理   总被引：1，自引：0，他引：1  

吴敬文  潘苏成 《现代测绘》2005,28(6):45-46,48

DXF文件是AUTOCAD与高级语言程序设计之间的接口文件,在测量工作中,充分利用DXF文件对测量数据进行辅助处理计算,可以达到事半功倍的效果.  相似文献   

GGM02 – An improved Earth gravity field model from GRACE     

B. Tapley  J. Ries  S. Bettadpur  D. Chambers  M. Cheng  F. Condi  B. Gunter  Z. Kang  P. Nagel  R. Pastor  T. Pekker  S. Poole  F. Wang 《Journal of Geodesy》2005,79(8):467-478

A new generation of Earth gravity field models called GGM02 are derived using approximately 14 months of data spanning from April 2002 to December 2003 from the Gravity Recovery And Climate Experiment (GRACE). Relative to the preceding generation, GGM01, there have been improvements to the data products, the gravity estimation methods and the background models. Based on the calibrated covariances, GGM02 (both the GRACE-only model GGM02S and the combination model GGM02C) represents an improvement greater than a factor of two over the previous GGM01 models. Error estimates indicate a cumulative error less than 1 cm geoid height to spherical harmonic degree 70, which can be said to have met the GRACE minimum mission goals. Electronic Supplementary Material Supplementary material is available in the online version of this article at  相似文献   

黑龙江气候变暖的时空变化特征   总被引：15，自引：0，他引：15  

潘华盛  张桂华 《黑龙江气象》2002,(3):3-6,11

进入80年代以来，黑龙江气温明显变暖，近120年来年平均气温上升1.4℃，春季次之，气温突变在1990年前后，从年、各季平均气温变化趋势与全国北半球及全球气温变化进行比较，年及冬季我国增暖中心在黑龙江，春季增暖中心在内蒙古北部及黑龙江省；夏秋增暖不明显，但仍有上升趋势，近50年来，50～70年代黑龙江省及全国各大区域普遍增暖不明显，80年代开始黑龙江省增暖明显，三北地区次之，90年代黑龙江增暖更加明显，而全国及其他区域上升已达到80年代北方增温幅度，这里从黑龙江变暖的事实，突变时间，与全球、北半球、全国区域的气温及雪盖海温变化关系来揭示黑龙江气候变化的时空特点。  相似文献   

Simulation of the east asian summer monsoon using a variable resolution atmospheric GCM   总被引：6，自引：0，他引：6  

T. Zhou  Z. Li 《Climate Dynamics》2002,19(2):167-180

The East Asia summer monsoon (EASM) is simulated with a variable resolution global atmospheric general circulation model (GCM) developed at the Laboratoire de Météorologie Dynamique, France. The version used has a local zoom centered on China. This study validates the model's capability in reproducing the fundamental features of the EASM. The monsoon behaviors over East Asia revealed by the ECMWF reanalysis data are also addressed systematically, providing as observational evidence. The mean state of the EASM is generally portrayed well in the model, including the large-scale monsoon airflows, the monsoonal meridional circulation, the cross-equatorial low-level jets, the monsoon trough in the South China Sea, the surface cold high in Australia, and the upper-level northeasterly return flow. While the performance of simulating large-scale monsoonal climate is encouraging, the model's main deficiency lies in the rainfall. The marked rainbelt observed along the Yangtze River Valley is missed in the simulation. This is due to the weakly reproduced monsoonal components in essence and is directly related to the weak western Pacific subtropical high, which leads to a fragile subtropical southwest monsoon on its western flank and results in a weaker convergence of the southwest monsoon flow with the midlatitude westerlies. The excessively westward extension of the high, together with the distorted Indian low, also makes the contribution of the tropical southwest monsoon to the moisture convergence over the Yangtze River Valley too weak in the model. The insufficient plateau heating and the resulting weak land-sea thermal contrast are responsible for the weakly reproduced monsoon. It is the deficiency of the model in handling the low-level cloud cover over the plateau rather than the horizontal resolution and the associated depiction of plateau topography that results in the insufficient plateau heating. Comparison with the simulation employing regular coarser mesh model reveals that the local zoom technique improves, in a general manner, the EASM simulation.  相似文献   

A mathematical hysteretic model for elastomeric isolation bearings     

J. S. Hwang  J. D. Wu  T.‐C. Pan  G. Yang 《地震工程与结构动力学》2002,31(4):771-789

An analytical model for high damping elastomeric isolation bearings is presented in this paper. The model is used to describe mathematically the damping force and restoring force of the rubber material and bearing. Ten parameters to be identified from cyclic loading tests are included in the model. The sensitivity of the ten parameters in affecting the model is examined. These ten parameters are functions of a number of influence factors on the elastomer such as the rubber compound, Mullins effect, scragging effect, frequency, temperature and axial load. In this study, however, only the Mullins effect, scragging effect, frequency and temperature are investigated. Both material tests and shaking table tests were performed to validate the proposed model. Based on the comparison between the experimental and the analytical results, it is found that the proposed analytical model is capable of predicting the shear force–displacement hysteresis very accurately for both rubber material and bearing under cyclic loading reversals. The seismic response time histories of the bearing can also be captured, using the proposed analytical model, with a practically acceptable precision. Copyright © 2002 John Wiley & Sons, Ltd.  相似文献   

湘中锑(金)矿床成矿物质来源——Ⅰ.微量元素及其实验地球化学证据   总被引：9，自引：0，他引：9  

马东升  潘家永  解庆林  何江 《矿床地质》2002,21(4):366-376

为了查明湘中盆地中-低温梯（金）矿床的成矿物质来源，文章应用高分辨率ICP-MS、ICP-AES等方法对岩石与矿石进行了系统测定，并结合作者以往分析数据和实验地球化学结果，对该区盆地及周边基底地层与矿床中的微量元素分布特征及其水/岩反应效应进行了综合分析和系统研究。结果表明：Sb、Au等成矿元素在元古界基底碎屑岩中具有高的背景含量，在近似成矿条件下的水/岩反应实验中，成矿元素的淋出率达20%～90%，元古界基底碎屑岩中的金（锑、钨）矿床的周围蚀变围岩中出现明显的金负异常区。而盆地内泥盆系统地层中的高锑含量仅局限于锑矿床（化）及其蚀变围岩中；湘中锑（金）矿床中的矿石与基底碎屑岩具有相似的稀土元素球粒陨石标准化配分曲线特征，以上微量元素地球化学特征充分证明该区锑（金）矿床锑、金等成矿物质主要来源于元古界底碎屑岩。  相似文献   

Spatial structure of the old open cluster NGC 2420     

Z. I. Peikov  R. M. Rusev  T. Ruseva 《Astronomy Reports》2002,46(4):267-274

The spatial structure of the intermediate and outer regions of the old open cluster NGC 2420 is analyzed using data from the catalog of Paparó. The differential and integrated distributions of the projected [ΔF(r) and F(r)] and spatial [Δf(r) and f(r)] stellar densities are obtained for various subsystems of cluster stars using Kholopov’s star-count method. Analysis of these curves shows that: (1) the cluster has at least three distinct spatial zones with different stellar-density gradients, (2) the each cluster subsystem has a layered structure, and (3) the spatial structure of the cluster changes systematically in the transition to subsystems containing fainter main-sequence stars. Empirical relations describing the structure of the cluster are also derived. Similar structural features can also be found in other globular and open clusters.  相似文献