近景摄影测量在宋陵石刻测绘中应用的几个问题     

邵锡惠  龚志辉 《测绘学院学报》1995,(1)

本文论述了在宋陵石刻近景摄影测量中的几个技术问题，并进行了精度估算，实际应用证明这种方法是有效的。  相似文献   

NGC 4650 A: A nearly edge-on ring galaxy?     

S. Laustsen  R. M. West 《Journal of Astrophysics and Astronomy》1980,1(2):177-187

The peculiar galaxy NGC 4650 A (α=12^h 42^m. 1; = δ—40° 26′; 1950·0) has been studied by means of direct and spectral observations with the ESO 3·6-m telescope. It is interpreted as a prolate, elliptical galaxy surrounded by a warped ring of H II regions, dust and stars. The distance is 47 Mpc (H ₀=55 km s⁻¹ Mpc⁻¹). The ring is seen nearly edge-on (inclination 85°) and it rotates. It has a diameter of about 21 kpc and is bluer than the elliptical galaxy for which the (M/L _v) ratio is ∼12 in solar units. The observed configuration may be the result of interaction with the nearby galaxy, NGC 4650.  相似文献   

Yielding oscillator subjected to simple pulse waveforms: numerical analysis & closed‐form solutions     

George Mylonakis  Elia Voyagaki 《地震工程与结构动力学》2006,35(15):1949-1974

Numerical and analytical solutions are presented for the elastic and inelastic response of single‐degree‐of‐freedom yielding oscillators to idealized ground acceleration pulses. These motions are typical of near‐fault earthquake recordings generated by forward rupture directivity and may inflict damage in the absence of substantial structural strength and ductility capacity. Four basic pulse waveforms are examined: (1) triangular; (2) sinusoidal; (3) exponential; and (4) rectangular. In the first part of the article, a numerical study is presented of the effect of oscillator period, strength, damping, post‐yielding stiffness and number of excitation cycles, on inelastic response. Results are presented in the form of dimensionless graphs and regression formulas that elucidate the salient features of the problem. It is shown that conventional R–µ relations may significantly underestimate ductility demand imposed by near‐fault motions. The second part of the article concentrates on elastic‐perfectly plastic oscillators. Closed‐form solutions are derived for post‐yielding response and associated ductility demand. It is shown that all three ground motion histories (i.e. acceleration, velocity, and displacement) control oscillator response—contrary to the widespread view that ground velocity alone is of leading importance. The derived solutions provide insight on the physics of inelastic response, which is often obscured by the complexity of numerical algorithms and actual earthquake motions. The model is evaluated against numerical results from near‐field recordings. A case study is presented. Copyright © 2006 John Wiley & Sons, Ltd.  相似文献   

高密度电法勘探技术及其应用   总被引：19，自引：0，他引：19  

赵光辉 《矿产与地质》2006,20(2):166-168

简述了高密度电法勘探技术的基本原理。从电极排列、数据预处理及反演处理方法等方面介绍了该技术在应用中应注意的关键技术问题及其处理方法,并通过在长-邵高速公路勘察的应用实例,来说明高密度电法勘探技术在岩溶洞穴、地质灾害等探测领域具有较好的探测效果。  相似文献   

2003年江淮梅雨暴雨与湿位涡的关系   总被引：11，自引：3，他引：11  

张端禹  丁治英  张兴强  徐海明 《南京气象学院学报》2006,29(4):526-532

统计了2003年发生在江淮地区的梅雨暴雨，根据暴雨中心对流稳定度及降雨性质将暴雨分为4种类型。分析湿位涡与梅雨暴雨中的惯性不稳定、对称不稳定、对流不稳定的关系发现：第1类暴雨往往与对称不稳定有关，第2类暴雨与对流不稳定有关，且这两类暴雨高层多具有强惯性不稳定，降水相对较大；第3、第4类暴雨是稳定性降雨，高层一般不具备惯性不稳定，雨量一般较小。高层的惯性不稳定对降水的加强作用明显。  相似文献   

2003年一次梅雨大暴雨成因的动力学研究   总被引：6，自引：5，他引：6  

张端禹  丁治英  王丛梅 《南京气象学院学报》2006,29(6):827-832

运用中尺度非静力模式MN5对2003年梅雨期一次大暴雨天气进行数值模拟，在降雨模拟基本正确的基础上分析暴雨发生原因。结果表明：该次梅雨大暴雨属于切变类暴雨，对流层低层有能量锋区、高层有惯性不稳定活动，暴雨区位于低空急流的左前方、高空急流的右前方。暴雨中心物理量要素的时间一高度演变显示：低层正涡度、辐合，高层负涡度、辐散，深厚的上升运动，等相当位温线抬升，湿位涡及其正、斜压分量3者负值加大均有利于降雨加强；暴雨减弱阶段，这些要素一般向相反方向转变。该次大暴雨的直接影响系统具有明显的中尺度时、空特点，大暴雨的发生与高层惯性不稳定和低层对流不稳定有关。  相似文献   

Differences Between Mode I and Mode II Crack Propagation     

K. B. Broberg 《Pure and Applied Geophysics》2006,163(9):1867-1879

Although mode I and mode II crack propagation show many similarities, in particular when analysed by linear elastic fracture mechanics, they differ significantly in the micro-structural behaviour. These differences, which are clearly noticeable in the fracture surface morphology, lead to fundamental differences in the macroscopic behaviour. Thus, mode II crack expansion under remote loading, appears to obey micro-structural scaling laws, implying that the dimensions of the process region stay essentially constant during crack expansion, rather than increasing with crack length. Therefore, expanding mode II cracks can almost reach the Rayleigh velocity, and actually also intersonic velocities. An expanding mode I crack, on the other hand, seems to obey continuum scaling laws, implying that the dimensions of the process region increase in proportion to crack length, leading to self-similar crack expansion at a velocity significantly below the Rayleigh speed and dependent on the remote load.  相似文献   

电磁波CT成像技术在防水工程场地勘查中的应用     

夏金儒  陈石羡 《地质找矿论丛》2006,21(Z1):171-173

电磁波CT成像技术是基于地下介质的物性差异,利用各种波源透视探测目的体及地质现象的一种地球物理方法,文章介绍了电磁波CT成像技术的原理和工作方法、某防水工程场地电磁波CT成像勘查实例及应用效果.  相似文献   

Stellar models for very low-mass main-sequence stars: the role of model atmospheres     

Brocato  Cassisi  & Castellani 《Monthly notices of the Royal Astronomical Society》1998,295(3):711-724

We present very low-mass stellar models as computed using non-grey model atmospheres for selected assumptions about the stellar metallicities. The role of atmospheres is discussed and the models are compared with models based on the Eddington approximation, and with similar models that have appeared in the recent literature. Theoretical predictions concerning both the HR diagram location and the mass–luminosity relation are presented and discussed in terms of expectations in selected photometric bands. Comparison with available observational data concerning both galactic globular clusters and dwarfs in the solar neighbourhood reveals a satisfactory agreement together with the existence of some residual mismatches.  相似文献   

HST colour–magnitude diagrams of six old globular clusters in the LMC     

K. A. G. Olsen  P. W. Hodge  M. Mateo  E. W. Olszewski  R. A. Schommer  N. B. Suntzeff  & A. R. Walker 《Monthly notices of the Royal Astronomical Society》1998,300(3):665-685

We report on HST observations of six candidate old globular clusters in the Large Magellanic Cloud (LMC): NGC 1754, 1835, 1898, 1916, 2005 and 2019. Deep exposures with the F555W and F814W filters provide us with colour–magnitude diagrams that reach to an apparent magnitude in V of ∼25, well below the main-sequence turn-off. These particular clusters are associated with significantly high LMC field star densities and care was taken to subtract the field stars from the cluster colour–magnitude diagrams accurately. In two cases there is significant variable reddening across at least part of the image, but only for NGC 1916 does the differential reddening preclude accurate measurements of the CMD characteristics. The morphologies of the colour–magnitude diagrams match well those of Galactic globular clusters of similar metallicity. All six have well-developed horizontal branches, while four clearly have stars on both sides of the RR Lyrae gap. The abundances obtained from measurements of the height of the red giant branch above the level of the horizontal branch are 0.3 dex higher, on average, than previously measured spectroscopic abundances. Detailed comparisons with Galactic globular cluster fiducials show that all six clusters are old objects, very similar in age to classical Galactic globulars such as M5, with little age spread among the clusters. This result is consistent with ages derived by measuring the magnitude difference between the horizontal branch and main-sequence turn-off. We also find a similar chronology by comparing the horizontal branch morphologies and abundances with the horizontal branch evolutionary tracks of Lee, Demarque &38; Zinn. Our results imply that the LMC formed at the same time as the Milky Way Galaxy.  相似文献