1975年8月河南省特大暴雨雨强极值的重新估算   总被引：1，自引：0，他引：1  

王兴荣  高守亭 《热带气象学报》2007,23(2):196-200

通过对云中气载液态水含量以及水汽和气载液态水之间的平衡方程的讨论,建立了改进的可降水量Ia公式。按照改进的公式,重新估算了1975年8月河南省特大暴雨7日20时雨强。结果表明,分别以遂平气象站记录的8 m/s和按物象估算的12 m/s地面风速为基础的改进的板桥水库附近8月7日20时雨强估算值Iae1=75.0 mm/h和Iae1=95.8 mm/h很接近实际的雨强极值Ioe=99.7 mm/h。  相似文献   

融合形状和光谱的高空间分辨率遥感影像分类   总被引：13，自引：0，他引：13  

黄昕  张良培  李平湘 《遥感学报》2007,11(2):193-200

提出了一种像元形状指数及基于形状和光谱特征融合的高（空间）分辨率遥感影像分类方法。形状和光谱是遥感影像纹理的具体表现形式,尤其在高分辨率影像中地物细节得到充分表达,相邻像元的关系及其共同表征的形状特性成为分类的重要因素。本文用像元及其邻域的关系来描述其空间结构,同时为了更全面地利用影像特征,提出了基于支持向量机的形状和光谱融合分类方法。实验证明,该方法计算简便且能有效表达高分辨率影像的地物特征,提高分类精度。  相似文献   

块系岩体非协调动力响应特征试验研究     

王凯兴  窦林名  潘一山  OPARIN V N 《岩土力学》2020,41(4):1227-1234

岩体在块系构造状态下的动力传播存在块体和块体间软弱介质的非协调变形现象，对岩体结构的动力稳定产生重要影响。目前块系岩体的非协调动力传播响应研究尚不充分，导致不能进行有效的动力响应特征识别。通过试验对块系岩体非协调动力传播过程岩块动力响应特征进行研究，分别从动力传播速度、岩块加速度振幅衰减、岩块振动位移响应、岩块振动持续时间、块体动能显现、块体振动频域响应特性等方面对比纵波传播，给出块系岩体非协调动力传播的特征分析。通过分析可知，块系介质非协调变形运动产生的动力传播现象相比于纵波传播是一种低频低速波，并伴随着岩块的大位移运动，同时岩块振动持续时间较长，蕴含着动能与势能的相互转换过程，这些现象构成了块系岩体非协调动力传播的重要特征。该研究将为识别岩体非协调动力传播特征及块系岩体的冲击预警波动特征识别提供参考。  相似文献   

Early star formation and the evolution of the stellar initial mass function in galaxies     

Richard B. Larson 《Monthly notices of the Royal Astronomical Society》1998,301(2):569-581

It has frequently been suggested in the literature that the stellar IMF in galaxies was top-heavy at early times. This would be plausible physically if the IMF depended on a mass-scale such as the Jeans mass that was higher at earlier times because of the generally higher temperatures that were present then. In this paper it is suggested, on the basis of current evidence and theory, that the IMF has a universal Salpeter-like form at the upper end, but flattens below a characteristic stellar mass that may vary with time. Much of the evidence that has been attributed to a top-heavy early IMF, including the ubiquitous G-dwarf problem, the high abundance of heavy elements in clusters of galaxies, and the high rate of formation of massive stars in high-redshift galaxies, can be accounted for with such an IMF if the characteristic stellar mass was several times higher during the early stages of galaxy evolution. However, significant variations in the mass-to-light ratios of galaxies and large amounts of dark matter in stellar remnants are not as easily explained in this way, because they require more extreme and less plausible assumptions about the form and variability of the IMF. Metal-free 'population III' stars are predicted to have an IMF that consists exclusively of massive stars, and they could help to account for some of the evidence that has been attributed to a top-heavy early IMF, as well as contributing importantly to the energetics and chemical enrichment of the early Universe.  相似文献   

Mass segregation in young stellar clusters     

Ian A. Bonnell  & Melvyn B. Davies 《Monthly notices of the Royal Astronomical Society》1998,295(3):691-698

We investigate the evolutionary effect of dynamical mass segregation in young stellar clusters. Dynamical mass segregation acts on a time-scale of order the relaxation time of a cluster. Although some degree of mass segregation occurs earlier, the position of massive stars in rich young clusters generally reflects the cluster's initial conditions. In particular, the positions of the massive stars in the Trapezium cluster in Orion cannot be due to dynamical mass segregation, but indicate that they formed in, or near, the centre of the cluster. Implications of this for cluster formation and for the formation of high-mass stars are discussed.  相似文献   

Mass functions of five distant northern open star clusters     

Ram Sagar  & W. K. Griffiths 《Monthly notices of the Royal Astronomical Society》1998,299(3):777-788

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中国东南陆缘的深部结构与动力学过程     

王椿镛  陈运泰  邵占英 《大地测量与地球动力学》1998,(2)

对我国东南陆缘地区的人工地震测深、大地电磁测深、重磁测量、地热测量、地学大断面编制以及天然地震的层析成像等大量深部构造研究结果作综合分析。地热异常、地壳内存在低速层和高导层、强烈地震频繁发生等现象说明,这一地区是现代构造运动的活动区。中国东南陆缘的现今应力场主压应力方向为ＮＷＷ－ＳＥＥ,认为是菲律宾板块对欧亚板块的挤压,以及冲绳海槽的扩张等联合作用的结果。因此,这一地区地壳运动的驱动力是太平洋板块和菲律宾板块向欧亚板块推挤产生的。  相似文献   

佘山重力垂直梯度偏小的原因及其对大地测量的影响     

张赤军 《大地测量与地球动力学》1998,(2)

根据推导的公式计算了由山体质量引起的梯度效应,结果与实测值甚为接近。分析了佘山重力垂直梯度偏小的原因,认为这是由于山体质量分布引起的。最后讨论了垂直梯度偏小对重力值的高度归算和大地水准面的影响。  相似文献   

不同群体团头鲂生长性能分析     

朱春华 《广东海洋大学学报》1998,(1)

用随机区组试验方法,比较四种不同的选育群体团头鲂的后代和一个对照群体团头鲂的生长性能。结果表明：在同一环境条件下,远交群体比近交群体生长优势明显（|xi-xj|＞D0.01）;亲本年龄大（3足龄）的群体后代生长性能优于亲本年龄小（2足龄）的群体后代（|xi-xj|＞D0.05）;对照群体团头鲂与近交群体后代生长性能相当。  相似文献   

Toward an Ecological Explanation of Agricultural Unemployment in Bangladesh     

Abu Muhammad Shajaat Ali 《The Professional geographer》1998,50(2):176-191

Cultural ecology theoretical framework was found suitable to explain unemployment in agriculture in three villages in Bangladesh. Path analysis and multiple regression statistics were used to examine the direct, indirect, and total effects of eight independent human, social, environmental, and technology variables as well as their aggregate contribution on agricultural unemployment. The multiple regression model explains 86.2% of the total variation in unemployment in agriculture; they were followed by environmental constraints and labor saving technology variables.  相似文献