加速度记录测定近震震级在江苏地区的计算研究     

詹小艳  徐顺强  章东  王凯 《大地测量与地球动力学》2021,41(5):539-543

基于江苏强震台网和江苏测震台网的地震记录,采用时间域内实时仿真WA记录方法,对2007~2018年记录到的M2.3以上地震进行近震震级测定。为了定量分析基于加速度测定近震震级的可靠性,首先采用国标规定的新震级测定方法和量规函数测定了基于加速度记录的震级,并将结果与江苏测震台网基于速度记录测定的结果进行对比分析,得到线性拟合关系式：ML(ACC)=0.987ML＋1.371;另外计算了15 324组基于加速度测定的震级与人工编目震级之间的绝对偏差,结果显示,偏差在±0.5级以内的结果占87%;通过4阶多项式拟合后发现,在小于200 km范围内测定的震级略低于人工编目的结果,震中距超过200 km后无系统偏差。总体而言,两者结果的一致性较好,表明利用加速度记录仿真WA位移记录来计算近震震级是可行的,得到的结果也是可靠的。  相似文献   

云南两次局地暴雨过程水汽输送特征分析     

马志敏  朱莉  连钰  牛法宝  王将 《中低纬山地气象》2021,45(6):50-58

采用常规观测资料、NCEP再分析资料,结合数值试验,对2012年5月24日和2015年9月27日云南两次局地暴雨过程水汽输送特征进行分析。结果表明：（1）两次过程主要受副热带高压影响,强降雨及其水汽输送伴随副热带高压西伸而中断,“5.24”过程动力条件主要由天气尺度系统提供,“9.27”过程动力条件主要为地形抬升作用;（2）两次过程水汽源地均为孟加拉湾、南海、西太平洋,“5.24”过程以西南路径水汽输送为主,输送距离较远,“9.27”过程以东南路径水汽输送为主,输送距离较短,局地特征更显著;（3）“9.27”过程水汽通量及最大雨量值均高于“5.24”过程,水汽通量与强降雨相关性较好,对强降雨具有一定指示意义;（4）两次过程水汽输送均集中在600hPa以下层,以经向偏南水汽输送为主,水汽输送增强时间较强降雨开始时间提前48～72h;（5）数值模拟结果与常规分析一致,同时可显示水汽垂直输送特征,低层以偏南路径为主,中层西南路径增多,中层以上出现偏西路径,存在沿西风带来自印度半岛及青藏高原的水汽贡献。  相似文献   

敦煌莫高窟潜在地震变形数值模拟   总被引：1，自引：0，他引：1  

王爱国  石玉成  马巍 《工程地质学报》2005,13(2):240-246

在研究莫高窟地区地震地质条件及潜在地震危险性分析的基础上,基于地震的断层弹性位错理论,采用位移水平分布的抛物线模型,假定三危山断层分别发生5.5、6.0和6.5级地震情况下,用三维有限元的方法分析计算了莫高窟地区的潜在地震变形。给出了在震级5.5、6.0及6.5级三种情况断层逆冲和水平走滑两种活动方式下,莫高窟区的地震位移和应变值,供石窟的抗震设防加固设计参考。  相似文献   

土钉支护现场测试及三维数值模拟分析   总被引：12，自引：3，他引：9  

李志刚秦四清  张冰峰 《工程地质学报》2004,12(1):69-73

在进行土钉轴力和边坡位移测试的基础上 ,进行了土钉支护的三维数值模拟研究 ,对边坡位移、土钉轴力、塑性区分布等分别作了较为深入的探讨 ,认识到土钉与土体相互作用形成了一个完整的支护体系 ;基坑失稳破坏并非传统意义上的土体和土钉的破坏 ,而是土钉支护体系的整体性破坏 ;土钉支护体系的形成正是通过土钉的分担作用、应力传递与扩散作用来实现的 ,这是土钉支护作用的实质.  相似文献   

Phytoplankton, nutrients and hydrography in the frontal zone between the Southwest Indian Subtropical gyre and the Southern Ocean     

J. F. Read  M. I. Lucas  S. E. Holley  R. T. Pollard 《Deep Sea Research Part I: Oceanographic Research Papers》2000,47(12):2341-2367

A survey was made of the Southwest Indian Ocean frontal region between 30 and 50°E containing the Agulhas Return, Subtropical and Subantarctic Fronts. From CTD, SeaSoar and extracted samples the distribution of nitrate, silicate and chlorophyll a is shown to be strongly linked to the front and water mass structure, varying zonally and meridionally. Surface chlorophyll a concentrations were low to the north and south leaving a band of elevated chlorophyll between the Subtropical and Subantarctic Fronts. The low concentration of chlorophyll a to the north, in Subtropical Water, was clearly due to nitrate limitation. Between the Subtropical and Subantarctic Fronts, where the chlorophyll a concentrations were highest, the surface layer showed silicate depletion limiting diatom growth. South of the Subantarctic Front there were deep extending, low concentrations of chlorophyll a, but despite plentiful supplies of macro-nutrients and a well-stratified surface layer, high concentrations of chlorophyll a were absent. Changes from west to east were associated with the meandering of the Southern Ocean Fronts, especially the Subtropical Front, and their strength and proximity to each other. Concentrations of chlorophyll a peaked where the Agulhas Return, Subtropical and Subantarctic Fronts were in close proximity. Combined frontal structures appear to have particularly pronounced vertical stability and are associated with enhanced upwelling of nutrients and leakage of nutrients across the front. Light levels are high within the shallow stable layer. Such conditions are clearly favourable for biological growth and support the development of larger-celled phytoplankton communities.  相似文献   

倾角函数展开及其在分析法轨道预报中的应用          下载免费PDF全文

郑峰椿  汤靖师 《天文学报》2023,64(5):51-35

田谐项摄动是分析法轨道预报中的重要部分,其中包含大量倾角函数及其偏导数的计算.由于具有精度更高、速度更快的优点,倾角函数一般通过递推方法计算.以文献中提出的改进Gooding方法为基础,将其给出的程序稍加改进,在计算2–50阶倾角函数时缩短了约24%的计算时间.考虑到分析法预报过程中轨道平倾角变化很小,以泰勒展开式计算倾角函数,可极大提高计算速度,较大程度地减小分析法预报耗时,且引力场阶次越高,减小幅度越大,取50阶时预报耗时缩短了48%.另一方面,以2阶展开式计算倾角函数时,与改进Gooding法相比,分析法预报星历偏差很小.对于500 km高度的低轨卫星,分别以改进Gooding法和2阶泰勒展开式计算倾角函数,预报3天,当地球引力场阶次不高于50时,二者预报星历偏差RMS (Root Mean Square)低于1 mm,且随着轨道高度的增加,预报星历偏差RMS逐渐减小.  相似文献   

Development of a river delta: a case study of Cimanuk river mouth,Indonesia     

Nita Yuanita  Tawatchai Tingsanchali 《水文研究》2008,22(18):3785-3801

This paper describes delta development processes with particular reference to Cimanuk Delta in Indonesia. Cimanuk river delta, the most rapidly growing river delta in Indonesia, is located on the northern coast of Java Island. The delta is subject to ocean waves of less than 1 m height due to its position in the semi‐enclosed Java Sea in the Indonesian archipelago. The study has been carried out using a hydrodynamic model that accounts for sediment movement through the rivers and estuaries. As an advanced approach to management of river deltas, a numerical model, namely MIKE‐21, is used as a tool in the management of Cimanuk river delta. From calibration and verification of hydrodynamic model, it was found that the best value of bed roughness was 0·1 m. For the sediment‐transport model, the calibration parameters were adjusted to obtain the most satisfactory results of suspended sediment concentration and volume of deposition. By comparing the computed and observed data in the calibration, the best values of critical bed shear stress for deposition, critical bed shear stress for erosion and erosion coefficient were 0·05 N m^?2, 0·15 N m^?2, and 0·00001 kg m^?2 s^?1, respectively. The calibrated model was then used to analyse sensitivity of model parameters and to simulate delta development during the periods 1945–1963 and 1981–1997. It was found that the sensitive model parameters were bed shear stresses for deposition and erosion, while the important model inputs were river suspended sediment concentration, sediment characteristics and hydrodynamic. The model result showed reasonable agreement with the observed data. As evidenced by field data, the mathematical model proves that the Cimanuk river delta is a river‐dominated delta because of its protrusion pattern and very high sediment loads from the Cimanuk river. It was concluded that 86% of sediment load from the Cimanuk river was deposited in the Cimanuk delta. Copyright © 2008 John Wiley & Sons, Ltd.  相似文献   

Influence of size on the constitutive equations of concrete or rock dowels     

Letícia Fleck Fadel Miguel  Jorge Daniel Riera  Ignacio Iturrioz 《国际地质力学数值与分析法杂志》2008,32(15):1857-1881

The numerical fracture analysis of non‐homogeneous rock or concrete dowels subjected to shear and compression is described in detail. The method of analysis allows the consideration of scale and rate effects due to material non‐homogeneity and fracture. The proposed approach is verified by comparing numerical predictions with experimental results reported in the literature for a series of small rock samples, since experimental evidence for large bodies is not yet available (2007). Results generated by Monte Carlo simulation using the so‐called discrete element method to model the dowels suggest that a simple three parameters law can be used to predict the relationship between tangential stress at the base and lateral distortion. It is observed that the larger the size of the cubes, the smaller both the peak tangential stress and the rupture distortion. Size effects are also evaluated in samples with vertical restraint. The influence of loading rate is likewise numerically assessed for two sample sizes. The effect is compatible with experimental evidence available for concrete using small samples. Copyright © 2008 John Wiley & Sons, Ltd.  相似文献   

高校贫困生存在的主要道德情感问题及其对策     

饶华  阎钢 《成都信息工程学院学报》2007,22(3):410-415

目前,随着贫困生数量的急剧增加,高校在重视解决贫困生经济困难的同时,往往忽略了他们内心深处潜藏的情绪感受.他们中的大多数产生了不同于一般大学生的道德情感问题.因此,贫困生的道德情感状况、造成此种状况的原因以及培养贫困生的道德情感的路径和方法,便成为对贫困生问题开展深入研究的全新的独特视域.  相似文献   

Towards a new standard model for black hole accretion     

Zdenka Kuncic  Geoffrey V. Bicknell 《Astrophysics and Space Science》2007,311(1-3):127-135

We briefly review recent developments in black hole accretion disk theory, emphasizing the vital role played by magnetohydrodynamic (MHD) stresses in transporting angular momentum. The apparent universality of accretion-related outflow phenomena is a strong indicator that large-scale MHD torques facilitate vertical transport of angular momentum. This leads to an enhanced overall rate of angular momentum transport and allows accretion of matter to proceed at an interesting rate. Furthermore, we argue that when vertical transport is important, the radial structure of the accretion disk is modified at small radii and this affects the disk emission spectrum. We present a simple model demonstrating how energetic, magnetically-driven outflows modify the emergent disk emission spectrum with respect to that predicted by standard accretion disk theory. A comparison of the predicted spectra against observations of quasar spectral energy distributions suggests that mass accretion rates inferred using the standard disk model may be severely underestimated.  相似文献