常加速度模型的简化自协方差最小二乘法     

林旭  罗志才  姚朝龙 《测绘学报》2014,43(11):1144-1150

“当前”统计模型自适应算法并非真正意义上的自适应目标跟踪算法,其性能与其中关键参数的选择有着直接的关系。本文以常加速度模型对机动载体进行建模,顾及其状态噪声协方差矩阵满足特定结构,提出了简化的自协方差最小二乘噪声协方差估计方法,该方法通过建立新息的相关函数序列与未知噪声协方差矩阵间的函数模型,并结合最小二乘法进行噪声协方差估计。数值仿真结果表明,当载体进行阶跃加速度运动或变加速度运动时,本文所提方法的目标跟踪精度均优于“当前”统计模型自适应算法。  相似文献   

华南沿海2011年7月15—18日持续暴雨过程中的季风槽与中尺度对流系统相互作用   总被引：1，自引：0，他引：1  

蒙伟光  张艳霞  袁金南  李春晖  梁巧倩  吴乃庚 《气象学报》2014,72(3):508-525

应用NCEP FNL再分析资料及位涡分离反演等方法,对华南沿海2011年7月15—18日持续暴雨过程中季风槽与中尺度对流系统的相互作用进行了研究,主要针对暴雨发生期间季风槽气旋性涡度向上发展的机理及其对季风槽维持发展和中尺度对流系统活动的影响进行分析。结果发现,季风槽的中尺度对流系统发展于弱斜压性环境中,大多在槽东西两端涡度中心区发展最强。南侧盛行的西南低空急流为对流反复发生提供了对流发展的“可维持性”条件,是对流得以组织发展成为中尺度对流系统的重要原因。涡度收支诊断表明,季风槽气旋性涡度生成主要由中尺度对流系统低层辐合引起。位涡分离反演结果证实,季风槽气旋性环流增强主要由与中尺度对流系统潜热加热相关的扰动位涡造成,并随着中尺度对流系统加热峰值高度升高而向上发展,是大尺度环流对中尺度对流系统潜热加热动力响应的结果。在季风槽东西两端,由于中尺度对流系统发展强烈且持续,具有更高的加热效率,引起的气旋性涡度向上发展最为明显。其结果可引起中尺度对流系统西南一侧向北非地转风发展,并在地转偏向力作用下增强西风,维持低空急流的发展,为对流反复发生提供条件。这些都说明季风槽大尺度环流与中尺度对流系统相互作用在中尺度对流系统和持续暴雨形成过程中有重要作用。  相似文献   

土体参数对地表加速度峰值和反应谱的影响   总被引：9，自引：1，他引：8  

刘红帅  薄景山  吴兆营  刘德东 《地震研究》2005,28(2):167-171

运用一维土层地震反应的等效线性化波动方法,研究了单层均质土密度、动剪切模量比和阻尼比、土层厚度和土层剪切波速等参数变化对土层地表加速度峰值和反应谱的影响,所得到的结论对于指导地震安全性评价中的勘察试验工作、提高土层地震反应的计算精度具有一定的参考价值。  相似文献   

Regional Tectonic Stability Evaluation of the Middle Reaches of the Yarlung Zangbo River Hydropower Planning     

XU Wei  DENG Jianghong 《《地质学报》英文版》2013,87(Z1):659-659

  相似文献   

Determination of passive earth pressure with lower bound finite elements limit analysis and modified pseudo-dynamic method     

《Geomechanics and Geoengineering》2013,8(3):218-229

ABSTRACT

The present study deals with the determination of passive earth pressure under seismic condition by following the lower bound finite elements limit analysis and modified pseudo-dynamic methodology. In accordance with the lower bound finite elements formulation, the stress field was modelled using a three-noded triangular elements, while the passive pressure was determined via linear optimisation. The parametric study was performed, for a vertical rigid retaining wall, by varying the magnitude of seismic acceleration in horizontal direction (k_h) between 0 and 0.3, while the vertical seismic acceleration (k_v) was kept equal to 0 or 0.5 k_h. Furthermore, the damping coefficient for dry cohesionless backfill was kept ξ = 10%. The obtained results in various cases were found to be in good agreement with those found in the literature. It is expected that this method can be further used for solving other important geotechnical stability problems.  相似文献   

太阳米波和分米波Ⅱ型、Ⅲ型射电暴及其精细结构观测研究进展     

高冠男  林隽  汪敏  谢瑞祥 《天文学进展》2012,30(1):35-47

太阳米波和分米波的射电观测是对太阳爆发过程中耀斑和日冕物质抛射现象研究的重要观测手段。米波和分米波的太阳射电暴以相干等离子体辐射为主导,表现出在时域和频域的多样性和复杂性。其中Ⅱ型射电暴是激波在日冕中运动引起电磁波辐射的结果。在Ⅱ型射电暴方面,首先对米波Ⅱ型射电暴的激波起源问题和米波Ⅱ型射电暴与行星际Ⅱ型射电暴的关系问题进行了讨论;其次,结合Lin-Forbes太阳爆发理论模型对Ⅱ型射电暴的开始时间和起始频率进行讨论:最后,对Ⅱ型射电暴信号中包含的两种射电精细结构,Herringbone结构(即鱼骨结构)和与激波相关的Ⅲ型射电暴也分别进行了讨论。Ⅲ型射电暴是高能电子束在日冕中运动产生电磁波辐射的结果。在Ⅲ型射电暴方面,首先介绍了利用Ⅲ型射电暴对日冕磁场位形和等离子体密度进行研究的具体方法;其次,对利用Ⅲ型射电暴测量日冕温度的最新理论进行介绍;最后,对Ⅲ型射电暴和Ⅱ型射电暴的时间关系、Ⅲ型射电暴和粒子加速以及Ⅲ型射电暴信号中包含的射电精细结构(例如斑马纹、纤维爆发及尖峰辐射)等问题进行讨论并介绍有关的最新研究进展。  相似文献   

Flow and deformation failure of sandy slopes   总被引：2，自引：0，他引：2  

G. Biondi  E. Cascone  M. Maugeri 《Soil Dynamics and Earthquake Engineering》2002,22(9-12):1103-1114

The effects of earthquake induced pore pressure on seismic and post seismic stability conditions of cohesionless slopes are investigated with reference to the infinite slope scheme. In cohesionless slopes the shear strength reduction caused by pore pressure build-up may lead the slope to a deformation failure or to a flow failure if liquefaction conditions are approached. Two critical values of the seismic induced pore pressure ratio are introduced to evaluate the effect of shear strength reduction on the slope failure mechanism. The results are given in the form of stability charts and a procedure for the evaluation of the seismic stability condition is described. The procedure gives useful information about the failure mechanism that slopes may exhibit and the displacement analysis which should be carried out.  相似文献   

滑坡危险性分析中地震动的概率性估算及地震滑坡的危险性评判   总被引：5，自引：0，他引：5  

王赞军  江志萍  张家庆  辛莉 《高原地震》1998,(1)

论述了滑坡危险性分析中如何科学地估算地震力的问题。主要思路概括为：将滑坡体视为一个完整体系的结构物（或震动对象）,将滑坡场点视为一个工程场点,利用比较成熟的地震危险性概率分析方法计算滑坡体未来若干年内可能遭遇的不同超越概率水平下的地震峰值加速度,这种不确定性的地震加速度是由地震预报的不确定性带入的,由此计算地震力和惯性力。最后,对地震触发滑坡的机理展开讨论。  相似文献   

On the origin of the 511-keV emission in the Galactic Centre     

Reba M. Bandyopadhyay  Joseph Silk  James E. Taylor  Thomas J. Maccarone 《Monthly notices of the Royal Astronomical Society》2009,392(3):1115-1123

Diffuse 511-keV line emission, from the annihilation of cold positrons, has been observed in the direction of the Galactic Centre for more than 30 yr. The latest high-resolution maps of this emission produced by the SPI instrument on INTEGRAL suggest at least one component of the emission is spatially coincident with the distribution of ∼70 luminous, low-mass X-ray binaries detected in the soft gamma-ray band. The X-ray band, however, is generally a more sensitive probe of X-ray binary populations. Recent X-ray surveys of the Galactic Centre have discovered a much larger population (>4000) of faint, hard X-ray point sources. We investigate the possibility that the positrons observed in the direction of the Galactic Centre originate in pair-dominated jets generated by this population of fainter accretion-powered X-ray binaries. We also consider briefly whether such sources could account for unexplained diffuse emission associated with the Galactic Centre in the microwave (the Wilkinson Microwave Anisotropy Probe 'haze') and at other wavelengths. Finally, we point out several unresolved problems in associating Galactic Centre 511-keV emission with the brightest X-ray binaries.  相似文献   

A kinetic approach to cosmic-ray-induced streaming instability at supernova shocks   总被引：1，自引：0，他引：1  

E. Amato  P. Blasi 《Monthly notices of the Royal Astronomical Society》2009,392(4):1591-1600

We show that a purely kinetic approach to the excitation of waves by cosmic rays in the vicinity of a shock front leads to predict the appearance of a non-Alfvénic fast-growing mode which has the same dispersion relation as that previously found by Bell in 2004 by treating the plasma in the magnetohydrodynamic approximation. The kinetic approach allows us to investigate the dependence of the dispersion relation of these waves on the microphysics of the current which compensates the cosmic ray flow. We also show that a resonant and a non-resonant mode may appear at the same time and one of the two may become dominant on the other depending on the conditions in the acceleration region. We discuss the role of the unstable modes for magnetic field amplification and particle acceleration in supernova remnants at different stages of the remnant evolution.  相似文献