基于实测资料的南海海浪周期关系研究          下载免费PDF全文

黄必桂  石新刚  谢波涛  胡琴 《海洋学研究》2016,34(3):6-10

海浪周期在海洋工程设计中有着重要作用,而不同的海洋工程设施在设计时所选用的周期参数也不同,因此不同周期间的换算关系也就显得尤为重要。本文利用南海北部油气田区1 a的实测海浪周期数据,研究了其谱峰周期、有效周期、跨零周期和最大波高周期等的相互关系,并与相关规范和文献研究结果进行对比,给出了南海海浪周期间的关系式,从而为海洋工程设计提供了支持,也为南海海浪周期关系研究提供了参考。  相似文献   

南迦巴瓦峰第四纪隆升期次划分的热年代学证据   总被引：1，自引：0，他引：1       下载免费PDF全文

康文君  徐锡伟  于贵华  谭锡斌  李康 《地球物理学报》2016,59(5):1753-1761

喜马拉雅东构造结南迦巴瓦峰核心区附近一个高程剖面上的8个片麻岩样品裂变径迹中值年龄介于0.71~2.07Ma之间,平均封闭径迹长度在14.51~15.87μm之间,标准偏差都小于0.84μm;其冷却年龄和径迹长度所作"香蕉图"显示出三期快速的抬升期,分别发生在距今0.71 Ma、1.23 Ma、2.05 Ma.结合已有磷灰石裂变径迹冷却年龄等值线图显示出南迦巴瓦峰核心区呈复式背斜状快速隆升,而外围拉萨地体和冈底斯构造单元隆升速率慢的空间分布特征等,分析认为这种差异隆升主要受构造作用主导,气候变化造成的均衡抬升起次要作用.  相似文献   

位移和加速度融合的自适应多速率Kalman滤波方法          下载免费PDF全文

林旭  罗志才 《地球物理学报》2016,59(5):1608-1615

多速率Kalman滤波方法可用于低采样率的位移和高采样率的加速度数据融合,而未知的噪声协方差信息则显著制约着多速率Kalman滤波精度.本文通过将多速率Kalman滤波转换为传统的单速率Kalman滤波,建立了Kalman滤波增益的自协方差矢量与未知的加速度谱密度和观测噪声参数间的线性函数模型,并采用最小二乘估计方法对未知的噪声协方差参数进行估计,进而有效地提高了多速率Kalman滤波精度.数值仿真和震动台实验结果验证了本文方法的正确性和有效性.  相似文献   

Seismic directional random noise suppression by radial‐trace time–frequency peak filtering using the Hurst exponent statistic          下载免费PDF全文

Chao Zhang  Hongbo Lin  Baojun Yang 《Geophysical Prospecting》2016,64(3):571-580

Radial‐trace time–frequency peak filtering filters a seismic record along the radial‐trace direction rather than the conventional channel direction. It takes the spatial correlation of the reflected events between adjacent channels into account. Thus, radial‐trace time–frequency peak filtering performs well in denoising and enhancing the continuity of reflected events. However, in the seismic record there is often random noise whose energy is concentrated in certain directions; the noise in these directions is correlative. We refer to this kind of random noise (that is distributed randomly in time but correlative in the space) as directional random noise. Under radial‐trace time–frequency peak filtering, the directional random noise will be treated as signal and enhanced when this noise has same direction as the signal. Therefore, we need to identify the directional random noise before the filtering. In this paper, we test the linearity of signal and directional random noise in time using the Hurst exponent. The time series of signals with high linearity lead to large Hurst exponent value; however, directional random noise is a random series in time without a fixed waveform and thus its linearity is low; therefore, we can differentiate the signal and directional random noise by the Hurst exponent values. The directional random noise can then be suppressed by using a long filtering window length during the radial‐trace time–frequency peak filtering. Synthetic and real data examples show that the proposed method can remove most directional random noise and can effectively recover the reflected events.  相似文献   

高能质子能谱特征在日冕物质抛射影响预报中的应用          下载免费PDF全文

薛炳森 《地球物理学报》2012,55(3):738-743

日冕物质抛射(CME)的规模和对地有效性是地磁暴预报中重点关注的特征.本项研究的目的是通过对行星际高能质子通量和能谱的特征与演化规律的分析,得到CME对粒子的加速能力,评估CME可能对地磁场造成的影响.在工作中,统计分析了ACE/EPAM的1998-2010年的质子数据,对质子能谱进行了拟合,得到了能谱指数,并对能谱指数及其变化特征所对应的CME和地磁暴进行了相关统计.通过研究发现:(1)能谱指数随着太阳活动水平而变化,高年最大,达到-2.6,而且涨落幅度也达到±0.4,而在太阳活动低年则稳定在-3.0左右;(2)CME对粒子的加速对应着能谱指数的升高,幅度达到20%时,CME引起地磁暴的可能性较大;(3)冕洞高速流到达地球时,高能质子通量也会升高,但能谱指数同时会有下降;(4)以2004年全年的能谱指数为例,对能谱指数在地磁暴预报中的应用进行了评估,结论认为,能谱指数的升高是CME引发地磁暴的必要条件,可以作为地磁暴预报的参数使用.  相似文献   

Effects of aftershocks on peak ductility demand due to strong ground motion records from shallow crustal earthquakes     

Katsuichiro Goda  Colin A. Taylor 《地震工程与结构动力学》2012,41(15):2311-2330

Aftershocks induced by a large mainshock can cause additional damage to structures and infrastructure, hampering building reoccupation and restoration activities in a post‐disaster situation. To assess the nonlinear damage potential due to aftershocks, this study investigates the effects of aftershocks by using real as well as artificially generated mainshock–aftershock sequences. The real mainshock–aftershock sequences are constructed from the Pacific Earthquake Engineering Research Center—Next Generation Attenuation database for worldwide shallow crustal earthquakes; however, they are deemed to be incomplete because of missing records. To supplement incomplete real dataset, artificial sequences are generated on the basis of the generalized Omori's law, and a suitable aftershock record selection procedure is then devised to simulate time‐series data for mainshock–aftershock sequences. The results from nonlinear dynamic analysis of inelastic single‐degree‐of‐freedom systems using real and artificial sequences indicate that the incremental effects of aftershocks on peak ductility demand using the real sequences are relatively minor and that peak ductility demand estimates based on the generalized Omori's law are greater, particularly in the upper tail, than those for the real sequences. The results based on the generalized Omori's law also suggest that the aftershock effects based on the real sequences might underestimate the aftershock impact because of the incompleteness of the real dataset. Copyright © 2012 John Wiley & Sons, Ltd.  相似文献   

Solar wind influence on atmospheric processes in winter Antarctica     

O. Troshichev   《Journal of Atmospheric and Solar》2008,70(18):2381-2396

Galactic cosmic rays (GCRs) altered by solar wind are traditionally regarded as the most plausible agent of solar activity influence on the Earth's atmosphere. However, it is well known that severe reductions in the GCRs flux, known as Forbush decreases (FDs), are caused by solar wind of high speed and density, which sweeps away the GCRs on its way. Since the FD beginnings are registered at the Earth's orbit simultaneously with dramatic disturbances in the solar wind, the atmospheric effects, assigned to FDs, can be, in reality, the results of the solar wind influence on the atmospheric processes. This paper presents a summary of the experimental results demonstrating the strong influence of the interplanetary electric field on atmospheric processes in central Antarctica, where the large-scale system of vertical circulation is formed during winter seasons. The influence is realized through acceleration of the air masses, descending into the lower atmosphere from the troposphere, and the formation of cloudiness above the Antarctic Ridge, where the descending air masses enter the surface layer. The acceleration is followed by a sharp increase of the atmospheric pressure near-pole region, which gives rise to the katabatic wind strengthening above the entire Antarctica. The cloudiness formation results in the sudden warmings in the surface atmosphere, since the cloud layer efficiently backscatters the long wavelength radiation from the ice sheet, but does not affect the adiabatic warming process of the descending tropospheric air masses. When the drainage flow strengthening the circumpolar vortex around the periphery of the Antarctic continent decays, the surface easterlies typical of the coast stations during the winter season are replaced by southerlies and the cold Antarctic air masses flow out to the Southern ocean.  相似文献   

汶川8.0级地震强震动特征初步分析   总被引：19，自引：3，他引：16  

于海英  王栋  杨永强  卢大伟  解全才  张明宇  周宝峰  江纹乡  程翔  杨剑 《震灾防御技术》2008,3(4):321-336

本文对国家强震动台网中心收集的2008年5月12日14时28分04秒汶川8．0级地震中获取的420组三分量加速度记录进行了处理和初步分析。在这次地震中布设在龙门山断裂带及其周围地区的50多个台站获得了大于100gal的加速度记录,有46组三分量加速度记录的断层距小于100km,使中国大陆近断层区域所获得的强震动加速度记录的数量成倍增加。本文依据这批数据,对汶川大地震强震动特性进行了初步分析,给出了此次地震断层附近地区的PGA衰减规律,并利用此规律模拟了断层附近的加速度峰值,绘制了PGA分布图、竖向PGA与水平向PGA比值图;给出了汶川地震断层附近的加速度反应谱、上盘效应、竖向效应、速度大脉冲效应等地震动特征,这些特征可作为抗震设计规范修订的依据并供灾区重建时参考。  相似文献   

利用VSP资料直达波的包络峰值处瞬时频率提取介质品质因子   总被引：10，自引：3，他引：7       下载免费PDF全文

高静怀  杨森林  王大兴 《地球物理学报》2008,51(3):853-861

本文采用一个具有4个待定参数的函数去逼近震源子波,利用黏弹介质中单程波传播理论推导出了地震子波包络峰值处瞬时频率(EPIF)和品质因子之间的解析关系;同时,为提高瞬时频率的估计精度和抗噪性能,在小波域中发展了一种计算瞬时频率的方法,并在此基础上提出了估算VSP资料Q值的方法,简称小波域包络峰值处瞬时频率法(WEPIF)．合成的VSP数据衰减估计结果表明,与对数谱比法和中心频率偏移法相比较,WEPIF法受到界面反射波影响相对较小、计算结果稳定、精度相对较高．将WEPIF法用于某气田的单炮零偏6级VSP资料Q值估计,结果表明,吸收强弱与储层含气性高低有良好的对应关系．  相似文献   

倾斜断层不对称分布引起的几何效应-上下盘效应.   总被引：1，自引：0，他引：1       下载免费PDF全文

王栋  谢礼立  胡进军 《地震学报》2008,30(3):271-278

首先介绍了具有加权平均意义的均方根距离Drms. 与断层距Drup和发震断层距Dseis相比, 均方根距离可以真实地反映观测点与倾斜断层的整体靠近程度. 然后利用断层距、 发震断层距和均方根距离, 通过回归分析分别对1999年集集地震加速度峰值的上下盘效应进行研究. 残差分析表明上盘的加速度峰值明显大于相同断层距或发震断层距处下盘的加速度峰值, 而相同均方根距离处的上下盘观测点的加速度峰值没有明显差异. 这说明上下盘效应是一种由于倾斜断层的不对称分布引起的几何效应, 因此进行地震动衰减分析时, 如果采用均方根距离作为观测点与断层之间的距离标准, 上下盘效应对近断层地震动的影响可以忽略.   相似文献