Analysis of seismic dynamical systems     

M. Urquizú  A. M. Correig 《Journal of Seismology》1998,2(2):159-171

A procedure is presented for the analysis of complex stationary time series for which the Fourier power spectra reveals broadband noise or broadened pulses. We first determine the Hurst exponent from which we may know whether the time series under study is mainly random or if the data points present correlations. If the data are correlated, a chaotic analysis will reveal whether they may be interpreted as a low dimensional nonlinear system (defined by a low correlation dimension and a finite and positive Kolmogorov entropy and largest positive Lyapunov exponent) or as a stochastic process. We have studied three kind of temporal series: inter-event time series of infrasonic pulses recorded at Stromboli volcano, and, S-coda waves and microseisms, that have been recorded at the eastern Pyrenees. Results show that microseisms and Coda waves can be modeled as a low dimensional deterministic system, Correlation dimensions 2.3, 3.2, respectively. At the contrary infrasonic has resulted stochastic. This chaotic character can be attributed to the medium properties. Coda waves with scattering through a fractal distribution of scatters or to multiple reflection inside resonators (for example sedimentary basins) and microseisms as a propagation of wave guide of variable cross section which have the same temporal characteristics as a nonlinear forced oscillator.  相似文献   

HEIFE绿洲和沙漠地区大气边界层湍流混沌特性研究   总被引：8，自引：1，他引：7  

高志球  王介民 《高原气象》1998,17(4):397-402

利用“黑河实验”期间张掖、沙漠观测站加强观测期间１９９１年６月２０日０９：００至１９９１年１０月２日０９：００时段内水平风速的观测资料,计算分析了有关测量混沌的特征量：关联维数。Ｌｙａｐｕｎｏｖ指数和Ｋｏｌｍｏｇｏｒｏｗ熵。  相似文献   

Generalisation of a Nonlinear Dynamo Model     

Tanner  Sarah E. M.  Hughes  D. W. 《Studia Geophysica et Geodaetica》1998,42(3):343-349

In order to gain a better understanding of the physical processes underlying fast dynamo action it is instructive to investigate the structure of both the magnetic field and the velocity field after the dynamo saturates. Previously, computational results have been presented (Cattaneo, Hughes and Kim, 1996) that indicate, in particular, that Lagrangian chaos is suppressed in the dynamical regime of the dynamo. Here we extend their model by removing the assumption of neglecting the inertial term. This allows for an investigation into the effect of this term on the evolution of the dynamo via a comparison of the two models. Our results indicate that this term plays a crucial role in the physics of the dynamo.  相似文献   

沈阳大气气溶胶光学特性及其影响因子   总被引：4，自引：0，他引：4  

赵胡笳  马雁军  王扬锋  朱轶明 《气象与环境学报》2015,(3):43-49

利用2010年3—10月沈阳大气成分监测站CE－318太阳光度计观测资料,计算沈阳大气气溶胶光学厚度和波长指数等大气光学特性参数,结合地面气象观测资料,分析大气气溶胶光学特性及其影响因子。结果表明：沈阳气溶胶光学厚度在3—6月较高,8月较低,9—10月气溶胶光学厚度略有增加;除4月和8月外,气溶胶光学厚度与风速基本呈反相关;气溶胶光学厚度与可吸入颗粒物（particulate matter,PM）质量浓度变化趋势基本一致;气溶胶光学厚度日平均值距平的绝对值、改变率均与降水强度成正比;地面能见度与气溶胶光学厚度呈负相关。由气溶胶浑浊度系数计算的能见度在4—6月与实际观测的能见度基本吻合,由气溶胶标高计算的水平能见度整体小于实际观测的水平能见度。  相似文献   

月表虹湾Hurst指数分析          下载免费PDF全文

奚晓旭  刘少峰  韦蔚  李珂  焦中虎  李力 《地学前缘》2012,19(6):137-143

月球遥感是在登月技术还不完善的情况下,利用遥感数据,通过各种分析来研究月球演化、内部结果和表面特征的方法。粗糙度是地表隆升、沉降、侵蚀和火山喷射物覆盖在行星表面留下的记录,因此对行星表面粗糙度的定量分析可以精确反映其地质演化过程。而Hurst指数则是粗糙度的精确反映。文中利用LOLA制作的DEM,以月球正面虹湾为例,选取水平方向的12条剖面和垂直方向的15条剖面对其各粗糙度参数进行计算,并结合月表成熟度对Hurst指数与底层年龄的相关性进行了分析,得出如下结论:(1)在1km的剖面长度上,虹湾地区均方根高程的平均值在3m左右;在0.2～3km研究尺度范围内,虹湾地区的坡度不超过2°,说明该地表起伏度小。(2)虹湾地区的Hurst指数跨度比较大,尤其在垂直方向(南北)上,在0.4到0.9之间,表明其构造样式丰富。(3)在0.2～3km研究尺度范围内,Hurst指数自北往南增大、自西往东增大,表示在虹湾地区粗糙度自西北向东南方向增大。(4)虹湾地区地质年龄为自西北向东南方向变小,与Hurst指数增大方向一致。(5)在月表年轻撞击坑地区月表成熟度与Hurst指数大致呈负相关关系。  相似文献   

修正的内梅罗指数法及其在城市地下饮用水源地水质评价中的应用   总被引：5，自引：0，他引：5  

闫欣荣 《地下水》2010,32(1):6-7

为了克服内梅罗指数法和平均指数法存在的不足,对内梅罗指数法进行了修正。将公式中的算术平均修改为加权平均,各评价指标的权重是根据污染因子的危害性与该污染因子的排放标准呈反比例关系来确定的。并将修正后的公式用于西安市地下饮用水源地的水质评价中。结果表明,改进后的方法更能客观地评价水质状况,既突出了最大污染因子,又增强了危害性较强因子的作用,是合理的。  相似文献   

应用等性块段指数法划分新场井田的构造类型     

蒋幕飞  李正武 《四川地质学报》2010,30(2):237-239

介绍了等性块段指数法定量划分井田构造类型的基本原理。利用该法对筠连矿区新场井田的构造类型进行定量评价,得出该井田构造指数为1．98,属中等构造,证明原勘探所定构造类型基本正确。  相似文献   

非线性Lyapunov稳定性及Stern''''s Modons的稳定性判据     

罗德海 《成都信息工程学院学报》1993,(4)

本文在构造正压大气运动的浅水波模式的Hamilton守恒量和积分不变的Casimir泛函的基础上,建立了一个积分不变的Lyapunov函数,通过使用变分法,找出了正压旋转流体运动的非线性Lyapunov稳定性判据,并进一步讨论了Stern's Modons的稳定性。  相似文献   

关联指数误差和样本容量     

吴云  周硕愚  孙建中 《大地测量与地球动力学》1994,(1)

根据关联指数的定义，推导了ＧＰ法计算关联指数时的观测数据误差与关联指数误差的关系，导出了任意两个嵌入空间维上关联指数之差的表达式，并提出了一种确定样本容量限的方法。  相似文献   

Homoclinic and heteroclinic orbits in the photogravitational restricted three-body problem     

K. E. Papadakis 《Astrophysics and Space Science》2006,302(1-4):67-82

We study numerically the asymptotic homoclinic and heteroclinic orbits around the hyperbolic Lyapunov periodic orbits which emanate from Euler's critical points L ₁ and L ₂, in the photogravitational restricted plane circular three-body problem. The invariant stable-unstable manifolds associated to these Lyapunov orbits, are also presented. Poincaré surface of sections of these manifolds on appropriate planes and several homoclinic and heteroclinic orbits for the gravitational case as well as for varying radiation factor q ₁, are displayed. Homoclinic-homoclinic and homoclinic-heteroclinic-homoclinic chains which link the interior with the exterior Hill's regions, are illustrated. We adopt the Sun-Jupiter system and assume that only the larger primary radiates. It is found that for small deviations of its value from the gravitational case (q ₁ = 1), the radiation pressure exerts a significant impact on the Hill's regions and on these asymptotic orbits.  相似文献