分数布朗运动的小波分析     

王桥  胡毓钜 《武汉大学学报(信息科学版)》1995,(1)

给出了分数布朗运动的连续和离散小波分析，讨论了有关的性质，并将结果用于分维估值、分数布朗运动小波变换系数的相关性研究等方面．  相似文献   

VENTILATION FLOW IN A BAROCLINIC VORTEX RELATED TO TROPICAL CYCLONE MOTION   总被引：1，自引：0，他引：1       下载免费PDF全文

田永祥 《Acta Meteorologica Sinica》1995,(3)

The tropical cyclone motion is numerically simulated with a quasi-geostrophic baroclinic model.The flow field of a tropical cyclone is decomposed into its axisymmetric and asymmetric components.The relation between the ventilation flow vector and the motion vector of the tropical cyclone is inves-tigated.The results of numerical experiments indicate:(1) There are both large-scale beta gyres andsmall-scale gyres in the asyrnmetric flow field.(2) The interaction between small-scale gyres andlarge-scale beta gyres leads to the oscillation of translation speed and translation direction for the tropi-cal cyclone.(3) There are the large deviations between the ventilation flow vector calculated bymeans of Fiorino and Elsberry's method and the motion vector of tropical cyclone.(4) The ventila-tion flow vector computed using the improved method closely correlates with the motion vector of thetropical cyclone.  相似文献   

阴山山链隆起机制及有关问题探讨   总被引：9，自引：0，他引：9  

张振法 《内蒙古地质》1995,(Z1)

阴山隆起为异常地幔发育区，软流层上凸、岩石圈变薄、幔汁上侵、地幔底辟，垂直运动激烈；阴山隆起又处在南北两大板块夹击挤压构造带上，水平运动强烈。所以，阴山隆起是中新生代垂直运动和水平运动共同作用的结果。随着阴山山链的隆起，在其南缘形成了呼包、临河等地堑式盆地。  相似文献   

非平衡热力学在短期灾害性天气预报中的应用     

钱维宏 《地球科学进展》1993,8(1):39-42

综述了非平衡热力学应用于天气预报的若干进程以及在短期灾害性天气预报应用中的明显效果。  相似文献   

新地震区划图的几个基本问题     

高孟潭  鄢家全 《中国地震》1993,9(2):97-103

我国新的地震区划图(1990年版)是采用地震危险性慨率分析方法编制的。该图给出的是场点地震烈度值,该值在50年内被突破的概率为0.1。人们普遍关注该图与我国曾经编制的地震区划图(1957年版,1977年版)的区别,该图超越概率概念的内含和外延以及超越概率水平为什么采用50年超越概率0.1。本文围绕这些问题进行了讨论。分析结果表明,前两张地震区划图编图的基本着眼点都是地震预测,而新的地震区划着眼于场点的地震动预测。新的地震区划图是按场点地震危险性分析方法给出的,它所表示的地震危险性只能针对具体的场点,不能完全反映区域的地震危险性特征。而弄清场点地震危险性和区域地震危险性的差异是正确进行区域防灾对策的基础。作者希望这些讨论能对正确使用新的地震区划图有所裨益。  相似文献   

Unrestricted Planar Problem of a Symmetric Body and a Point Mass. Triangular Libration Points and Their Stability     

Krzysztof Goździewski  Andrzej J. Maciejewski 《Celestial Mechanics and Dynamical Astronomy》1999,75(4):251-285

  相似文献   

双向近场地震作用下HDR隔震梁桥地震响应研究     

李琛  徐文平  孟宪锋  赵国辉  李宇 《震灾防御技术》2020,15(1):67-76

以HDR隔震梁桥多自由度（MDOF）模型和等效双线性单自由度（SDOF）模型为研究对象，以典型近场地震动作为输入，研究HDR支座双向耦合效应对HDR隔震梁桥地震响应的影响。研究结果表明:不考虑双向耦合效应的HDR支座滞回曲线呈典型双线性；考虑双向耦合效应的HDR支座滞回曲线面积小于不考虑双向耦合效应的HDR支座滞回曲线面积。不考虑双向耦合效应的顺桥向HDR支座位移峰值d_b大于考虑双向耦合效应时，但横桥向的结果相反。近场地震作用下，对梁桥进行HDR支座隔震设计时，忽略双向耦合效应计算得到的墩底剪力峰值和弯矩峰值均偏于保守。可忽略HDR支座双向耦合效应对HDR隔震梁桥近场地震能量的影响。  相似文献   

Wavelet analysis of the standard map: Structure and scaling     

A. D. Gilbert  C. Froeschlé  U. Frisch 《Celestial Mechanics and Dynamical Astronomy》1993,56(1-2):263-272

Wavelet analysis is applied to distributions of points generated by iterating the standard map. The initial condition is chosen so that the points fill the largest chaotic region. When the standard map parameterk=1.3, the distribution of points contains many voids corresponding to islands in the chaotic region. The wavelet transform is dominated by contributions from these islands. Fork=10 the chaos fills phase space and no structure is apparent; the wavelet transform reveals statistical fluctuations in the distribution of points.  相似文献   

Adiabatic invariants for the nonconservative Kepler's problem     

Djordje S. Djukic 《Celestial Mechanics and Dynamical Astronomy》1993,56(4):523-540

This paper considers adiabatic invariants for the classical Kepler problem with resisting forces. The analysis is based on the theory of integrating factors and theory of adiabatic invariants in the Krylov-Bogoliubov-Mitropolski variables. The adiabatic invariants are series with respect to a small parameter. Also, for every particular case of nonconservative forces, it is shown that, with a complete set of adiabatic invariants, an approximate solution of the problem can be obtained. Four problems are analyzed in detail where approximate solutions are compared with numerical.  相似文献   

One more explanation of superluminal motion     

V. Krishan 《Journal of Astrophysics and Astronomy》1988,9(4):231-236

The occurrence of superluminal motion in extragalactic radio sources is believed to be quite common. Among others, the geometrical scattering of radio radiation can also cause superluminal expansion and or motion and halo formation, In this paper, the effectiveness of the stimulated Raman scattering in producing these features is investigated. The scattering medium is a plasma whose position, density and temperature decide the rate and angle of scattering. When the radiation from a stationary and constant source gets scattered from a stationary plasma, a halo is formed around the source. However, the scattering of a rotating radiation beam does produce superluminal motion of the virtual source. It is found that the plasma should have the characteristics of the emission-line regions and the intercloud medium in order to Raman scatter the radiation. Since the scattering is polarization dependent, it is possible to estimate the rotation of the electric vector along the direction of the apparent motion of a radio source.  相似文献