Intra-seasonal variability of the abyssal currents in COMRA’s contract area in the Clarion-Clipperton Zone     

Fangfang Kuang  Jing Cha  Junpeng Zhang  Aijun Pan  Hangyu Chen  Xiwu Zhou  Chunsheng Jing  Xiaogang Guo 《海洋学报(英文版)》2022,41(11):1-11

In this paper, the intra-seasonal variability of the abyssal currents in the China Ocean Mineral Resources Association (COMRA) polymetallic nodule contact area, located in the western part of the Clarion and Clipperton Fraction Zone in the tropical East Pacific, is investigated using direct observations from subsurface mooring instruments as well as sea-surface height data and reanalysis products. Mooring observations were conducted from September 13, 2017 to August 15, 2018 in the COMRA contact area (10°N, 154°W). The results were as follows: (1) At depths below 200 m, the kinetic energy of intra-seasonal variability (20?100 d) accounts for more than 40% of the overall low-frequency variability, while the ratio reaches more than 50% below 2 000 m. (2) At depths below 200 m, currents show a synchronous oscillation with a characteristic time scale of 30 d, lasting from October to the following January; the energy of the 30-d oscillation increases with depth until the layer of approximately 4 616 m, and the maximum velocity is approximately 10 cm/s. (3) The 30-d oscillation of deep currents is correlated with the tropical instability waves in the upper ocean.  相似文献   

绥中一次暴雪伴雷电天气过程的成因分析     

孟振雄  于亚薇  唐帅 《内蒙古气象》2014,(1):7-11

为了探讨绥中一次暴雪伴雷电天气过程的成因,利用常规观测资料、NCEP每6h间隔的1°×1°的再分析资料和营口多普勒雷达的资料,分析此过程的天气形势特点、高低空急流的作用、雷达回波的特征及反映动力、热力和水汽条件的相关物理量场的特征。结果发现:雷电发生在对流层中层的西南风急流和底层偏东风均处在最强的时刻,当对流云团发展到-20℃温度层时,温差起电产生雷电;雷电发生在低层850hPa附近存在的逆温层消失之后,同时配合低层水汽的辐合,产生了暴雪天气;雷电和强降雪发生在大气底层南风和北风转换的过程中,强降雪的时间与冷空气扩散加强的时间比较一致,当冷空气扩散到整个大气底层时强降雪结束;引起雷电和强降雪的对流不稳定层结主要处在对流层中层,并为上升运动的发生提供了动力和热力条件,促使雷电发生和强降雪的维持。  相似文献   

Z���ζϲ�ϵͳ����Ӧ�䶸��ʱ�շֲ�����ֵģ��     

王学滨  马冰  吕家庆  顾路 《大地测量与地球动力学》2014,34(1):63-67

????Z???ζ????????????????ο?????FLAC??3D??????о????????????????????????9??????????????????????й???????????????о?????????????λ???????м????????????????????м??????????????????????????????Щ??????????й???????Щ???????????й??????????????????????????д??????????????????????????  相似文献   

高光谱大气红外探测仪(AIRS)反演大气不稳定度指数在强对流天气个例中的应用试验   总被引：1，自引：0，他引：1  

刘辉  寿亦萱  漆成莉 《气象》2014,40(6):678-686

使用探空、NCEP-FNL,数据和高光谱分辨率大气垂直探测仪(AIRS)标准反演数据计算大气不稳定度指数,对2011年6月23日北京强对流天气发生前的本地及上游大气中不稳定能量进行分析研究。分析发现:利用08、14和20时探空数据计算的北京站不稳定度指数显示了在"6·23暴雨"过程发生前后北京上空不稳定能量变化,上游关键区无探空数据;利用NCEP和AIRS数据计算的不稳定度指数显示,强对流天气发生前,在北京的上游关键区大气处于极端不稳定状态(K指数大于40,SI指数小于一5),有利于强对流天气发生。文章的研究结果表明,探空数据时空分辨率较低,不利于监测强对流天气的发生;质量控制后AIRS数据计算的不稳定度指数可以监测对流天气的发生;空间分辨率较低的NCEP数据监测小范围大气不稳定层结能力较低。综上所述,AIRS反演产品具有弥补探空资料时空分辨率不足的优势,利用AIRS L2反演产品计算晴空大气不稳定度指数产品可以监测到"6·23暴雨"天气发生前上游关键区大气层结稳定度状态,为预报员决策提供有效的辅助信息。  相似文献   

排桩内支撑基坑典型失稳原因及处理对策分析          下载免费PDF全文

虞利军  王茸  陈敏军 《探矿工程》2014,41(6):77-79

排桩内支撑支护结构是软土地区建筑工程中常用的一种基坑支护结构型式。从设计和施工2方面对影响排桩内支撑支护结构稳定的因素进行了分析,并结合某基坑工程破坏实例,对排桩内支撑支护结构典型失稳原因进行了分析探讨,提出了处理对策。开挖结果表明处理措施安全有效。  相似文献   

Spatial pattern formation of a ratio-dependent predator—prey model     

林望 《海洋学报(英文版)》2010,29(9)

This paper presents a theoretical analysis of evolutionary process that involves organisms distribution and their interaction of spatially distributed population with diffusion in a Holling-III ratio-dependent predator--prey model, the sufficient conditions for diffusion-driven instability with Neumann boundary conditions are obtained. Furthermore, it presents novel numerical evidence of time evolution of patterns controlled by diffusion in the model, and finds that the model dynamics exhibits complex pattern replication, and the pattern formation depends on the choice of the initial conditions. The ideas in this paper may provide a better understanding of the pattern formation in ecosystems.  相似文献   

A benchmark comparison of numerical methods for infinite Prandtl number thermal convection in two-dimensional Cartesian geometry     

B. J. Travis  C. Anderson  J. Baumgardner  C. W. Gable  B. H. Hager  R. J. O'Connell 《地球物理与天体物理流体动力学》2013,107(3-4):137-160

Abstract

A comparison is made between seven different numerical methods for calculating two-dimensional thermal convection in an infinite Prandtl number fluid. Among the seven methods are finite difference and finite element techniques that have been used to model thermal convection in the Earth's mantle. We evaluate the performance of each method using a suite of four benchmark problems, ranging from steady-state convection to intrinsically time-dependent convection with recurring thermal boundary layer instabilities. These results can be used to determine the accuracy of other computational methods, and to assist in the development of new ones.  相似文献   

静力平衡近似下大气中非线性对称运动的稳定性、分岔和突变     

彭晓林  罗德海 《成都信息工程学院学报》1991,(Z1)

本文在考虑基本气流具有非线性切变情况下,导出了对称运动所满足的非线性常微分方程,并用非线性系统的稳定、分岔、突变理论,严格地讨论了非线性对称运动的稳定性、分岔和突变问题,获得了一个推广的对称不稳定判据,找到了突变产生的条件。  相似文献   

An explanation of the dimensions of penumbral filaments     

Zhou Dao-qi 《Chinese Astronomy and Astrophysics》1991,15(4):453-460

Unstable pertubation modes exist in the magnetic field of penumbral electric current and I think the penumbral filaments are formed from the development of such modes. Under the short wave approximation the non-adiabatic dispersion equation is solved in the radial and transverse directions of the sunspot. From the condition of instability the length and width of the penumbral filament can be evaluated and it is found that the filament mode is static in the direction of the length and is non-moving in the direction of the width, that the penumbral filaments are a feature of the sunspot magnetic flow under gravity and that the presence of the filaments implies the existence of a twisted magnetic field.  相似文献   

Plasma instability at the inner edge of the accretion disk—I     

S. C. Tripathy  C. B. Dwivedi  A. C. Das  A. R. Prasanna 《Journal of Astrophysics and Astronomy》1993,14(2):103-114

In this paper, the analytical and numerical results of the stability analysis of the accretion disk at the inner boundary is presented. Including the effect of finite conductivity in the disk dynamics, a simple calculation considering only the radial perturbation has been carried out. Within local approximation, it is concluded that the disk is stable to Kelvin-Helmholtz and resistive electromagnetic modes whereas the magnetosonic mode can destabilise the disk structure.  相似文献