登陆热带风暴Bilis（2006）暴雨特征及其可能原因   总被引：3，自引：1，他引：2  

滕代高  罗哲贤  代刊  黄新晴 《南京气象学院学报》2008,31(3):369-380

利用NCEP/NCAR 1°×1°格点再分析资料、FY-2C TBB（black bright temperature）资料及中国740站降水资料,对0604号强热带风暴Bilis登陆后的暴雨特征及其可能原因进行诊断分析,结果表明：（1）Bilis登陆过程中强降水中心位于风暴中心西北侧沿岸,主要影响福建和浙江两省;进入内陆后强降水中心向风暴中心以西转移,最后在风暴中心西南侧聚集,主要影响广东东北部、福建、江西和湖南南部。（2）西北太平洋副热带高压的稳定少动为Bilis陆上西行过程中产生持续性降水提供了稳定的背景场。（3）Bilis西南部季风环流的发展增强为Bilis登陆后强降水的产生提供了必要的水汽条件。（4）涡合并和自激增长形成的中尺度系统与风暴涡旋的相互作用,是Bilis登陆后产生强降水的可能机制。  相似文献   

Tripolar vortex in plasma flow     

J. Vranje 《Planetary and Space Science》1999,47(12):1531-1535

Strongly nonlinear processes in a two-component plasma with sheared flow, in the low-frequency limit, in comparison with the ion gyro frequency Ω_i, and for perturbations propagating perpendicularly to the ambient magnetic field are studied. In the linear domain such a system is prone to the development of instability of the Kelvin–Helmholtz type. In the nonlinear regime this instability can saturate into stationary travelling solutions of the form of vortex chains and tripolar vortices, which are found in this paper.  相似文献   

Vortical mechanism for collimation and acceleration of jets     

M. G. Abrahamyan 《Astrophysics》2008,51(3):357-371

A vortical mechanism for the collimation and acceleration of astrophysical jets is proposed on the basis of exact solutions of the hydrodynamic equations in a homogeneous gravitational field taking viscosity into account. Velocity profiles in the form of a jet structure with a uniformly rotating trunk whose pressure decreases in time, and longitudinal and converging radial flows of matter, are examined. Because of the radial flow, the angular velocity of the trunk and the velocity of the longitudinal flow of matter can accelerate exponentially or in the manner of an “explosive” instability. Flows of this type have low energy dissipation and can serve as unique channels for the acceleration and collimation of jet eruptions from young stars, as well as from active galactic nuclei and quasars. __________ Translated from Astrofizika, Vol. 51, No. 3, pp. 431–444 (August 2008).  相似文献   

On the merger of subsurface isolated vortices     

Daniele Ciani  Xavier Carton  Jacques Verron 《地球物理与天体物理流体动力学》2016,110(1):23-49

Vortex merger is a phenomenon characterizing the whole class of geophysical vortices, from atmospheric storms and large oceanic eddies up to small scale turbulence. Here we focus on the merger of subsurface oceanic anticyclones in an idealized primitive equations model. This study has been motivated by past and recent observations of colliding lens-like anticyclones off of Gibraltar Strait. The critical conditions for merger (critical merger distance and time needed for merger) are determined. We will show that the predictions of classical two-dimensional merger are not verified for subsurface isolated vortices. For instance, critical merger distances will be reduced because of the vortex potential vorticity (PV) structure. The post-merger characteristics of the vortex (radius, extension and PV), are also determined. Merger-related effects, like production of peripheral filaments and small-scale eddies are also investigated and suggest the contribution of merger in both direct and inverse energy cascades.  相似文献   

夏季青藏高原低涡的切向流场及波动特征分析   总被引：4，自引：0，他引：4  

陈功  李国平 《气象学报》2011,69(6):956-963

从大气动力学原理出发,将高原低涡视为受热源强迫的边界层内涡旋,建立了柱坐标下满足梯度风平衡的低涡控制方程组,分析高原低涡切向流场的基本特征.在此基础上,通过求解线性化涡旋模式,得出高原低涡中各类波动的频散关系及其特征,同时定性讨论了热力作用对混合波动的影响以及混合波动与高原低涡流场特征的联系.使用中尺度数值模式WRF分...  相似文献   

The latest Carboniferous–Early Permian Dorud Group of the eastern Alborz (Iran): biostratigraphy and taxonomy of smaller foraminifers     

Zohreh Alipour  Seyyed Mahmood Hosseini‐Nezhad  Daniel Vachard  Koorosh Rashidi 《Geological Journal》2013,48(4):385-402

The latest Carboniferous–Early Permian Dorud Group in the Chaman‐Saver area of eastern Alborz, Iran is more than 222 m thick and includes thick sequences of oncolitic limestone, sandy limestone, sandstones and shales. The Emarat and Ghosnavi formations of this Group are dated here as latest Gzhelian to early Sakmarian Stages. During the Asselian Stage, the sea level fell abruptly and epeirogenic episodes occurred. These events generated a broad, shallow carbonate platform suitable for the growth and diversity of smaller foraminifers in the Chaman‐Saver area which, consequently, displays faunal differences with the rest of the Alborz Mountains. Three foraminiferal biozones are proposed: Nodosinelloides potievskayae–Vervilleina bradyi Zone (latest Gzhelian), Calcitornella heathi–Nodosinelloides sp. Zone (latest Gzhelian–Asselian), and Rectogordius iranicus n. gen. n. sp.–Hemigordius schlumbergeri Zone (early Sakmarian). The new taxa described herein include: Pseudovidalina iranica n. sp., P. damghanica n. sp., Rectogordius iranicus n. gen. n. sp. and Tezaquina sp. 1. Copyright © 2012 John Wiley & Sons, Ltd.  相似文献   

“7.17”西北夏季沙尘暴数值模拟   总被引：4，自引：3，他引：1  

赵建华  张强  李耀辉  刘世祥  隆霄 《中国沙漠》2009,29(6):1221-1228

 对2005年7月17日发生在西北地区近20 a来夏季最强的沙尘暴过程进行了数值模拟研究,结果得到:①沙尘暴发生前,沙源处于高温控制下;②起沙是水平低涡和垂直涡叠加而成的一种类似于Benard对流泡的系统扫掠沙源的结果;③起沙主要发生在水平低涡移动方向的右部。  相似文献   

Large-scale structure of magnetospheric plasma     

T. E. Moore  D. C. Delcourt 《Surveys in Geophysics》1995,16(3):363-387

Recent investigations of magnetospheric plasma structure are summarized under the broad categories of empirical models, transport across boundaries, formation, and dynamics of the plasma sheet. This report reviews work in these areas during the period 1991 to 1993. Fully three-dimensional empirical models and simulations have become important contributors to our understanding of the magnetospheric system. Some new structural concepts have appeared in the literature: the entry boundary and geopause, the plasma sheet region 1 vortices, the low-energy layer, the adiabaticity boundary or wall region, and a region in the tail to which we refer as the injection port. Traditional structural concepts have also been the subject of recent study, notably the plasmapause, the magnetopause, and the plasma sheet. Significant progress has been made in understanding the nature of plasma sheet formation and dynamics, but the acceleration of electrons to high energy remains somewhat mysterious.  相似文献   

Structure of a pair of anticyclonic vortices in northern part of the South China Sea in autumn of 1994     

Fu Gang  Toshio Yamagata 《海洋学报(英文版)》2002,21(2):203-216

A pair of remarkable meso-scale anticyclonic vortices, one formed closely to another, inthe northern part of the South China Sea during the period from the later August to early September of 1994 were documented by the in situ observation data. Their spatial structures were examined in detail from the horizontal and two nearly perpendicular/vertical angles of view. It was shown that the horizontal scales of these two vortices were around 100, 50 km, and their vertical scales were about 500, 1000 m, respectively. Two "warm core" structures associated with these two vortices were found in their horizontal and vertical analyses. The closer spacing of these two vortices (namely, 60 km), which was smaller than the Rossby radius of deformation, suggested that they might merge with each other during their next evolution stages and form into a larger vortex eventually.  相似文献   

The rotational quenching of the rotation-induced kinetic alpha-effect     

V. V. Pipin  G. Rüdiger  L. L. Kitchatinov 《地球物理与天体物理流体动力学》2013,107(1-2):119-133

Abstract

A theory of the non-diffusive anisotropic kinetic alpha-effect (“Γ-effect”) for densitystratified rotating turbulent fluids is developed. No limitations on the rotation rate are imposed and the fully nonlinear dependence of the Γ-effect on the angular velocity is studied. When the Coriolis number, ω? = 2τ ω, is small the dimensionless “dynamo number”, Cτ, characterising the power of the Γ-effect, grows with ω?. The dependence, however, reaches a maximum for ω? ～ 2. For still higher rotation rates C_Λ decreases as 1/ω?. In opposition, the corresponding number, C_x, of the hydromagnetic α² -dynamo problems remains finite for very large ω?. Hence, for fast rotation the hydrodynamic Γ-effect is small while the hydromagnetic α-effect remains large. In consequence, the large-scale magnetic and velocity structures are expected to be generated with roughly equal power in slowly rotating objects. In the rapid rotators, however, generation of the large-scale flows is problematic.  相似文献