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排序方式: 共有137条查询结果,搜索用时 15 毫秒
11.
Frontal upwelling is an important phenomenon in summer in the Yellow Sea (YS) and plays an essential role in the distribution of nutrients and biological species. In this paper, a three-dimensional hydrodynamic model is applied to investigate the characteristics and influencing factors of frontal upwelling in the YS. The results show that the strength and distribution of frontal upwelling are largely dependent on the topography and bottom temperature fronts. The frontal upwelling in the YS is stronger and narrower near the eastern coast than near the western coast due to the steeper shelf slope. Moreover, external forcings, such as the meridional wind speed and air temperature in summer and the air temperature in the preceding winter and spring, have certain influences on the strength of frontal upwelling. An increase in air temperature in the previous winter and spring weakens the frontal upwelling in summer; in contrast, an increase in air temperature in summer strengthens the frontal upwelling. When the southerly wind in summer increases, the upwelling intensifies in the western YS and weakens in the eastern YS. The air temperature influences the strength of upwelling by changing the baroclinicity in the frontal region. Furthermore, the meridional wind speed in summer affects frontal upwelling via Ekman pumping. 相似文献
12.
Analysis of ocean fronts' uncertainties indicates that they result from indiseemibility of their spatial position and fuzzi-ness of their intensity. In view of this, a flow hierarchy for uncertainty representation of ocean fronts is proposed on the basis of fuzzy-rough set theory. Firstly, raster scanning and blurring are carried out on an ocean front, and the upper and lower approximate sets, the indiscernible relation in fuzzy-rough theories and related operators in fuzzy set theories are adopted to represent its uncer-tainties, then they are classified into three sets: with members one hundred pereent belonging to the ocean front, belonging to the ocean front's edge and definitely not belonging to the ocean front. Finally, the approximate precision and roughness degree are util-ized to evaluate the ocean front's degree of uncertainties and the precision of the representation. It has been proven that the method is not only capable of representing ocean fronts' uncertainties, but also provides a new theory and method for uncertainty representation of other oceanic phenomena. 相似文献
13.
Shocks propagating in the interstellar medium (ISM) play an important role in the life of molecular clouds. Through a theoretical study of interaction between clouds and shocks we can understand, for example, the density distribution of observed molecular clouds and the first steps of star formation. The only way to study of interaction in detail is via a numerical hydrodynamical simulation. In this paper we present the first results of a hydrocode which is able to follow the processes after the collision between the cloud and shock front.Our main theoretical result is that the chemical processes (e.g. H2 dissociation) can affect the dynamical processes significantly. Global parameters of the cloud are calculated for the comparision of the simulation and the observations. 相似文献
14.
K. V. Krasnobaev 《Astronomy Letters》2002,28(9):594-600
The effect of a time-varying radiation flux incident on an ionization front on the generation of ionization-shock front oscillations in the interstellar medium is analyzed analytically and numerically. We take into account both variations in the flux of ionizing radiation directly from the source that produces the ionization front and the absorption of energetic photons by the post-front plasma. Based on our calculations, we show that the time dependence of the radiation flux can be an additional factor (apart from small inhomogeneities in the interstellar medium) that contributes to the amplification of oscillations and to the kinetic energy input to the observed turbulent motions in H II regions. 相似文献
15.
16.
Transverse secondary circulations involving surface convergence, observed in a well-mixed estuary in North Wales, are made visible by the collection of surface material along an axial line which extends continuously for many kilometres through the estuary. The circulation and axial convergence, however, are seen only during the flood phase of the tide and no similar behaviour has been observed during the ebb phase.Convergent circulations in the estuary are associated with small but steady transverse density gradients in the cross-section, produced by non-uniform advection of the longitudinal gradient through the channel. A diagnostic model, using measured mean distributions of cross-sectional density, indicates surface transverse velocities (~0.1 ms?1) similar to those observed in the estuary. The model further predicts appreciable transverse divergent currents at a fractional depth of 0.75: a prediction which has been tested in the estuary using a vertical array of accurately resolving current direction indicators. 相似文献
17.
18.
一次典型梅雨锋锋面结构分析 总被引:16,自引:5,他引:11
1999年梅雨期在长江中下游维持着一条典型的梅雨锋 ,锋面和梅雨雨带呈东西走向 ,从中国的四川省一直延伸到日本。锋面两侧的温度及湿度对比明显 ,并且其上有数个中间尺度的低涡沿梅雨锋依次向东移动发展 ,在长江中下游造成严重的梅雨暴雨和洪涝。文中分析了 1999年这次典型梅雨锋的锋面结构。结果表明 ,从温度场看 ,由于梅雨区对流和降水的显著发展 ,梅雨锋的低层温度对比几近消失 ,其中上部仍具有典型的上宽下窄的锋面结构 ,锋面随高度向北倾斜。在低层经向温度场呈现复杂的暖 -冷 -暖的结构 ,即北部华北平原为地面感热加热造成的相对较暖的变性极地大陆气团 ,中间为冷空气南下和降水冷却造成的相对较冷的梅雨区 ,南部是相对较暖的热带海洋气团。在这种温度场下 ,由北部低层变性暖气团与梅雨区偏冷空气形成了明显的温度对比区 ,文中定义这个区域为梅雨赤道锋。因而 ,在低层东亚梅雨区的锋区结构由梅雨赤道锋和减弱的梅雨锋构成。在 6 0 0hPa以上前者消失 ,只有单一的极锋型的梅雨锋结构。在此分析的基础上文中给出了东亚梅雨期锋面结构模型图。另外还指出 ,从假相当位温场分析 ,主要表现出梅雨区的深厚对流。降雨引起了高θse带及其南北高θse梯度区 ,其北侧高θse梯度区大致相当于梅雨锋 ,而南侧高θs 相似文献
19.
Dynamic link between the level of ductile crustal flow and style of normal faulting of brittle crust
In a rheologically layered crust, compositional layers have an upper, elasto-plastic part and a lower, viscous one. When broken, the upper elastic part undergoes flexure, which is upward for the foot-wall and downward for the hanging wall. As a consequence of bending, stresses will develop locally that can overcome the strength of the plate and, therefore, impose the migration of active fault. In the lower, viscous part of each compositional layer, rocks can potentially flow. Numerical modelling of the behaviour of a crust made up of two compositional layers, during and following extension, shows that flow can take place not only in the lower crust but also, and more importantly, in the lower part of the upper crust. The ability of crustal rocks to flow influences the style and kinematics of rifted regions. When no flow occurs, subsidence will affect the extending areas, both hanging wall and foot-wall will subside with respect to an absolute reference frame such as sea level, and there will be a strict proportionality between extension and thinning. In addition, the downward movement of the fault blocks will decrease the local stresses created in the foot-wall and increase those of the hanging wall, thereby imposing a migration of fault towards the hanging wall. This is the behaviour of extensional settings developed on stabilised crust and which evolved in a passive margin. When flow does take place, middle crustal rocks will move towards the rifting zone causing isostatically driven upward movements that will be superimposed on movements associated with crustal and lithospheric thinning. Consequently, fault blocks will move upwards and the crust will show more extension than thinning. The upward movements will decrease the stresses developed in the hanging walls and increase those of the foot-wall. Faults will then migrate towards the foot-wall. Such a mode of deformation is expected in regions with thickened crust and has its most apparent expression in core complexes. 相似文献
20.
We investigated the dynamics of upwelling fronts near a coast. This work was first motivated by laboratory experiments [Bouruet-Aubertot, Linden, Dyn. Atmos. Oceans, 2002] in which the front is produced by the adjustment of a buoyant fluid initially confined within a bottomless cylinder. It was shown that cyclonic eddies consisting of coastal waters are enhanced when the front is unstable near the coast (the outer vertical boundary). The purpose of this paper is to provide further insights into this process. We reproduced the experimental configuration using a three-dimensional model of the primitive equations. We first show that for coastal fronts more potential energy, in terms of the maximum available potential energy, is released than for open-ocean fronts. Therefore, waves of larger amplitude are generated during the adjustment and the mean flow that establishes has a higher kinetic energy in the former case. Then as baroclinic instability starts and wave crests reach the boundary, cyclonic eddies are enhanced as in the laboratory experiments and in a similar way. However, in contrast to the laboratory experiments, offshore advection of cyclonic eddies can occur in two stages, depending on the spatial organization of the baroclinic wave. When the baroclinic wave consists of the sum of different modes and is thus highly asymmetric, the offshore advection of cyclonic eddies occurs just after their enhancement at the boundary, as in the laboratory experiments. By contrast, when a single-mode baroclinic wave develops, neighboring cyclonic eddies first merge before being advected offshore. Very different behavior is observed for open-ocean fronts. First a mixed baroclinic–barotropic instability grows. Then the eddies transfer their energy to the mean flow and the barotropic and baroclinic instabilities start again. An excellent agreement is obtained with the main result obtained in the laboratory experiments: the ratio between growth rates of surface cyclonic and anticyclonic vorticity increases as the instability develops nearer to the coast. 相似文献