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Dynamics of 'critical' trajectories

机译:“关键”轨迹的动力学

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Two diagnostic dynamic models for flow in hyperbolic and elliptic regions of a geophysical fluid are developed and compared. As the main interest here is in local dynamical processes, these models are used to study trajectories near stagnation points in the flow field. The simplest model presumes a balance between the Coriolis and geopotential accelerations. This model is equivalent to the classic approach that characterizes these regimes by the quadratic equation for the eigenvalues of the velocity gradient. However, since that model imposes geostrophic dynamics, the eigenvalues of the velocity gradient can be replaced by the local curvature or Hessian of the geopotential scaled by Coriolis. The general model adds both local and inertial accelerations to the dynamical balance. In contrast to the classic result the consequent frequency equation is a quartic that involves both the Hessian of the geopotential field, the components of the velocity gradient, and Coriolis. Roots of this equation give two distinct time scales, which are interpreted as Lagrangian time scales. Motion of the geopotential field produces a third Eulerian time scale. Critical trajectories are those whose initial positions and velocities are such that they are independent of the Lagrangian time scales. These simple models establish that within hyperbolic and elliptic regions of the geopotential field there may be trajectories whose time scales differ radically from even their nearest neighbors. A characteristic of critical trajectories in the ocean is that they often are found near stagnation points. These may be hard to identify even in model simulations, but a similar quantity, the null in the geopotential gradient, might be easier to obtain. To analyze the relation between the critical trajectories, stagnation points, and gradient null, evolution models for the later two objects are proposed. For a steady geopotential all three coincide. However with a time varying geopotential, they are distinct even though all have the same time scale. The analysis provides a metric for the separation of all three objects.
机译:开发并比较了地球物理流体双曲线和椭圆形区域中流动的两个诊断动态模型。由于这里的主要兴趣在于局部动力学过程,因此这些模型用于研究流场中停滞点附近的轨迹。最简单的模型假定科里奥利加速度和地势加速度之间达到平衡。此模型等效于经典方法,该方法通过速度梯度特征值的二次方程式来表征这些状态。但是,由于该模型强加了地转动力学,因此速度梯度的特征值可以替换为由科里奥利定标的地势的局部曲率或Hessian。通用模型将局部和惯性加速度都添加到动态平衡中。与经典结果相反,结果频率方程是一个四次方程,涉及地势场的Hessian,速度梯度的分量和科里奥利。该方程的根给出了两个不同的时标,它们被解释为拉格朗日时标。地势场的运动产生了第三欧拉时标。临界轨迹是指其初始位置和速度与拉格朗日时间标度无关的轨迹。这些简单的模型确定,在地势场的双曲线和椭圆形区域内,可能存在一些轨迹,这些轨迹的时间尺度甚至与其最近的邻居都不相同。海洋中的关键轨迹的一个特征是它们经常在停滞点附近被发现。即使在模型仿真中,也可能很难识别出这些,但是类似的数量(地势梯度中的零)可能更容易获得。为了分析临界轨迹,停滞点和梯度零点之间的关系,提出了后两个物体的演化模型。对于稳定的地势,所有这三个都重合。但是,随着时间的变化,即使它们都具有相同的时间标度,它们也是不同的。该分析为所有三个对象的分离提供了度量。

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