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惯性重力波与涡旋运动

Inertia-Gravity Waves and Vortical Flows

  • 摘要: 本文基于尺度分析和量阶估计研究了正压地球流体在适应过程与演变过程中的惯性重力波与涡旋运动,着重探讨了在地转适应过程和准地转演变过程两个不同动力学阶段中各种因素对于地转偏差以及惯性重力波波源的贡献. 对于线性小扰动情况,若不计\beta效应,f平面上的小扰动经地转适应过程达到常定的地转平衡,该常定的地转平衡状态将保持下去,不再激发出惯性重力波等非地转运动. 计入\beta效应,\beta平面上的小扰动,经适应过程后进入准地转演变过程,非常定的演变过程将造成位势场起伏,进而产生地转偏差并激发出新的惯性重力波. 对于完全的非线性情况,不计\beta效应,在演变过程阶段,由于运动为非常定,本已处于准地转状态的涡旋运动通过非线性作用即通过广义位势涡度平流项的作用,在位势涡度守恒的约束下,通过改变位势通量散度而产生新的地转偏差,从而激发出新的惯性重力波. 对于Burger数Bu \ll 1即运动尺度L远大于Rossby变形半径L_d的情况,必须同时计入\beta效应和广义位势涡度平流的影响,二者在位势涡度守恒的约束下,通过改变位势通量散度产生地转偏差,激发出新的惯性重力波.

     

    Abstract: Based on scale analysis and order estimation, the inertia-gravity waves and vortical flows of barotropic geophysical fluid are investigated in the adjustment and evolution processes, and the contribution of various factors to the ageostrophic modes and the source of inertia-gravity waves in the two different dynamic stages of geostrophic adjustment and quasi-geostrophic evolution are discussed. For the linear small perturbation case, if the \beta effect is not considered, the small perturbations in the f plane establish the steady geostrophic balance through the adjustment process, and the steady-state of geostrophic balance will be maintained, and no more ageostrophic modes of motion, such as inertia-gravity waves, will be excited. Considering the \beta effect, the motion on the \beta plane transitions the stage of quasi-geostrophic evolution process after the adjustment process, and the unsteady evolution process will cause fluctuations of the geopotential field, which in turn generate the ageostrophic perturbations and excite the new inertia-gravity waves. In the full nonlinear case, excluding \beta effect, in the evolution stage, under the constraint of conservation of potential vorticity, the unsteady quasi-geotrophic flows generate new ageostrophic modes of motion by altering the divergence of geopotential flux due to the generalized potential vorticity advection, thereby excites new inertia-gravity waves. For the Burger number Bu \ll 1, i.e., the spatial scale L is much greater than L_d, the Rossby radius of deformation, the effects of both the \beta effect and the advection of generalized potential vorticity have to be accounted for, which generate ageostrophic modes of motion by altering the potential flux divergence within the constraints of potential vorticity conservation, thereby exciting inertia-gravity waves.

     

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