The spontaneous generation of inertia-gravity waves during frontogenesis forced by large strain: numerical solutions
The spontaneous generation of inertia-gravity waves during frontogenesis forced by large strain: numerical solutions
复制标题
大应变迫使锋生过程中惯性重力波的自发产生:数值解
DOI:
10.1017/jfm.2015.197
复制
发表时间:
2015
影响因子:
3.7
通讯作者:
Shakespeare C
中科院分区:
文献类型:
--
作者:
Shakespeare C
A fully nonlinear numerical model is used to investigate spontaneous wave generation during two-dimensional frontogenesis forced by a horizontal strain field. The model uses the idealised configuration of an infinitely long straight front and uniform potential vorticity, with a uniform imposed convergent strain across the front. Shakespeare & Taylor (J. Fluid Mech., vol. 757, 2014, pp. 817–853) formulated a generalised analytical model (ST14) for this system that extends the classical Hoskins & Bretherton (J. Atmos. Sci., vol. 29, 1972, pp. 11–37) model (HB) to large strain rates (), the confinement of the secondary circulation and the spontaneous generation of waves, predicted by ST14, are shown to be important corrections to the HB solution. These inviscid predictions are also robust for an equilibrated front where strain-forced frontogenesis is balanced by diffusion. For strong strains the wavefield becomes of leading-order importance to the solution. In this case the frontal circulation is tightly confined, and the vertical velocity is an order of magnitude larger than in the HB model. The addition of a strain field that weakens with time allows the release and propagation of the spontaneously generated waves. We also consider fronts with both large vorticity and strain rate, beyond the validity of the ST14 model.