台风中涡旋波1波扰动的形成机制及其变化特征

The formation mechanism and change characteristics of the wavenumber-1 vortex Rossby wave in the typhoon

  • 摘要: 通常将台风中的螺旋云带看成是一种称为涡旋罗斯贝波的波动,双臂对应的切向波数为2,单臂对应的切向波数为1,目前这种波动发生发展的物理机制仍不很清楚,值得进一步研究。利用柱坐标下的正压流体涡度方程,研究了台风中涡旋罗斯贝波1波扰动的正压不稳定性及发展变化问题。结果表明,当基本流径向涡度梯度小于0时,由于涡度扰动的速度场对于基本涡度场的平流效应,1波(m=1)扰动可从基本流吸取能量而出现不稳定快速增长。但由于扰动旋臂的缠卷作用,径向速度将很快变小,因此,不稳定增长将受到一定的时间限制;波动的发展速度与半径有关,中心附近的波动先发展且向外传播,距中心较远的波动稍后发展。整体上看,波动由中心向外扩展,大尺度台风的螺旋云带比小尺度台风的螺旋云带发展更快。

     

    Abstract: The spiral cloud bands usually are regarded as one type of wave named the vortex Rossby waves among which the double arm corresponds to the tangential wavenumber-2, and the single arm corresponds to tangential wavenumber -1. At the present the vortex Rossby wave’s mechanism still needs further studies. This article, by applying the barotropic fluid vorticity equation of cylindrical coordinates, studied the bartropic instability and change process of the vortex Rossby wave in a typhoon, and the results show that when the vorticity gradient of the basic flow is below zero, the vortex Rossby wave of wavenumber-1 may absorb energy from the base flow and then grow very quickly, which is attributed to the strong advection effect that vorticity is transferred from basic flow to fluctuation. Because the base flow entangles tight the perturbation, the radial velocity fast turns to be very small and therefore the unstable growth rate will be limited. In addition, the speed of fluctuation’s development is related to its radius. The fluctuation near the vortex center develops firstly and then disseminates while the non-centric fluctuation develops later. Also, the research indicates that the spiral cloud bands of a large scale typhoon develops faster than those of a small scale typhoon do.

     

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