Instabilities of low-latitude easterly jets in the presence of moist convection and topography and related cyclogenesis, in a simple atmospheric model

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2021-09-17 DOI:10.1080/03091929.2021.1959574
M. Rostami, V. Zeitlin
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引用次数: 1

Abstract

A simple two-layer model, the moist-convective rotating shallow water, which allows for low-cost high-resolution numerical simulations of the dynamics of the moist atmosphere in the presence of topography, is used to identify and understand dynamical processes governing the evolution of easterly waves propagating on the background of a low-latitude easterly jet crossing a land-sea boundary, a setup crudely representing the African Easterly Jet over the West-African plateau and the Atlantic ocean. We perform a thorough linear stability analysis and identify the unstable modes of the jet, which we use then for initialisation of fully nonlinear numerical simulations. In this way, we determine nonlinear evolution of unstable perturbations of the jet, both in the “dry” and moist-convective environments and highlight essential differences between the two cases. We identify a mechanism of formation of intense lower-layer cyclonic vortices at the northern flank of the jet and determine the influence of the land-sea contrast upon this process.
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在一个简单的大气模式中,存在湿润对流和地形以及相关的气旋形成的低纬度偏东急流的不稳定性
一个简单的两层模型,即水汽对流旋转浅水,允许低成本的高分辨率数值模拟地形存在下的潮湿大气动力学,用于识别和理解控制在低纬度东风急流穿越陆海边界的背景下传播的东风波演变的动力过程。这个装置大致代表了西非高原和大西洋上空的非洲东部急流。我们进行了彻底的线性稳定性分析,并确定了射流的不稳定模式,然后将其用于完全非线性数值模拟的初始化。通过这种方式,我们确定了在“干燥”和湿对流环境下射流不稳定扰动的非线性演变,并强调了两种情况之间的本质区别。我们确定了急流北侧强烈低层气旋涡旋的形成机制,并确定了海陆对比对这一过程的影响。
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来源期刊
Geophysical and Astrophysical Fluid Dynamics
Geophysical and Astrophysical Fluid Dynamics 地学天文-地球化学与地球物理
CiteScore
3.10
自引率
0.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: Geophysical and Astrophysical Fluid Dynamics exists for the publication of original research papers and short communications, occasional survey articles and conference reports on the fluid mechanics of the earth and planets, including oceans, atmospheres and interiors, and the fluid mechanics of the sun, stars and other astrophysical objects. In addition, their magnetohydrodynamic behaviours are investigated. Experimental, theoretical and numerical studies of rotating, stratified and convecting fluids of general interest to geophysicists and astrophysicists appear. Properly interpreted observational results are also published.
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