Thermal versus isothermal rotating shallow water equations: comparison of dynamical processes by simulations with a novel well-balanced central-upwind scheme

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2020-06-15 DOI:10.1080/03091929.2020.1774876
A. Kurganov, Yongle Liu, V. Zeitlin
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引用次数: 10

Abstract

ABSTRACT We introduce a new high-resolution well-balanced central-upwind scheme for two-dimensional rotating shallow water equations with horizontal temperature/density gradients – thermal rotating shallow water equations. The scheme maintains the equilibrium states in the presence of topography and temperature/density variations, and allows for high-resolution tracking of the active scalar field together with velocity and pressure fields. We use the new scheme to highlight both the similarities and differences in the predictions of the thermal and isothermal shallow water models for the fundamental dynamical processes: evolution of isolated vortices in the midlatitude β-plane in the presence of topography and relaxation of localised pressure and temperature perturbations in the equatorial β-plane.
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热与等温旋转浅水方程:用一种新的良好平衡的中心迎风方案模拟动力学过程的比较
摘要:本文提出了一种新的高分辨率的具有水平温度/密度梯度的二维旋转浅水方程的良好平衡中心迎风格式——热旋转浅水方程。该方案在存在地形和温度/密度变化的情况下保持平衡状态,并允许高分辨率跟踪活动标量场以及速度和压力场。我们使用新的方案来强调热和等温浅水模式对基本动力过程的预测的异同:在地形存在下中纬度β平面孤立涡的演化和赤道β平面局部压力和温度扰动的松弛。
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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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