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A new general circulation model of Jupiter's atmosphere based on the UKMO Unified Model: Three-dimensional evolution of isolated vortices and zonal jets in mid-latitudes

机译:基于UKMO统一模型的木星大气新环流模型:中纬度孤立涡和纬向射流的三维演化

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We have been developing a new three-dimensional general circulation model for the stratosphere and troposphere of Jupiter based on the dynamical core of a portable version of the Unified Model of the UK Meteorological Office. Being one of the leading terrestrial GCMs, employed for operational weather forecasting and climate research, the Unified Model has been thoroughly tested and performance tuned for both vector and parallel computers. It is formulated as a generalized form of the standard primitive equations to handle a thick atmosphere, using a scaled pressure as the vertical coordinate. It is able to accurately simulate the dynamics of a three-dimensional fully compressible atmosphere on the whole or a part of a spherical shell at high spatial resolution in all three directions. Using the current version of the GCM, we examine the characteristics of the Jovian winds in idealized configurations based on the observed vertical structure of temperature. Our initial focus is on the evolution of isolated eddies in the mid-latitudes. Following a brief theoretical investigation of the vertical structure of the atmosphere, limited-area cyclic channel domains are used to numerically investigate the nonlinear evolution of the mid-latitude winds. First, the evolution of deep and shallow cyclones and anticyclones are tested in the atmosphere at rest to identify a preferred horizontal and vertical structure of the vortices. Then, the dependency of the migration characteristics of the vortices are investigated against modelling parameters to find that it is most sensitive to the horizontal diffusion. We also examine the hydrodynamical stability of observed subtropical jets in both northern and southern hemispheres in the three-dimensional nonlinear model as initial value problems. In both cases, it was found that the prominent jets are unstable at various scales and that vorteces of various sizes are generated including those comparable to the White Ovals and the Great Red Spot.
机译:我们已经基于英国气象局统一模型的便携式版本的动力核心,为木星的平流层和对流层开发了一个新的三维总体环流模型。作为用于运营天气预报和气候研究的领先的地面GCM之一,统一模型已经过矢量和并行计算机的全面测试和性能调整。它使用比例压力作为垂直坐标,被公式化为标准原始方程的广义形式,以处理浓厚的大气。它能够在所有三个方向上以高空间分辨率准确地模拟整个或部分球形壳的三维完全可压缩气氛的动力学。使用当前版本的GCM,我们根据观察到的温度垂直结构检查理想化配置下的木星风特征。我们最初的重点是中纬度地区孤立涡的演变。在对大气的垂直结构进行了简短的理论研究之后,使用有限区域循环通道域对中纬度风的非线性演化进行了数值研究。首先,在静止大气中测试深,浅旋风分离器和反旋风分离器的演变,以确定涡旋的首选水平和垂直结构。然后,针对模型参数研究了旋涡迁移特性的依赖性,发现其对水平扩散最为敏感。我们还检查了在三维非线性模型中作为初始值问题的北半球和南半球观测到的副热带急流的水动力稳定性。在这两种情况下,都发现突出的喷流在各种规模上都是不稳定的,并且产生了各种大小的旋涡,包括与白色椭圆形和大红色斑点相当的旋涡。

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