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Numerical Simulation of Tropical Cyclone Development with the Use of Primitive Equations

机译:利用原始方程的热带气旋发展的数值模拟

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Based upon arguments by Syono and Yamasaki (1966), numerical experiments for simulating the developmental process of tropical cyclones are carried out with the use of primitive equations. Thermal effects of deep cumulus clouds are incorporated in the same manner as proposed by Ooyama (1964), and Charney and Eliassen (1964). The numerical experiments are performed using a four-layer model. The effect of surface friction is included through the equations of motion applied to the lowest level. Latent heat released by cumulus clouds is distributed to two tropospheric layers, and the heat partition ratio is assumed to be timeindependent.In a case in which 57 per cents of released latent heat is given to the upper troposphere and 43 per cents to the lower one, a given weak vortex develops to the mature stage in about 8 days. The structure of the computed tropical cyclone is similar to that of observed tropical cyclones. The deviation from the gradient wind balance is notable in the upper level near the center. The ratio of kinetic energy production to released latent heat increases with time and it attains 3 per cents at the mature stage.In order to investigate the relation between the gr iwth rate (and structure) of computed tropical cyclones and various physical parameters (such as mixing ratio of water vapor of surface air q, heat partition ratio to the lower troposphere 1, static stability S, the Coriolis parameter f and the drag coefficient CD), several numerical experiments are carried out. The horizontal scale of computed tropical cyclones is decreased with decrease of the Coriolis parameter. The experiments further reveal that the growth rate of cyclones is very sensitive to the static stability of the lower layer. In a case in which 70% of released latent heat is given to the upper layer, a given vortex does not develop. The growth rate of computed tropical cyclones is increased with increase of q, l and CD.
机译:基于Syono和Yamasaki(1966)的论证,利用原始方程进行了模拟热带气旋发展过程的数值实验。深积云的热效应与Ooyama(1964)以及Charney and Eliassen(1964)提出的方法相同。数值实验是使用四层模型进行的。通过应用到最低级别的运动方程,可以包括表面摩擦的影响。积云释放的潜热被分配到两个对流层,并且热分配比被认为与时间无关。在这种情况下,对流层高层释放的潜热为57%,下层对流层释放的潜热为43% ,大约8天后,给定的弱涡就会发展到成熟阶段。计算得到的热带气旋的结构与观测到的热带气旋的结构相似。与梯度风平衡的偏差在中心附近的上层明显。动能产生与释放潜热的比率随时间增加,在成熟阶段达到3%。为了研究热带气旋的增长率(和结构)与各种物理参数(例如地面空气水蒸气的混合比q,对流层下部的热分配比1,静态稳定性S,科里奥利参数f和阻力系数CD),进行了几个数值实验。计算的热带气旋的水平尺度随着科里奥利参数的减小而减小。实验还表明,旋风分离器的生长速率对下层的静态稳定性非常敏感。在释放的潜热的70%提供给上层的情况下,不会产生给定的涡流。随着q,l和CD的增加,计算得到的热带气旋的增长率增加。

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