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Numerical Simulation of Andhra Severe Cyclone (2003): Model Sensitivity to the Boundary Layer and Convection Parameterization

机译:安德拉强旋风的数值模拟(2003年):模型对边界层的敏感性和对流参数化

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The Andhra severe cyclonic storm (2003) is simulated to study its evolution, structure, intensity and movement using the Penn State/NCAR non-hydrostatic mesoscale atmospheric model MM5. The model is used with three interactive nested domains at 81, 27 and 9 km resolutions covering the Bay of Bengal and adjoining Indian Peninsula. The performance of the Planetary Boundary Layer (PBL) and convective parameterization on the simulated features of the cyclone is studied by conducting sensitivity experiments. Results indicate that while the boundary layer processes play a significant role in determining both the intensity and movement, the convective processes especially control the movement of the model storm. The Mellor-Yamada scheme is found to yield the most intensive cyclone. While the combination of Mellor-Yamada (MY) PBL and Kain-Fritsch 2 (KF2) convection schemes gives the most intensive storm, the MRF PBL with KF2 convection scheme produces the best simulation in terms of intensity and track. Results of the simulation with the combination of MRF scheme for PBL and KF2 for convection show the evolution and major features of a mature tropical storm. The model has very nearly simulated the intensity of the storm though slightly overpredicted. Simulated core vertical temperature structure, winds at different heights, vertical winds in and around the core, vorticity and divergence fields at the lower and upper levels—all support the characteristics of a mature storm. The model storm has moved towards the west of the observed track during the development phase although the location of the storm in the initial and final phases agreed with the observations. The simulated rainfall distribution associated with the storm agreed reasonably with observations.
机译:使用宾州/ NCAR非静水中尺度大气模型MM5模拟了安得拉严重气旋风暴(2003),以研究其演变,结构,强度和运动。该模型与分辨率为81、27和9 km的三个交互式嵌套域一起使用,覆盖孟加拉湾和毗邻的印度半岛。通过进行敏感性实验研究了行星边界层(PBL)的性能和对流旋风模拟特征的对流参数化。结果表明,尽管边界层过程在确定强度和运动方面都起着重要作用,但对流过程尤其控制着模型风暴的运动。发现Mellor-Yamada方案产生了最强烈的旋风。 Mellor-Yamada(MY)PBL和Kain-Fritsch 2(KF2)对流方案的组合产生了最强烈的风暴,而MRF PBL和KF2对流方案在强度和航迹方面产生了最佳模拟。结合MRF方案对PBL和KF2进行对流的模拟结果显示了成熟热带风暴的演变和主要特征。该模型几乎完全模拟了风暴的强度,尽管有点高估了。模拟的岩心垂直温度结构,不同高度的风,岩心内部和周围的垂直风,上下两层的涡度和发散场均支持成熟风暴的特征。尽管开发初期和最终阶段的风暴位置与观测结果一致,但在开发阶段,模型风暴已向观测轨道的西侧移动。与暴风雨有关的模拟降雨分布与观测值合理吻合。

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