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完整Coriolis力作用下非线性Rossby波的精确解 被引量:17

Exact solutions to the nonlinear Rossby waves with a complete representation of the Coriolis force
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摘要 从包含完整Coriolis力的Boussinesq近似的斜压大气运动方程组出发,利用半地转近似导出β效应和地球旋转水平分量fH=2Ωcosφ共同作用下的大气非线性Rossby波动所满足的KdV方程,求得了椭圆余弦波解和孤立波解.结果分析表明,若扰动与纬度有关,Coriolis参数分量fH将影响波动传播的频率特征,并加强水平散度对斜压Rossby波的作用;如果扰动与纬度无关,则Coriolis参数分量fH的影响消失. A horizontal component of the earth's rotation is included in a set of Boussinesq fluid equations, which have a constant horizontal component of the Coriolis parameter, while the vertical component varies with latitude. The nonlinear Rossby waves described by the KdV equation are derived. Its periodic-wave and soliton solution are also obtained. The results show that the fH =2Ω cosφ effect can be important if the perturbations are functions of the latitude. We also find that when the perturbations are independent of latitude, the fH effect disappears.
作者 赵强 于鑫
出处 《地球物理学报》 SCIE EI CAS CSCD 北大核心 2008年第5期1304-1308,共5页 Chinese Journal of Geophysics
基金 国家自然科学基金项目(40475023)资助
关键词 CORIOLIS力 β效应 ROSSBY波 Coriolis force, β effect, Rossby waves
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参考文献19

  • 1Phillips N A. The equations of motion for a shallow rotating atmosphere and the 'traditional approximation'. J. Atmos. Sci.. 1966, 23:626-628
  • 2Phillips N A, Reply to G. Veronis's comments on Phillips (1966). J. Atmos. Sci. , 1968, 25:1155-1157
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  • 4Wangsness R K. Comments on "The equations of motion for a shallow rotating atmosphere and the ' traditional approximation'". J. Atmos. Sci., 1970, 27:504-506
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二级参考文献11

  • 1[1]Phillips, N. A. , The equations of motion for a shallow rotating atmosphere and the "traditional approximation", J. Atmos. Sci. , 1966, 23, 626~628.
  • 2[2]Phillips, N. A. , Reply to G. Veronis' s comments on Phillips (1966), J. Atmos. Sci. , 1968, 25, 1155~ 1157.
  • 3[3]Veronis, G. , Comments on Phillips's (1966) proposed simplification of the equations of motion for a shallow ro tating atmosphere, J. Atmos. Sci. , 1968, 25, 1154~1155.
  • 4[4]Wangsness, R. K. , Comments on "The equations of motion for a shallow rotating atmosphere and the ‘ tradition al approximation'", J. Atmos. Sci. , 1970, 27, 504~506.
  • 5[5]Sun, W. -Y. , Unsymmetrical symmetric instability, Quart. J. Roy. Meteor. Soc. , 1995, 121, 419~431.
  • 6[6]White, A. A. , and R. A. Bromley, Dynamically consistent, quasi-hydrostatic equations for global models with a complete representation of the Coriolis force, Quart. J. Roy. Meteor. Soc. , 1995, 121, 399~418.
  • 7[7]Draghici, I. , Non-hydrostatic Coriolis effects in an isentropic coordinate frame, Meteor. Hydrol. , 1987, 17, 45~54.
  • 8[8]Leibovich, S. , and S. K. Lele, The influence of the horizontal component of the Earth's angular velocity on theinstability of the Ekman layer, J. Fluid Mech. , 1985, 150, 41~87.
  • 9[9]Burger, A. P. , The potential vorticity equation: from planetary to small scale, Tellus, 1991, 43A, 191~197.
  • 10[10]Grimshaw, R. H. J., A note on the β-plane approximation, Tellus, 1975, 27, 351~357.

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