Mechanism for the formation of equatorial superrotation in forced shallow-water turbulence with Newtonian cooling
Mechanism for the formation of equatorial superrotation in forced shallow-water turbulence with Newtonian cooling
复制标题
牛顿冷却强迫浅水湍流中赤道超自转的形成机制
DOI:
10.1175/jas-d-14-0235.1
复制
发表时间:
2015
影响因子:
3.1
通讯作者:
Izumi Saito and Keiichi Ishioka
中科院分区:
文献类型:
--
作者:
高山和雄;三村菜摘;萩原康子;立花雅史;櫻井文教;神田勝弘;川端健二;水口裕之;辻 かおる;Izumi Saito and Keiichi Ishioka
Forced shallow-water turbulence on a rotating sphere with Newtonian cooling is examined with the aim of elucidating the mechanism of the robust formation of equatorial superrotation reported by R. K. Scott and L. M. Polvani. It is shown that the Newtonian cooling term distorts the structure of the Hough modes. This distortion can be visualized as either the westward or eastward tilting of the equiphase line with increasing absolute value of latitude; the structural change of the Hough modes leads to the acceleration of the zonal-mean flow. A statistical analysis based on a weak-nonlinear theory predicts that stochastically excited Hough modes generate a prograde equatorial jet, the profile of which is quantitatively consistent with that of the ensemble-averaged zonal-mean flow obtained in nonlinear time evolutions. The predicted prograde equatorial jet originates mainly from the acceleration produced by Rossby modes, the equiphase line of which is tilted westward by the Newtonian cooling term. This tilt of the equiphase line of the Hough modes is clarified and a comparison between the acceleration mechanism presented in the present paper and that in other numerical studies in which equatorial superrotation emerges is made.