Features of the Equatorial Intermediate Current Associated with Basin Resonance in the Indian Ocean

Author:

Huang Ke1,Han Weiqing2,Wang Dongxiao1,Wang Weiqiang13,Xie Qiang413,Chen Ju1,Chen Gengxin1

Affiliation:

1. a State Key Laboratory of Tropical Oceanography, South China Sea Institute of Oceanology, Chinese Academy of Sciences, Guangzhou, China

2. b Department of Atmospheric and Oceanic Sciences, University of Colorado Boulder, Boulder, Colorado

3. c Laboratory for Regional Oceanography and Numerical Modeling, Qingdao National Laboratory for Marine Science and Technology, Qingdao, China

4. d Institute of Deep-Sea Science and Engineering, Chinese Academy of Sciences, Sanya, China

Abstract

AbstractThis paper investigates the features of the Equatorial Intermediate Current (EIC) in the Indian Ocean and its relationship with basin resonance at the semiannual time scale by using in situ observations, reanalysis output, and a continuously stratified linear ocean model (LOM). The observational results show that the EIC is characterized by prominent semiannual variations with velocity reversals and westward phase propagation and that it is strongly influenced by the pronounced second baroclinic mode structure but with identifiable vertical phase propagation. Similar behavior is found in the reanalysis data and LOM results. The simulation of wind-driven equatorial wave dynamics in the LOM reveals that the observed variability of the EIC can be largely explained by the equatorial basin resonance at the semiannual period, when the second baroclinic Rossby wave reflected from the eastern boundary intensifies the directly forced equatorial Kelvin and Rossby waves in the basin interior. The sum of the first 10 modes can reproduce the main features of the EIC. Among these modes, the resonant second baroclinic mode makes the largest contribution, which dominates the vertical structure, semiannual cycle, and westward phase propagation of the EIC. The other 9 modes, however, are also important, and the superposition of the first 10 modes produces downward energy propagation in the equatorial Indian Ocean.

Funder

National Natural Science Foundation of China

Natural Science Foundation of Guangdong Province

Open Fund of the Key Laboratory of Ocean Circulation and Waves, Chinese Academy of Sciences

Major State Research Development Program of China

Research Project of State Key Laboratory of Tropical Oceanography

Publisher

American Meteorological Society

Subject

Oceanography

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