4.3 Article

Temporal variability of the current in the northeastern South China Sea revealed by 2.5-year-long moored observations

Journal

JOURNAL OF OCEANOGRAPHY
Volume 71, Issue 4, Pages 361-372

Publisher

SPRINGER
DOI: 10.1007/s10872-015-0295-3

Keywords

Northeastern South China Sea; Seasonal variabilities; Intraseasonal variabilities; Mesoscale eddies; Circulation

Categories

Funding

  1. National Key Basic Research Program of China (Program 973) [2014CB745003]
  2. National Key Scientific Research Project the South China Sea Deep [91028008]
  3. National Natural Science Foundation of China [41176010, 41176008]
  4. Strategic Priority Research Program of the Chinese Academy of Sciences [XDA11010202]
  5. Sanya Institute of Deep-Sea Science and Engineering [SIDSSE-201207]

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The current in the northeastern South China Sea (NSCS) has been extensively studied by both observations and numerical models, but its vertical structure and temporal variability are still not well understood because of the lack of long-term and full-depth direct observations. From August 2010 to March 2013, the current velocity in the NSCS was directly observed by Acoustic Doppler Current Profilers from a subsurface mooring at 117A degrees 52.07'E, 21A degrees 06.68'N. The observed current velocity was coherent in the vertical direction and nearly showed the same sign in the nearly full water column (960 m). The observed current presented strong intraseasonal variabilities (ISVs) within periods between 30 and 90 days. Analysis of the altimeter observation suggested that the ISVs were closely related to the propagating mesoscale eddies. Corresponding to the seasonally varying circulation in the NSCS, the ISV-removed current roughly showed a semiannual cycle. The seasonal U (V) averaged over 80-200 m depths reached the peak in March and October (January and July) and the trough in July and February (April and August), respectively, with a peak-to-trough amplitude of 0.14 m/s (0.19 m/s). Dynamical modes analysis suggested that the observed current velocity showed dominated energy in the barotropic mode during most of the observation period but enhanced energy in the first baroclinic mode during eddy events because of the enhanced vertical shear of velocity.

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