Intra-seasonal variability of the abyssal currents in COMRA’s contract area in the Clarion-Clipperton Zone
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Abstract: In this paper, the intra-seasonal variability of the abyssal currents in the China Ocean Mineral Resources Association (COMRA) polymetallic nodule contact area, located in the western part of the Clarion and Clipperton Fraction Zone in the tropical East Pacific, is investigated using direct observations from subsurface mooring instruments as well as sea-surface height data and reanalysis products. Mooring observations were conducted from September 13, 2017 to August 15, 2018 in the COMRA contact area (10°N, 154°W). The results were as follows: (1) At depths below 200 m, the kinetic energy of intra-seasonal variability (20−100 d) accounts for more than 40% of the overall low-frequency variability, while the ratio reaches more than 50% below 2 000 m. (2) At depths below 200 m, currents show a synchronous oscillation with a characteristic time scale of 30 d, lasting from October to the following January; the energy of the 30-d oscillation increases with depth until the layer of approximately 4 616 m, and the maximum velocity is approximately 10 cm/s. (3) The 30-d oscillation of deep currents is correlated with the tropical instability waves in the upper ocean.
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Figure 1. ETOPO1 depth of the eastern tropical Pacific Ocean, position of the mooring site (red triangle) and the section in c (a); depth around the mooring site (b); climatologic temperature (from World Ocean Atlas 2009) at a meridional section of 154°W (0°−20°N) and the observation range of current metres (red line represents the observation range of 75-kHz ADCPs at upper layers and the red dots below 1 200 m represent the location of Aquadopp current meters) (c).
Figure 3. Kinetic energy of intra-seasonal variability (ISV), low-frequency variability and their ratio. The blue circle line represents kinetic energy of low-frequency variability (Ke-low); the blue asterick line represents kinetic energy of ISV (Ke-isv); the red triangle line represents the ratio of Ke-isv and Ke-low.
Figure 6. Continuous wavelet transform of meridional velocity at surface current (a) and currents at 50−100 m (b), 450−500 m (c), 900−1 000 m (d), 1 854 m (e) , 4 616 m (f). The colour filled maps represent the wavelet power spectrum (WPS), and the curves on the right represent the global wavelet spectrum (GWS). In the colour maps, the thick black contours denote the 5% significance level against red noise. The cone of influence where edge effects might distort the picture is shown in lighter shades.
Figure 10. Spatial amplitude (a), spatial phase (b), spatial reconstruction (c), temporal amplitude (d), temporal phase (e), frequency-spectra density (f) of the first complex empirical orthogonal function (CEOF) mode of meridional velocity at 4 000 m. The mooring site is marked with a triangle in a, b and c. The cpd means counts per day.
Figure 14. Spatial patterns of 35 m (a) and 4 000 m (b) meridional velocity; homogeneous (c) and heterogeneous (d) correlation map for the 4 000 m velocity, the 95% significance level is shown as red contours; time evolution of the expansion coefficients of 35 m and 4 000 m meridional velocity (e). All is for the first leading SVD mode. The mooring site is marked with a red triangle in a and b. SVD: Singular Value Decomposition; SCF: Squared Covariance Fraction (measuring the amount of squared covariance for which each mode accounts).
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