论文标题
沿轨道卫星的季节性和中尺度洋流的季节性和空间依赖性
Seasonality and spatial dependence of meso- and submesoscale ocean currents from along-track satellite altimetry
论文作者
论文摘要
沿轨道波数光谱密度(SSH)从Jason-2高度学数据估算为空间位置和日历月的函数,以了解整个全球海洋中的中尺度和子尺度级平衡动力学的季节性。具有显着模式1和模式2的斜压潮的区域被拒绝,将分析限制为室外。 Where balanced motion dominates, the SSH spectral density is averaged over all pass segments in a region for each calendar month, and is fit to a 4-parameter model consisting of a flat plateau at low wavenumbers, a transition at wavenumber $k_0$ to a red power law spectrum $k^{-s}$, and a white spectrum at high wavenumbers that models the altimeter noise.将模型参数的每月时间序列与混合层的演变进行比较。混合层加深后,光谱斜率$ s $的年度模式达到了最低限度,并且在范围内,每年的乐队模式在$ [2K_0,4 k_0] $和$ [k_0,2 k_0] $ peak $ \ sim $ 2和$ \ sim $ 2和$ \ sim $ 4个月后,最大的年度混合层深度(分别是Mighter Myde Mode Mode Mode Mode Mode Mode Mode)。该分析与冬季混合层不稳定性的能量一致,然后是与先前的建模研究和原位测量相一致的级级别级联。将这些结果与先前的建模,原位和对特定区域的卫星研究进行了比较,并且在测量不确定性中与它们广泛一致。
Along-track wavenumber spectral densities of sea surface height (SSH) are estimated from Jason-2 altimetry data as a function of spatial location and calendar month, to understand the seasonality of meso- and submesoscale balanced dynamics across the global ocean. Regions with significant mode-1 and mode-2 baroclinic tides are rejected, restricting the analysis to the extratropics. Where balanced motion dominates, the SSH spectral density is averaged over all pass segments in a region for each calendar month, and is fit to a 4-parameter model consisting of a flat plateau at low wavenumbers, a transition at wavenumber $k_0$ to a red power law spectrum $k^{-s}$, and a white spectrum at high wavenumbers that models the altimeter noise. The monthly time series of the model parameters are compared to the evolution of the mixed layer. The annual mode of the spectral slope $s$ reaches a minimum after the mixed layer deepens, and the annual mode of the bandpassed kinetic energy in the ranges $[2k_0,4 k_0]$ and $[k_0,2 k_0]$ peak $\sim$2 and $\sim$4 months, respectively, after the maximum of the annual mode of the mixed layer depth. This analysis is consistent with an energization of the submesoscale by a winter mixed layer instability followed by an inverse cascade to the mesoscale, in agreement with prior modeling studies and in situ measurements. These results are compared to prior modeling, in situ, and satellite investigations of specific regions, and are broadly consistent with them within measurement uncertainties.