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CAN WE INFER OCEAN DYNAMICS FROM ALTIMETER WAVENUMBER SPECTRA

机译:我们可以从高度计波数光谱推断海洋动力学吗?

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Wavenumber spectral slopes of sea surface height (SSH) and kinetic energy (KE) have been used to infer “interior” or surface quasi-geostrophic (QG or SQG) dynamics of the ocean. However, noise-corrected altimeter SSH in a fixed mesoscale band of 70 to 250 km have much flatter slopes than the QG or SQG predictions over most of the ocean. Spectra estimated from an eddy resolving global ocean circulation model (the HYbrid Coordinate Ocean Model) with embedded tides, suggest that the flatter slopes arise from two additional sources: (1) presence of strong internal waves and tides and (2) shift of the inertial sub-range to smaller scales. Separating the high and low frequency variability yields a different pattern with flatter spectra at high frequency and steeper spectrum at low frequency. For low mesoscale KE, the inertial subrange moves to smaller scales based upon the enstrophy spectra. Thus, it is difficult to infer the ocean dynamics from the altimeter spectral slope over a fixed wavenumber band.
机译:海表面高度(SSH)和动能(KE)的波数谱斜率已被用于推断海洋的“内部”或表面拟地球节脑(QG或SQG)动态。然而,固定的MESCHELE频段的噪声校正的高度计SSH在70到250公里的70至250公里中具有比大多数海洋的QG或SQG预测得多得多得多。从嵌入式潮汐的涡流解决全球海洋循环模型(混合坐标海洋模型)估计的光谱表明,漂浮斜率从两个额外的来源出现:(1)强大的内部波和潮汐的存在和惯性的换档子范围到更小的尺度。分离高频率变化,在低频下高频和陡峭频谱处具有平坦光谱的不同模式。对于低MESSCLE KE,惯性子区域基于敌对光谱移动到较小的尺度。因此,难以在固定波数带上从高度计谱斜率推断出海洋动力学。

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