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Mesoscale eddies observed by moored current-meters at abyssal depths in the western North Pacific during 1978-1985

机译:1978年至1985年期间,北太平洋西部深渊处的系泊电流表观测到的中尺度涡

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Observations by moored current-meters were carried out repeatedly in mid-ocean of the western North Pacific, providing 50 velocity records. A continuous velocity record for almost seven years was obtained at 5000 m depth. The overall mean velocity is directed to the north with a speed of less than 1 cm s~(-1). The kinetic energy of low-frequency velocity-fluctuations, or mesoscale eddies is more than 30 times larger than that of mean flow. Frequency spectra of eddy kinetic energy show that most of the energy is contained in mesoscale bands (periods of 31-235 days), with zonal (meridional) dominance of energy in the longer (shorter) period band. An array observation at 4000 m depth shows that the local change of relative vor-ticity of mesoscale eddies is balanced mainly with the advection of planetary vorticity, although the horizontal advection of relative vorticity and higher-order horizontal divergence may play some role. Those results suggest that the mesoscale eddies are understood as primarily plane barotropic Rossby waves with possible modification.
机译:在北太平洋西部大洋中部反复进行了系泊电流计的观测,提供了50条速度记录。在5000 m的深度获得了近7年的连续速度记录。总体平均速度以小于1 cm s〜(-1)的速度指向北。低频速度波动或中尺度涡旋的动能比平均流动能大30倍以上。涡动能的频谱显示,大部分能量包含在中尺度带(31-235天的时间段)中,而在较长(较短)周期带中能量的区域(子午)占主导地位。在4000 m深度的阵列观测表明,中尺度涡旋的相对涡度的局部变化主要与行星涡旋的平流平衡,尽管相对涡旋的水平对流和高阶水平发散可能起一定作用。这些结果表明,中尺度涡流主要被理解为平面正压罗斯贝波,并可能进行了修改。

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