High-Resolving modeling of the surface semidiurnal M2 tide in the East-Siberian Sea

B. Kagan, A. A. Timofeev
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Abstract

In the framework of a high-resolving version of the 3D finite-element hydrostatic model QUODDY-4 we have simulated the fields of dynamic characteristics (amplitudes and phases of tidal elevations and barotropic tidal velocity ellipses) corresponding to the surface semidiurnal M2 tide in the no-ice East-Siberian Sea. It is shown that the obtained tidal chart has a complex structure, determined by 4 real amphidromes of left rotation which are induced by interference of counter-coming progressive Poincare waves in the southern part of the sea, 1 fake amphidrome with the center upon the Novaya Sibir Isl. and 4 small-scale amphidromes caused by interference of counter-coming Kelvin waves, from which 3 are formed in the narrow straits in the region of Bolshoy and Maly Lyahovsky Isls. and 1 near the entrance of the Chaunskaya Guba. Tidal amplitudes in the vicinity of the Novaya Sibir Isl. achieve 20–30 cm, whereas in the remaining part of the sea they are comparatively small and do not exceed 5–10 cm. Accordingly, the field of barotropic tidal velocities in the north-western part of the sea basically consists of high values (they are tens of cm/s), but in the other parts of the sea barotropic velocities are small (lower then 10 cm/s) and their field has a band structure. The fields of the averaged (over a tidal cycle) integrated in depth constituents of the barotropic tidal energy budget (namely, the barotropic tidal energy density, the advective transport and the horizontal wave flux per unit length of this energy and the rate of its dissipation due to the bottom friction) are presented. Also, a comparison of predicted tidal elevations with the mareographic level measurement data states that an estimate of their agreement may be considered as satisfactory taking into account that the tidal amplitudes in the sea as a whole are small.
东西伯利亚海M2海面半日潮的高分辨率模拟
在高分辨率三维流体静力模型QUODDY-4的框架下,我们模拟了东西伯利亚海无冰M2海面半日潮的动力特征场(潮汐高程的幅值和相位以及正压潮汐速度椭圆)。结果表明,所得到的潮汐图结构复杂,由海面南部反来的渐进庞加莱波干涉引起的4个真正的左旋角和1个以新西伯利亚岛为中心的假角决定。在反来开尔文波干扰下形成的4个小水坑,其中3个形成于Bolshoy和Maly Lyahovsky群岛的狭窄海峡。一个在Chaunskaya Guba入口附近。新西伯利亚岛附近的潮汐振幅。达到20-30厘米,而在海洋的其余部分,它们相对较小,不超过5-10厘米。因此,西北海区正压潮速度场基本由高值潮(几十cm/s)组成,而其他海区正压潮速度场较小(小于10 cm/s),且呈带状结构。给出了正压潮汐能平衡(即正压潮汐能密度、该能量单位长度的平流输运和水平波通量以及由于底部摩擦引起的耗散率)的平均场(在一个潮汐周期内)。此外,将预测的潮汐高程与气象测量的潮位测量数据进行比较表明,考虑到整个海洋的潮汐振幅很小,对两者一致性的估计可能是令人满意的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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