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Measurements of the Directional Spectrum across the Equilibrium Saturation Ranges of Wind-Generated Surface Waves

机译:风力面波的平衡饱和范围内方向谱的测量

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摘要

It is now well accepted that to better understand the coupling between the atmosphere and the ocean, and improve coupled ocean-atmosphere models, surface wave processes need to be taken into account. Here, properties of the directional distributions of the surface wave field across the equilibrium and saturation ranges are investigated from airborne lidar data collected during the ONR Southern California 2013 (SoCal2013) experiment, conducted off the coast of Southern California in November 2013. During the field effort, detailed characterization of the marine atmospheric boundary layer was performed from Research Platform (R/P) Floating Instrument Platform (FLIP), moored at the center of the aircraft operational domain. The wind speed ranged from approximately 1-2 to up to 11ms(-1), while the significant wave height varied from 0.8 to 2.5m during the 10 days of data collection considered in the analysis. The directional wavenumber spectrum exhibits a clear, bimodal distribution that extends well beyond what was reported in previous studies, with the azimuthal separation between the lobes reaching approximate to pi for the highest wavenumbers that could be resolved: approximately 10-12 rad m(-1). The results demonstrate that opposing wave components can be found in one storm system rather than requiring waves from opposing storms, with implications for ocean acoustics. With the broad wavenumber range of the directional spectra obtained from the lidar, the transition from the equilibrium to saturation ranges over a range of wind forcing conditions is found to occur for k(n)u(*)(2)/g approximate to 1-2 x 10(-3), where k(n) is the wavenumber at the upper limit of the equilibrium range, u* the friction velocity, and g the gravitational acceleration. The results are discussed in the context of Phillips' model of the equilibrium range of wind-generated gravity waves.
机译:为了更好地理解大气与海洋之间的耦合并改善海洋与大气的耦合模型,现在已经被广泛接受,需要考虑表面波过程。在此,根据在2013年11月在南加州海岸进行的ONR南加州2013(SoCal2013)实验期间收集的机载激光雷达数据,研究了在平衡和饱和范围内表面波场的方向分布的特性。尽力而为,对海洋大气边界层的详细表征是通过停泊在飞机操作域中心的研究平台(R / P)浮动仪表平台(FLIP)进行的。在分析中考虑的10天数据收集期间,风速范围从大约1-2到最高11ms(-1),而显着的波高从0.8到2.5m不等。方向波数频谱显示出清晰的双峰分布,其范围远远超出了先前研究中所报道的范围,对于可以解决的最高波数,波瓣之间的方位角间隔接近pi,大约可以解决10-12 rad m(-1) )。结果表明,可以在一个风暴系统中找到相反的波浪成分,而不是需要来自相反风暴的波浪,这会影响海洋声学。在从激光雷达获得的方向性光谱的宽波数范围的情况下,发现在k(n)u(*)(2)/ g近似于1的情况下,在一定的风力条件下会发生从平衡到饱和范围的过渡-2 x 10(-3),其中k(n)是平衡范围上限的波数,u *摩擦速度,g是重力加速度。在菲利普斯的风力引力波平衡范围模型的背景下讨论了结果。

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  • 来源
    《Journal of Physical Oceanography 》 |2017年第8期| 2123-2138| 共16页
  • 作者单位

    Univ Calif San Diego, Scripps Inst Oceanog, La Jolla, CA 92093 USA;

    Univ Calif San Diego, Scripps Inst Oceanog, La Jolla, CA 92093 USA;

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  • 正文语种 eng
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