Wind-generated waves are often treated as stochastic processes. There is particular interest in their spectral density functions, which are often expressed in some parametric form. Such spectral density functions are used as inputs when modelling structural response or other engineering concerns. Therefore, accurate and precise recovery of the parameters of such a form, from observed wave records, is important. Current techniques are known to struggle with recovering certain parameters, especially the peak enhancement factor and spectral tail decay. We introduce an approach from the statistical literature, known as the de-biased Whittle likelihood, and address some practical concerns regarding its implementation in the context of wind-generated waves. We demonstrate, through numerical simulation, that the de-biased Whittle likelihood outperforms current techniques, such as least squares fitting, both in terms of accuracy and precision of the recovered parameters. We also provide a method for estimating the uncertainty of parameter estimates. We perform an example analysis on a data-set recorded off the coast of New Zealand, to illustrate some of the extra practical concerns that arise when estimating the parameters of spectra from observed data.
翻译:风产生的波浪往往被视为随机过程。人们对其光谱密度功能特别感兴趣,这些功能往往以某种参数的形式表示。在模拟结构反应或其他工程关切时,这种光谱密度功能被用作投入。因此,从观测到的波记录中准确和准确地恢复这种表的参数非常重要。目前的技术是努力恢复某些参数,特别是峰值增强系数和光谱尾部衰变。我们从统计文献中引入了一种方法,即所谓的降压惠特尔概率,并解决了在风产生的波中实施这种功能的一些实际关切。我们通过数字模拟表明,从已观测到的参数的精确度和精确度来看,去偏移的惠特尔概率比当前技术(例如最小的方形)要好。我们还提供了一种估算参数估计不确定性的方法。我们对在新西兰沿海记录的一个数据集进行了举例分析,以说明在从观测到的数据中估算光谱参数时所产生的一些额外的实际关切。