4.7 Article

Wave spectrum analysis for southern Caspian Sea

期刊

OCEAN ENGINEERING
卷 272, 期 -, 页码 -

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PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.oceaneng.2022.113490

关键词

Caspian sea; Spectral density function; Pierson -Moskowitz; JONSWAP Spectrum; Waves spectrum; Spectral analysis

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In this study, the general form of the spectrum was used to mathematically describe the spectrum of the Caspian Sea waves. Five spectral models were compared and it was found that the Krylov model performed the best for narrow spectra, the Donelan model performed the best for broad spectra, and the PM model performed the best for medium-width spectra.
The general form of spectrum S(omega) = A omega-p exp(-B omega-q) was used in the present study to mathematically describe the spectrum of the Caspian Sea waves, and its fit to observations was obtained by assigning different values to pair (p,q). For this purpose, five spectral models, including Donelan, Pierson-Moskowitz (PM), Krylov, Davidan, and Neumann were considered corresponding to (4,4), (5,4), (7,4), (6.5,5.5), and (6,2). In the first step, the default coefficients were found to lack the required accuracy, therefore, they were optimized. The performance comparison of these five models showed that the spectral width index (v) provides a good insight into the performance of the models such that the Krylov model exhibited the highest accuracy for narrow spectra (v < 0.4). For broad (v > 0.45) and medium-width spectra (0.4 < v < 0.45), the Donelan model and PM model yielded the best result, respectively. The highest rate of error was related to the Davidan model; therefore, it was excluded from the study. The Neumann model had similar performance to the Donelan model. Additionally, it was observed that the models are sometimes incapable of accurately estimating the spectrum in high frequency band. In validation of Philips (-omega- 5) and Toba (-omega-4) theories, the frequency dependence of spectrum in the equilibrium range was found to take the form of omega- 7, omega- 4, and omega- 5 in narrow, broad and medium-width spectra, respectively.

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