Theoretical model and simulation of ship underwater radiated noise

Jun Ping Sun, Jun Yang, Jian Heng Lin*, Guo Jian Jiang, Xue Juan Yi, Peng Fei Jiang

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

13 Citations (Scopus)

Abstract

Ship underwater radiated noise is one of the most important ocean ambient noise sources, and building a reasonable model for the ship underwater radiated noise is helpful for understanding the physical mechanism and reducing research cost of ship underwater radiated noise. The quasi-periodic random sound pulse sequence signals act well in explaining the rhythm and the power spectrum variation of the ship underwater radiated noise, and reveal that there are not any real sinusoidal components in ship radiated noise signals, which come from the non-linear transformation of the signals, and the analysis of some representative experimental data of ship radiated noise also supports this idea. Based on this, the explosion-type cosine pulses are used as the units of quasi-periodic random sound pulse sequences. This model can generate the power spectrum with a peak, and the peak location can change with ship velocity or ship type. The power spectrum variation characteristics of quasi-periodic random sound pulse sequences consisting of the explosion-type cosine pulses are in good agreement with the measured ship underwater radiated noise data, which shows that this model is of important practical value.

Original languageEnglish
Article number124301
JournalWuli Xuebao/Acta Physica Sinica
Volume65
Issue number12
DOIs
Publication statusPublished - Jun 20 2016
Externally publishedYes

Bibliographical note

Publisher Copyright:
© 2016 Chinese Physical Society.

ASJC Scopus Subject Areas

  • General Physics and Astronomy

Keywords

  • Experimental data
  • Explosive cosine pulse signal
  • Quasi-periodic random sound pulse sequence

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