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Noise-Source Detection in an Oceanic Waveguide Using Interferometric Processing

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Abstract

The signal-to-noise ratio as a result of interferometric processing of noise-source field in an oceanic waveguide is estimated. The minimum duration of noise-source realization, which determines the maximum noise immunity, is evaluated. The noise-source signal detection based on the Neyman–Pearson criterion is considered. The range of input signal-to-noise ratios for the case where a single detector provides acceptable data on the source parameters is analyzed. An expression for the detection curves (dependences of the correct-detection probability on the signal-to-noise ratio at a fixed false-alarm probability) is derived. The corresponding numerical calculations are carried out.

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Funding

This study was supported by the Russian Foundation for Basic Research (project nos. 19-08-00941, 19-29-06075).

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Authors and Affiliations

  1. Prokhorov General Physics Institute of the Russian Academy of Sciences, 119991, Moscow, Russia

    V. M. Kuz’kin, G. A. Lyakhov & S. A. Pereselkov

  2. Voronezh State University, 394006, Voronezh, Russia

    S. A. Pereselkov & S. A. Tkachenko

  3. Institute of Marine Technology Problems, Far East Branch, Russian Academy of Sciences, 690091, Vladivostok, Russia

    Yu. V. Matvienko

Authors
  1. V. M. Kuz’kin
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  2. G. A. Lyakhov
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  3. S. A. Pereselkov
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  4. Yu. V. Matvienko
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  5. S. A. Tkachenko
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Corresponding author

Correspondence to V. M. Kuz’kin.

Additional information

Translated by Yu. Sin’kov

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Kuz’kin, V.M., Lyakhov, G.A., Pereselkov, S.A. et al. Noise-Source Detection in an Oceanic Waveguide Using Interferometric Processing. Phys. Wave Phen. 28, 68–74 (2020). https://doi.org/10.3103/S1541308X20010057

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  • DOI: https://doi.org/10.3103/S1541308X20010057

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