Broadband spectrograms from surface ships are employed in convolutional neural networks (CNNs) to predict the seabed type, ship speed, and closest point of approach (CPA) range. Three CNN architectures of differing size and depth are trained on different representations of the spectrograms. Multitask learning is employed; the seabed type prediction comes from classification, and the ship speed and CPA range are estimated via regression. Due to the lack of labeled field data, the CNNs are trained on synthetic data generated using measured sound speed profiles, four seabed types, and a random distribution of source parameters. Additional synthetic datasets are used to evaluate the ability of the trained CNNs to interpolate and extrapolate source parameters. The trained models are then applied to a measured data sample from the 2017 Seabed Characterization Experiment (SBCEX 2017). While the largest network provides slightly more accurate predictions on tests with synthetic data, the smallest network generalized better to the measured data sample. With regard to the input data type, complex pressure spectral values gave the most accurate and consistent results for the ship speed and CPA predictions with the smallest network, whereas using absolute values of the pressure provided more accurate results compared to the expected seabed types.
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Seabed type and source parameters predictions using ship spectrograms in convolutional neural networksa)
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February 2021
February 18 2021
Seabed type and source parameters predictions using ship spectrograms in convolutional neural networksa)
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Machine Learning in Acoustics
David F. Van Komen
;
David F. Van Komen
b)
1
Physics and Astronomy, Brigham Young University
, Provo, Utah, 84604, USA
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Tracianne B. Neilsen
;
Tracianne B. Neilsen
c)
1
Physics and Astronomy, Brigham Young University
, Provo, Utah, 84604, USA
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Daniel B. Mortenson;
Daniel B. Mortenson
1
Physics and Astronomy, Brigham Young University
, Provo, Utah, 84604, USA
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Mason C. Acree;
Mason C. Acree
1
Physics and Astronomy, Brigham Young University
, Provo, Utah, 84604, USA
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David P. Knobles;
David P. Knobles
2
Knobles Scientific and Analysis
, Austin, Texas, 78731, USA
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Mohsen Badiey;
Mohsen Badiey
3
Department of Electrical Engineering, University of Delaware
, Newark, Delaware 19716, USA
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William S. Hodgkiss
William S. Hodgkiss
4
Marine Physical Laboratory, Scripps Institution of Oceanography, University of California, San Diego
, La Jolla, California 92093, USA
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David F. Van Komen
1,b)
Tracianne B. Neilsen
1,c)
Daniel B. Mortenson
1
Mason C. Acree
1
David P. Knobles
2
Mohsen Badiey
3
William S. Hodgkiss
4
1
Physics and Astronomy, Brigham Young University
, Provo, Utah, 84604, USA
2
Knobles Scientific and Analysis
, Austin, Texas, 78731, USA
3
Department of Electrical Engineering, University of Delaware
, Newark, Delaware 19716, USA
4
Marine Physical Laboratory, Scripps Institution of Oceanography, University of California, San Diego
, La Jolla, California 92093, USA
a)
This paper is part of a special issue on Machine Learning in Acoustics.
b)
Electronic mail: [email protected], ORCID: 0000-0003-0610-0806.
c)
ORCID: 0000-0002-9729-373X.
J. Acoust. Soc. Am. 149, 1198–1210 (2021)
Article history
Received:
October 14 2020
Accepted:
January 22 2021
Citation
David F. Van Komen, Tracianne B. Neilsen, Daniel B. Mortenson, Mason C. Acree, David P. Knobles, Mohsen Badiey, William S. Hodgkiss; Seabed type and source parameters predictions using ship spectrograms in convolutional neural networks. J. Acoust. Soc. Am. 1 February 2021; 149 (2): 1198–1210. https://doi.org/10.1121/10.0003502
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