Comparison of maximum entropy and ResNet-18 inferences of sediment sound speed using surface ship noise

The impact of individual seabed properties on sound propagation in the ocean depends on many factors including source-receiver range and frequency band of interest. In this talk, estimates of the sound speed ratio across the water-sediment interface are obtained using a maximum entropy approach and...

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Published in:The Journal of the Acoustical Society of America Vol. 151; no. 4; p. A267
Main Authors: Neilsen, Tracianne B., Mortenson, Michael C., Nuttall, Jacob R., Amos, Stephen M., Transtrum, Mark K., Knobles, David P., Hodgkiss, William
Format: Journal Article
Language:English
Published: 01-04-2022
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Abstract The impact of individual seabed properties on sound propagation in the ocean depends on many factors including source-receiver range and frequency band of interest. In this talk, estimates of the sound speed ratio across the water-sediment interface are obtained using a maximum entropy approach and ResNet18, a supervised machine learning model. The input data are spectrograms of surface ship noise from shipping lanes. Synthetic spectrograms are modeled using a ship noise source spectrum and a range-independent normal mode model, ORCA, with a wide range of environments and ship parameters. Experimental data from the New England Mud Patch are used with both inverse methods. The maximum entropy approach uses data-model mismatch to obtain a posterior probability distribution for the parameters of interest. The ResNet18 is trained on the synthetic spectrograms, augmented with additive noise, and then applied to the experimental data. A comparison of the results from these two methods for a variety of ships using different frequency bands will be presented, along with a discussion of the advantages and limitations of each method.
AbstractList The impact of individual seabed properties on sound propagation in the ocean depends on many factors including source-receiver range and frequency band of interest. In this talk, estimates of the sound speed ratio across the water-sediment interface are obtained using a maximum entropy approach and ResNet18, a supervised machine learning model. The input data are spectrograms of surface ship noise from shipping lanes. Synthetic spectrograms are modeled using a ship noise source spectrum and a range-independent normal mode model, ORCA, with a wide range of environments and ship parameters. Experimental data from the New England Mud Patch are used with both inverse methods. The maximum entropy approach uses data-model mismatch to obtain a posterior probability distribution for the parameters of interest. The ResNet18 is trained on the synthetic spectrograms, augmented with additive noise, and then applied to the experimental data. A comparison of the results from these two methods for a variety of ships using different frequency bands will be presented, along with a discussion of the advantages and limitations of each method.
Author Mortenson, Michael C.
Knobles, David P.
Amos, Stephen M.
Nuttall, Jacob R.
Transtrum, Mark K.
Hodgkiss, William
Neilsen, Tracianne B.
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  givenname: Tracianne B.
  surname: Neilsen
  fullname: Neilsen, Tracianne B.
  organization: Phys. and Astronomy, Brigham Young Univ., N251 ESC, Provo, UT 84602tbn@byu.edu
– sequence: 2
  givenname: Michael C.
  surname: Mortenson
  fullname: Mortenson, Michael C.
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  givenname: Jacob R.
  surname: Nuttall
  fullname: Nuttall, Jacob R.
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  givenname: Stephen M.
  surname: Amos
  fullname: Amos, Stephen M.
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  givenname: Mark K.
  surname: Transtrum
  fullname: Transtrum, Mark K.
  organization: Phys. and Astronomy, Brigham Young Univ., Provo, UT
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  givenname: David P.
  surname: Knobles
  fullname: Knobles, David P.
  organization: Phys., Knobles Sci. and Anal., Austin, TX
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  givenname: William
  surname: Hodgkiss
  fullname: Hodgkiss, William
  organization: Marine Physical Lab., Scripps Inst. of Oceanogr., San Diego, CA
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Title Comparison of maximum entropy and ResNet-18 inferences of sediment sound speed using surface ship noise
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