De-noising receiver function data using the unsupervised deep learning approach

SUMMARY The converted wave data (P-to-s or S-to-p), traditionally termed as receiver functions, are often contaminated with noise of different origin that may lead to the erroneous identification of phases and thus influence the interpretations. Here, we utilize an unsupervised deep learning approac...

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Vydané v:Geophysical journal international Ročník 229; číslo 2; s. 737 - 749
Hlavní autori: Dalai, Bijayananda, Kumar, Prakash, Srinu, Uppala, Sen, Mrinal K
Médium: Journal Article
Jazyk:English
Vydavateľské údaje: Oxford University Press 20.01.2022
Predmet:
Theoretical seismology
Body wave
Structure of the Earth
Neural networks
Computational seismology
ISSN:0956-540X, 1365-246X
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Shrnutí:SUMMARY The converted wave data (P-to-s or S-to-p), traditionally termed as receiver functions, are often contaminated with noise of different origin that may lead to the erroneous identification of phases and thus influence the interpretations. Here, we utilize an unsupervised deep learning approach called Patchunet to de-noise the converted wave data. We divide the input data into several patches, which are input to the encoder and decoder network to extract some meaningful features. The method de-noises an image patch by patch and utilizes the redundant information on similar patches to obtain the final de-noised results. The method is first tested on a suite of synthetic data contaminated with various amounts of Gaussian and realistic noise and then on the observed data from three permanent seismic stations: HYB (Hyderabad, India), LBTB (Lobatse, Botswana, South Africa) and COR (Corvallis, Oregon, USA). The method works very well even when the signal-to-noise ratio is poor or with the presence of spike noise and deconvolution artifacts. The field data demonstrate the effectiveness of the method for attenuating the random noise especially for the mantle phases, which show significant improvements over conventional receiver function based images.
ISSN:0956-540X
1365-246X
DOI:10.1093/gji/ggab494