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Modelling secondary microseismic noise by normal mode summation

Title: Modelling secondary microseismic noise by normal mode summation
Authors: Gualtieri, A; Stutzmann, M; Capdeville, F; Ardhuin, A; Schimmel, A; Mangeney, Anne; Morelli, Andrea
Contributors: Institut de Physique du Globe de Paris (IPGP); Institut national des sciences de l'Univers (INSU - CNRS)-IPG PARIS-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Centre National de la Recherche Scientifique (CNRS); Dipartimento di Fisica e Astronomia Bologna; Alma Mater Studiorum Università di Bologna Bologna (UNIBO); Laboratoire de Planétologie et Géodynamique UMR 6112 (LPG); Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST); Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS); Laboratoire d'Océanographie Spatiale (LOS); Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER); Institute of Earth Sciences Jaume Almera; Consejo Superior de Investigaciones Científicas Madrid (CSIC); Istituto Nazionale di Geofisica e Vulcanologia - Sezione di Bologna (INGV); Istituto Nazionale di Geofisica e Vulcanologia
Source: ISSN: 0956-540X.
Publisher Information: HAL CCSD; Oxford University Press (OUP)
Publication Year: 2013
Collection: Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe)
Subject Terms: Surface waves and free oscillations; Seismic attenuation; Theoretical seismology; Wave propagation; [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]
Description: International audience ; Secondary microseisms recorded by seismic stations are generated in the ocean by the interaction of ocean gravity waves. We present here the theory for modelling secondary microseismic noise by normal mode summation. We show that the noise sources can be modelled by vertical forces and how to derive them from a realistic ocean wave model. We then show how to compute bathymetry excitation effect in a realistic earth model by using normal modes and a comparison with Longuet–Higgins approach. The strongest excitation areas in the oceans depends on the bathymetry and period and are different for each seismic mode. Seismic noise is then modelled by normal mode summation considering varying bathymetry. We derive an attenuation model that enables to fit well the vertical component spectra whatever the station location. We show that the fundamental mode of Rayleigh waves is the dominant signal in seismic noise. There is a discrepancy between real and synthetic spectra on the horizontal components that enables to estimate the amount of Love waves for which a different source mechanism is needed. Finally, we investigate noise generated in all the oceans around Africa and show that most of noise recorded in Algeria (TAM station) is generated in the Northern Atlantic and that there is a seasonal variability of the contribution of each ocean and sea.
Document Type: article in journal/newspaper
Language: English
Relation: insu-01397324; https://hal-insu.archives-ouvertes.fr/insu-01397324; https://hal-insu.archives-ouvertes.fr/insu-01397324/document; https://hal-insu.archives-ouvertes.fr/insu-01397324/file/Geophys.%20J.%20Int.-2013-Gualtieri-1732-45.pdf
DOI: 10.1093/gji/ggt090
Availability: https://hal-insu.archives-ouvertes.fr/insu-01397324; https://hal-insu.archives-ouvertes.fr/insu-01397324/document; https://hal-insu.archives-ouvertes.fr/insu-01397324/file/Geophys.%20J.%20Int.-2013-Gualtieri-1732-45.pdf; https://doi.org/10.1093/gji/ggt090
Rights: info:eu-repo/semantics/OpenAccess
Accession Number: edsbas.61CECCC5
Database: BASE