Analyse Du Bruit Microsismique Associé À La Houle Dans L'océan Indien

Total Page:16

File Type:pdf, Size:1020Kb

Analyse Du Bruit Microsismique Associé À La Houle Dans L'océan Indien Analyse du bruit microsismique associ´e`ala houle dans l'oc´eanIndien C´elineDavy To cite this version: C´eline Davy. Analyse du bruit microsismique associ´e `a la houle dans l'oc´ean Indien. G´eophysique [physics.geo-ph]. Universit´ede La R´eunion,2015. Fran¸cais. <tel-01391911> HAL Id: tel-01391911 http://hal.univ-reunion.fr/tel-01391911 Submitted on 4 Nov 2016 HAL is a multi-disciplinary open access L'archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destin´eeau d´ep^otet `ala diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publi´esou non, lished or not. The documents may come from ´emanant des ´etablissements d'enseignement et de teaching and research institutions in France or recherche fran¸caisou ´etrangers,des laboratoires abroad, or from public or private research centers. publics ou priv´es. Université de La Réunion – Laboratoire Géosciences Réunion – Institut de Physique du Globe de Paris Ecole Doctorale Sciences Technologies Santé THÈSE Pour obtenir le grade de DOCTEUR DE L’UNIVERSITÉ DE LA REUNION Spécialité : Sciences de la Terre Par Céline DAVY Analyse du bruit microsismique associé à la houle dans l’océan Indien Soutenue publiquement le 26 novembre 2015, devant le jury composé de : Fabrice ARDHUIN Directeur de Recherches CNRS, IFREMER Rapporteur Karin SIGLOCH Associate Professor, Université d’Oxford Rapporteur Éric BEUCLER Maître de Conférences, Université de Nantes Examinateur Éléonore STUTZMANN Professeur, IPGP Examinateur Guilhem BARRUOL Directeur de Recherches CNRS, Université de La Réunion Directeur Fabrice R. FONTAINE Maître de Conférences, Université de La Réunion Co-Directeur Avant-propos Débutée en mars 2012, cette thèse a été réalisée au laboratoire Géosciences de l’Université de La Réunion, sous la direction de Guilhem Barruol et Fabrice R. Fontaine. Le financement de cette thèse a été assuré par l’École Doctorale STS de l’Université de La Réunion. Les données sismologiques utilisées dans le cadre de ce travail ont été acquises dans le cadre des programmes suivants : RHUM-RUM [Barruol and Sigloch, 2013], cofinancé par l’Agence National de la Recherche (projet ANR-11-BS56-0013) et par le DFG (Deutsche Forschungsgemeinschaft), avec le soutien du CNRS-INSU, des TAAF, de l’iPEV et de l’AWI. GEOSISM-Éparses, cofinancé par le CNRS-INSU, CNRS-INEE, les TAAF et par le projet RHUM-RUM, avec le soutien de l’OSU Réunion. HOULE REUNION, financé par la Région Réunion, l'OSU-Réunion, le programme INSU-SYSTER. Remerciements Je tiens tout d’abord à remercier Guilhem Barruol sans qui l’aboutissement de cette thèse n’aurait pas été possible, pour son encadrement sans faille, ses conseils avisés, son efficacité et pour toute l’aide qu’il m’a apportée dans l’apprentissage du travail de chercheur. Mes remerciements vont également à Fabrice Fontaine pour avoir assuré la co-direction de cette thèse et pour son accompagnement dans la prise en main des outils du sismologue. Je remercie vivement Fabrice Ardhuin et Karin Sigloch d’avoir accepté d’évaluer ce travail en tant que rapporteurs, ainsi qu’Éric Beucler et Éléonore Stutzmann en tant qu’examinateurs. Je tiens également à remercier Éléonore Stutzmann pour sa collaboration, ses conseils pertinents et sa disponibilité lors de mes passages à l’IPGP. D’une façon générale, la préparation de ce travail de recherche m’a amenée à rencontrer un grand nombre de scientifiques de tout horizon, avec lesquels les échanges ont toujours été très enrichissants. Je tiens à les en remercier ici. Un grand merci à Emmanuel Cordier pour son aide précieuse dans tout ce qui concerne l’aspect modélisation de la houle et pour ses nombreux conseils dans l’utilisation du logiciel Matlab, toujours donnés dans la bonne humeur ! Je remercie toute l’équipe RESIF de Grenoble pour leur aide technique dans le traitement et la mise à disposition des données sismologiques acquises dans le cadre de cette thèse. Je remercie chaleureusement toute l’équipe du laboratoire Géosciences de l’Université de La Réunion pour leur accueil et pour l’aide qu’ils m’ont apportée durant ces trois années. Enfin, d’un point de vue plus personnel, je remercie toutes les personnes qui ont contribué à rendre cette expérience professionnelle si enrichissante, tant sur le plan des rencontres et des découvertes que pour les bons moments passés ensemble. Une spéciale dédicace à ma famille créole d’adoption : Sylvie, Bruno et toute leur tribu, ainsi qu’à Jean-Luc des Petits débrouillards et à l’équipe « Paré pas Paré » de la Croix Rouge pour avoir rendu ce séjour à La Réunion inoubliable : mi aime zot tout ! Je remercie naturellement mes parents, à qui je dois d’être arrivée jusqu’ici, et ma Nénène d’amour, pour leur soutien incommensurable et pour tout ce qu’ils représentent pour moi. Je vous aime fort. Big up à l’homme de ma vie [Charles, 2015] qui a rendu tout cela possible … TABLE DES MATIERES Table des matières PARTIE 1 : INTRODUCTION GÉNÉRALE ...................................................................... 1 1.1 Contexte et problématique générale ..................................................................................................... 2 1.2 Étude bibliographique du bruit microsismique ............................................................................... 6 1.2.1. Origine et nature du bruit (de la découverte à la théorie : 1870-1950) ............................ 6 1.2.2. Les microséismes secondaires ............................................................................................................... 9 1.2.3. Les microséismes primaires ..................................................................................................................13 1.2.4. Observations du bruit microsismique (de 1950 à nos jours) ................................................14 1.2.5. Modélisation : de la houle au bruit microsismique .....................................................................16 1.2.6. Utilisations du bruit microsismique..................................................................................................18 PARTIE 2 : LES SOURCES DE MICROSÉISMES SECONDAIRES À L’ÉCHELLE DE L’OCÉAN INDIEN, Relations avec les tempêtes océaniques ............................................................. 19 2.1 Détection lointaine des sources de microséismes secondaires ............................................... 20 2.1.1. Introduction .................................................................................................................................................20 2.1.2. Localisation des sources de microséismes secondaires : méthodes utilisées .................21 2.1.3. Localisation des sources de microséismes secondaires à l’échelle de l’océan Indien par l’analyse de la polarisation .....................................................................................................................................23 2.1.4. Localisation des sources de microséismes secondaires par analyses spectrales .........43 2.2 Détection in situ des sources de microséismes secondaires : le cas des cyclones ........... 63 2.2.1. Les cyclones comme sources de microséismes secondaires ...................................................63 2.2.2. Le suivi spatio-temporel du passage d’un cyclone tropical depuis les observations fond de mer .............................................................................................................................................................................69 2.3 Le suivi des variations climatiques sur le long terme .................................................................. 88 PARTIE 3 : LES SOURCES DE MICROSÉISMES PRIMAIRES DANS L’OCÉAN INDIEN, Impact direct de la houle sur la côte ................................................................................ 90 3.1 Étude bibliographique sur les sources de microséismes primaires ...................................... 91 3.2 Méthodes d'études des sources de microséismes primaires .................................................... 95 3.3 Utilisation d’une station sismique comme houlographe : application aux îles Éparses et à Mayotte ............................................................................................................................................................................ 98 3.3.1. Présentation des îles Éparses ...............................................................................................................98 3.3.2. Installation des stations sismiques dans les îles Éparses et à Mayotte ......................... 106 TABLE DES MATIERES 3.3.3. Suivi des houles australes et cycloniques dans les îles Éparses à partir du bruit microsismique .................................................................................................................................................................... 111 3.3.4. Fonctions de transfert dans les îles Éparses .............................................................................. 136 PARTIE 4 : ANALYSE DE HOULES EXTRÊMES SUR L’ÎLE DE LA RÉUNION .................. 158 4.1 Introduction................................................................................................................................................ 159 4.1.1 Contexte climatique : les houles à La Réunion ............................................................................ 159 4.2 Présentation des observations ..........................................................................................................
Recommended publications
  • The Origin of Deep Ocean Microseisms in the North Atlantic Ocean
    Proc. R. Soc. A (2008) 464, 777–793 doi:10.1098/rspa.2007.0277 Published online 8 January 2008 The origin of deep ocean microseisms in the North Atlantic Ocean 1, 2 1 BY SHARON KEDAR *,MICHAEL LONGUET-HIGGINS ,FRANK WEBB , 3 4 1 NICHOLAS GRAHAM ,ROBERT CLAYTON AND CATHLEEN JONES 1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA 2Institute for Nonlinear Science, University of California, San Diego, La Jolla, CA 92093-0402, USA 3Hydrologic Research Center, San Diego, CA 92130-2069, USA 4Seismological Laboratory, California Institute of Technology, Pasadena, CA 91125-2100, USA Oceanic microseisms are small oscillations of the ground, in the frequency range of 0.05–0.3 Hz, associated with the occurrence of energetic ocean waves of half the corresponding frequency. In 1950, Longuet-Higgins suggested in a landmark theoretical paper that (i) microseisms originate from surface pressure oscillations caused by the interaction between oppositely travelling components with the same frequency in the ocean wave spectrum, (ii) these pressure oscillations generate seismic Stoneley waves on the ocean bottom, and (iii) when the ocean depth is comparable with the acoustic wavelength in water, compressibility must be considered. The efficiency of microseism generation thus depends on both the wave frequency and the depth of water. While the theory provided an estimate of the magnitude of the corresponding microseisms in a compressible ocean, its predictions of microseism amplitude heretofore have never been tested quantitatively. In this paper, we show a strong agreement between observed microseism and calculated amplitudes obtained by applying Longuet-Higgins’ theory to hindcast ocean wave spectra from the North Atlantic Ocean.
    [Show full text]
  • Predicting Short-Period, Wind-Wave-Generated Seismic Noise in Coastal Regions ∗ Florent Gimbert A,B, , Victor C
    Earth and Planetary Science Letters 426 (2015) 280–292 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Predicting short-period, wind-wave-generated seismic noise in coastal regions ∗ Florent Gimbert a,b, , Victor C. Tsai a,b a Seismological Laboratory, California Institute of Technology, Pasadena, CA, USA b Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA a r t i c l e i n f o a b s t r a c t Article history: Substantial effort has recently been made to predict seismic energy caused by ocean waves in the 4–10 s Received 19 March 2015 period range. However, little work has been devoted to predict shorter period seismic waves recorded Received in revised form 5 June 2015 in coastal regions. Here we present an analytical framework that relates the signature of seismic noise Accepted 6 June 2015 recorded at 0.6–2 s periods (0.5–1.5 Hz frequencies) in coastal regions with deep-ocean wave properties. Available online 7 July 2015 Constraints on key model parameters such as seismic attenuation and ocean wave directionality are Editor: P. Shearer provided by jointly analyzing ocean-floor acoustic noise and seismic noise measurements. We show that Keywords: 0.6–2 s seismic noise can be consistently predicted over the entire year. The seismic noise recorded in this ocean waves period range is mostly caused by local wind-waves, i.e. by wind-waves occurring within about 2000 km of seismic noise the seismic station.
    [Show full text]
  • Noise Generation in the Solid Earth, Oceans, and Atmosphere, from Non
    Under consideration for publication in J. Fluid Mech. 1 Noise generation in the solid Earth, oceans, and atmosphere, from non-linear interacting surface gravity waves in finite depth FABRICE ARDHUIN1 A N D T. H. C. HERBERS2 1Ifremer, Laboratoire d’Oc´eanographie Spatiale, Plouzan´e, France 2Department of Oceanography, Naval Postgraduate School, Monterey, California 93943, USA (Received 22 June 2012; revised 22 September 2012; accepted ? ) Oceanic pressure measurements, even in very deep water, and atmospheric pressure or seismic records, from anywhere on Earth, contain noise with dominant periods between 3 and 10 seconds, that is believed to be excited by ocean surface gravity waves. Most of this noise is explained by a nonlinear wave-wave interaction mechanism, and takes the form of surface gravity waves, acoustic or seismic waves. Previous theoretical works on seismic noise focused on surface (Rayleigh) waves, and did not consider finite depth effects on the generating wave kinematics. These finite depth effects are introduced here, which requires the consideration of the direct wave-induced pressure at the ocean bottom, a contribution previously overlooked in the context of seismic noise. That contribution can lead to a considerable reduction of the seismic noise source, which is particularly relevant for noise periods larger than 10 s. The theory is applied to acoustic waves in the atmosphere, extending previous theories that were limited to vertical propagation only. Finally, the noise generation theory is also extended beyond the domain of Rayleigh waves, giving the first quantitative expression for sources of seismic body waves. In the limit of slow phase speeds in the ocean wave forcing, the known and well-verified gravity wave result is obtained, which was previously derived for an incompressible ocean.
    [Show full text]
  • Wind Wave - Wikipedia 1 of 16
    Wind wave - Wikipedia 1 of 16 Wind wave In fluid dynamics, wind waves, or wind-generated waves, are water surface waves that occur on the free surface of bodies of water. They result from the wind blowing over an area of fluid surface. Waves in the oceans can travel thousands of miles before reaching land. Wind waves on Earth range in size from small ripples, to waves over 100 ft (30 m) high.[1] When directly generated and affected by local waters, a Large wave wind wave system is called a wind sea. After the wind ceases to blow, wind waves are called swells. More generally, a swell consists of wind-generated waves that are not significantly affected by the local wind at that time. They have been generated elsewhere or some time ago.[2] Wind waves in the ocean are called ocean surface waves. Wind waves have a certain amount of randomness: Video of large waves from Hurricane Marie along the coast of Newport subsequent waves differ in height, duration, and shape Beach, California with limited predictability. They can be described as a stochastic process, in combination with the physics governing their generation, growth, propagation, and decay—as well as governing the interdependence between flow quantities such as: the water surface movements, flow velocities and water pressure. The key statistics of wind waves (both seas and swells) in evolving sea states can be predicted with wind wave models. Although waves are usually considered in the water seas Ocean waves of Earth, the hydrocarbon seas of Titan may also have wind-driven waves.[3] Contents Formation Types https://en.wikipedia.org/wiki/Wind_wave Wind wave - Wikipedia 2 of 16 Spectrum Shoaling and refraction Breaking Physics of waves Models Seismic signals See also References Scientific Other External links Formation The great majority of large breakers seen at a beach result from distant winds.
    [Show full text]
  • The Near-Coastal Microseism Spectrum: Spatial and Temporal Wave Climate Relationships Peter D
    JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 107, NO. B8, 10.1029/2001JB000265, 2002 The near-coastal microseism spectrum: Spatial and temporal wave climate relationships Peter D. Bromirski Integrative Oceanography Division, Scripps Institution of Oceanography, University of California, San Diego, La Jolla, California, USA Fred K. Duennebier Department of Geology and Geophysics, University of Hawaii at Manoa, Honolulu, Hawaii, USA Received 17 August 2000; revised 16 February 2001; accepted 20 August 2001; published 22 August 2002. [1] Comparison of the ambient noise data recorded at near-coastal ocean bottom and inland seismic stations at the Oregon coast with both offshore and nearshore buoy data shows that the near-coastal microseism spectrum results primarily from nearshore gravity wave activity. Low double-frequency (DF), microseism energy is observed at near-coastal locations when seas nearby are calm, even when very energetic seas are present at buoys 500 km offshore. At wave periods >8 s, shore reflection is the dominant source of opposing wave components for near-coastal DF microseism generation, with the variation of DF microseism levels poorly correlated with local wind speed. Near-coastal ocean bottom DF levels are consistently 20 dB higher than nearby DF levels on land, suggesting that Rayleigh/Stoneley waves with much of the mode energy propagating in the water column dominate the near-coastal ocean bottom microseism spectrum. Monitoring the southward propagation of swell from an extreme storm concentrated at the Oregon coast shows that near-coastal DF microseism levels are dominated by wave activity at the shoreline closest to the seismic station. Microseism attenuation estimates between on-land near-coastal stations and seismic stations 150 km inland indicate a zone of higher attenuation along the California coast between San Francisco and the Oregon border.
    [Show full text]
  • A Method for Harmonic Noise Elimination in Slip Sweep Data
    Societ y of Exploration Geophysicists International Exposition and 81st Annual Meeting 2011 (SEG San Antonio 2011) San Antonio, Texas, USA 18-23 September 2011 Volume 1 of 5 ISBN: 978-1-61839-184-1 Printed from e-media with permission by: Curran Associates, Inc. 57 Morehouse Lane Red Hook, NY 12571 Some format issues inherent in the e-media version may also appear in this print version. Copyright© (2011) by the Society of Exploration Geophysicists All rights reserved. Printed by Curran Associates, Inc. (2011) For permission requests, please contact the Society of Exploration Geophysicists at the address below. Society of Exploration Geophysicists P. O. Box 702740 Tulsa, Oklahoma 74170-2740 Phone: (918) 497-5554 Fax: (918) 497-5557 www.seg.org Additional copies of this publication are available from: Curran Associates, Inc. 57 Morehouse Lane Red Hook, NY 12571 USA Phone: 845-758-0400 Fax: 845-758-2634 Email: [email protected] Web: www.proceedings.com Table of Contents Simultaneous Source Applications and Techniques ACQ 1.1 (0001–0005) ACQ 1.5 (0020–0025) A method for harmonic noise elimination in slip sweep data On the separation of simultaneous-source data by inversion Shang Yongsheng, Wang Changhui*, and Zhang Mugang, BGP, CNPC; Zhou Gboyega Ayeni and Ali Almomin, Stanford University; Dave Nichols, Xuefeng, Li Zhenchun, Li Fenglei, and Dong Lieqian, China University of WesternGeco Petroleum ACQ 1.6 (0026–0031) ACQ 1.2 (0006–0010) Iterative separation of blended marine data: Discussion on the Sparsity-promoting recovery from simultaneous data: A coherence-pass filter compressive sensing approach Panagiotis Doulgeris*, Araz Mahdad, and Gerrit Blacquiere, Delft University Haneet Wason*, Felix J.
    [Show full text]
  • How Deep Ocean-Land Coupling Controls the Generation of Secondary Microseism Love Waves ✉ Florian Le Pape 1,2 , David Craig1,2 & Christopher J
    ARTICLE https://doi.org/10.1038/s41467-021-22591-5 OPEN How deep ocean-land coupling controls the generation of secondary microseism Love waves ✉ Florian Le Pape 1,2 , David Craig1,2 & Christopher J. Bean 1,2 Wind driven ocean wave-wave interactions produce continuous Earth vibrations at the seafloor called secondary microseisms. While the origin of associated Rayleigh waves is well understood, there is currently no quantified explanation for the existence of Love waves in the – 1234567890():,; most energetic region of the microseism spectrum (3 10 s). Here, using terrestrial seismic arrays and 3D synthetic acoustic-elastic simulations combined with ocean wave hindcast data, we demonstrate that, observed from land, our general understanding of Rayleigh and Love wave microseism sources is significantly impacted by 3D propagation path effects. We show that while Rayleigh to Love wave conversions occur along the microseism path, Love waves predominantly originate from steep subsurface geological interfaces and bathymetry, directly below the ocean source that couples to the solid Earth. We conclude that, in contrast to Rayleigh waves, microseism Love waves observed on land do not directly relate to the ocean wave climate but are significantly modulated by continental margin morphologies, with a first order effect from sedimentary basins. Hence, they yield rich spatio-temporal infor- mation about ocean-land coupling in deep water. 1 Geophysics Section, Dublin Institute for Advanced Studies, Dublin 2, Ireland. 2 iCRAG centre, University College Dublin, Dublin 4, Ireland. ✉ email: fl[email protected] NATURE COMMUNICATIONS | (2021) 12:2332 | https://doi.org/10.1038/s41467-021-22591-5 | www.nature.com/naturecommunications 1 ARTICLE NATURE COMMUNICATIONS | https://doi.org/10.1038/s41467-021-22591-5 better understanding of ocean generated seismic noise were analyzed for the period of March 2016 to March 2017.
    [Show full text]
  • Distributed Sensing of Microseisms and Teleseisms with Submarine Dark fibers
    CORE Metadata, citation and similar papers at core.ac.uk Provided by e_Buah - Biblioteca Digital de la Universidad de Alcalá ARTICLE https://doi.org/10.1038/s41467-019-13262-7 OPEN Distributed sensing of microseisms and teleseisms with submarine dark fibers Ethan F. Williams1*, María R. Fernández-Ruiz 2, Regina Magalhaes 2, Roel Vanthillo3, Zhongwen Zhan 1, Miguel González-Herráez2 & Hugo F. Martins4 Sparse seismic instrumentation in the oceans limits our understanding of deep Earth dynamics and submarine earthquakes. Distributed acoustic sensing (DAS), an emerging 1234567890():,; technology that converts optical fiber to seismic sensors, allows us to leverage pre-existing submarine telecommunication cables for seismic monitoring. Here we report observations of microseism, local surface gravity waves, and a teleseismic earthquake along a 4192-sensor ocean-bottom DAS array offshore Belgium. We observe in-situ how opposing groups of ocean surface gravity waves generate double-frequency seismic Scholte waves, as described by the Longuet-Higgins theory of microseism generation. We also extract P- and S-wave : phases from the 2018-08-19 Mw8 2 Fiji deep earthquake in the 0.01-1 Hz frequency band, though waveform fidelity is low at high frequencies. These results suggest significant potential of DAS in next-generation submarine seismic networks. 1 Seismological Laboratory, California Institute of Technology, 1200 E. California Boulevard, Pasadena, CA 91125-2100, USA. 2 Department of Electronics, University of Alcalá, Polytechnic School, 28805 Alcalá de Henares, Spain. 3 Marlinks, Sint-Maartenstraat 5, 3000 Leuven, Belgium. 4 Instituto de Óptica, CSIC, 28006 Madrid, Spain. *email: [email protected] NATURE COMMUNICATIONS | (2019) 10:5778 | https://doi.org/10.1038/s41467-019-13262-7 | www.nature.com/naturecommunications 1 ARTICLE NATURE COMMUNICATIONS | https://doi.org/10.1038/s41467-019-13262-7 ne of the greatest outstanding challenges in seismology is gauge length) by integration.
    [Show full text]
  • Global Trends in Extremal Microseism Intensity Richard C
    GEOPHYSICAL RESEARCH LETTERS, VOL. 37, L14303, doi:10.1029/2010GL043472, 2010 Click Here for Full Article Global trends in extremal microseism intensity Richard C. Aster,1 Daniel E. McNamara,2 and Peter D. Bromirski3 Received 30 March 2010; revised 25 May 2010; accepted 7 June 2010; published 21 July 2010. [1] Globally ubiquitous seismic background noise peaks principally due to seismic surface waves. This excitation, near 7 and 14 s period are generated via distinct the microseism, is observed globally, even in deep conti- mechanisms that transfer storm‐generated gravity wave nental interiors (Figure 1), and has long been recognized as energy to the seismic wave field. We utilize continuous a proxy of ocean wave and storm intensity [Gutenberg, digital ground motion data recorded by the Global 1947]. The single‐frequency (SFM; primary) and double‐ Seismographic Network and precursor instrumentation to frequency microseism (DFM; secondary) power spectral chronicle microseism power extreme events for 1972– density peaks are largely unaffected by common anthropo- 2009. Because most land‐observed microseism surface‐ genic noise sources [Withers et al., 1996; McNamara and wave energy is generated at or near coasts, microseism Buland, 2004]. SFMs are generated at the causative ocean metrics are particularly relevant to assessing changes in swell period via direct pressure fluctuations at the ocean coastal ocean wave energy. Extreme microseism winter bottom in shallow water resulting from breaking and/or storm season event counts reveal the widespread influence shoaling waves [Hasselmann, 1963]. The amplitude of the of the El Niño Southern Oscillation (ENSO). Individual much stronger DFM is proportional to the square of standing‐ station and ensemble slopes trend positive for this study wave components of the ocean wave field [Longuett‐Higgins, period for Northern Hemisphere stations.
    [Show full text]
  • Ambient Seismic Noise Interferometry Using Rotational Ground Motion
    Ambient seismic noise interferometry using rotational ground motion Céline Hadziioannou, Paul Neumann University of Hamburg, Germany Joachim assermann, Heiner !gel "udwig$%aximilians-University %unich, Germany Ulrich 'chreiber Technical University %unich, Germany … and the *+%Y team - .ideo recording of presentation here 0or scan the QR code23 Note4 most references are lin5s to the publications2 - Ne# sensing technologies 6 beyond conventional seismic translation measurements- Here: rotational ground motion Can we detect the wea5 ocean-generated seismic noise with the e&isting rotation sensors7 Can we /erform ambient noise interferometry #ith rotational motions7 !nterferometry with rotations 8 strain4 Paitz, Sager, 9ichtner: GJI 2<=> +bserving rotations4 Ring lasers G meter Observatory instruments: Ring lasers Ring lasers o?er a point measurement of rotational ground motion @ RLAS in Wettzell Germany: vertical com/onent rotation =; meter most sensitive worldwide co-located seismometer4 A( @ RO"Y near Munich Germany: RLAS Brst 3-com/onent rotation RO"# co-located seismometer4 9U* D*+%,4 A Multi-Component Ring Laser for Geodesy and Geophysics”, earthAr&iv D"ord of the Rings”, Science, 2<=F +bserving rotations4 Ring lasers Observatory instruments: Ring lasers @ RLAS in Wettzell Germany: vertical com/onent rotation most sensitive worldwide co-located seismometer4 A( @ RO"Y near Munich Germany: Brst 3-com/onent rotation co-located seismometer4 9U* Here: focus on vertical component: 'H- and Love waves %an we pic' up the ocean microseism? PP'L
    [Show full text]
  • Tsunami Glossary: a Glossary of Terms and Acronyms Used in The
    Intergovernmental Oceanographic Commission technical series 37 Tsunami Glossary A Glossary of Terms and Acronyms Used in the Tsunami Literature UNESC01991 The designations employed and the presentation of the material in this publication do not imply the expression of any opinion whatsoever on the part of the Secretariats of UNESCO and IOC concerning the legal status of any country or territory, or its authorities, or concerning the delimitations of the frontiers of any country or territory. For bibliographic purposes this document should be cited as follows: Tsunami Glossary, IOC Tech. Ser. 37, UNESCO, 1991 (English) Published in 1991 by the United Nations Educational, Scientific and Cultural Organization 7, place de Fontenoy, 75700 Paris Printed in UNESCO’s Workshops © UNESCO 1991 Printed in France SC/91/WS/27 PREFACE Tsunami Science is a relatively new field dating only a few decades. It is only in the last fifty years that the tsunami scientific literature proliferated. Many terms from other disciplines were adopted, modified, revised, and applied to the studies of the tsunami phenomena. Many other terms were redefined in the context of the components of this new scientific field. This glossary is intended to list as many as possible of the terms found in the tsunami literature and provide their specific definitions. It is intended for students, scientists, administrators and for anyone interested in tsunami. This book contains concise definitions of more than 2,000 terms. It includes terms from a multitude of disciplines. Primary, specialized and frequently-used tsunami terms are given with bolder headwords. Less frequently used terms are not highlighted.
    [Show full text]
  • Impacts of the Cryosphere and Atmosphere on Observed Microseisms Generated in the Southern Ocean
    manuscript submitted to JGR: Earth Surface Impacts of the cryosphere and atmosphere on observed microseisms generated in the Southern Ocean Ross J. Turner1;2, Martin Gal1;3, Mark A. Hemer4, and Anya M. Reading1;2 1School of Natural Sciences, University of Tasmania, Private Bag 37, Hobart, TAS 7001, Australia 2Institute for Marine and Antarctic Studies, University of Tasmania, Private Bag 129, Hobart, TAS 7004, Australia 3Institute of Mine Seismology, 50 Huntingfield Avenue, Huntingfield, TAS 7055, Australia 4CSIRO Oceans and Atmosphere Flagship, Hobart, TAS 7004, Australia Key Points: • Seasonal sea ice coverage is the dominant control on the microseism intensity in East Antarctica • Microseism events with extremal intensity are most prevalent in East Antarctica during March-April • East Antarctic extremal microseism events increase during the austral autumn for a negative SAM climate index arXiv:2108.08590v1 [physics.geo-ph] 19 Aug 2021 Corresponding author: R. J. Turner, [email protected] {1{ manuscript submitted to JGR: Earth Surface Abstract The Southern Ocean (in the region 60-180◦E) south of the Indian Ocean, Aus- tralia and the West Pacific is noted for the frequent occurrence and severity of its storms. These storms give rise to high-amplitude secondary microseisms from sources including the deep ocean regions, and primary microseisms where the swells impinge on submarine topographic features. A better understanding of the varying microseism wavefield enables improvements to seismic imaging, and development of proxy observ- ables to complement sparse in-situ wave observations and hindcast models of the global ocean wave climate. We analyse 12-26 years of seismic data from 11 seismic stations either on the East Antarctic coast or sited in the Indian Ocean, Australia and New Zealand.
    [Show full text]