Depth sensitivity of seismic coda waves to velocity perturbations in an elastic heterogeneous medium



Similar documents
Brief Review of Global Earth Velocity Structures and Seismology

Marine broadband seismic: Is the earth response helping the resolution revolution? N. Woodburn*, A. Hardwick, and R. Herring, TGS

Determination of source parameters from seismic spectra

DEM modelling of the dynamic penetration process on Mars as a part of the NASA InSight Mission

7.2.4 Seismic velocity, attenuation and rock properties

STUDY OF DAM-RESERVOIR DYNAMIC INTERACTION USING VIBRATION TESTS ON A PHYSICAL MODEL

Passive image interferometry and seasonal variations of seismic velocities at Merapi Volcano, Indonesia

Sound Power Measurement

Sputtering by Particle Bombardment I

A Time b). Redatuming Direct with Ghost by Correlation T AB + T BC

II. Earth Science (Geology) Section (9/18/2013)

CHAPTER 6 THE TERRESTRIAL PLANETS

AN APPLICATION MANUAL FOR BUILDING ENERGY AND ENVIRONMENTAL MODELLING

Acoustic Terms, Definitions and General Information

Semester 2. Final Exam Review

Which physics for full-wavefield seismic inversion?

This article appeared in a journal published by Elsevier. The attached copy is furnished to the author for internal non-commercial research and

The earthquake source

The Dynamic Crust 2) EVIDENCE FOR CRUSTAL MOVEMENT

Periodical meeting CO2Monitor. Leakage characterization at the Sleipner injection site

Seismic Waves Practice

Building Design for Advanced Technology Instruments Sensitive to Acoustical Noise

GCMs with Implicit and Explicit cloudrain processes for simulation of extreme precipitation frequency

Use of OpenFoam in a CFD analysis of a finger type slug catcher. Dynaflow Conference 2011 January , Rotterdam, the Netherlands

Development of EM simulator for sea bed logging applications using MATLAB

GPR Polarization Simulation with 3D HO FDTD

Nuevas tendencias de la Minería Subterránea profunda Planeación, operación y estabilización del macizo rocoso

PROHITECH WP3 (Leader A. IBEN BRAHIM) A short Note on the Seismic Hazard in Israel

Satish Pullammanappallil and Bill Honjas. Optim LLC, Reno, Nevada, USA. John N. Louie. J. Andrew Siemens. Siemens & Associates, Bend, Oregon, USA

3. Experimental Results

THERMAL STRATIFICATION IN A HOT WATER TANK ESTABLISHED BY HEAT LOSS FROM THE TANK

Introduction to Petroleum Geology and Geophysics

Waveform inversion of shallow seismic refraction data using hybrid heuristic search method

Interaction of Energy and Matter Gravity Measurement: Using Doppler Shifts to Measure Mass Concentration TEACHER GUIDE

Antennas & Propagation. CS 6710 Spring 2010 Rajmohan Rajaraman

Measuring Optical and Thermal Properties of High Temperature Receivers

DYNAMIC CRUST: Unit 4 Exam Plate Tectonics and Earthquakes

Tsunami Practice Questions and Answers Revised November 2008

Kinetic effects in the turbulent solar wind: capturing ion physics with a Vlasov code

4.3 Results Drained Conditions Undrained Conditions References Data Files Undrained Analysis of

Corso di Fisica Te T cnica Ambientale Solar Radiation

2 Absorbing Solar Energy

EFFECT OF SURFACE COVER ON GROUND TEMPERATURE SEASON S FLUCTUATIONS

Cloud-Resolving Simulations of Convection during DYNAMO

Limitations of Equilibrium Or: What if τ LS τ adj?

The APOLLO cloud product statistics Web service

A HELE-SHAW MODEL OF HEAT CONVECTION IN POROUS MEDIA UNDER GEOTHERMAL CONDITIONS

OPTIMIZATION OF VENTILATION SYSTEMS IN OFFICE ENVIRONMENT, PART II: RESULTS AND DISCUSSIONS

Transform Boundaries

How To Model An Ac Cloud

Heating & Cooling in Molecular Clouds

Subsalt Interferometric Imaging using Walkaway VSP and Offset Free Cable geometry: A Modeling Study

Measurement of the effect of biomass burning aerosol on inhibition of cloud formation over the Amazon

Laboratory scale electrical resistivity measurements to monitor the heat propagation within porous media for low enthalpy geothermal applications

Solarstromprognosen für Übertragungsnetzbetreiber

Name: Date: Class: Finding Epicenters and Measuring Magnitudes Worksheet

The APOLLO cloud product statistics Web service The APOLLO cloud product statistics Web service

The formation of wider and deeper clouds through cold-pool dynamics

Energy Transport. Focus on heat transfer. Heat Transfer Mechanisms: Conduction Radiation Convection (mass movement of fluids)

Magnitude 7.2 GUERRERO, MEXICO

Full azimuth angle domain decomposition and imaging: A comprehensive solution for anisotropic velocity model determination and fracture detection

APPLICATION OF DATA MINING TECHNIQUES FOR BUILDING SIMULATION PERFORMANCE PREDICTION ANALYSIS.

Waves disturbances caused by the movement of energy from a source through some medium.

Overview. What is EMR? Electromagnetic Radiation (EMR) LA502 Special Studies Remote Sensing

How To Design A Room Air Conditioning System

CFD Based Air Flow and Contamination Modeling of Subway Stations

Waves - Transverse and Longitudinal Waves

Real-time Ocean Forecasting Needs at NCEP National Weather Service

Solar Wind Heating by MHD Turbulence

Effects of Cell Phone Radiation on the Head. BEE 4530 Computer-Aided Engineering: Applications to Biomedical Processes

CHAPTER 9 FEM MODELING OF SOIL-SHEET PILE WALL INTERACTION

Ravi Kumar Singh*, K. B. Sahu**, Thakur Debasis Mishra***

Simulation of Offshore Structures in Virtual Ocean Basin (VOB)

1. The diagram below shows a cross section of sedimentary rock layers.

Biomedical Optics Theory

MODULE VII LARGE BODY WAVE DIFFRACTION

The ever increasing importance of reservoir geomechanics

An Introduction to Twomey Effect

ebb current, the velocity alternately increasing and decreasing without coming to

Impact of microphysics on cloud-system resolving model simulations of deep convection and SpCAM

COMPUTATIONAL FLOW MODEL OF WESTFALL'S 4000 OPEN CHANNEL MIXER R1. By Kimbal A. Hall, PE. Submitted to: WESTFALL MANUFACTURING COMPANY

W009 Application of VTI Waveform Inversion with Regularization and Preconditioning to Real 3D Data

An Analysis of the Rossby Wave Theory

Electromagnetic Radiation (EMR) and Remote Sensing

Chapter 2. Plate Tectonics. Plate Tectonics: Learning Goals

GEOPHYSICAL TESTING OF ROCK AND ITS RELATIONSHIPS TO PHYSICAL PROPERTIES FINAL REPORT

Development and optimization of a hybrid passive/active liner for flow duct applications

Blackbody radiation. Main Laws. Brightness temperature. 1. Concepts of a blackbody and thermodynamical equilibrium.

Optimum Solar Orientation: Miami, Florida

Magnitude 8.8 OFFSHORE MAULE, CHILE

Field Data Recovery in Tidal System Using Artificial Neural Networks (ANNs)

Transcription:

Depth sensitivity of seismic coda waves to velocity perturbations in an elastic heterogeneous medium Anne Obermann* Thomas Planès* Eric Larose Christoph Sens-Schönfelder Michel Campillo Montpellier August 212 *PhD Students

Motivation Central question in monitoring of ambient seismic noise: Depth of the temporal changes! Monitoring of ambient seismic noise during slow slip events in the Guerrero region Mexico (Rivet et al. (211)) Apparent temporal change of velocity (tt) Coda: Rayleigh waves Locating the depth of the change (lower crust)

Depth Motivation Rivet et al. assumption Coda: mainly Rayleigh waves Heterogeneous medium Coda: Rayleigh wave Bulk wave conversions Influence on the depth sensitivity of coda waves

2 D Simulations v p v ' p v p d h z =16km x Model parameters -2D velocity model with random velocity fluctuations -free surface 3 absorbing boundaries = 3 m σ = 2% v p = 65 m/s h = 2 m = 2/3 dv/v=1.5% f=2hz x=16km SPECFEM 2D Komatitsch et al.

normalized displacement Stretching Technique 1 5.5 5.6 5.7 t in s -1 ' 3 6 9 t in s Hadziiannou et al. (JASA 29)

Apparent velocity variations versus depth Result from the simulation 6 x 1-3 std dev data 4 2 1 2 3 depth (km)

Apparent velocity variations versus depth Result from the simulation 6 x 1-3 std dev data 4 1 D surface wave regime 2 2 D diffusion regime of body waves 1 2 3 depth (km)

Apparent velocity variations versus depth Result from the simulation 6 x 1-3 std dev data 4 1 D surface wave regime 2 2 D diffusion regime of body waves 1 2 3 depth (km) Model Surf ( 1 ) α=fitting parameter; partition coefficient Bulk

S R Bulk Regime: Sensitivity Kernel ) ( ) ( ) ( ) ( t r s p du u t r x p u x s p t x r s K t Pacheco and Snieder (25) Intensity Propagator ) ( t r s p Diffusion radiative transfer... ) ( V bulk t x r s K t v dv v dv local relative velocity change in the volume element ΔV around x

epsilon Surface Wave Sensitivity Regime 3.5 4 x 1-3 3 std dev Data Radiative Transfer 2.5 2 1.5 1.5 1 2 3 4 depth (km) = apparent velocity change

epsilon epsilon Surface Wave Sensitivity Regime 3.5 3 x 1-3 std dev Data Radiative Transfer.15.1 Surface wave sensitivity 2.5 2 1.5 1 2 3 depth (m).5 1 2 3 depth (m) = apparent velocity change

epsilon epsilon Surface Wave Sensitivity Regime 3.5 3 x 1-3 std dev Data Radiative Transfer Model.15.1 Surface wave sensitivity 2.5 2 1.5 1 2 3 depth (m).5 1 2 3 depth (m) = apparent velocity change

epsilon normalized displacement Model 4 x 1-3 3 std dev Data Model 1 2-1 ' 3 6 9 t in s 1 1 2 3 4 depth (km) = apparent velocity change Model Surf ( 1 1-α =.75 α =.25 ) α=fitting parameter; partition coefficient Bulk

partition coefficient Evolution of the partition coefficient 1 =5% =1% =15% =2% =3%.5 1- (bulk) (surf) 2 4 6 2 4 6 2 4 6 2 4 6 2 4 6 time in coda (s) Model Surf ( 1) Bulk

partition coefficient partition coefficient Evolution of the partition coefficient 1 =5% =1% =15% =2% =3%.5 1- (bulk) (surf) 2 4 6 2 4 6 2 4 6 2 4 6 2 4 6 time in coda (s) 1.8.6.4.2 =5% =1% =15% =2% =3% Mean free time t*=l*/c 1 2 3 4 5 6 t/t*

Shallow or deep perturbation? Perturbation at shallow depth (2 m) Perturbation at great depth (15 m)

Shallow or deep perturbation? Application to lunar data Passive Seismic Experiment of the Apollo 17 Sens-Schönfelder & Larose (28) Velocity variations as a consequence of temperature variations induced by solar irradiation influence limited to shallow subsurface only

Conclusion We can relate the depth sensitivity of coda waves to a combination of bulk-wave and surface-wave sensitivity Changes can be detected at large depth Time dependence of the relative velocity change in the coda - possibility to discriminate a shallow and a deep perturbation Apply the new sensitivity kernel to seismic monitoring in regions with strong scattering (volcanoes fault zones). Obermann et al. (212). Depth sensitivity of seismic coda waves to velocity perturbations in an elastic heterogeneous medium. Submitted to GJI Piton de la Fournaise La Reunion Island

absorbing Bulk Regime: Diffusion vs Radiative transfer absorbing absorbing absorbing

Bulk Regime: Diffusion vs Radiative transfer Simulation of the bulk regime without free surface source and receiver in the middle obs 1.4 x 1-3 1.2 1.8.6 std dev Data ( bulk ) radiative transfer approx. diffusion approx. = apparent velocity change.4.2 4 6 8 1 12 14 depth (km) No free parameters = direct fit!