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Seismic source inversion in mining environments Simone Cesca Institute of Geophysics, University of Hamburg [email protected] http://mine.zmaw.de. Outline The MINE project background, structure and project aims Seismic source inversion problem theory and methods - PowerPoint PPT Presentation
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Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Seismic source inversion in mining environments
Simone Cesca
Institute of Geophysics, University of Hamburg
http://mine.zmaw.de
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Outline
The MINE project
• background, structure and project aims
Seismic source inversion problem
• theory and methods
• point and kinematic source inversion using the Kiwi tools
Source inversion in mining environments
• an application to coal mining induced seismicity (Ruhr, Germany)
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
The MINE project, a quick overview
MINing Environment: continuous monitoring and simultaneous inversion
Funding, positions, timeline
• German Ministery of Education and Science (BMBF – Geotechnologien Programme)
• Junior Research project, 1 Leading Scientist + 3 PhDs
• 3+3 years duration (started 1.7.2010)
Aims
• Mining monitoring (seismicity, fracturing, stress perturbation) and imaging
Adapt full waveform techniques from classical seismology and to mining
Combine information from different data streams
Provide portable software tools to analyse mine datasets
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Research lines
Detection and location using full waveforms
Signal characterization
Moment tensor inversion
Extended source parameters
Spatio-temporal patterns of seismicity
Stress inversion (seismicity patterns and focal mechanisms)
Local earthquake tomography
WP1
Detection, Location,
Characterization
WP3
Stress inversion
WP2
Source
Inversion
WP4
Tomography
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Hamm,
Ruhr region
Courtesy M. Bischoff
Biscoff et al. (2010)
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Pyhäsalmi
Deep metal mine in Europe
Collaboration with NORSAR (Kuhn, Oye, Roth, Nath)
3D velocity model
Multi-stream monitoring system
Seismic
Internal deformation
Thermal measurements
Others
Figure T. Mäki (2000)
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Cerville
SALT
MARLS
LIMESTONE(DOLOMIE)
190 m
125 m
50 m
Courtesy P. Jousset
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Source inversion in seismology
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Source inversion in seismology, overview
Global CMT catalogue, shallow earthquakes, 1976-2005
Slip map
kinematic model
(Li et al. 2002)
Source: http://cgsweb.moeacgs.gov.tw/
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Source inversion in seismology, what do we need?
Moment tensor / Kinematic sourceInversion routine
Plotting and result evaluation
Data access(waveform and
metadata)Data preprocessing
Green's functions(database)
Inversion method,Inv. Parameters
(e.g. BP, tapers, ...)
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
OpenSource
Running under Linux
Python + Fortran implementation http://kinherd.org
Source inversion in seismology using the Kiwi tools
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Point source model, double couple & moment tensor
More complete point source model is represented by a moment tensor (MT)
MT = MTDC + MTCLVD + MTISO
Earthquakes is often well modeled in terms of shear cracks, using a point source representation (DC model).
after Hasegawa et al. (1989)
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Extended source model, definitions
Extended sources may be reproduced by superposition of several point sources distributed along a planar (or bended) rupture surface. Each point source start radiating when reached by the rupture front. Radiation lasts for a given (rise) time.
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
The eikonal source model
Circular area, plus constraints
Rupture velocity scales with shear velocity
Despite its flexibility, the eikonal source model is described by only 13 parameters (considering constraints and earth model as fixed and known)
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
One earthquake, five solutions
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Source model parameters and inversion priorities
Source model parameters (13)
Time Lat Lon Depth M0 Strike Dip Rake NucX NucY RuptV RiseTRad
General source description
Source location Radiation pattern Rupture process
Scale of source model
Point source Finite source
Information from data
Low frequencies High frequencies
Inversion priority
Step 1, 2 Step 3
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Greece,
Shallow earthquakes
2003-2007
extended sources
Cesca et al. JGR 2010
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Source inversion, natural and induced seismicity
Cesca et al. submitted
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Source inversion in mining environment
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Bischoff et al. 2010
Ruhr region
Coal mining induced seismicity monitored by Ruhr University since 1983
About 1000 events are recorded between 0.7<ML<3.3 every year
Hamm region (blue circle)
>7000 events in 2006-2007 (14 months)
913 events 0.0<ML<2.0
DC inversion
MT inversion
Kinematic inversion and rupture modeling
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Seismicity follows longwall mining,
Epicenters are spreaded over an area of about 2x2km
6 broadband stations (5 Guralp CMG, pink; 1 Trillium 40, purple)
9 short-period (Mark L-4C-3D, orange)
3 subsurface stations (yellow)
We work here at 0.5-2Hz or 1-4Hz, only BB stations are used
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Seismicity follows longwall mining
Additional clusters
Average depth above mining level
Bimodal frequency-magnitude distribution
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Inversion strategy
Depth M0 Strike Dip RakeTime Lat LonTime Lat Lon NucX NucY RuptV RiseTRad
Time Lat Lon Depth M0 Strike Dip Rake NucX NucY RuptV RiseTRad
Time Lat Lon Depth M0 Strike Dip Rake NucX NucY RuptV RiseTRad
Time Lat Lon Depth M0 Strike Dip Rake NucX NucY RuptV RiseTRadTime Lat Lon Depth M0
Step 1, Focal mechanism (DC and full moment tensor)
amplitude spectra inversion, whole waveform
Depth M0 Strike Dip Rake
1
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Inversion strategy
Depth M0 Strike Dip RakeTime Lat LonTime Lat Lon NucX NucY RuptV RiseTRad
Time Lat Lon Depth M0 Strike Dip Rake NucX NucY RuptV RiseTRad
Time Lat Lon Depth M0 Strike Dip Rake NucX NucY RuptV RiseTRad
Time Lat Lon Depth M0 Strike Dip Rake NucX NucY RuptV RiseTRadTime Lat Lon Depth M0
Step 1, Focal mechanism (DC and full moment tensor)
amplitude spectra inversion, whole waveform
Depth M0 Strike Dip Rake
1
Step 2, Polarity control / Centroid location
time domain inversion, whole waveforms
Depth M0 Strike Dip RakeTime Lat Lon
2
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Inversion strategy
Depth M0 Strike Dip RakeTime Lat LonTime Lat Lon NucX NucY RuptV RiseTRad
Time Lat Lon Depth M0 Strike Dip Rake NucX NucY RuptV RiseTRad
Time Lat Lon Depth M0 Strike Dip Rake NucX NucY RuptV RiseTRad
Time Lat Lon Depth M0 Strike Dip Rake NucX NucY RuptV RiseTRadTime Lat Lon Depth M0
Step 1, Focal mechanism (DC and full moment tensor)
amplitude spectra inversion, whole waveform
Depth M0 Strike Dip Rake
1
Step 2, Polarity control / Centroid location
time domain inversion, whole waveforms
Depth M0 Strike Dip RakeTime Lat Lon
2
Step 3, Kinematic model
amplitude spectra or time domain inversion, including high freqencies
NucX NucY RuptV RiseTRadTime Lat Lon Depth M0 Strike Dip Rake
3
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
DC inversion results overview
Successful inversion for 578 (over 913)
Magnitude range, Mw 0.3-1.8
Very similar mechanisms
Normal faults (80%) or oblique-normal
One steep plane, one sub-horizontal
Different strike are observed, strike angles are related to mining geometry
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Wehling-Benatelli (2011)
Courtesy D. Becker
Waveform similarity analysis and
cluster analysis (relocated events)
Consistent focal mechanisms for
Major clusters
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Moment tensor / extended source parameters
Full MT solutions significant for more than 100 events
Non-DC terms results are still ambiguous
Possible inversion artefact rather than source features
Preliminar kinematic inversion for 24 largest events (Ml > 1.0)
Kinematic model is significant for 8 events, only
In almost all cases (7), the vertical rupture plane is preferred
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Conclusions
Full waveform moment tensor inversion successfully applied to mining induced seismicity at local scale (<2km) for low magnitude events (at now, down to Mw 0.3).
DC and MT focal mechanisms were successfully obtained for 587 selected events
Results are in good agreement with reference, when available (about 100 events), based on first polarities and S wave polarization.
Better results are obtained for a layered model and frequency range 0.5-2Hz
Focal mechanisms are characterized by similar ruptures. Normal faulting with one steep fault plane. In general, striking angles are linked to the mining geometry.
Non-DC resolution to be judged
Preliminar kinematic modeling for largest events (Ml≥1.0) point to a similar rupture mechanism along sub-vertical planes.
Cesca, 2011. Source inversion in mining environments
AIM 2nd annual meeting, 29-30.9.2011, Institute of Geophysics, Academy of Sciences of the Czech Republic, Praha
Thanks to:
A. T. Şen, Prof. Dr. T. Dahm, Dr. S. Heimann, F. Grigoli, S. Maghsoudi, A. Rohr,
M. Bischoff, T. Meier, S. Wehling-Benatelli
BMBF project MINE
GEOTECHNOLGIEN programme
The Kiwi tools are currently used at:
University of Hamburg, University of Potsdam, BGR Hannover, GFZ Potsdam,
University of Coimbra, Aristotle University of Thessaloniki ,Ruhr University Bochum
Further info on software and applications:
http://mine.zmaw.de
http://kinherd.org
Cesca et al., JGR 2010
Cesca et al., J. Seismol. 2010
Cesca et al., J. Seismol., submitted