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Automated Earthquake Response Systems

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Automated Earthquake Response Systems Tom Heaton, Caltech Hiroo Kanamori, Caltech Egill Hauksson, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ – PowerPoint PPT presentation

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Title: Automated Earthquake Response Systems


1
Automated Earthquake Response Systems
  • Tom Heaton, Caltech
  • Hiroo Kanamori, Caltech
  • Egill Hauksson, Caltech
  • Georgia Cua, ETH, Switzerland
  • Masumi Yamada, Kyoto Univ
  • Maren Böse, Caltech

2
Earthquake Alerting a different kind of
prediction
  • What if earthquakes were really slow, like the
    weather?
  • We could recognize that an earthquake is
    beginning and then broadcast information on its
    development on the news.
  • an earthquake on the San Andreas started
    yesterday. Seismologists warn that it may
    continue to strengthen into a great earthquake
    and they predict that severe shaking will hit
    later today.

3
Shakeout Simulation (Aagaard and Graves)
  • ..\Documents\2008\ShakeOut_LosAngeles_lowres.mov

4
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5
If the earthquake is fast, can we be faster?
  • Everything must be automated
  • Data analysis that a seismologist uses must be
    automated
  • Communications must be automated
  • Actions must be automated
  • Common sense decision making must be automated

6
How would the system work?
  • Seismographic Network computers provide estimates
    of the location, size, and reliability of events
    using data available at any instant estimates
    are updated each second
  • Each user is continuously notified of updated
    information . Users computer estimates the
    distance of the event, and then calculates an
    arrival time, size, and uncertainty
  • An action is taken when the expected benefit of
    the action exceeds its cost
  • In the presence of uncertainty, false alarms must
    be expected and managed

7
What we need is a special seismologist
  • Someone who has good knowledge of seismology
  • Someone who has good judgment
  • Someone who works very, very fast
  • Someone who doesnt sleep
  • We need a Virtual Seismologist

8
Ground motion envelope our definition
Full acceleration time history
Efficient data transmission 3 components each
of Acceleration, Velocity, Displacement, of 9
samples per second
envelope definition max.absolute value over
1-second window
9
Estimating M from ratios of P-wave motions
  • P-wave frequency content scales
  • with M (Allen and Kanamori, 2003, Nakamura,
    1988)
  • Find the linear combination of log(acc) and
    log(disp) that minimizes the variance within
    magnitude-based groups while maximizing
    separation between groups (eigenvalue problem)
  • Estimating M from Zad

10
  • Voronoi cells are nearest neighbor regions
  • If the first arrival is at SRN, the event must
    be within SRNs Voronoi cell
  • Green circles are seismicity in week prior to
    mainshock

11
What about Large Earthquakes with Long Ruptures?
  • Large events are infrequent, but they have
    potentially grave consequences
  • Large events potentially provide the largest
    warnings to heavily shaken regions
  • Point source characterizations are adequate for
    Mlt7, but long ruptures (e.g., 1906, 1857) require
    finite fault

12
Strategy to Handle Long Ruptures
  • Determine the rupture dimension by using
    high-frequencies to recognize which stations are
    near source
  • Determine the approximate slip (and therefore
    instantaneous magnitude) by using low-frequencies
    and evolving knowledge of rupture dimension
  • We are using Chi-Chi earthquake data to develop
    and test algorithms

13
10 seconds after origin
20 seconds after origin
Near-field Far-field
Near-field Far-field
14
30 seconds after origin
40 seconds after origin
Near-field Far-field
Near-field Far-field
15
  • Once rupture dimension is known
  • Obtain approximate slip from long-periods
  • Real-time GPS would be very helpful
  • Evolving moment magnitude useful for estimating
    probable rupture length
  • Magnitude critical for tsunami warning

16
Real-time prediction of ultimate rupture
B?se and Heaton, in prep.
Remaining Rupture Length
slip
Is the rupture on the San Andreas fault?
17
Distributed and Open Seismic Network
  • Just in the gedanken phase
  • Tens of thousands of inexpensive seismometers
    running on client computers.
  • Sensors in buildings, homes, buisinesses
  • Data managed by a central site and available to
    everyone.
  • It will change the world!

18
Conclusions
  • Earthquake warning is an extension of current
    systems that provide rapid information in
    earthquakes (e.g. ShakeMap)
  • Significant warning times can be achieved for
    moderate to light shaking
  • Heavily damaged areas in moderate events (M 6)
    will not receive warning
  • Heavily damaged areas in great earthquakes (M
    7.5) will receive
  • Strategies to determine rupture dimension and
    slip look very promising
  • User decision making should be based on
    cost/benefit analysis need to develop a
    community that develops optimal responses
  • Managing expectations is critical users must
    understand what EEW wont do.

19
Probabilistic Rupture Prediction ? Probabilistic
Ground Shaking
B?se and Heaton, in prep.
20
  • We are experimenting with different Linear
    Discriminant analyses to distinguish near-field
    from far-field records

21
Percent of area receiving warning time T or
greater (log N6.89-Mw)
Pseudovelocity cm/sec
Warning time T sec
Heaton, 1985
22
3 sec after initial P detection at SRN
  • Prior information
  • Voronoi cells
  • Gutenberg-Richter

Single station estimate
M, R estimates using 3 sec observations at SRN
No prior information
8 km M4.4
  • Prior information
  • Voronoi cells
  • No Gutenberg-Richter

9 km M4.8
Note star marks actual M, RSRN
23
Virtual Seismologist (VS) method for seismic
early warning
  • Bayesian approach to seismic early warning
    designed for regions with distributed seismic
    hazard/risk
  • Modeled on back of the envelope methods of
    human seismologists for examining waveform data
  • Shape of envelopes, relative frequency content
  • Robust analysis
  • Capacity to assimilate different types of
    information
  • Previously observed seismicity
  • State of health of seismic network
  • Known fault locations
  • Gutenberg-Richter recurrence relationship

24
Data set for learning the envelope
characteristics Most data are from TriNet, but
many larger records are from COSMOS
  • 70 events, 2 lt M lt 7.3, R lt 200 km
  • Non-linear model estimation (inversion) to
    characterize waveform envelopes for these events
  • 30,000 time histories

25
Average Rock and Soil envelopes as functions of
M, R rms horizontal
acceleration
26
Distinguishing between P- and S-waves
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33
  • Sum of 9 point source envelopes
  • Vertical acceleration

34
horizontal acceleration ampl rel. to ave. rock
site
Vertical P-wave acceleration ampl rel. to ave.
rock site
horizontal velocity ampl rel. to ave. rock site
vertical P-wave velocity ampl rel. to ave. rock
site
35
Strategy for acceleration envelopes
  • High-frequency energy is proportional to rupture
    are (Brune scaling)
  • Sum envelopes from 10-km patches
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