creating the virtual seismologist tom heaton, caltech georgia cua, eth, switzerland masumi yamada,...

33
Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

Upload: terence-hawkins

Post on 03-Jan-2016

251 views

Category:

Documents


1 download

TRANSCRIPT

Page 1: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

Creating the Virtual Seismologist

Tom Heaton, CaltechGeorgia Cua, ETH, SwitzerlandMasumi Yamada, Kyoto Univ

Maren Böse, Caltech

Page 2: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

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.”

Page 3: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

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

Page 4: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

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 …. User’s 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

Page 5: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

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 doesn’t sleep

• We need a Virtual Seismologist

Page 6: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

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

Page 7: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

Full acceleration time history

envelope definition– max.absolute value over 1-second window

Ground motion envelope: our definition

Efficient data transmission3 components each ofAcceleration, Velocity, Displacement, of9 samples per second

Page 8: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

70 events, 2 < M < 7.3, R < 200 kmNon-linear model estimation (inversion) to characterize waveform envelopes for these events~30,000 time histories

Data set for learningthe envelope characteristics

Most data are fromTriNet, but many larger records are from COSMOS

Page 9: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

Average Rock and Soil envelopes as functions of M, R rms horizontal acceleration

Page 10: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

Distinguishing between P- and S-waves

Page 11: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

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

Estimating M from ratios of P-wave motions

Page 12: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

SRN

STGLLS

DLA

PLS

MLS

CPP

WLT

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

Page 13: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

3 sec after initial P detection at SRN

M, R estimates using 3 sec observations at SRN

Epi dist est=33 km

M=

5.5

Note: star marks actual M, RSRN

Prior information:-Voronoi cells-Gutenberg-Richter

Prior information:-Voronoi cells-No Gutenberg-Richter

8 kmM=4.4

9 kmM=4.8

Single station estimate:

No prior information

Page 14: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

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 M<7, but long ruptures (e.g., 1906, 1857) require finite fault

Page 15: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

Warning time T [sec]

Pse

udov

eloc

ity [c

m/s

ec]

Heaton, 1985

Percent of area receiving warning time T or greater (log N*=6.89-Mw)

Page 16: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

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

Page 17: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

• We are experimenting with different Linear Discriminant analyses to distinguish near-field from far-field records

Page 18: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

10 seconds after origin 20 seconds after origin

Near-fieldFar-field

Near-fieldFar-field

Page 19: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

Near-fieldFar-field

Near-fieldFar-field

30 seconds after origin 40 seconds after origin

Page 20: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

• 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

Page 21: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

Real-time prediction of ultimate rupture

Bӧse and Heaton, in prep.

slip

Is the rupture on the San Andreas fault?

Page 22: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

22

Probabilistic Rupture Prediction → Probabilistic Ground Shaking

Bӧse and Heaton, in prep.

Page 23: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

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!

Page 24: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

Conclusions• Bayesian statistical framework allows integration of many

types of information to produce most probable solution and error estimates

• 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

• Need to carry out Bayesian approach from source estimation through user response. In particular, the Gutenberg-Richter recurrence relationship should be included in either the source estimation or user response.

• If a user wants ensure that proper actions are taken during the “Big One”, false alarms must be tolerated

• Managing expectations is critical … users must understand what EEW won’t do.

Page 25: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech
Page 26: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech
Page 27: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech
Page 28: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech
Page 29: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech
Page 30: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech
Page 31: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

• Sum of 9 point source envelopes

• Vertical acceleration

Page 32: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

horizontal 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

Vertical P-wave acceleration ampl rel. to ave. rock site

Page 33: Creating the Virtual Seismologist Tom Heaton, Caltech Georgia Cua, ETH, Switzerland Masumi Yamada, Kyoto Univ Maren Böse, Caltech

Strategy for acceleration envelopes

• High-frequency energy is proportional to rupture are (Brune scaling)

• Sum envelopes from 10-km patches