background seismicity rates from interevent-time statistics · 2017. 4. 3. · short interevent...

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Page 1: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Background seismicity rates frominterevent-time statistics:

Spatial patterns appear stationary through time

Jeanne HardebeckUnited States Geological Survey

Page 2: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Background earthquake rate

Assumes two earthquake classes:

1) Background events: occur as direct response toloading (e.g. tectonic, magmatic.)

2) Triggered events: caused by other earthquakes.

Page 3: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Background earthquake rate

Important for:• Time-independent seismic hazard assessment.• Background rate changes related to loadingrate changes => fault physics; time-dependentseismic hazard.• Background rate changes related to stressshadows => static versus dynamic stresstriggering debate.

Page 4: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Background earthquake rate

Difficult to measure:• Background rate obscured by triggered events.• Standard declustering methods (Reasenberg,Gardner & Knopoff) rely on two unknown,subjectively adjustable parameters: the length-scale and time-scale that define a “triggered”event.• A poster today: Van Stiphout “How far can wetrust declustering algorithms?”

Page 5: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Earthquake interevent-time distribution

- Time between successive events i and i+1: Δti = ti+1 - ti.- N earthquakes, catalog duration T, given area and magnitude range.- Normalize by average interevent time, τi=Δti*(N/T).

Page 6: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Short interevent times: clustered => power law.Long interevent times: Poissonian => exponential.

Gamma distribution combinespower law and exponential:

Gamma distribution formulationfrom Hainzl et al., BSSA 2006,following Corral, PRL, 2004.

Earthquake interevent-time distribution

Page 7: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Method of Hainzl et al., BSSA 2006:Background fraction found objectivelyand easily from mean and variance ofinterevent-time distribution:

Follows from gamma distribution:

Earthquake interevent-time distribution

Page 8: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Follows from gamma distribution:

Gamma distribution is apoor fit to our data!

Earthquake interevent-time distribution

Method of Hainzl et al., BSSA 2006:Background fraction found objectivelyand easily from mean and variance ofinterevent-time distribution:

Page 9: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Earthquake interevent-time distributionTheoretical distribution:

Another form of the theoreticaldistribution from Gutenberg-Richter and Omori laws wasderived by Saichev and Sornette,JGR 2007.

Page 10: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma
Page 11: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

2000 ETAS simulations: Hainzl et al method works well, but requires acorrection based on direct p-value (not usually known for real data.)

Page 12: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Northern California

1980-2007

Page 13: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Method used for USseismic hazard maps.

ObjectiveSubjective, using recommended parameters: Reasenberg Gardner & Knopoff

Page 14: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma
Page 15: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Calaveras

Parkfield

High rate

Page 16: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma
Page 17: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Calaveras Fault

Page 18: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

San Andreas Fault: Parkfield

Page 19: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma
Page 20: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Schorlemmer et al., JGR 2004

Page 21: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Conclusions:

• The Hainzl et al method can accurately recover thebackground fraction, for ETAS simulations, but requires acorrection based on the direct p-value.

• Gamma distribution poorly fits the observed and ETASinterevent-time distributions, especially for high direct p-value.

• The background rate in Northern California is spatiallyvariable, but appears generally stable through time.

• Parkfield seismicity is remarkably stationary: earthquakelocations, background rate, and b-value.

Page 22: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Future Work - Methodology:

• Develop a method to use the theoretical interevent-timedistribution (rather than gamma distribution) to findbackground fraction and direct p-value.

• Develop a quantitative measure of uncertainty for theestimated background rate. Explore sources of error such ascatalog incompleteness.

Page 23: Background seismicity rates from interevent-time statistics · 2017. 4. 3. · Short interevent times: clustered => power law. Long interevent times: Poissonian => exponential. Gamma

Future Work - Applications:

• Quantify the stability of background rate through time.• New background rates for seismic hazard estimates.• Search for temporal changes in background rate, especiallyin areas of changing stressing rate:

- Volcanic areas: does background rate change due toloading from magma movement?- Subduction zones: does background rate change due toloading from episodic slow-slip events?

- Stress shadows: do they exist?• Etc…