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Global grid of master events for waveform cross correlation: design and testing Kitov, I., D. Bobrov, and M. Rozhkov International Data Centre Preparatory Commission for the Comprehensive Nuclear-Test-Ban Treaty Organization Provisional


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Global grid of master events for waveform cross correlation: design and testing

Kitov, I., D. Bobrov, and M. Rozhkov

International Data Centre Preparatory Commission for the Comprehensive Nuclear-Test-Ban Treaty Organization Provisional Technical Secretariat Vienna International Centre P.O. Box 1200 A-1400 Vienna AUSTRIA ivan.kitov@ctbto.org

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Acknowledgements The authors are grateful to the IDC and especially to all analysts reviewing XSEL and REB events. This presentation has been produced with the assistance of the European Union, EU Council Decision 2010/CFSP of 26 July 2010. Disclaimer The content of this presentation is the sole responsibility of the authors and can in no way be taken to reflect the views of the European Union and the CTBTO Preparatory Commission.

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Background

Comprehensive Nuclear-Test-Ban Treaty

The Comprehensive Nuclear-Test-Ban Treaty (CTBT) obligates each State Party not to carry out any nuclear explosions, independently of their size and purpose. The Technical Secretariat (TS) of the Comprehensive Nuclear-Test-Ban Treaty Organization will carry out the verification of the CTBT. The International Data Centre (IDC) is an integral part of the (currently Provisional) TS. It receives, collects, processes, analyses, reports on and archives data from the International Monitoring System (IMS). The IDC is responsible for automatic and interactive processing of the IMS data and for standard IDC products. The IDC is also required by the Treaty to progressively enhance its technical capabilities.

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Objectives

To built a global grid of master events for waveform cross correlation To assess the performance of waveform cross correlation as a technique of seismic monitoring using the global grid of master events

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Outline

  • 1. Motivation
  • 2. Global seismic monitoring: IMS
  • 3. Global seismicity: IDC view
  • 4. Cross correlation at teleseismic distances
  • 5. Actual and grand master events
  • 6. Machine learning and classification
  • 7. Synthetic master events
  • 8. Underground nuclear explosions as master events
  • 9. Global cross correlation grid. Design

10.Testing. February 12, 2013

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Cross correlation as an IDC technique

Motivation

  • Regional studies demonstrate significant improvement in

detection, location, and magnitude estimation.

At least an order of magnitude!

  • Many IMS primary stations are arrays enhancing the capability
  • f cross correlation analysis
  • For arrays, correlation distance depends on phase and its

slowness

  • At teleseismic distances, high level of cross correlation is
  • bserved for signals from events spaced by 100 km and even

more

  • Remote events may have similar signals
  • Small events can be considered as point sources
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IMS, seismic network

Green circles – primary arrays Green triangles – primary 3-C stations Small green circles – auxiliary arrays The primary network includes many arrays

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Global seismicity: the IDC view

Waveform cross correlation relies on high quality master events REB events with zero depth: yellow – a neighbor closer than 50 km; red – no neighbor within 50 km

Monitoring is global. How to populate the aseismic area with quality master event?

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Waveform cross correlation

6 s 6 s CC STA LTA SNR=STA/LTA≥3.0

Detection: CC > CCtr SNR_CC > SNRtr

Multichannel waveforms Master template Four frequency bands Adjusted template length Waveform quality check CC for individual channels Averaged CC trace Detection Multichannel CC-detector better sees signals from slave events close to the master

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Actual and grand masters: Sumatera 2012

  • 2

2 4 6 86 88 90 92 94 96 lat, deg long, deg Regular grid REB Real masters main shock

  • 2

2 4 6 86 88 90 92 94 96 lat, deg long, deg

1181 REB events between April 11 and May 24 , 2012

  • 7 IMS array stations
  • 16 master events: actual and grand

masters

  • 2763 XSEL hypotheses
  • 409 (~15%) randomly chosen XSEL

events were reviewed by analysts

  • 119 new REB events
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Machine learning: classification

Nsta XSEL Tree Bagger SVM Naive Bayes 1066 1406 848 1 489 487 613 2 382 253 540 3 2080 324 208 452 4 514 347 256 198 5 129 115 113 80 6 31 31 31 24 7 9 9 9 8 Total 2763 826 617 762

ASAR CMAR GERES MKAR SONM WRA ZALV

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Grand masters: Atlantic Ocean

Cross correlation of signals from remote events 931 REB events; 3 array stations with SNR>3

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Grand masters: Atlantic Ocean

Cross correlation coefficient for 931 events in seismic region 32 Events are ordered by latitude: north to south Matrix of cross correlation coefficients (color coded) Signals correlation does not dependent on the distance between events

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Cross correlation: explosion signals

  • 100 waveforms
  • 25 underground

nuclear explosions

  • 6.2 > mb > 4.5
  • 2015 m > H > 150 m
  • 60 stations
  • 16º > ∆ > 100º

Towards seismic monitoring of underground nuclear explosions

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Cross correlation of explosion signals

Synthetic seismograms: ∆ =30º, 45º, 60º, 90º H=0.1, 0.3, 0.6, 1.0, 2.0 km fc= 0.8 Hz to 4.8 Hz

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Cross correlation of explosion signals

Principal Component Analysis 10 best components for real and synthetic waveforms CCs for 100 real waveforms correlated with real PC CCs for 100 real waveforms correlated with synthetic PC Synthetics demonstrate excellent performance when used for waveforms cross correlation

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Global Cross Correlation Grid

Master: Ten primary seismic arrays at P-wave distances (6 to 96 degrees)

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Global Cross Correlation Grid Segment R = 100 km

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Global Cross Correlation Grid Testing, February 12, 2013

REB - 134 events Grid: 25000 nodes Group 1 = WRA, TORD, MKAR, ILAR, GERES, PDAR, CMAR, SONM, AKASG, BRTR, GEYT Group 2 = ASAR, ZALV, YKA, ARCES, TXAR, KSRS Group 3 = USRK, FINES, NVAR, NOA, MJAR Defining parameters: Templates: simplest 1D synthetic waveform for all arrays, theoretical time delays Detections: SNRmin = 0.5; SNR_CCmin=2.5; CCmin = 0.2; FKSTATmin = 2.5; AZRESmax= 20.0º; SLORESmax = 2.0 s/º; Events: dTorigin = 6s; NSTAmin= 3; AZGAPmax= 330º RESULTS: Total arrivals and hypotheses: 22,900,402 arrivals; 107,969 events; After conflict resolution: SNR_CC>2.5 SNR_CC>3.0 SNR_CC>3.5 SNR>2 XSEL 6,141 events 766 122 2351 REB Matched 92 90 77 101 DPRK 2013: time - 02:57:50.799 , d=24.92 km, OTres=0.1s; nsta=9: AKASG, BRTR, CMAR, GERES, GEYT, ILAR, MKAR, SONM, WRA

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Global Cross Correlation Grid

  • V0.1: All master templates are synthetics same at all stations, a version of f-k

analysis

  • V0.2: Master templates are station/master specific synthetics in 1D velocity

model

  • V0.3: Master templates are station/master/source (e.g. explosion) specific

synthetics calculated for 2D velocity structure (e.g. ak135+CRUST 2.0)

  • V1.1: Real master templates are used where possible
  • V1.2: Grand master events are applied where possible
  • V2.0: The set of principal components are optimized where possible as
  • btained by the PCA applied to the complete set of actual and historical

data

  • V3.0: Synthetic + real master templates based on principal components with

classification algorithms trained on actual data

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Discussion

  • IMS array stations make possible automatic processing based on

waveform cross correlation

  • Cross correlation is a powerful technique allowing to reduce the

detection threshold and relative location accuracy by an order of magnitude, i.e. to find by 50% to 100% more (smaller) REB events

  • Grand master and synthetic master events may reduce the

magnitude threshold of seismic monitoring by 0.4 units of magnitude

  • The Global Cross Correaltion Grid is flexible (e.g. master density,

templates, number of stations, thresholds, etc.) to fulfill various tasks including effective monitoring of UNEs