Description of a software package for signal detection and association using waveform cross correlation. Recovery of aftershock sequences of the largest events: Sumatra 2004 and Tohoku 2011. Finding of a small aftershock of the September 9, 2016 DPRK test.
Organic Name Reactions for the students and aspirants of Chemistry12th.pptx
Recovery of aftershock sequences using waveform cross correlation: from catastrophic earthquakes to smallest aftershocks
1. Automatic recovery of aftershock sequences at the International Data Centre: from concept to pipeline
Dmitry Bobrov, Ivan Kitov, and Mikhail Rozhkov
International Data Centre, Preparatory Commission for the Comprehensive Nuclear Test-Ban Treaty Organization
Abstract
Aftershocks of larger earthquakes represent an important source of
information on the distribution and evolution of stresses and
deformations in pre-seismic, co-seismic and post-seismic phases. For the
International Data Centre (IDC) of the Comprehensive Nuclear-Test-Ban
Organization (CTBTO) largest aftershocks sequences are also a challenge
for automatic and interactive processing. The highest rate of events
recorded by two and more seismic stations of the International
Monitoring System (IMS) from a relatively small aftershock area may
reach hundreds per hour (e.g. Sumatra 2004 and Tohoku 2011).
Moreover, there are thousands of reflected/refracted phases per hour with
azimuth and slowness within the uncertainty limits of the first P-waves.
Misassociation of these later phases, both regular and site specific, as the
first P-wave results in creation of numerous wrong event hypotheses in
automatic IDC pipeline. In turn, interactive review of such wrong
hypotheses is direct waste of analysts’ resources. Waveform cross
correlation (WCC) is a powerful tool to separate coda phases from actual
P-wave arrivals and to fully utilize the repeat character of waveforms
generated by events close in space. Array seismic stations of the IMS
enhance the performance of the WCC in two important aspects – they
reduce detection threshold and effectively suppress arrivals from all
sources except master events. A prototype of IDC specific aftershock tool
has been developed and merged with standard IDC pipeline. The tool
includes several procedures: creation of master events consisting of
waveform templates at ten and more IMS stations; cross correlation (CC)
of real-time waveforms with these templates, association of arrivals
detected at CC-traces in event hypotheses; building events matching IDC
quality criteria; and resolution of conflicts between events hypotheses
created by neighbouring master-events. The final cross correlation
standard event lists (XSEL) is a start point of interactive analysis. Since
global monitoring of underground nuclear tests is based on historical and
synthetic data, each aftershock sequence can be tested for the CTBT
violation with big earthquakes as an evasion scenario.
Disclaimer: The views expressed on this poster are those of the authors and do not necessary reflect the views of the PTS CTBTO
AUTOMATIC RECOVERY OF THE BIGGEST SEQUENCIESWAVEFORM CROSS CORRELATION AND AFTERSHOCKS
MASTER EVENTS SMALL AFTERSHOCK OF THE DPRK SEPT 9, 2016 UNDERGROUND TEST
Preparatory Commission for the Comprehensive Nuclear-Test Ban Treaty Organization, Provisional Technical Secretariat,
Vienna International Centre, P.O. Box 1200, A-1400 Vienna, Austria. E-mail: ivan.kitov@ctbto.org www.ctbto.org
S31A-2703
Conclusion
A bigger aftershock sequence is a challenge for IDC
automatic and interactive processing.
Waveform cross correlation is an effective technique to
accurately recover even the biggest aftershock sequences with
thousands of events.
Cross correlation bulletin (XSEL) includes only REB-
compatible (EDC) events.
XSEL provides more REB-compatible events than GA.
XSEL provides higher quality and consistency for REB
events.
XSEL completeness grows with time as new and higher
quality master events are available.
XSEL events need no global location and have smaller
confidence ellipses as related to master events.
The analysts’ workload may be reduced by several times with
higher location accuracy and bulletin completeness.
Waveforms cross correlation is a powerful tool for REB
quality check and expert technical analysis.
Cross correlation works best with arrays.
Configuration of IMS arrays should not be changed to
preserve the same set of master events and templates.
Cross correlation is an effective monitoring method for weak
aftershock activity.
The method of waveform cross correlation (WCC) allows
remote monitoring of weak seismic activity induced by
moderate size earthquakes as well as underground
explosions. For nuclear explosions, this type of monitoring
is considered as a principal task of on-site inspection under
the Comprehensive nuclear-test-ban treaty.
On September 11, 2016, a seismic event with body wave
magnitude 2.1 was found in automatic WCC processing
near the epicenter of the underground explosion conducted
by the DPRK on September 9, 2016. This event occurred
approximately two days after the test. The automatic
procedure based on WCC was developed by the IDC and
runs in testing mode since 2011.
Using the WCC method, two array stations of the
International Monitoring System (IMS), USRK and KSRS,
detected Pn-wave arrivals, which were associated with a
unique event. Standard automatic processing at the
International Data Centre (IDC) did not create an event
hypothesis, but in the following interactive processing
based on WCC detections, an IDC analyst was able to
create a two-station event with local magnitude ML=2.4
(after magnitude correction at station USRK). Location and
other characteristics of this small seismic source indicate
that it is likely an aftershock of the preceding explosion.
Building on the success of automatic detection and phase
association, we carried out an extended analysis, which
included later phases and closest non-IMS stations. The
final cross correlation solution uses four stations, including
MDJ (The People's Republic of China) and SEHB
(Republic of Korea), with the epicenter approximately 2
km to north-west from the epicenter of the Sept. 9 test. We
also located the aftershock epicenter by standard IDC
program LocSAT using the arrival times obtained by cross
correlation. The distance between the DPRK and LocSAT
aftershock epicenters is 25.5 km, i.e. by an order of
magnitude larger than that obtained by the WCC relative
location method.
Component-to-component, E-W (H1), N-S (H2), Z,
comparison of signals from the DPRK5 and its
aftershock as measured at IMS stations USRK (a) and
KSRS (b). Pn- and Pg-waves from the aftershock at
channels H1 (E-W) and H2 (N-S) of USRK are
similar to those from the DPRK5 - c).
The local association grid around the DPRK4. The
distance between circles and nodes is approximately 15
km. Red star shows the node with the automatically
found event hypothesis. The RMS origin time residual for
the two-station event is 0.054 s.
Component-to-component, E-W (H1), N-S (H2),
and Z, comparison of signals from the DPRK5 and
its aftershock as measured at stations SEHB and
MDJ. The Pn-wave arrival at SEHB is poor,
nevertheless found by WCC.
Relative positions of the test site (star), two IMS
arrays (open circles), and two 3-C stations (open
triangles).
The position of the aftershock (red dot) relative to
the DPRK5 epicenter (blue dot). The distance
between two events is ~2 km as estimated from
cross correlation arrivals at four stations. Color bar
shows the RMS origin time residual measured in
seconds.
Absolute locations of the DPRK5 (red star) and
aftershock (blue circle) with 90% confidence
ellipses as obtained by IDC location software
LocSAT. The result of aftershock relative location
is shown by green circle.
a)
b)
c)
For purposes of signal association and event
location, each grid point is extended by a subnet
with five circles of nodes spaces by ~25 km.
Coordinates of all nodes for all masters are fixed
and saved in WCC database. For each node, the
master-station travel times are corrected for the
distance between the global grid point and the
node. These corrected travel times are used in
arrival association by origin times.
All nodes are processed individually, but may use
the same set of physical signals (arrivals) obtained
by cross correlation. The node with the largest
number of associated stations and the lowermost
scattering (RMS) of origin times wins and is saved
as an event hypothesis. Other hypotheses are
rejected.
The fifths circle is ~100 km in radius (i.e. very
close to the grid points of adjacent masters) and all
winning hypotheses obtained at this circle, which
are many, are rejected in further conflict resolution
because they must be found by the adjacent
masters in the first place
Global Grid of Master Events is designed for finding and
location of seismic events based on cross-correlation (CC).
The whole globe is subdivided uniformly by cells
surrounding the grid points. The IMS stations consider the
hypotheses of seismic event occurrence within these cells
based on matched filter detection with the pre-established
Master Event signals (template). The template is a set of
certain data, including array multi-channel waveforms,
azimuth and slowness estimations, event-station travel
times, and magnitude. When the predefined and master-
station dependent WCC detection threshold is exceeded as
triggered by the current seismogram, the multi-stage
location procedure is started.
The choice of adequate templates is one of the key points
of detection and location procedures. Real masters work
best for similar events – earthquakes for earthquakes and
explosions for explosions. All kind of sources and thus
seismograms can be simulated numerically. These
synthetic master events most useful in aseismic zones,
where real master events are not available.
GLOBAL SEISMICITY MEASURED BY IMS NETWORK
WAVEFORM CROSS CORRELATION
DETECTION USING CROSS CORRELATION COEFFICIENT
PHASE ASSOCIATION, CONFLICT RESOLUTION
Global seismicity is unevenly distributed with a few zones, where catastrophic earthquakes with Mw>7 can happen. Such
events are usually accompanied by extensive aftershock sequences (black areas in the map), which are repeated events
with similar signals within a relatively tight territory. Waveform cross correlation (WCC) is a natural method to detect
signals and associate them with events.
We select high quality waveform templates (left panel) from a number of master events measured at IMS stations and
run cross correlation over real-time signals (right panel). For an array, we calculate CC on each trace and then average
them over all traces to get an aggregate CC. Selection of master events is crucial for the WCC method.
Detection is carried out with STA/LTA method adapted at the IDC. Detection threshold depends on station (3-C,
array). When detected on a CC-trace, all signals are processed by standard procedures to estimate their attributes,
After extensive quality checking, valid detections are associated with events with a Local Association
(LA) procedure based on empirical travel times between master events and IMS stations. IDC event
definition criteria (EDC) are applied. When several masters compete for the same physical arrival,
conflict resolution is applied as based on event quality, i.e. number of phases, RMS origin time
residual.
HISTORICAL EVENTS AUTOMATIC EVENTS (SEL3) GLOBAL GRID (DETECTION)
Currently, IDC database includes more than 500,000 seismic
events. We have selected 6,000 master events, also with depth, to
cover the observed seismicity. Example of historical events
(open black circles) available before Tohoku 2011. Green circles
- IDC interactive events.
REGULAR GRID OF MASTER EVENTS, GRAND MASTER
IDC produces automatic event list, SEL3, which may contain
a number of quality event hypothesis, which can be used as
master events. Example of Tohoku 2011 SEL3 – open red
circles.
When historical or automatic events are not available in some zones, one (Grand Master) or several best quality
events can be moved from their estimated positions to nodes of a regular grid to cover these blind spots. Grand Master
creates a uniform master set with uniform resolution over the studied area and can be extended to global level.
NEPAL 2015
GG (LOCATION)
TOHOKU 2011
Selection of master events (red circles) from the REB
Recovery of the aftershock sequence (blue circles)
Selection of master events (red circles) from the REB.
Recovery of the aftershock sequence (blue circles)
Nepal 2015: input of IMS stations to XSEL and REB
Tohoku 2011: input of IMS stations to XSEL and REB
NEPAL
(2015115)
TOHOKU
(2011070)
SUMATRA
(2004361)
REB ALL 286 797 724
REB
aftershocks
209 725 625
REB with
SEL3 evid’s
132 538 497
SEL3 ALL 262 887 910
SEL3 in
AREA
109 628 526
XSEL 362 1408 1459
REB FOUND 197 694 592
REB NOT
FOUND
12 31 33
STATISTICS OF PERFORMANCE
NEPAL: 12 events
NOT FOUND REB EVENTS
TOHOKU: 31 event
The pipeline based of the waveform cross correlation
method is more effective in automatic finding real
event hypotheses (XSEL vs. SEL3 with the same
evid’s and XSEL vs. REB FOUND)) matching the
IDC Event Definition Criteria and creates much less
invalid event hypothesis (SEL3 ALL vs REB).
Overall, the completeness of the REB increases (REB
vs. XSEL) with decreasing analyst workload.
By design, the WCC is also characterized by higher
potential of adjustment to specific sources, e.g.
earthquakes and explosions. When recovering
intensive aftershock sequences (hundreds of events
per day) with standard seismological methods based
on detections related to the change in energy flux one
might miss bigger man-made events. Fine tuning of
templates to specific sources is able to reduce the
threshold of detection for the events of interest.