Parkfield Borehole Network
The operation of the High Resolution Seismic Network (HRSN) at
Parkfield, California began in 1987,
as part of the U.S. Geological Survey initiative known as the
Parkfield Prediction Experiment (PPE) (Bakun and Lindh, 1985).
Figure 5.1 shows the location of the network,
its relationship to the San Andreas fault, sites of significance
from previous and ongoing research using the HRSN, relocated earthquake locations
from 1987-1998.5, routine locations of seismicity since August 2002,
and the epicenter of the 1966 M6 earthquake that motivated the PPE.
The HRSN records exceptionally high-quality data, owing to its
13 closely spaced three-component borehole sensors (generally emplaced
in the extremely low attenuation and background noise environment at 200 to 300 m
depth (5.1)), its high-frequency
wide bandwidth recordings (0-125 Hz), and its low magnitude detection threshold
(recording events below magnitude -1.0).
Several aspects of the Parkfield
region make it ideal for the study of small earthquakes and their
relationship to tectonic processes. These include the fact that the
network spans the expected nucleation region of a repeating
magnitude 6 event and a significant portion of the transition from locked to creeping
behavior on the San Andreas fault, the availability of
three-dimensional P and S velocity models (Michelini and McEvilly, 1991), a
seismicity catalogue that is complete to very low magnitudes and
that includes at least half of the M6 seismic cycle, a well-defined and
simple fault segment,
a homogeneous mode of seismic energy release as indicated by the
earthquake source mechanisms (over 90
right-lateral strike-slip),
and the planned drilling zone and penetration and instrumentation site
of the San Andreas Fault deep observatory at depth experiment
(SAFOD) (see: http://www.earthscope.org/safod/index.html or
http://www.iris.iris.edu/HQ/EarthScope/EarthScope.saf.html).
Figure 5.1:
Map showing the San Andreas Fault trace, the location of the original
10 Parkfield HRSN stations (filled diamonds) and the 3 new sites installed
to enhance coverage of the region containing the SAFOD facility (open
diamonds), along with the BDSN station PKD (filled square).
The locations of the 8 source points
for the Vibroseis wave propagation monitoring experiment are
represented by small black triangles. The epicenter of the 1966 M6
Parkfield main shock is located at the large open circle. The location
of the pilot hole and SAFOD drill site is shown by the filled star,
and the location of the 2 alternative M2 repeating earthquake targets (70 meters
apart) are shown as concentric circles. Because of the SAFOD experiment,
the 4 km by 4 km dashed box surrounding the SAFOD zone is a region of particular
interest to BSL researchers.
Routine locations of earthquakes recorded by the expanded and
upgraded 13 station HRSN are shown as open black circles.
Locations of events recorded by the earlier vintage 10 station HRSN, relocated
using an advanced 3-D double-differencing
algorithm applied to a cubic splines interpolated 3-D velocity model
(Michelini and McEvilly, 1991), are shown as gray points.
Station GHIB (Gold Hill, not shown) is located on the San Andreas Fault about
8 km to the Southeast of station EADB.
 |
In a series of journal articles and Ph.D. theses, we have
presented the cumulative, often unexpected, results of U.C. Berkeley's
HRSN research efforts
(see: www.seismo.berkeley.edu/seismo/faq/parkfield_bib.html).
They trace the evolution of a new and exciting picture of
the San Andreas fault zone responding to its plate-boundary
loading, and they are forcing new thinking on the dynamic
processes and conditions within the fault zone at the sites of
recurring small earthquakes.
The HRSN was installed in deep (200-300m) boreholes beginning in 1986. Sensors are
3-component geophones in a mutually orthogonal gimbaled package. This
ensures that the sensor corresponding to channel DP1 is aligned vertically
and that the others are aligned horizontally. In November
1987, the Varian well vertical array was installed and the first
VSP survey was conducted, revealing clear S-wave anisotropy in the
fault zone (Daley and McEvilly, 1990). During 1988, the original
network was completed to a ten station
3-component 500 sps set of stations telemetered into a central
detection/recording system operating in triggered mode and incorporating
a deep (572 m) sensor in
the Varian well string into the network. The Varian system was
slaved in 1988, for about two years, to the Vibroseis control
signals, allowing simultaneous recording of vibrator signals on
both systems. For several years beginning in 1991, low-gain event
recorders (from PASSCAL) were installed at several of the sites
to extend the dynamic range to
about 4.5. The
data acquisition system operated quite reliably until late 1996,
when periods of unacceptably high down time developed. During this period
as many as
7 of the remote, solar-powered telemetered stations were occasionally
down simultaneously
due to
marginal solar generation capacity, old batteries, and
recording system outages of a week or more were not uncommon. In July of 1998
the original data acquisition system
failed permanently. This system
was a modified VSP recorder acquired from LBNL, based on a 1980-
vintage LSI-11 cpu and a 5 MByte removable Bernoulli system disk
with a 9-track tape drive, configured to record both triggered
microearthquake and Vibroseis data (discontinued in 1994, Karageorgi et
al., 1997). The system was remote and completely autonomous, and
data
tapes were mailed about once a month to Berkeley for processing and analysis. The old
system also had a one-sample timing
uncertainty and a record length limitation because the tape write system
recovery after event detection was
longer than the length of the record, leaving the system off-line after record
termination and until write recovery was completed.
In December of 1998, the original HRSN acquisition system was replaced
by 10 stand-alone PASSCAL RefTek systems with continuous recording.
To process these data, development of a major data handling procedure was
required,
in order to identify the microearthquakes down to M = -1,
since continuous telemetry to
the Berkeley Seismological Laboratory (BSL) and application of a central site detection
scheme was not an option at that time.
In July, 1999 we had to reduce the network to four RefTeks at critical
sites that would ensure continuity in monitoring at low magnitudes and
the archive of characteristic events for studying the evolution of
their recurrence intervals. Properties of the 10 original sites are
summarized in Table 5.2.
Table 5.1:
Stations of the Parkfield HRSN.
Each HRSN station is listed with its station code, network id, location,
date of initial operation, and site description.
The latitude and longitude (in degrees) are given in the WGS84 reference frame,
the surface elevation (in meters) is relative to mean sea level, and the depth
to the sensor (in meters) below the surface.
Coordinates and station names for the 3 new sites are given at the bottom.
| Site |
Net |
Latitude |
Longitude |
Surf. (m) |
Depth (m) |
Date |
Location |
| EADB |
BP |
35.89525 |
-120.42286 |
499 |
245 |
01/1988 - |
Eade Ranch |
| FROB |
BP |
35.91078 |
-120.48722 |
542 |
284 |
01/1988 - |
Froelich Ranch |
| GHIB |
BP |
35.83236 |
-120.34774 |
433 |
63 |
01/1988 - |
Gold Hill |
| JCNB |
BP |
35.93911 |
-120.43083 |
559 |
224 |
01/1988 - |
Joaquin Canyon North |
| JCSB |
BP |
35.92120 |
-120.43408 |
487 |
155 |
01/1988 - |
Joaquin Canyon South |
| MMNB |
BP |
35.95654 |
-120.49586 |
731 |
221 |
01/1988 - |
Middle Mountain |
| RMNB |
BP |
36.00086 |
-120.47772 |
1198 |
73 |
01/1988 - |
Gastro Peak |
| SMNB |
BP |
35.97292 |
-120.58009 |
732 |
282 |
01/1988 - |
Stockdale Mountain |
| VARB |
BP |
35.92614 |
-120.44707 |
511 |
572 |
01/1988 - |
Varian Well |
| VCAB |
BP |
35.92177 |
-120.53424 |
790 |
200 |
01/1988 - |
Vineyard Canyon |
| CCRB |
BP |
35.95716 |
-120.55161 |
601 |
251 |
05/2001 - |
Cholame Creek |
| LCCB |
BP |
35.98006 |
-120.51423 |
637 |
252 |
08/2001 - |
Little Cholame Creek |
| SCYB |
BP |
36.00942 |
-120.53661 |
947 |
252 |
08/2001 - |
Stone Canyon |
|
Table 5.2:
Instrumentation of the Parkfield HRSN. Most HRSN
sites have L22 sensors and were originally digitized with a RefTek 24
system. After the failure of the WESCOMP recording system,
PASSCAL RefTek recorders were installed. In July of 1999, 6 of the
PASSCAL systems were returned to IRIS and 4 were left at critical
sites.
The upgraded network uses a Quanterra 730 4-channel system.
For the three new stations (bottom) horizontal orientations are approximate
(N45W and N45E) and will be determined more accurately in the near future.
| Site |
Sensor |
Z |
H1 |
H2 |
RefTek 24 |
RefTek 72-06 |
Quanterra 730 |
|
|
|
|
|
| EADB |
Mark Products L22 |
-90 |
170 |
260 |
01/1988 - 12/1998 |
12/1998 - 07/1999 |
03/2001 - |
|
|
|
|
|
| FROB |
Mark Products L22 |
-90 |
338 |
248 |
01/1988 - 12/1998 |
12/1998 - 07/1999 |
03/2001 - |
|
|
|
|
|
| GHIB |
Mark Products L22 |
90 |
failed |
unk |
01/1988 - 12/1998 |
12/1998 - 07/1999 |
03/2001 - |
|
|
|
|
|
| JCNB |
Mark Products L22 |
-90 |
0 |
270 |
01/1988 - 12/1998 |
12/1998 - 06/2001 |
03/2001 - |
|
|
|
|
|
| JCSB |
Geospace HS1 |
90 |
300 |
210 |
01/1988 - 12/1998 |
12/1998 - 07/1999 |
03/2001 - |
|
|
|
|
|
| MMNB |
Mark Products L22 |
-90 |
175 |
265 |
01/1988 - 12/1998 |
12/1998 - 06/2001 |
03/2001 - |
|
|
|
|
|
| RMNB |
Mark Products L22 |
-90 |
310 |
40 |
01/1988 - 12/1998 |
12/1998 - 07/1999 |
03/2001 - |
|
|
|
|
|
| SMNB |
Mark Products L22 |
-90 |
120 |
210 |
01/1988 - 12/1998 |
12/1998 - 06/2001 |
03/2001 - |
|
|
|
|
|
| VARB |
Litton 1023 |
90 |
15 |
285 |
01/1988 - 12/1998 |
12/1998 - 07/1999 |
03/2001 - |
|
|
|
|
|
| VCAB |
Mark Products L22 |
-90 |
200 |
290 |
01/1988 - 12/1998 |
12/1998 - 06/2001 |
03/2001 - |
|
|
|
|
|
| CCRB |
Mark Products L22 |
-90 |
N45W |
N45E |
- |
- |
05/2001 - |
|
|
|
|
|
| LCCB |
Mark Products L22 |
-90 |
N45W |
N45E |
- |
- |
08/2001 - |
|
|
|
|
|
| SCYB |
Mark Products L22 |
-90 |
N45W |
N45E |
- |
- |
08/2001 - |
|
|
|
|
|
|
Thanks to emergency funding from the USGS NEHRP, we have replaced
the original 10-station system with a modern 24-bit acquisition system
(Quanterra 730 4-channel digitizers, advanced software using flash disk
technology, spread-spectrum telemetry, Sun Ultra 10/440 central
processor at the in-field collection point, with 56K frame-relay
connectivity to Berkeley). The new system is now online and recording
data continuously at a central site located on the California
Department of Forestry (CDF) fire station in Parkfield.
We have also added three new borehole stations at the NW end of the
network as part of the SAFOD
project, with NSF support, to improve resolution at the planned
drilling target on the fault. Figure 5.1 illustrates
the location of the proposed drill site (star), the new borehole sites,
and locations of earthquakes recorded by the initial and the
upgraded/expanded HRSN.
These three new stations
use similar hardware to the main network, with the addition
of an extra channel for electrical signals. Station descriptions and
instrument properties are summarized in Tables 5.1 and
5.2. All HRSN Q730 data loggers employ FIR filters to extract data at
250 and 20 Hz (Table 5.3).
Table 5.3:
Data streams currently being acquired at each HRSN site.
Sensor type, channel name, sampling rate, sampling mode, and
type of FIR filter are given. C indicates continuous;
T triggered; Ac acausal; Ca causal. "?" indicates orthogonal
vertical and 2 horizontal components.
| Sensor |
Channel |
Rate (sps) |
Mode |
FIR |
| Geophone |
DP? |
250.0 |
T |
Ca |
| Geophone |
BP? |
20.0 |
C |
Ac |
|
The remoteness of the drill site and new stations require an intermediate
data collection point at Gastro Peak, with a microwave link to the CDF
facility. The HRSN stations use SLIP to transmit TCP and UDP data packets over
bidirectional spread-spectrum radio links between the on-site data
acquisition systems and the central recording system at the CDF.
Six of the sites
transmit directly to a router at the central recording site. The other seven
sites transmit to a router at Gastro Peak, where the data are aggregated and
transmitted to the central site over a 4 MBit/second digital 5.4 GHz microwave
link. All HRSN data are recorded to disk at the CDF site. A modified
version of the REDI real-time system detects events from the HRSN data,
creates event files with waveforms from the HRSN
and sends the event data in near real-time to UC Berkeley.
Currently the continuous data is being migrated to DLT tape when local disk space
fills up, and the tapes are mailed to the BSL for long-term storage.
Efforts are being made to acquire funding to make this data Internet accessible
to the research community through the NCEDC.
The upgraded system is compatible with the data flow and archiving common to
all the elements of the BDSN/NHFN and the NCEDC, and is providing remote
access and control of the system. It is also providing data with better
timing accuracy and longer records, which are to eventually flow seamlessly
into NCEDC. The new system also solves the problems of timing resolution, dynamic
range, and missed detections, in addition to providing the added advantage
of conventional data flow (the old system recorded SEGY format).
Over the past year, activities associated with the operation of the HRSN
primarily involved three components: 1) routine operations and maintenance
of the network, 2) enhancement of the network's performance for detection
and recording of very low magnitude earthquakes, and 3) routine data processing
and analysis.
In addition to the routine maintenance tasks required
to keep the HRSN in operation, various
refinements and adjustments to the networks infrastructure
and operational parameters have been needed this year to
correct for pathologies that continue to manifest themselves in
the recently upgraded and expanded system.
A feature of the new system that has been particularly useful
both for routine maintenance and for pathology identification has
been the Internet connectivity of the central site processing computer
and the station data loggers with the computer network at BSL. Through
this connection, select
data channels and on-site warning messages from the central site processor
are sent directly to BSL for evaluation by project personnel.
If, upon these evaluations, more detailed information
on the HRSN's performance is required, it can also be directly accessed.
Analysis of this remotely acquired information has been extremely useful
for trouble shooting by allowing field personnel to schedule and plan
the details of maintenance visits to Parkfield.
The connectivity also allows certain data acquisition parameters to be modified
remotely when needed, and commands can be sent to the central site computer
and data loggers to modify or restart processes when necessary.
The network connectivity allows analysts at the BSL to routinely
perform checks on the system health of the HRSN and its data quality.
One example of a technique used by BSL analysts involves the use of
teleseismic arrivals from deep focus earthquakes. Since seismic waves
from such events impose a near simultaneous and vertically incident
plane wave of relatively uniform amplitude on all HRSN
stations, seismograms from these events can be used to assess
relative station responses across the network and help identify pathologies
in station polarities, individual component failures and other response
characteristics.
Figure 5.2 shows an example of a recent teleseism
recorded on the DP1 (vertical) channel across the network. Not shown
are recordings from stations MMNB and VARB. The initial display of
seismograms from this teleseism showed these station components to be
responding abnormally at the time of the earthquake. Based on this
teleseismic result other remotely acquired information was uploaded
from the HRSN and it was determined that these components were indeed
malfunctioning. Subsequent field visits were then scheduled and the
necessary repairs made.
Figure 5.2:
Displayed are 30 seconds of 0.5-2.0 Hz BP filtered vertical ground velocity data
for a
6.9 deep focus teleseism which occurred 6/23/2003 at 12:12 UT
at a depth of 685 km in the vicinity of the Rat Islands in the Aleutian
Islands chain (51.44N,176.78E). The traces have been ordered by
increasing distance (top to bottom), their waveforms are absolute
scaled to allow comparisons between the response functions between stations.
The great circle distance to the HRSN is approximately 46.5
degrees with an azimuth of
310
. The recording of this
teleseism on the Northern Hayward Fault Network is show in Figure
4.2.
 |
The network connectivity also allows remote monitoring of the background
noise levels being recorded by the HRSN stations. For example shown in
Figure 5.3 are power spectral density plots of background
noise for vertical components of the 7 HRSN stations that are most critical
for monitoring seismicity in the region containing SAFOD. The PSD analysis
gives a rapid assessment of the HRSN seismometer responses across their
wide band-width. By routinely generating these plots with data telemetered
from Parkfield, changes in the seismometer responses, often indicating problems with
the acquisition system, can be easily identified, and corrective measures can
then be planned and executed on a relatively short time-frame.
Figure:
Background noise PSD plot for the seven continuously
telemetered BP.DP1 data streams from Parkfield. The data are 20 minute
samples starting at 2003.225.0900 (2 AM PDT).
The plots show the
background noise PSD as a function of frequency for the the highest
available sampling rate (250 sps) vertical component data which are
continuously telemetered to Berkeley.
Note the relatively low PSD levels and the overall consistency for all the
HRSN stations. By comparison, the PSD curves among the borehole Northern
Hayward Fault Network (NHFN) land and bridge
stations (Figure 4.3) are much more variable and show a generally
higher background noise level. On the other hand, PSD curves for the MPBO
stations of the NHFN are much more consistent with the HRSN PSD's (Figure 8.6). The
differences among the various station PSD's can, in large part, be
explained by the relative cultural noise
levels at the various stations, by the depth of the borehole sensors, and
by whether the boreholes remain open holes (noisier) or have been filled
with cement. The 2 Hz minimum in the PSD plots for the HRSN sensor results
from the 2 Hz sensors used at these sites. Below 2 Hz, noise levels rise
rapidly and the peak at 3 sec (.3 Hz) is characteristic of teleseismic noise
observed throughout California. In the 2 to 5 Hz range, VCAB
and JCNB have historically shown higher background noise which is believed
to result from excitation modes in the local structure.
A small 60 Hz blip can be seen in the SCYB curve
due to its close proximity to a power-line.
 |
Triggered event data for the HRSN is also telemetered in near real time
to the BSL, and this allows for rapid evaluation of the triggered data.
This year we have implemented a semi-automated waveform and trigger review
procedure using a graphical user interface (GUI). This procedure is now
being used to review the triggered waveform data daily to discriminate
between earthquake and non-earthquake events and to pick P and S phases
of the local events. In the process, our analyst/field technician also
makes note of obvious problems with station/component specific earthquake
recording, and this malfunction information is used to identify maintenance
needs for the HRSN.
Over the past year significant efforts were made to identify and reduce noise
problems arising from the new and expanded data acquisition system.
Detection, monitoring, and high-resolution recording of
earthquakes down to the smallest possible magnitudes with the highest
possible signal-to-noise (especially in the region of the proposed SAFOD
drilling) is a major objective of the HRSN data collection effort.
Consequently, elimination of all sources of unnaturally occurring system noise
is a primary goal. The minimization of data loss due to station
outages and data-dropouts is also critical to this objective.
The sophisticated HRSN data acquisition involves integration of a
number of distinct components at each station (i.e., sensor, preamp,
solar panels, solar regulator, batteries, Freewave radio, antenna,
lightening arresters, and associated cabling, connectors and grounds) and
radio telemetry apparatus between the seismic stations, telemetry relay stations,
and the central processing site on the CDF site in Parkfield.
This complex integration of station and communication components
combined with a variety of associated concerns (e.g., ground loops,
cable resistances, radio feedback into recording equipment at stations, radio interference between stations,
marginal line of site paths, cloud cover and solar power, the integration of older
(pre-upgrade) hardware components with new
components, old component deterioration and failures, and malfunctioning and
unexpected performance characteristics of newer components) all make
identification of specific causes of
network generated (i.e. artificial) noise difficult
to identify.
Exhaustive and iterative testing of HRSN performance has
identified two primary causes for observed artificial noise remaining in the system
(i.e. solar regulator spiking and preamp self-noise generation).
We have designed and have implemented or are in the process of implementing
fixes for these problems. We are also continuing to improve the HRSN
event detection sensitivity by refining the HRSN triggering scheme.
Regularly occurring spikes occurring during the daylight hours were observed
in the continuous data streams and found to be due to the solar regulators. We have
tested a variety of solar regulator designs and have identified the Prostar 30 as
having the optimal cost-benefit. We have purchased and installed several of these devices
at several of the HRSN sites with the ultimate goal of installing the Prostar's at all
the HRSN stations as time and funding permit.
We found that a significant source of artificial noise was coming from the station
pre-amplifiers. In the upgraded system, preamps from the older
network were used. During integration
of the older preamps with the increased dynamic range capabilities of
the 24-bit Quanterra system, gain settings of the preamps were reduced
from x10,000 to x80 in order to match signal sensitivity of the new system with
the older one. While these lower preamp gain levels are still within
the operational design of the preamps, they are no longer in
their optimal range and a significant contribution of
preamp's self-generated noise is present in the recorded seismograms.
Initially, this was not expected to be a significant problem.
However, we have subsequently found that even the small increase
in preamp noise that results from the preamp gain reduction
significantly impacts the sensitivity of the network for detecting
and recording the smallest locatable events.
Figure 5.4 shows the preamp noise reduction effect
observed on background noise signals at three vertical components
of the HRSN when gains are raised from x80 to x1,000.
Considerable
signal hash is seen at gain levels of x80 (top waveform in each station pair),
and significantly reduced when gains are increased to x1,000 (lower
waveforms). Since we are also interested in recording large earthquakes on-scale,
simply increasing gain levels on all stations is
not the preferred solution, since doing so causes the recording system to saturate
at much lower magnitudes. Instead we are attempting to redesign the preamps using modern components
to reduce the noise levels at the lower gain levels. However our attempts at redesign
have not yet yielded satisfactory results.
Since a primary objective of the HRSN is to monitor the evolving patterns of the numerous small earthquakes that occur
at very low magnitudes, and since this objective also complements the scientific objectives
of the recently funded SAFOD experiment, it is important to address the
preamp noise problem in a timely manner. We have opted, therefore, to raise the gain levels for the near-term
on all
the station preamps from x80 to x1,000. These gain changes are
currently (late August, 2003) being implemented, and we estimate that
the number of small earthquakes we will detect will increase by
a factor of 2 to 3. We will continue investigating preamp redesigns until a suitable
alternative is found at which time we will install the new preamps and lower the preamp gain
back to x80-allowing both the increased detection of small events and the on-scale recording
of events up to about magnitude 4 to 4.5.
Figure 5.4:
Preamp noise reduction test. Shown are 30 seconds of vertical
background signal recorded at stations EADB, FROB and JCNB on day 229
of 2003 at 0700 UTC (top of station pairs, recorded at x80 gain and
scaled up by 1000/80 for comparison to the x1000 preamp gain levels)
and 0700 UTC on day 233 (bottom of station pairs, recorded at x1000
preamp gain). Note the substantial reduction in background noise, due
primarily to the lower preamp generated noise at higher preamp gain.
 |
Additional efforts underway to increase event detection
sensitivity include: 1) development of a station specific filtering
scheme for input into the triggering algorithm, 2) refinement of the multi-station
trigger association algorithm to include subnet triggering, and
3) incorporation of the pilot
hole array data into the network triggering scheme to capture the
smallest events in the SAFOD drilling area.
Monitoring the evolution of microseismicity, particularly
in the SAFOD drilling and target zone, is a primary objective of the HRSN project.
In addition, the continued analysis of the HRSN data for determining detailed seismic
structure, for the study of similar and characteristic microearthquake systematics, for
estimation of deep fault slip
rate evolution, and for various studies of fault zone and earthquake
physics is also of great interest to seismologists. Before advanced
studies of the Parkfield microseismicity can take place, however,
initial processing, analysis and routine cataloging of the earthquake
data must be done. An integral part of this process is quality control
of the processed data, including a final check of the routine catalog
results.
At this time, continuous data streams on all 39 components are being recorded
at 20 and 250 sps on disk on the local HRSN computer at the CDF facility and when
the local disk space is full, the continuous data is migrated onto
DLT tape. The 20 sps data are transmitted continuously to the BSL over
the frame-relay linked and archived at the NCEDC. In addition, the vertical
component channels for the 7 stations critical to resolving seismicity
in the SAFOD area are also being transmitted continuously to the BSL
at 250 sps
over the frame relay-circuit for purposes of quality control and fine tuning the triggering
algorithm for the detection of the smallest possible events around SAFOD.
Shortly after being recorded to disk, event triggers for the individual station
data are determined and a multi-station trigger association routine then processes the station
triggers and identifies potential earthquakes. For each potential earthquake trigger, 30 second
waveform segments are then collected for all stations and components, assigned a unique
event identifier (compatible with the NCEDC classification scheme) and saved as an event
gather. Event gathers are then periodically telemetered to BSL and included directly
into the NCEDC earthquake database (dbms) for analysis and processing.
An ongoing effort has been the development of a new earthquake triggering
scheme, with the goal of routinely detecting SAFOD area events to magnitudes
below -1.0. A first cut version of the new scheme has been
implemented and is already detecting earthquakes at an increased
rate-nearly 3 times the number of earthquakes detected before the
upgrade.
In order to facilitate the processing and archiving of this large number of events
(approx. 150 per month), BSL personnel have recently developed
a Graphical User Interface (GUI). The GUI
is integrated with the NCEDC dbms and allows review of the waveforms from
every triggered event. Initial analysis of the data using the GUI involves
review of the waveforms and classification of the event as an earthquake
or non-earthquake event. The GUI also allows the analyst to log
potential network problems that become apparent from the seismograms.
The HRSN analyst then classifies the event as a local, distant-local,
regional, or teleseismic event and then systematically hand picks the
P- and S-phases for the local and distant local events.
Picking of the numerous microearthquake events is no mean task. On
average about 7 P-phases and 4 S-phases are picked for each event, putting
the total number of annual phase picks for the HRSN data on the order of 19,000
to 20,000.
We have experimented with algorithms that make initial auto-picks of
the phase arrivals, but have so far found picking by hand to be an
advantage since it forces the analyst to review each pick carefully
while at the same time allowing him to assess the state of health of
recording on each station-component in detail. In all our tests, repicked
autopicks have also invariably resulted in catalog locations that are significantly
more scattered and that have higher residuals than locations done with purely
hand-picked data.
A peculiarity of processing very small earthquake data, is that multiple events
commonly occur within a few seconds of one another (Figure 5.5).
The close timing of these events does not allow the local triggering algorithm
to recover from one event before another occurs. As a result, the central site
processor often does not trigger uniquely for each event. In such cases only one,
30 sec waveform gather and one earthquake identifier will be created for all the
events. These multiple earthquake records (MER) account for only 3 to 5
of the total
seismicity recorded by the HRSN. However, there are times when this rate rises
to over 10
. In order to assign each event in an MER a unique event identifier
for the NCEDC dbms and to make picking and automated processing of these events more manageable
an additional feature of the GUI was developed that allows the analyst to "clone"
MER into separate gathers for each event.
Figure 5.5:
Five events occurring on the same MER. The P phase of the first event
was not captured on this record. These five events occurred as part of
a swarm of 47 small events recorded by the HRSN that occurred on day
211 of 2003. Of these 47 events, the NCSN catalog contains only 2.
Events shown are all less than magnitude 0.
 |
Once false triggers have been removed and picks for the events completed,
quality control on the picks is made to ensure that all picks have
phase and weights assigned, that extraneous characters have been removed
from the pick files, that double station-phase picks have not inadvertently
been made, and that no repicks of the same event had been accidentally
made during any cloning that was performed.
Initial locations are then performed and phase residuals analyzed in order
to determine whether severe pick outliers must be removed or adjusted.
Unstable location solutions based on events with few picks are also assessed
to see if the addition of marginal phases will improve the stability of the
location determination.
After any required pick adjustments have been made, the events are then
relocated, and combined with error information to allow ranking of the
confidence of location quality.
These procedures have all been put in place and tested over the past
year for the new HRSN configuration. Currently we have located 9 months
of data recorded by the new HRSN (over 1300 events) and are staying current with ongoing
seismicity and also moving backwards in time to pick and locate the
earlier data collected since early 2001.
We now have enough data and are confident enough with the procedures
to begin organizing the locations for formal inclusion into the NCEDC dbms
and dissemination to the community. These efforts are now underway. We
are also in the early stages of establishing a scalar seismic moment catalog for
the new HRSN events that is also to be included in the NCEDC dbms.
We continue to examine the ongoing earthquake data being
collected by the HRSN in search of possible earthquake precursors.
This includes quality control and evaluation of the routine earthquake
catalog locations and analyses of the spatial and temporal distribution
of the microseismicity in relation to the occurrence of larger
earthquakes in the area and heightened alert levels declared as part of
the Parkfield Prediction Experiment. Even before our planned
enhancement of HRSN performance, the new central detection system that
operates at the telemetry hub, along with real-time telemetry of
selected high-sensitivity channels to Berkeley for monitoring, allows
event detection below magnitude 0.0. As a result, the rate of
earthquake detection by the HRSN exceeds that of the NCSN by about a
factor of 3 in the 30 km stretch of the SAF centered at the location of
the 1966 M6 Parkfield event (Figure 5.6). The additional
rate of HRSN event detection significantly increases both the spatial
and temporal coverage of the changing seismicity patterns and provide
unique additional information on the earthquake pathology at very low
magnitudes. With our planned noise reduction and triggering
enhancement, we estimate the proportion of HRSN located events
relative to the NCSN catalog to increase by an additional factor of 2.
Differences between earthquake locations evident in Figure 5.6 are
largely attributable to the more advanced 3-D P- and S- wave velocity
model used in determining the HRSN locations and the more accurate
hand-picked P- and S- phases made possible by the high sampling rate
(250 sps) and horizontal component borehole recordings of the HRSN.
Figure 5.6:
Comparison of NCSN and HRSN catalog locations for the period
September through November of 2002. During this period, magnitude M3.8 and M4.2
earthquakes occurred at about
and
km NW, respectively (gray
disks). The proposed SAFOD drilling target is shown as an asterisks
and a 4x4 km gray box of 6km depth is shown surrounding the target (corresponding
to the 4x4 km box in Figure 5.1).
The region shown is centered on the hypocentral region of the 1966
Parkfield M6 earthquake that occurred at 0 km at about 9 km depth. The
lower magnitude detection and greater rate of microearthquake detection
by the HRSN provides increased spatial coverage and detail in the
temporal pattern of the evolution of seismic activity in the region.
Station coverage in the region is comparable for both networks, yet the
more accurate S- phase picks possible on the horizontal HRSN component seismograms
and the use of a 3-D P and S velocity model for hypocentral inversion
provides a sharper picture of the fault zone structure. On average the
current detection rate of locatable earthquakes by the HRSN is about 3
times that of the NCSN. Planned enhancements for the HRSN are
expected to increase rate of locatable earthquakes by an additional
factor of 2 to 3.
 |
Thomas V. McEvilly, who passed away in February 2002,
was the PI on the
HRSN project for many years, and without his dedication and hard
work the creation and continued operation of the HRSN would not have
been possible. His contributions continue to be appreciated in the
extreme and the fruits of his labor many-fold.
Under Bob Nadeau's
and Doug Dreger's general supervision, Rich Clymer, Wade Johnson,
Bob Uhrhammer, Doug Neuhauser, Don Lippert, Bill Karavas, John Friday,
Pete Lombard, and Lane Johnson all contribute to the operation of the HRSN.
Bob Nadeau prepared this chapter with the assistance of Bob Uhrhammer and
Wade Johnson.
During the period of this report, the operation and maintenance of the
HRSN and the processing and archiving of its
data was supported in large part by
the USGS, through the NEHRP External Grants Program
(grants: 02HQGR0067 and 03HQGR0065). NSF also provided
support for the expansion of the HRSN near the SAFOD drill site
through grant EAR-9814605.
Bakun, W. H., and A. G. Lindh, The Parkfield, California,
prediction experiment, Earthq. Predict. Res., 3, 285-304, 1985.
Daley, T.M. and T.V. McEvilly, Shear wave anisotropy in the Parkfield Varian Well
VSP, Bull. Seism. Soc. Am., 80, 857-869, 1990.
Karageorgi, E., R. Clymer and T.V. McEvilly, Seismological studies at
Parkfield. IV: Variations in controlled-source waveform parameters
and their correlation with seismic activity, 1987-1994, Bull.
Seismol. Soc. Am., 87, 39-49, 1997.
Michelini, A. and T.V. McEvilly, Seismological studies at Parkfield: I.
Simultaneous inversion for velocity structure and hypocenters using B-splines parameterization,
Bull. Seismol. Soc. Am., 81, 524-552, 1991.
Berkeley Seismological Laboratory
215 McCone Hall, UC Berkeley, Berkeley, CA 94720-4760
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