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Parkfield Borehole Network
As part of the U.S. Geological Survey initiative known as the
Parkfield Prediction Experiment (Bakun and Lindh, 1985), the operation of the
High Resolution Seismic Network (HRSN) at Parkfield, California,
and the collection and analysis of its recordings began in 1987.
Figure 4.1 shows the location of the network and
its relationship to the San Andreas fault.
The HRSN records exceptionally high-quality data, owing to its
10 closely spaced three-component borehole sensors, its very
broad band recordings (0-125 Hz), and its sensitivity (recording
events below magnitude -0.5) due to the extremely low attenuation
and background noise levels at the 200-300 m sensor depths
(Karageorgi et al., 1992). Several aspects of the Parkfield
region make it ideal for the study of small earthquakes and their
relation to tectonic processes. These include the fact that the
network spans the expected nucleation region of a repeating
magnitude 6 event and the transition from locked to creeping
behavior on the San Andreas fault, the availability of
three-dimensional P and S velocity models, a very complete
seismicity catalogue, a well-defined and simple fault segment, and a
homogeneous mode of seismic energy release as indicated by the
earthquake source mechanisms (over 90
right-lateral strike-slip).
In a series of journal articles and Ph. D. theses, we have
presented the cumulative, often unexpected, results of this
effort. 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. Recent results are described
in Chapter III.
Figure 4.1:
Map showing the location of the Parkfield HRSN stations (filled
diamonds) and the 3 planned sites (open diamonds), along with the BDSN
stations PKD and PKD1 (filled squares). The location of the proposed
SAFOD drill site is shown by a star.
 |
Table 4.1:
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 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 planned sites are approximate.
| Site |
Net |
Latitude |
Longitude |
Elev (m) |
Depth (m) |
Date |
Location |
| EAD |
BP |
35.89525 |
-120.42286 |
499 |
254 |
01/1988 - |
Eade Ranch |
| FRO |
BP |
35.91078 |
-120.48722 |
542 |
258 |
01/1988 - |
Froelich Ranch |
| GHI |
BP |
35.83236 |
-120.34774 |
433 |
370 |
01/1988 - |
Gold Hill |
| JCN |
BP |
35.93911 |
-120.43083 |
559 |
335 |
01/1988 - |
Joaquin Canyon North |
| JCS |
BP |
35.92120 |
-120.43408 |
487 |
332 |
01/1988 - |
Joaquin Canyon South |
| MMN |
BP |
35.95654 |
-120.49586 |
731 |
510 |
01/1988 - |
Middle Mountain |
| RMN |
BP |
36.00086 |
-120.47772 |
1198 |
1125 |
01/1988 - |
Gastro Peak |
| SMN |
BP |
35.97292 |
-120.58009 |
732 |
450 |
01/1988 - |
Stockdale Mountain |
| VAR |
BP |
35.92614 |
-120.44707 |
511 |
-61 |
01/1988 - |
Varian Well |
| VCA |
BP |
35.92177 |
-120.53424 |
790 |
590 |
01/1988 - |
Vineyard Canyon |
| CCR |
BP |
35.957 |
-120.544 |
|
|
Planned |
Cholame Creek |
| LCC |
BP |
35.977 |
-120.507 |
|
|
Planned |
Little Cholame Creek |
| SCY |
BP |
36.016 |
-120.538 |
|
|
Planned |
Stone Canyon |
|
Table 4.2:
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 in Dec 1998, 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 new
Quanterra-based systems will be installed in the fall of 2000.
| Site |
Sensor |
Z |
H1 |
H2 |
RefTek 24 |
RefTek 72-06 |
|
|
|
|
|
| EAD |
Mark Products L22 |
-90 |
170 |
260 |
01/1998 - 12/1998 |
12/1998 - 07/1999 |
|
|
|
|
|
| FRO |
Mark Products L22 |
-90 |
338 |
248 |
01/1998 - 12/1998 |
12/1998 - 07/1999 |
|
|
|
|
|
| GHI |
Mark Products L22 |
90 |
failed |
unk |
01/1998 - 12/1998 |
12/1998 - 07/1999 |
|
|
|
|
|
| JCN |
Mark Products L22 |
-90 |
0 |
270 |
01/1998 - 12/1998 |
12/1998 - |
|
|
|
|
|
| JCS |
Geospace HS1 |
90 |
300 |
210 |
01/1998 - 12/1998 |
12/1998 - 07/1999 |
|
|
|
|
|
| MMN |
Mark Products L22 |
-90 |
175 |
265 |
01/1998 - 12/1998 |
12/1998 - |
|
|
|
|
|
| RMN |
Mark Products L22 |
-90 |
310 |
40 |
01/1998 - 12/1998 |
12/1998 - 07/1999 |
|
|
|
|
|
| SMN |
Mark Products L22 |
-90 |
120 |
210 |
01/1998 - 12/1998 |
12/1998 - |
|
|
|
|
|
| VAR |
Litton 1023 |
90 |
15 |
285 |
01/1998 - 12/1998 |
12/1998 - 07/1999 |
|
|
|
|
|
| VCA |
Mark Products L22 |
-90 |
200 |
290 |
01/1998 - 12/1998 |
12/1998 - |
|
|
|
|
|
|
The HRSN was installed in boreholes beginning in 1986. 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. During 1988, the network was completed to ten 3-component
500 sps radio-telemetered stations into a central
detection/recording system, 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. In 1991, low-gain event recorders (from PASSCAL)
were installed to extend the dynamic range to ML about 4.5. The
data acquisition system operated quite reliably until late 1996,
when periods of unacceptably high downtime developed, with as many as
7 of the remote, solar-powered telemetered stations down due to
marginal solar generation capacity and old batteries, and
recording system outages of a week or more became common. In 1998
it failed permanently. The original acquisition system that failed
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 (discontinued in 1997) data. The
system was remote and completely autonomous - tapes were mailed to
Berkeley. The old system had one-sample timing uncertainty, and record
length limitation because the tape write after event detection was
longer than the length of the record, and we were off-line for the write
time.
Table 4.3:
Typical data streams acquired at each HRSN site,
with channel name, sampling rate, and sampling mode. C
indicates continuous; T triggered.
| Sensor |
Channel |
Rate (sps) |
Mode |
| Geophone |
DP |
500.0 |
T |
|
In fall 1998, the original HRSN acquisition system was replaced
by 10 PASSCAL RefTek systems with continuous recording. This
required the development of a major data handling procedure,
in order to capture microearthquakes as small as M = -1.0 are
not seen on surface stations, since continuous telemetry to
the BSL 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 the archive of
characteristic events and temporal variations in recurrence.
Thanks to emergency funding from the USGS NEHRP, we are replacing
the original 10-station system with a modern 24-bit acquisition system
(Quanterra 730 digitizers, spread-spectrum telemetry, Sun Ultra 10/440 central
processor at the in-field collection point, with frame relay, ultimately
T1, connectivity to Berkeley). The new system should be online late in
2000, assuming we can find a suitable new central site given the USGS
lease problems at the old Haliburton facility.
The upgraded system will be compatible with the data flow and archiving common to
all the elements of the BDSN/HFN and the NCEDC.
This will provide remote access and control of the system and produce
data with better timing accuracy and longer records flowing seamlessly
into NCEDC. The new system solves the problems of timing resolution, dynamic range,
and missed detections, in addition to the advantage in the conventional
data flow (the old system recorded SEG-Y format).
We are adding three new borehole stations at the NW end of the
network as part of the deep fault-zone drilling (San Andreas Fault
Observatory at Depth - SAFOD)
project, with NSF support, to improve resolution of at the planned
drilling target on the fault. Figure 4.1 illustrates
the location of the proposed drill site (star) and the new borehole sites.
These three new stations will
use similar hardware to the main network, with the possible addition
of extra channels for electrical, pore-pressure and strain signals.
In addition, the remoteness of the drillsite and new stations will
require a telemetry collection point and wideband transmission from
the RMN site. We are trying to combine this link with the data
flowing from the temporary 15-station surface array being deployed
around the drillsite. The new borehole installations are also
planned for the fall of 2000.
More information about SAFOD project is available on the Web
at http://www.earthscope.org/safod.com.html.
Under Tom McEvilly's general supervision, Rich Clymer, Bob Nadeau,
Wade Johnson, and Doug Neuhauser contribute to the
operation of the HRSN. Tom McEvilly and
Lind Gee contributed to the preparation of this chapter.
Bakun, W. H., and A. G. Lindh, The Parkfield, California,
prediction experiment, Earthq. Predict. Res., 3, 285-304, 1985.
Karageorgi, E., R. Clymer and T.V. McEvilly, Seismological
studies at Parkfield. II. Search for temporal variations
in wave propagation using Vibroseis,
Bull. Seism. Soc. Am., 82, 1388-1415, 1992.
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