california institute of technologyture (hudson, 1977; hudson, 1979). in addition, the figure shows...
TRANSCRIPT
CALIFORNIA INSTITUTE OF TECHNOLOGY
EARTHQUAKE ENGINEERING RESEARCH LABORATORY
STRONG-MOTION EARTHQUAKE MEASUREMENT
USING A DIGITAL ACCELEROGRAPH
BY
WILFRED D. IWAN, MICHAEL A. MOSER
AND CHIA-YEN PENG
REPORT No. EERL 84-02
A Report on Research Conducted Undr aGrant from the National Science Foundation
PASADENA, CALIFORNIA
APRIL 1984
Strong-Motion Earthquake Measurement Usinga Digital Accelerograph
By Wilfred D. Iwan, Michael A. Moser, and Chia-Yen Peng
ABSTRACT
This paper presents results of a study of some of the characteristics of the
Kinemetrics PDR-1 digital strong-motion accelerograph. The paper gives the results of
laboratory tests of the background noise level of the instrument and compares these
results with previously reported observations for optical instruments. The determina-
tion of displacement from acceleration data is discussed and results of laboratory tests
are presented. Certain instrument anomalies are identified, data correction algorithms
proposed, and examples given. The paper also presents the results of a comparison of
earthquake records obtained from side-by-side digital and optical analog instruments.
Finally, some results obtained from a recent Chinese earthquake are discussed.
INTRODUCTION
The development of reliable, digital strong-motion accelerographs is having a very
significant impact on the measurement of strong ground motion. After analog amplifi-
cation, and conversion to digital format, the digital instruments record the data on
magnetic tape or a core memory in a computer-readable form, thus bypassing many of
the steps of the analog-to-digital conversion process associated with optical analog
accelerographs. Timing is generally quite accurate in these digital recorders, being of
the order of one part in 107. In addition, digital instruments commonly have a pre-
event memory so that the entire history of the motion is recorded along with the initial
state of the instrument. The resolution of the digital instruments is typically 66 dB (with
12 bits of digital data), and the dynamic range is increased by 36 dB through the use of
an autoranging analog amplifier.
Because of their inherent advantages, the use of digital instruments should become
very widespread throughout the world in the years to come. However, since these
instruments have only recently been put into service, their characteristics are not well
known. The purpose of this paper is to present results of a study of the recording char
acteristics of a typical strong-motion recorder / transducer instrument. The background
noise level of the recorded data is compared with that of optical recorders. Integration
of the recorded acceleration time history to obtain displacement is discussed and the
results of laboratory tests presented. Certain instrument anomalies are identified and
correction algorithms are proposed. Also presented is a comparison of side-by-side
recorded results obtained from analog and digital instruments.
NOISE LEVEL OF DIGITAL INSTRUMENT
Considerable laboratory and field experience has been gained with optical strong-
motion recorders. The limitations of these instruments are fairly well understood and
substantial effort has been expended to maximize the data return from such instru
ments using various filtering and correction algorithms (Hudson, 1979). Noise is intro
duced into the optical recording from a number of sources including transducer drift,
recording medium lateral drift and speed variation, trace density variations and the
digitization process. This noise limits the range of ground motion for which useful data
can be obtained. Generally speaking, the optical instruments will have difficulty pro-
-2-
viding useful data for earthquakes of M=4 or smaller even in the epicentral region and
for earthquakes of magnitude M=6.5 if further than 200 km from the source.
Digital instruments have inherent advantages so far is noise is concerned. Noise
associated with media drift, transport speed variation and trace density variation are
essentially eliminated with the digital format. Furthermore, digitization error is greatly
reduced by eliminating the intermediate step of optical recording.
In order to obtain quantitative data on the background noise of a typical digital
strong-motion recorder, a Kinemetrics PDR-1/FBA-13 instrument was tested. The
PDR-1 is a gain ranging recorder with 12 bit resolution and a 102 dB dynamic range.
The FBA-13 is a three-component force balance accelerometer unit. The accelerometers
nominally have a 50 Hz natural frequency and 70<Yo damping and are capable of dc
measurement. The transducers tested (Ser. Nos. 16345 and 16347) had a range of ±2g.
The FBA-13 transducer was mounted on an air suspension optical table in a quiet
laboratory environment. Samples of background noise with a duration of 20 seconds
were recorded using the PDR-l "run" mode, and subsequently processed to obtain the
time history of the noise and the pseudo-velocity response spectrum. Care was taken in
balancing the transducer so that maximum system gain was obtained. No data was
obtained at lower gains. The input low-pass filters of the recorder were set at their
maximum value of 50 Hz and the sample rate was 200 sps. No correction was intro
duced into the processing except for a uniform baseline shift to eliminate the dc compo
nent of the accelerogram.
-3-
Figure 1 shows the time history of the background noise acceleration for four differ
ent test runs. It is seen that the noise is generally associated with fluctuations in the last
bit of the digital data. Some low frequency drift is evident. Figure 2 shows the Fourier
Amplitude Spectrum of one of the noise time histories of Figure 1. This spectrum was
obtained using a Kaiser-Bessel filtered version of the data. The result shown is typical.
Figure 3 shows the superimposed zero-damped response spectra for the four differ
ent test runs. Also shown in Figure 3 is the band of average digitization noise plus one
standard deviation for a typical hand digitized optical record as reported in the litera
ture (Hudson, 1977; Hudson, 1979). In addition, the figure shows the 20% damped
average digitization noise spectrum which is claimed for the automatic digitization
system employed by the California Division of Mines and Geology.
It is seen from Figure 3 that there is a very striking difference in noise level between
the analog and digital systems. The difference varies from more than one order of
magnitude at short periods (high frequency) to about two orders of magnitude at long
periods (low frequency). It is clear from the figure that the digital instrument is capable
of accurately measuring the acceleration from much smaller events than the analog
instrument. It is also clear that the digital instrument should give superior results for
integrals of the acceleration; i.e., velocity and displacement. The digitization noise in
the displacement at a period of ten seconds is of the order of two inches for the optical
instrument but is closer to 0.02 inches for the digital instrument. It would therefore be
anticipated that the digital instrument could be used to extract significantly more
-4-
information about displacement than the analog instrument. This possibility is exam
ined in the next section.
COMPUTATION OF DISPLACEMENT FROM ACCELERATION
In principle, velocity and displacement time histories could be obtained directly
from an acceleration time history by numerical integration. However, for optically
recorded data, this usually results in errors which are unacceptably large. This is due to
the fact that digitization and other errors associated with optical recording increase
with period and therefore become amplified when the time history is integrated. In
addition, an initial portion of the acceleration time history is lost in the analog instru
ment due to the finite time required to trigger this instrument. The digital instrument
has a much lower inherent digitization noise. Furthermore, the pre-event memory
incorporated into most instruments eliminates the ambiguity in the initial conditions of
the record.
In order to examine the nature of the errors associated with integration of accelera
tion time histories obtained from digital instruments, a series of laboratory tests were
conducted using the PDR-l/FBA-13 instrument. The transducer was moved horizon
tally in a straight line on a very flat, level surface through a known displacement. The
recorder was triggered from the output of the accelerometer oriented in the direction of
motion. The acceleration data was then integrated to obtain the time history of velocity
and displacement. A typical result for a test with a relatively smooth displacement is
shown in Figure 4.
-5-
For the test results shown in Figure 4, the actual permanent displacement of the
transducer as 10±0.1 inches (25.4±0.3 em). It is seen that the integrated acceleration
time history gives an accurate measure of this permanent displacement. The only cor
rection applied to the data was to adjust the zero offset of the accelerogram by the
average value of the pre-event data (the first 1.0 seconds of the record were used for this
average) and apply an instrument correction to remove transducer distortion. The
input low-pass filter of the PDR-l was set at 50 Hz and the sample rate was 200 sps.
The PDR-l does not have a high-pass filter, so the dc output from the accelerometers is
retained. This is a necessary feature of the instrument if permanent displacement
information is desired.
It would not be possible to generate a displacement time history like that shown in
Figure 4 from an optical recording instrument due to absence of pre-event data and the
presence of sibrnificant long-period noise. In an attempt to minimize the effect of these
factors, optically recorded data is typically subjected to a number of corrections. These
include baseline corrections and low- and high-pass filtering. In order to obtain a better
understanding of the effect of these corrections, the acceleration time history of Figure 4
was processed using the standard correction algorithms employed in the report series
entitled "Corrected Accelerograms" published by the California Institute of Technology
(Trifunac and Lee, 1973). The results are shown in Figure 5. It is seen that the effect of
the correction algorithm is to "level out" the displacement time history thus eliminating
any permanent displacement and simultaneously reducing the magnitude of the
dynamic displacement.
-6-
ANOMALIES IN THE DIGITAL INSTRUMENT
Unfortunately, the excellent results of double integration of the acceleration indi-
cated in Figure 4 are not altogether typical. Rather extensive laboratory testing and
field use of the FBA-13 transducer has revealed an anomaly which has a significant
effect on data analysis. Figure 6 shows the result of direct numerical integration of a
permanent displacement test in which the transducer was moved with a rather rough
motion having associated high acceleration peaks. In this case, a very noticeable drift is
observed in the displacement time history which completely overshadows the actual
test permanent displacement which was again 25.4 cm.
Through further testing, it was determined that the baseline output of the FBA-13
could be observed to shift suddenly if a sufficiently large input acceleration pulse were
applied. This shift may be associated with minute slippage in the flexure support of the
transducer, or hysteretic behavior of the fine wires which attach to the moving trans
ducer element. The phenomenon is not fully understood and is currently under further
investigation by the manufacturer. However, the anomaly has a very strong effect on
the acceleration data when it is double integrated.
An attempt has been made to develop a correction algorithm which can compensate
for the observed anomaly without having an adverse effect on the ability of the instru
ment to predict permanent displacement. The proposed correction algorithm is quite
simple and based on the perceived mechanism of the anomaly. The acceleration data is
first corrected for the dc offset observed in the pre-event data. Typically, this is
accomplished by performing a time average on only the first one-half of the pre-event
-7-
data in order to eliminate the possibility of including any actual earthquake data. Next,
the final offset of the acceleration is determined. If there were no instrument anomaly,
this offset should now be zero since the pre-event and final offsets should be equal.
However, due to slippage or other effects, these offsets will not, in general, be the same.
If the dynamic or oscillatory component of the acceleration at the end of the record is
smaller than the final offset of the record, as in Figure 4, the acceleration record may be
used directly to determine the final offset. However, it has been found that it is usually
more accurate to estimate the final acceleration offset from the final slope of the velocity
record since it has a relatively smaller oscillatory component. Normally, the last 15
seconds of the time history are adequate to determine the acceleration offset.
Finally, the cumulative effect of the transducer anomaly during the time of strong
shaking is estimated from the offset in the final velocity. This is accomplished by
assuming that the intermediate baseline shifts can, on the average, be replaced by a rec
tangular acceleration pulse which occurs during the strongest portion of the
acceleration time history. The overall correction for the instrument anomaly is shown
schematically in Figure 7.
The time t1 and tz may be selected in a number of different ways and it has been
observed that the final results are generally fairly insensitive to this selection. Experi
ments have shown that very little base line offset of the transducer occurs for
accelerations less than 50 cm/secz. Therefore, one possible approach is to select tl and
tz such that a(t) is less than or equal to 50 cm/ sec2 for all t on the interval (tl' t2)' This
approach (Option One) works well when there is known to be a real final net displace-
-8-
ment. Another approach would be to select tl as the time of the first significant accel-
eration pulse and then select t2 so as to minimize the computed final displacement. This
approach (Option Two) is useful when the existence of a final displacement is not
known a priori. If there is a real final displacement, Option Two will usually yield a
value of t2 which is less than tI, signifying that Option One is more reasonable.
The correction for the final offset is normally determined by a least-squares fit of the
final portion of the velocity data of the form
The intermediate range correction is determined from the relation
The result of applying the correction algorithm to the acceleration time history of
Figure 6 is shown in Figure 8. Option One was used in the selection of t l and t2' The
corrected displacement results show good agreement with the actual permanent dis-
placement of 25.4 em. Very little low frequency (long period) information seems to
have been lost from the data by the correction algorithm. Indeed, this was one of the
goals in the development of the algorithm.
Additional examples of the results of prescribed displacement tests using the pro-
posed correction algorithm are given in Figures 9-12. The FHA transducer was initially
adjacent to a ruler and the recorder set in the "triggered" mode. The transducer was
then moved slightly away from the ruler and translated parallel to the ruler. Finally,
when the desired displacement was reached, the transducer was moved back against
-9-
the ruler. The test displacement in each case was 25.4±0.3 em. No special fixtures were
used to maintain a fixed orientation of the transducer while it was translated. Hence,
angular rotation of the transducer may account for some of the differences between the
actual and computed displacement. However, it is more likely that the single correction
algorithm used is not adequate when large amounts of transducer baseline shift take
place over a long duration.
Figure 9 shows the corrected version of the test shown in Figure 4. Figure 10 shows
a similar test with a fairly smooth displacement. Figure 11 shows a test in which the
motion was caused by a series of discrete impacts to the transducer. This test clearly
illustrates both the nature of the hypothesized instrument anomaly and the limitations
of the proposed simple correction algorithm. From the velocity time history, it is evi
dent that there is a different transducer offset associated with each impulse. Averaging
the effect of these individual shifts over the approximately 10 seconds of strong accel
eration to obtain a single effective shift am as prescribed by Option One is not adequate
for such a case. When the acceleration pulses are distinct, as in Figure II, it is possible
to apply an offset correction to each individual pulse in a manner analogous to that
used in the simple correction. Figure 12 shows the results of using such an approach on
the data of the test shown in Figure 11. The improvement in the computed time histo
ries of the velocity and displacement is apparent.
Table 1 gives a summary of the values of the correction parameters and the final
displacements obtained from double integration of the acceleration for the tests pre
sented in Figures 8-12. It is seen that the numerical values of the corrections af and am
-10-
are generally quite small. The displacement results have been observed to be fairly
insensitive to the selection of the threshold acceleration level which defines tl and t2'
It is believed that the simplified correction algorithms will be adequate for most
short-duration earthquake-like time histories of motion. In that case, the time duration
over which the central correction is applied will generally be smaller than for the high
level acceleration tests presented herein and the permanent ground displacement will
also take place over a shorter time interval. This will be illustrated by examples which
follow.
It should be emphasized that the suggested correction algorithm has been intro
duced only to eliminate an observed anomaly in the instrument. It is anticipated that
the source of this anomalous behavior will soon be eliminated so that correction of the
digital accelerogram will no longer be necessary.
COMPARISON OF ANALOG AND DIGITAL RECORDS
Following the Coalinga earthquake of May 2/ 1983/ a SMA-1 optical analog record-
ing accelerograph and a PDR-1/FBA-13 digital accelerograph were installed side-by
side in a residential garage near the center of the city to measure aftershocks. On
May 8/ 1983/ an aftershock of ML=5.5 with an epicenter approximately 11 km to the
north of the city was recorded simultaneously by both instruments. The results
obtained represent a unique opportunity for a direct comparison between the optical
analog and digital recording instruments.
The time histories of the ground acceleration, velocity and displacement for the digi
tal instrument are shown in Figures 13-15. The time histories shown were corrected
-11-
using the algorithm described herein with tl and t2 selected according to Option Two.
The sampling rate was 100 sps.
The time histories obtained from the analog instrument are presented in Figures 16
18. These results were obtained from accelerograms which were digitized and cor
rected by the California Division of Mines and Geology. This data was band-pass
filtered with a low frequency cut-off of 0.2-0.4 Hz and a high frequency cut-off of 23-25
Hz. The maximum acceleration, velocity and displacement obtained from the two dif
ferent instruments are compared in Table II.
In general, there is rather close agreement between the results obtained from the
analog and digital instruments. The greatest difference is, as expected, observed in the
displacement. The results obtained from the digital instrument show the presence of a
low frequency pulse with a duration of about 7 seconds while this pulse is filtered out
of the results from the optical analog instrument. The potential of the digital instru
ment to provide long period displacement information is clearly indicated.
In order to obtain a more complete understanding of the difference between the
analog and digital records, a correlation analysis was performed. The cross-correlation
coefficient between each pair of records was computed and the time difference for
maximum correlation determined. The analog record was shifted by this time differ
ence and then subtracted from the digital record to obtain the time difference accelera
tion. The results are shown in Figures 19-21.
The difference acceleration shown in Figures 19-21 is somewhat larger than might
have been anticipated from the relatively high correlation of the analog and digital
-12-
records. The most satisfactory explanation for this seems to be that there is a slowly
varying phase shift with time between the two records. Whether this is associated with
speed variations in the analog instrument, the digitization process or the instrument
correction is uncertain.
In Table 3 the maximum correlation time difference for each pair of records is com
pared to the time difference between the largest acceleration peak of the records. In
general, there is fairly close agreement between the two measures of time difference.
This agreement holds as well for the difference between the largest velocity peak but
not for the peak displacement.
The Fourier Amplitude Spectra of the digital, analog and difference acceleration
time histories are shown in Figure 22-24. It is noteworthy that the Fourier Amplitude
Spectrum associated with the difference acceleration is generally significantly larger
than the difference between the Fourier Amplitude spectra of the digital and analog
time histories. This is another indication of the presence of phase differences in the
records that are not accounted for by a time shift corresponding to the maximum corre
lation time. Although not shown herein, a significant phase variation was also
observed in the cross-spectrum of the digital and analog records even after the records
were shifted.
The zero-damped response spectra for the three components of this aftershock are
shown in Figures 25-27. The solid lines denote the spectra obtained from the digital
instrument and the dashed lines denote the spectra obtained from the analog instru
ment. Two spectra are shown for each analog record. The higher response spectrum
-13-
values were obtained using corrected accelerograms which were high-pass filtered with
a corner frequency of 0.07 Hz (14.3 sec period). The lower values were obtained using
the accelerograms filtered with a corner frequency of 0.4 Hz (2.5 sec period) which are
reproduced in Figures 16-18. It is understood that the corner frequency of 0.4 Hz was
selected by the California Division of Mines and Geology to correspond approximately
to the intersection of the 20% damped earthquake response spectrum and the nominal
noise response spectrum (see Figure 3). There is very close agreement between the
optical and digital response spectra for periods less than one second. However, there
are some very significant differences in the range of periods greater than one second.
The difference can be as large as an order of magnitude depending on the filtering used
and the period considered. In this particular case, the optical instrument results are
conservative compared to those of the digital instrument but this cannot be assured in
general.
The spectral differences observed are believed to be caused by the presence of low
frequency noise in the analog records which is not eliminated by the baseline and filter
ing corrections applied to this data. This conclusion is supported by the background
noise level results presented in Figure 3. The absence of pre-event data along cannot
account for the observed differences. The fact that the accelerograms filtered at 0.4 Hz
have nearly the correct displacement asymptote appears to be coincidental.
From an engineering point of view, the comparison of the response spectra suggests
that for an earthquake with this level of shaking, the optical instrument is capable of
providing quite adequate estimates of the response of structures with periods less than
-14-
one second. However, the optical instrument data may lead to significant errors in
estimates of the response of structures with longer periods even when the data is fil-
tered according to accepted techniques. Additional data from side-by-side comparisons
would be useful in extending these observations.
RESULTS FROM A RECENT CHINESE EARTHQUAKE
A number of PDR-1/FBA-13 instruments have been installed in China as part of a
joint US/PRe cooperative project in strong ground motion measurement. This project
is sponsored by the U.S. National Science Foundation and the Chinese State Seismologi-
cal Bureau through the Instate of Engineering Mechanics in Harbin. A number of
instruments have been installed in arrays in the aftershock region of the 1976 Tangshan
*earthquake. On October 19, 1982 a Ms=5.3 event occurred near the city of Lulong
northeast of Tangshan. The location of the epicenter of this aftershock and the locations
of instruments recording the event are shown in Figure 28. The epicentral location
shown was determined by analysis of the strong-motion array data. The focal depth
was estimated at approximately 10 km and the closest instrument (TS-12) was 4.2 km
from the postulated epicenter. A comprehensive study of the aftershocks of this event
has been made by Wu (1984).
The accelerograms obtained from station TS-12 are shown in Figures 29-31. The
results shown are quite unique in that one channel of the horizontal data was not
recorded at all during the earthquake due to an instrument malfunction. This data was
. This event was originally assigned a magnitude of ML=6.2 by the Chinese Institute of Geophysics buthas recently been downgraded.
-15-
reconstructed later using the parity information recorded by the PDR-1. Time histories
of the velocity and displacement are also shown in Figures 29-31. All of the records
were processed using the correction algorithm described herein. However, due to the
presence of some obviously incorrect data (and associated parity errors) early in the
pre-event data, this data was averaged from 1.0 to 2.5 seconds. Application of Option
Two for the selection of t] and t2 yielded t2 < tl' Therefore, a form of Option One was
used. The final result was insensitive to the precise values of tl and t2 selected.
The results shown in Figures 29-31 predict a net horizontal absolute permanent dis
placement in the direction S30E of 4.0 em and a net downward vertical permanent dis
placement of 1.0 em. The rise time associated with the permanent displacement is of the
order of 1.5 sec. All of these results appear to be consistent with the known fault behav
ior in the region and are not inconsistent with the predictions of theoretical source
models for an event of this magnitude. To the authors' knowledge, this is the first time
that such absolute ground displacement has been recovered from recorded data.
Results of this type present a unique opportunity for the calibration of seismic source
models.
CONCLUSIONS
Based on the observations reported herein, it is believed that the digital accel-
erograph will eventually become the standard instrument for strong-motion measure
ment. Even allowing for anomalies which exist in some current instruments, it appears
that the digital instrument is capable of providing accurate data over a much wider
range of amplitude and frequency than was previously thought possible. Expanded use
-16-
of digital instruments could have a beneficial impact on source modeling and wave
propagation studies as well as structural response studies.
REFERENCES
Hudson, D.E. (1979). Reading and Interpreting Strong .Motion Accelerograms, EarthquakeEngineering Research Institute, Berkeley.
Hudson, D.E. (1977). "Reliability of Records," Panel 1, Earthquakes, Froc. Sixth WorldConf on Earthquake Engr., New Delhi, India.
Trifunac, M.D. and V. Lee (1973). Routine Computer Processing of Strong-MotionAccelerograms, Earthquake Engineering Research Laboratory Report No. 73-03, Calif.Inst. of Tech., Pasadena.
Wang, P., L. Song and F.T. Wu 91984). Near Field Seismic Observation with a MobileLittle Aperture Network, Proc. of International Workshop on Earthquake Engineering,Shanghai, China, March 27-31,1984.
ACKNOWLEDGMENT
The authors wish to acknowledge Mr. Raul RelIes who installed the instruments in
the Coalinga aftershock region. The authors also express appreciation to Mr. Tony
Shakal of the California Division of Mines and Geology for processing the analog film
records obtained from the Coalinga aftershock. The Lulong records were obtained
under a cooperative project between the United States and the People's Republic of
China. The project is directed by Profs. Liu Huixian, Xie LiLi and Peng Keshong of the
Institute of Engineering Mechanics, Harbin, and Dr. D.A. Boore and Profs. W.D. Iwan
and T.-L. Teng in the U.s. The second author was supported under the IBM Resident
Study Program. This project was sponsored in part by the National Science Founda-
tion. The opinions expressed are those of the authors and do not necessarily reflect
those of the sponsoring agency.
-17-
TABLE 1. RESULTS OF DISPLACEMENT TEST
Testaf (em / see2 ) am(em/see2 ) tl (see) t2 (see) Compo Final
(Fig. No.) Displ. (em)8 -6.52 -7.52 2.03 7.48 23.79 -0.081 -0.08 2.13 5.78 25.8
10 -0.09 -0.18 1.98 3.92 25.811 - - - - 15.512 -1.10 - - - 25.9
TABLE 2 COMPARISON OF OPTICAL AND DIGITAL VALUES OF PEAKACCELERATION, VELOCITY AND DISPLACEMENT COALINGA AFTERSHOCK, MAY 8, 1984
COMPONENT DIGITAL REC. OPTICAL REC.
Max. Acee!. N35E 99.5 95.7
em/sec2 Up 73.3 -72.7S55E 117.3 114.6
Max. Vel. N35E 7.37 6.75
(em/sec) Up 2.17 2.20S55E 4.46 4.11
Max. Displ. N35E 0.97 -0.39
(em) Up 0.4 -0.17S55E 0.63 0.36
TABLE 3. COMPARISON OF TIME DIFFERENCE BETWEENANALOG AND DIGITAL
Time Difference (sec, ±0.01 sec)Component From Max. Correlation From Max. Accel. Peak
35 Deg. 4.06 4.05Up 4.06 4.01
125 Deg. 4.05 4.04
-18-
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CO. 0 2.0 4.0 6.0 8.0 10.0TIME (SEC)
0
0
Cl~
(J)\).
II\)
0nO
3:
I
"'"gJ.O 2.0 4.0 6.0 8.0 10.0TIME (SEC)
Figure 6 Displacement test showing effects of instrument anomaly.
Figure 7 Simple correction algorithm for instrumentanomaly.
n
~ P.+----...,.A-tJ.-++.+++++.J-A.iI-++lrl+if4:-HrIIH-lrf-hd!ArfYo-,-----~o V \lJ ,~rn"(J)
rnnJ,~__----.--------r-----r------.------r~§J.O 2.0 4.0 6.0 8.0 10.0
TIME (SEC)
....o
<rnr
nP~---_-A-,~H+-I-t-f+-A-.f+.4t-A-A-M~fJTp'-------3:0"(J)
rnn
J,.-1-------.--------r-----r------.------rco. a 2.0 4.0 6.0 8.0 10.0
TIME (SEC)
0'..__------.,.------------------o
(J)
"lJ.I
I\.lo
J,.4------.------.-----r------.------,co. a 2.0 4.0 6.0 8.0 10.0
TIME (SEC)
Figure 8 Displacement test of Figure 6 with proposedcorrection algorithm
:ONnono·n3:......... !='(1)0rnn.........(I)
rn01~I\)
gJ.O 2.0 4.0 6.0 8.0 10.0TI.ME (SEC)
....<0
rnr·n~~o.........Virnn
I....co. 0 2.0 4.0 6. a 8.0 10.0
TIME (SEC)
....0
0.:....(I)
\J· ~0
n3:
I....co. a 2.0 4.0 6. a 8.0 10. a
TIME (SEC)
Figure 9 Displacement test of Figure 4 with proposedcorrection algorithm.
:D conon·n~,?Wornn,(J)rnnlco~ CO. 0 2.0 4.0 6.0 8.0 10.0
TI·ME - (SEC)
....0
<rnr·n?~o,Wrnn
I....co. 0 2.0 4.0 6.0 8.0 10.0TIME (SEC)
0
0
Q'......~.."• I
l\.l0
n~
I....co. 0 2.0 4.0 6.0 8.0 10.0
TIME (SEC)
Figure 10 Displacement test with proposed correctionalgorithm.
:DCl)
nono·n3:--...!=lU)orr1n--...U)
rr1nl
Cl)
~gJ. 0 3.0 6.0 9.0 12.0 15.0TIME (SEC)
I\)
0<rr1r·n!=l3:0--...U)
rr1n
II\)
cu. 0 3.0 6.0 9.0 12.0 15.0TIME (SEC)
I\)
0
CJ......U)
""'U· 0
0
n3:
II\)
cu. 0 3.0 6.0 9.0 12.0 15.0TIME (SEC)
Figure 11 Displacement test with proposed simple correction algorithm.
:::D ronono·n3:,p(J)ornn,(J)rnnl
ro~gJ. 0 3.0 6.0 9.0 12.0 15,0
TIME (SEC)
I'.J0
-<rnr·nP3:0,(J)rnn
1I'.J
co. 0 3.0 6.0 9.0 12.0 15.0TIME (SEC)
"'"0
0~
(J)\)
· 0
0
n3:
I
"'"co. 0 3.0 6.0 9.0 12.0 15.0TIME (SEC)
Figure 12 Displacement test of Figure 11 with more extensive correction.
::Dn-ono COALINGA AFTERSHOCK MAY 8, 1983
DIGITAL RECORD 35DEGn3:,?(J)oITtn,(J)ITtnl-§P.O 5.0 10.0 15.0 20.0 25.0 30.0
TIME (SEC)
CX)
<0ITtr.
n?3:0,(J)ITtn
ICX)
&.0 5.0 10.0 15.0 20.0 25.0 30.0TIME (SEC)
....0
0.-(J)-u.
?0
n3:
I-dl· O 5.0 10.0 15.0 20.0 25.0 30.0TIME (SEC)
Figure 13 Digital accelerogram with integrated velocity anddisplacement. Coalinga aftershock of May 8, 1983;35 degrees.
Figure 14 Digital accelerogram with integrated velocity anddisplacement. Coalinga aftershock of May 8, 1983;up.
:Dn rv
0nO COALINGA AFTERSHOCK MAY 8,1983
DIGITAL RECCR> 125 DEGn::3:
"P(f)ornn
"(f)rnnl~rv
gJ.O 5.0 10.0 15.0 20.0 25.0 30.0TIME (SEC)
:n<0rnr.nP::3:0
"(f)rnn
IUl
Jl.O 5. 0 10.0 15.0 20.0 25.0 30.0TIME (SEC)
0
~~l--0
P0
n::3:
I0
~.O 5.0 10.0 15.0 20.0 25.0 30.0TIME (SEC)
Figure 15 Digital accelerogram with integrated velocity anddisplacement. Coalinga aftershock of May 8, 1983;125 degrees.
:D_nono exw...tQ Af1'ERSI«)Q( MAY 8..983·
MW.DG ft!CQR) 35 lEGn3:........ P(1)0rnn........(1)rnnl-~gJ. 0 5.0 10.0 15. O. 20.0 25.0 30.0
TIME (SEC)
?l<0rnr·nP3:0........(1)rnn
IcodJ·O 5.0 10.0 15.0 20.0 25.0 30.0
TIME (SEC)
-0
0......(1)""1J· 0
0
n3:
I-dJ·O 5.0 10.0 15.0 20.0 25.0 30.0TIME (SEC)
Figure 16 Analog acce1erogram with integrated velocity and displacement. Coalinga aftershock of May 8, 1983;35 degrees.
:DO)non 00AI....ItGA Afl'ERSHC)Q( MAY &.1983·
NW..DG f£0(R) lPn3:......... ?(J)ornn.........(J)rnnl~O)
5.0 10.0 15.0 20.0 25.0 30.0CO. aTIME (SEC)
~<0rnr·n?3:0.........(J)rnn
I
""dJ. a 5.0 10.0 15.0 20.0. 25.0 30.0TIME (SEC)
?""0
.......(J)\)
· 0
0
n3:
I0;"'0. a 5. a 10. a 15. a 20.0 25.0 30.0
TIME (SEC)
Figure 17 Analog accelerogram with integrated velocity and displacement. Coalinga aftershock of May 8, 1983; up.
:DI\)
nono OOAL.JGA Af1'ERH)Q( aMY 8.1983·
ANALOG REOQR) 125 lEGn3:,P(1)0rnn,(I)
rnnl~I\)
gJ.o 5.0 10.0 15.0 20.0 25.0 30.0TIME (SEC)
U1
<0rn,r·nP3:0,(I)
rnn
IU1
dJ·O 5.0 10.0 15.0 20.0 25.0 30.0TIME (SEC)
0
0)
CJ.......(I)
-0· 0
0
n3:
I0
~.o 5.0 10.0 15.0 20.0 25.0' 30.0TIME (SEC)
Figure 18 Analog acce1erogram with integrated velocity and displacement. Coalinga aftershock of May 8 t 1983;125 degrees.
COALINGA AFTERSHOCK HAY 8. 198335 DEGREES
:e_n o"-,-----:----.,.----..,._---__,_----_r__---_,_-------,no
COALINGA AFTERSHOCK HAY 8, 1983ANALOG 35 DEGREES
n3:,~
UlofTIn,UlfTI
nl+----~-----r------.,.----....._---__,_------i'-'~. 0 5.0 10.0 15.0 20. 0 25. 0 30. 0
TIME (SEC):::D ~.n o..,.----~-~---_r_--"-~----....._---__r---___...,
noCOALINGA AFTERSHOCK MAY 8, 1983DIGITAL 35 DEGREES
n3:
'~+-------"'.(1)0rTln........(1)
rTln ~+---___r----_r_--____:___r---~._--,-.-----;
'-'§}.o 5.0 10.0, 15.0 20.0 25.0 30.0TIME (SEC)
- ...,.----___r----......------.,.----.----__,_---___...,nOo::0::0
~+_-----:.,.----..,._---__,_----_r__---_,_---___i
~o. 0 2. 0 4.0 6.0 8.0TIME DELAY (SEC)
10.0 12.0
o...-U'! --.,. ..,._---__,_----.----_,_---___...,.,0•.,
COALINGA AFTERSHOCK MAr 8, 198335 DEGREES
n3: 0 "------"'1,. ""T
(1)0
rTln,(j)
rTll--'-- --.,.----..,._---___r----._---_,_-----tn (J1'
'-'C{). 0 5.0 10.0. 15.0 20.0 25.0 30.0TIME (SEC)
Figure 19 Correlation coefficient and difference between digital and analogaccelerograms. Coalinga aftershock, May 8, 1983; 35 degrees.
COALINGA AFTERSHOCK HAY 8.1983DIGITAL UP
:0 conO.,------,,..----....----.-------r-----.------,n
COALINGA AFTERSHOCK HAY 8. 1983ANALOG UP
n3:,~
(./)0
n1n,(./)
n1
~~+--------,r-------r----......------r------r-------lco. 0 5.0 10.0 15.0 20.0 25.0 30.0
TIME (SEC)
:0 eo.no..,.-------,r--------.----......------.-----.-----,n
n3:,~+---(./)0
n1n,(./)
n1~ ~-+-----r-------r-----r--------r----,-----r-------l
co. 0 5.0 10.0 15.0 20.0 25.0 30.0TIME (SEC)
nOo::0::0
U'JALINGA AFTERSHCJCK HAY 8.1983UP
2..+_------,____,------.----.--------.-----.------\~.o 2.0 4.0 6.0
TIME DELAY8. 0
(S EC)10.0 12.0
o........ C'O ____,------.----.-------r-----,-----,.,0•.,
rClQU t\GA RFTF.RS;-JOCf"i MAY b. ~ 98:3UP
n3: 0 -L. _, ..(1)0
f"Tln,(J)
f"Tl,noo+-------,____,------.----.-------r----......-----\~C().O 5.0 10.0 15.0 20.0 25.0 30.0
TIME (SEC)
Figure 20 Correlation coefficient and difference between digital and analogaccelerograms. Coalinga aftershock, May 8, 1983; up.
:01'.:;rc..,...-------,----..,----.....,------r-----,------,no
CORLINGR RFTERSHOCK MRY 8.1983ANRLOG 125 DEGREES
n3:........ ~"""'''-/f#IM(..f)crnn........(..f)
rnr,0+------r----..,--------r-----r-----,-----j~§J.O 5.0 10.0 15.0 20.0 25.0 30.0
TIME (SEC)
:D1\.lno..,.------r----..,-----,-----..-------,------,no
COALINGR RFTERSHOCK MRY e.1983DIGITAL 125 DEGREES
n3:........~~----~ ...~(..f)ornn........(..f)
rnn,0+------r----..,--------r-----r-----,-----j~ gJ. 0 5. 0 10.0 15. 0 20. 0 25. 0 30. 0
TIME tSECJ
........,.----------,----.,.-----,------r-------,------,nOa:::0:::0
°n'0°rnIfIf
MRY 8, 1983
10.04.0 6.0 8.0TI ME DELRY (SEC)
2.0dJ·OJ..-I----"""'T""----r------r------,---~-.------j
12.0
CJ":-'CDIfo..,.------r----..,-----.....,------r------,------,If
COALI NGR RFTERSHOCK MAY -8 •. 1983125 DEGREES
n3: 0 L---..._14l1N......... .,.(..f)o
rnn........(..f)
rn lnCD+------r----..,------,------r-----,-----j~q).0 5.0 10.0 15.C 20.C 25.0 3C.C
TIME (SEC)
Figure 21 Correlation coefficient' and difference between digital and analogaccelerograms. Coalinga aftershock, May 8, 1983; 125 degrees.
"GlC:~-r-----,.----..,.--------r----r----..,:::0.........
COALINGA AFTERSHOCK MAY 8.1983ANALOG 35 DEGREES
+-<-fc:ornl\.)
o
n ~S 'Irn 0 ~....L--....!,-_----:-..l._-r--l-"":"':":!.......:'~'..iIl'~"""'~-~-----ln'_C::O.O 5.0 10.0 15.0 20.0 25.0
FREQUENCY (HZ.
COALINGA AFTERSHOCK MAY 8.1983DIGITAL 35 DEGREES
"Glenc: o,.....-----,.----..,.--------r----r-----,:::D.......rn::D
.......-fc:ornl\.)
o
n3::'U)
rn°-lll~_---.:..~_......:....:........:_..,....!.....L.L...!~Uf~_=..::Oo::~¥-......_.._,"'9n'_C::O.O 5.0 10.0 15.0 20.0 25.0
FREQUENCY (HZ.)t:J
....... en-.-------..----..,.---------r----r-----"TI 0
"TI.C~ALINGA AFTERSHOCK MAY 8. 1983
n3:'(J)
f'T1 0 ...~~U~:.:....::!..lI!..!:.-=,.:f.-..IT:Ya~~IIWdIlool!!~~-_-~n· -f- CP. 0 5. 0 10. 0 15.0 20. 0 25. O'
FREQUENCY (HZ)
Figure 22 Fourier amplitude spectra of analog and digital acce1erogramsand difference. Coalinga aftershock, May 8, 1983; 35 degrees.
11QwCO,------"T----,------,----,------,:::D
~ I:Dl\..ll3: 0"'lJr.....--l .Corn-o
CORLINGR RFTERSHOCK MRT 8. 1983RNRLOG UP
5.0 10.0 15.0FREQUENC'( (HZ.)
20.0 25.0
CORLINGR RFTERSHOCK MRT 8. 1983OIGITRL UP
11QO)co,------r----,---------r----...-------,:::D.....rn:::D
n3:.......(J)
rn 0 ~~~--.:.--.:..J..,......:...---J:.L..:-.:+_-----!~~-.!...:..!.....!....!.::rl~!!laQWtJti!.'::Cl:::l~n'..... CU.O 5.0 10.0 15.0 20.0 25.0
FREQUENC'( (HZ.)o..... 0)Ilo,------r----,..------r-~--,-------,
11
CORLI NGR RFTERSHOCK MRY 8. 1983
:D3:"'lJr_• 0
n3:.......(J)
rn 0 ~~tt!.:.~~~~T~~~--!J!.!..J..Q._..:.---.:~-~~~~~~n·-¥-..... CU.O 5.0 10.0 15.0 20.0 25.0
FREQUENC'( (HZ)
Figure 23 Fourier amplitude spectra of analog and digital acce1erograms anddifference.. Coalinga aftershock, May 8, 1983; up.
"GlCT.I ----.. -r- --,- ,-- -,co::D.....rn::0
COALINGA AFTERSHOCK MAY 8. 1983ANALOG 125 DEGREES
.....
n::;::........(.f)
~ P,4::--!..--~:-'-...L.--+.::.::.:t~~~!"""""---""'!"""-0-----i250~q). 0 5.0 10.0 15.0 20. .
FREQUENCY (HZ. I"GlC g;.~------r-----r------r-.---._----__,::0.....
COALINGA AFTERSHOCK MAY 8. 1983DIGITAL 125 DEGREES
.....-iCornl'lo
n::;::........(.f)
rno~~--.:..~--!L:.-__l~'W:!~~..-.~~.......eT"'_...o.-"""__1n'~ q). 0 5. 0 10. 0 15. 0 20. 0 25. 0
FREQUENCY (HZ.)o..... CT.I,,0".
COALINGA AFTERSHOCK MAY 8. 1983
"Gc ....::0 0.
n::;::
"CJ)
rn 0 11!ll~~!!!:~::....Jl!!._~~~~t.;.'-dIll!lllll'o!!6wo~!I!!!!IIo...!!Ioofooj_...1n· -.'~q).0 5.0 10.0 15.0 20.0 25.0
FREQUENCY (HZ)Figure 24 Fourier amplitude spectra of analog and digital accelerograms and
difference. Coalinga aftershock, May 8,1983; 125 degrees.
.....a
C>
.....a-
COALINGA AFTERSHOCK MAY 8,1983
35DEG
.....r---r--r,...,.",rn--r-r-T'TT"rTTT--r-"""T"""T'"T"T"TT'rr----r-..,.-r-M'TTTl O....
....... .......
DIGITAL
---------- ANALOG 0.07 HZ (UPPER)
------- ANALOG 0.40 HZ (LOWER)....... .....0 a~ ....... ....... ....... ~.~
0 0 0 0 0I .,!.. C> - ....
N
PERreD (SEC)
tJ(j)
<
.- .......z~'-(j)
rnn
Figure 25 Zero-damped response spectra of analog anddigital acce1erograms. Coalinga aftershock,May 8, 1983; 35 degrees.
.- .-O.-----r--r~,..,..,.TTT'-_r__r_,...,..,~rr____,___,__rT'"T"lrTTT-_,..._,...'T""r........,.,...
COALINGA AFTERSHOCK MAY 8.1983
lP
-
..-
.-0.:.
DIGITAL
-------- ANALOG 0.07 HZ (UPPER)
------- ANALOG 0.40 HZ (LOWER)..... .-a ar .- ..- .- ~'~
a a 0 0 aI .:. t;> ... .....
PEAleo (SEC)
..-o
IJ I
(.J)
<
Figure 26 Zero-damped response spectra of analog anddigital acce1erograms. Coalinga aftershock,May 8, 1983; up.
........O~--'---'-""T"1rTTnT"-'-"'T'""'1I'"T'1!"TT1rr---'--'''''''''T"T"1'TTT-''''''''''''T'TTTTn...
COALINGA AFTERSHOCK MAY 8,1983
125DEG.... .....
---DIGITAL
---------- ANALOG 0.07 HZ <UPPER)
-- - - -- - ANALOG 0.40 HZ (LOWER)
.....OL---L--L...L.L-I-L.LI.L_...J.-...J.-L.L-Ll..LLL---l--l'-L..&...l.IL.U.L_-I...-I.....I-L.J...LI......
-'1; ;; ;; ;; ~.:.~ .~ -0 N
....o
,!.
PERI-eJD (SEC)
Figure 27 Zero-damped response spectra of analog anddigital acce1erograms. Coalinga aftershock,May 8, 1983; 125 degrees.
1180
119°
... '..
.... . .
...
Cha
ngll
., . ..
.......'
oo o
o
:...
..0
..,
..- ....
..
.'....
.....,
". .'.
.....
..o
'•
.....
....
....
....
. .'.o
ML
2.9
-3
.9o
4.0
-4
.9
a6
.29
~1,2
....
'.. --\
\V
/1
39
°30
'I
0~
....
f/0
>------
1..---
-f=~
I
Fig
ure
28T
ang
shan
aft
ers
ho
ck
arr
ay
show
ing
locati
on
of
Lu1
0ng
even
tan
dS
tati
on
11
.
Figure 29 Accelerogram with integrated velocity and displacement. Station 12. Lulong earthquake, October 19, 1982;North.
::DI\,)
nono w..c:JG EAR11iQUAI(E OCT 19.1982·
LPn3:,f'(J)orT1n,(J)rT1nl
I\,)
~2P.O 2.5 5.0 7.5 10.0 12.5 15.0TIME (SEC)
~<0rT1I·nf'3:0,(J)rT1n
II\,)
dJ·O 2.5 5. a 7.5 10.0 12.5 15.0TIME (SEC)
I\,)
0
0.-(J)-0· f'
0n3:
II\,)
dl· O 2.5 5.0 7.5 10.0 12.5 15.0TIME (SEC)
Figure 30 Accelerogram with integrated velocity and displace-ment. Station 12. Lu10ng earthquake. October 19. 1982;up.
:ONnono LU..ONG EARTHQUAKE OCT 19.1982.
EASTn3:'-.?(J)ornn'-.(J)rnn~ i I i I i~gJ. 0 2.5 S.O 7.5 10.0 12.5 15.0
TIME (SEC)
co<0f"TIr
n?~o'-.(J)f"TIn
1codJ·O 2. 5 5.0 7.5 10.0 12.5 15.0
TIME (SEC)
'!'"0
0.......th"""U.
?0
n~
I~
dJ·O 2.5 5.0 7.5 10.0 12.5 15.0TIME (SEC)
Figure 31 Accelerogram with integrated velocity and displacement. Station 12. Lulong earthquake, October 19, 1982;East.