Características de propagação blast
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Transcript of Características de propagação blast
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dependent on the size of joints in comparison with the wave
length.10 The first method is usually adopted to a single joint
characterised by a large size, whereas the second is used
when fractures are dense and small in size compared with
the shock wave length.
In comparison with the effects of rock joints on the
mechanical properties of rock mass, however, less atten-
tion has been paid to their effects on wave propagation.2
There are fewer reports on field test study of rock joint
effect on shock wave propagation. In the present study,
blast-induced ground motions were recorded on a rock
surface at different distances from the explosion centre,
and in different orientations with respect to the predomi-
nant strike of joints. In this paper, the results of field
measurement are presented and analysed, and the mechan-ism of rock joint effects on wave propagation are
discussed.
2 MEASUREMENT CONFIGURATION AND
INSTRUMENTATION
The field layout, as shown in Fig. 1, consists of a charge
borehole of 11 m in depth and seven measuring points on
the rock surface. The measuring points, labelled RS1RS5,
were set up along a measuring line which is parallel to the
predominant joint strike, to examine shock wave propaga-tion and attenuation in rock mass. The measuring points are
2.5, 5, 10, 25 and 50 m from the charge borehole, with the
corresponding absolute distances of 8.8, 9.8, 13.1, 26.4 and
50.7 m from the explosion centre, respectively. To examine
the orientation effects of rock joints, two extra measuring
points, labelled RS6 and RS7, were arranged surrounding the
explosion centre at a distance of 50 m. They are 45 and 90
with respect to the strike of predominant joint sets,
respectively.
At each point, two pieces of ENDEVCO piezoelectric
accelerometers were set up to record the radial (horizontal)
and vertical accelerations. The accelerometers were
mounted on magnetic bases which were tightly secured onthe steel plates cemented onto the rock surface. The detected
signals were amplified by ENDEVCO signal conditioners
and then transmitted to a data recorder. A TEKTRONIX
data logging system was used to record the ground motions.
The sampling rate was taken as 100 ms, and the recording
duration as 2 s for each channel. An automatic signal trig-
gering model of the data logger was selected to simulta-
neously record the acceleration wave histories from all the
accelerometers. The automatic trigging level was set as 0.1g
(g 9.8 m/s2) which was slightly higher than the environ-
mental noise level.
The rock at the site is of very good quality. Its average P-
wave velocity (Vp) is approximately 5790 m. The predomi-
nant joint sets are sub-vertical, with the spacing ranging
from 30 to 50 cm.
Three cylindrical charges were detonated with theequivalent TNT charge weights of 10, 20 and 40 kg, corre-
sponding to the loading densities of 5, 10 and 20 kg/m3,
respectively. The surface motions, i.e. the radial and vertical
accelerations induced by blasting, were monitored during
the tests.
The blast-induced accelerations were estimated using
Dowdings empirical equation11 which is widely applied
in mining and civil engineering:
A 0:81 g30:5 m
R
1:84c
3050 m=s
1:45
Q
4:54 kg
0:28 2:4
r
0:28
1
where A is the peak acceleration in g, Q (kg) is the charge
weight, R (m) is the distance from the explosion centre, c is
the P-wave velocity of rocks (c 5790 m/s), and r is the
rock density (r 2.6 g/cm3).
To avoid signal peak cut-off, the recording range of the
instruments was taken as six times the estimated value.
Particle velocities and displacements were derived by
numerical integration from the acceleration data. Since the
displacement might contain a large error resulting from
double integration, it was not treated as a parameter describ-ing ground motions in this study.
Fig. 1. Configuration of measurement.
408 Y. K. Wu et al.
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3 RESULTS AND DISCUSSION
3.1 Propagation velocity of shock waves
Points RS1RS5 were set on the same measurement line
with different distances from the charge centre, therefore,
the arrival times of shock waves at these points and their
corresponding distances, can be used to calculate the wave
propagation velocity in the rock mass. In Fig. 2, the arrival
times of shock waves versus the corresponding distances,
and the best fitted trend-lines, are presented. As can be seen,
the trend-lines of arrival times and distances from all tests,
are consistently parallel to each other. Regardless of the
different triggering times of the data logging system
during each test, the mean propagation velocity, i.e. the
average slope of the trend-lines, is 5520 10 m/s). It is
slightly (approximately 5%) smaller than the average P-
wave velocity of 5790 m/s obtained from seismic surveys.
The error is acceptable in the realm of engineering geology.
In the seismic surveys, mechanical impacts were used as the
energy sources. The results indicate that the wave propaga-
tion velocity in a rock mass is independent of the type of
energy source generating elastic waves. The consistent
velocities at different distances from the charge centre,
imply the homogeneity of rock mass in its property along
the measuring line.
3.2 Rock surface motions
Fig. 3 shows the peak horizontal and vertical accelerations
measured at the points RS1RS5 against the horizontal dis-
tance from the explosion centre, respectively. As can be
seen, the horizontal and vertical surface motions show dif-ferent attenuation trends. In the close vicinity of the charge
hole, the vertical component of ground motion is larger than
the horizontal. With the increase of the horizontal distance
from the charge hole, the horizontal component increases
initially then decreases, whereas the vertical component
decreases continuously with the distance. The initial
increase of horizontal motions is caused by the very large
incident angle of the shock wave. Theoretically, the hori-
zontal component is zero, if the shock wave is vertically
incident to the ground surface. From the present test results,
it can be seen that the maximum horizontal acceleration
occurs at approximately 10 m from the charge hole. it wasnoted that either the horizontal or vertical components of
ground motions could be larger. In general, at near-field to
the charge centre, vertical motion is more pronounced, and
horizontal motion becomes dominant at large distances
from the charge centre. The results are significant for esti-
mating ground motion effects on the surface structures at
different distances from the charge centre, because struc-
tures respond to horizontal and vertical vibrations differ-
ently. Usually, structures are more prone to horizontal
excitations as a result of their great weight, which, however,
requires a very large vertical motion to excite.
Assuming that the peak horizontal and vertical accelera-
tions Ah and Av at a point occur at the same time, theresultant peak acceleration can then be calculated by
A (A2h A
2v). This assumption may result in a larger esti-
mation of the absolute peak acceleration than the actual one.
From the engineering point of view, however, the assump-
tion will result in a conservative assessment of structural
safety. The resultant peak particle velocity can be similarly
calculated from the horizontal and vertical velocity
components.
It is well known that blast-induced accelerations and par-
ticle velocities are closely related to cube-root scaled
range,11 i.e. the absolute distance from the explosion
centre scaled by the cube-root of the charge weight. There-fore, the measured peak accelerations and peak velocities
are plotted against the scaled range in Figs 4 and 5, respec-
tively, where the particle velocities are obtained by numeri-
cally integrating the recorded accelerations after baseline
corrections. The recorded data can be used to derive empiri-
cal attenuation for peak accelerations and peak particle
velocities. The least-squares-fitted empirical attenuation
relations are given in the following:
A 2540:4 R=Q1=3
1:59(2)
PPV 487:71 R=Q1=3
1:25
(3)
where A is the peak acceleration in g, PPV(mm/s) is the peakparticle velocity, and R/Q1/3 (m/kg1/3) is the scaled range.
Fig. 2. Propagation velocity of shock waves.
Fig. 3. Horizontal and vertical acceleration attenuation withdistance.
Blast-induced shock waves 409
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The correlation factors (r) are 0.98 and 0.97, respectively.
The best fitted attenuation relations are also shown in Figs 4
and 5, respectively. For comparison, the empirical attenua-
tion equations of acceleration and particle velocity obtainedby Dowding11 are also drawn in Figs 4 and 5, where the
particle velocity attenuation equation is:
PPV 18:3 mm=s30:5 m
R
1:46Q
4:54 kg
0:48 2:4r
0:48
(4)
As can be seen, the accelerations obtained from the present
tests are in good agreement with Dowdings equation,
whereas the particle velocities are approximately 30%
50% smaller than those from eqn (4). However, the data
are still within the lower bound of the data that are used to
deduce this equation. The discrepancy in velocity data
could be attributed to the different charge conditions,
because the equation is based on blasting with a fully-
coupled charge of loading density 14001600 kg/m 3, and
the present blasting are decoupled with a very low-loading
density.
3.3 Frequency attenuation
Frequency content is an important characteristics of blast-
induced shock waves besides the amplitude. It affects the
performance and safety of structures under shock wave
excitation, because the structural response is highly
frequency-dependent. Some commonly applied criteria for
assessing the structure safety under the influence of shock
waves are also frequency dependent.12 When the principal
frequency of a shock wave is higher or lower than the modal
frequency of structures, the allowable critical vibration level
of structures is accordingly raised. Therefore, it is alsoimportant to analyse the change of frequency contents of
shock waves with the increase of distance to the charge
centre. The frequency contents were estimated by using
the power spectral density function:13
SX1X1(q) 1
T
M
m M
WMX1 q 2pm
T
X1 q
2pm
T
(5)
where X1(q) is the Fourier transformation of the accelera-
tion wave x1(t), X1(q) is its complex conjugate, q is the
circular frequency, Tis the duration of the time history, WM
is a smooth window, and 2M 1 is the number of smooth-ing points (here, M 1).
Fig. 6 shows the typical shock waves from Test 3
recorded at RS5, RS6 and RS7 at the incident angles of 0,
45 and 90, respectively. Fig. 7 shows the corresponding
power spectral density functions of these waves. As can be
seen, the principal frequency of the shock wave at RS5, RS6
and RS7 is approximately 510, 280 and 100 Hz,
respectively.
Fig. 8 shows the attenuation of the principal frequencies
of acceleration waves with the increase of distance. As can
be seen, the principal frequencies of acceleration waves
decrease dramatically in the near-field of detonation, andthen slowly when the distance from the charge centre is
more than 10 m. The result implies that high-frequency
components are damped out in the rock mass within 10 m
surrounding the explosion centre.
It is noteworthy that a smaller charge weight corresponds
to a higher principal frequency. Similar results were also
reported by other authors.12 This result is probably due to
the size of the damage zone and plastic region. A larger
charge results in a larger damage zone and plastic region
surrounding the charge centre, which can dramatically
attenuate the high-frequency components of the shock
wave.
3.4 Effects of rock joints orientation
The theory of wave propagation across a joint indicates that
the existence of a joint will change the amplitude and fre-
quency contents of the wave.10 This is confirmed from the
results measured at the field.
Fig. 9 shows the accelerations recorded at 50 m from the
charge centre versus the incident angles of the wave path,
relative to the joint strike. As can be seen, the accelerations
decrease by approximately 60%, while the incident angle
varies from 0 to 90. The decrease is faster when the angle
increases from 0 to 45 than when it increases from 45 to90. This trend is related to the increase of the joint number
Fig. 4. Acceleration versus scaled range.
Fig. 5. Particle velocity versus scaled range.
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that the shock wave propagates across. As shown in Fig. 1,
the joint number that shock waves propagate across
increases rapidly when the angle varies from 0
to 45,
and then slowly when the angle varies from 45 to 90.
Fig. 10 shows the principal frequencies of the accelera-
tion waves recorded at RS5, RS6 and RS7. The principal
frequencies at these points decrease approximately 70%
when the incident angle varies from 0 to 90. Similar to
the peak acceleration, the frequency attenuation is slightly
faster when the angle increases from 0 to 45, than when the
angle varies from 45 to 90.
The decreases of the peak acceleration and the principal
frequency with the increase of the incident angle, reflect the
comprehensive effects of joints. As can be seen, when the
wave propagation path is perpendicular to the joint strike,
the shock wave attenuates the fastest, whereas it attenuatesthe slowest when its propagation path is parallel with the
joint strike.
3.5 Discussion of mechanism
A laboratory study carried out by Fourney et al.14 can be
used to explain the joint effects on shock-wave propagation
observed in these tests. It has been found that, for a seismic
wave characterised by a principal wave length, there exists a
critical aperture width of joints, below which the amplitude
of the wave changes very little. For joints wider than the
critical value, the wave amplitude significantly decreases
Fig. 6. Typical shock waves (Test 3). Top: RS5 (0); middle: RS6(45); bottom: RS7 (90).
Fig. 7. Power spectrum of shock waves.
Fig. 8. Principal frequency versus distance.
Fig. 9. Accelerations versus incident angles (R 50 m).
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