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Article |
1 Istituto Nazionale di Geofisica e
Vulcanologia
via Bassini 15
20133 Milano, Italy
(D.B.)
2 GeoForschungsZentrum
Potsdam
Telegrafenberg
14473 Potsdam, Germany
(S.P., H.G.,
C.M.)
3 Ministry of Public Works and
Settlement
General Directorate of Disaster Affairs
Earthquake Research
Department
P.O. Box 763
Ankara, Turkey
(S.K.)
| Abstract |
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f
10 Hz and
QP(f) = 56f0.25 for 2.5
f
10 Hz. For ray paths in the range from 60 to 80 km, the
attenuation weakens but the interaction between seismic waves and propagation
medium is more complex. The multilapse time window analysis (MLTWA)
is applied to quantify the amount of scattering loss and intrinsic absorption
for S waves. The seismic albedo B0 decreases
from 0.5 at 1 Hz to 0.3 at 10 Hz, while the total quality factor
QT increases from about 56 to 408. The multiple lapse
time-window analysis (MLTWA) results provide only an average estimate
of the attenuation properties in the range from 10 to 80 km. In fact, by
neglecting the variation of attenuation with depth, the MLTWA results
underestimate attenuation for distances less than 40 km, and do not capture the
significant features caused by the integrated energy of the secondary arrivals
observed in the range from 40 to 60 km. | Introduction |
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, most studies found
values of Q0 less than 100, and values of
close to or even greater than 1. Examples are QS =
35f0.83 and Qc =
29f1.03 (for a lapse time of 20 sec) for the Erzincan region
(Akinci and Eyidogan, 1996) over
a distance range from 10 to 40 km and in the frequency range from 1.5 to 24 Hz,
and Qc = 41f1.08 and
QS = 50f1.09 for the Marmara
region
(Gündüz et al., 1998)
for the range from 20 to 110 km and the frequency range from 1.5 to 24 Hz.
Studies on Qc(f) that implemented the
single-scattering model generally found an increase in
Qc(f) with lapse time, suggesting an increase in
Q with depth
(Akinci and Eyidogan, 1996;
Gündüz et al., 1998).
Recently, a comparison between the attenuation characteristics of the western
and eastern parts of the NAF was performed
(Akinci et al., 2004)
using attenuative dispersion measurements of P waves. A slightly lower
Q in the western NAF with respect to eastern NAF
was observed.
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We first present results from the application of the generalized inversion technique (Castro et al., 1990; Anderson, 1991) to estimate the rate of decay with distance of the spectral amplitudes in northwestern Turkey for both P and S waves. Second, the attenuation-distance curves are parameterized in terms of geometrical spreading and anelastic attenuation, and the results for QP(f) and QS(f) are compared over the frequency range 1–10 Hz. Finally, we apply the multilapse time window analysis, MLTWA (Hoshiba, 1991; Fehler et al., 1992) to evaluate the relative contribution of intrinsic absorption and scattering to total S-wave attenuation. We follow the numerical approach introduced by Hoshiba (1991), based on the Monte Carlo technique, to synthesize the theoretical integrals of the energy density for the isotropic scattering and spatial uniformity of attenuation. Moreover, using the method developed by Hoshiba (1997), synthetic seismograms and integrated seismic-wave energy are also computed for a simple conceptual model consisting of two layers over a half-space, with the aim of discussing the discrepancy between the observed and thoretically predicted integrals of seismic energy against distance.
| Data |
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The spectra are collected from 14 stations (Fig. 2 and Table 1). We analyze the spectra of S- and P-wave windows with widths of 5 sec. If the travel-time difference between an S wave (tS) and P wave (tP) is less than 5 sec, we use the analyzed P window with a width of (tS – tP) sec. Each window is cosine tapered (5%) and Fourier transformed. Instrumental corrections are applied and the spectral amplitudes are smoothed using the Konno–Ohmachi window, b = 20 (Konno and Ohmachi, 1998). The signal-to-noise ratio (S/N) is greater than about 3 over the frequency range 1 to 10 Hz for S waves, and from 2 to 10 Hz for P waves. The two horizontal (east–west and north–south) and the vertical (Z) spectra are then vectorially summed.
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| Method |
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|
| (1) |
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| (2) |
j(f) is a scalar depending upon the spectral
amplitude of source j, and A(f,rij) is a
nonparametric description of attenuation. We discuss here the results for
A(f,rij) obtained solving the first step, whereas
the results of the second step, which was performed to split the residual
spectra Rij(f) =
U(f,rij)/A(f,rij) into
source Sj(f) and site
Zi(f) spectra, are discussed elsewhere
(Parolai et al., 2004).
The distance range from 10 to 142 km is discretized into 44 bins 3 km wide.
The attenuation is constrained to assume a value equal to 1 at 10 km,
irrespective of frequency, and the A(f,r) is constrained to be
a smooth function of distance by requiring a small second derivative with
respect to r. Equation
(1) is numerically solved for
each frequency separately using the least squares algorithm (LSQR)
(Paige and Saunders, 1982). For
all events and all stations, equation
(1) can be expressed in a matrix
form by
|
| (3) |
0, ...,
Nev–1], where
ai (i = 0,..., M) are the
unknown nonparametric attenuation coefficients, one for each distance knot
i, and
j (j = 0,...,
Nev – 1) are related to the unknown spectral amplitude
of source j. M and Nev are the number of
discrete distance intervals and the number of considered earthquakes,
respectively. | Reliability of the Results |
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][V]T.
Figures 3 and
4 show the unit covariance and
resolution matrices obtained by considering only singular values
i of the diagonal matrix [
]
greater than 0.01 times the maximum singular value. The resolution matrix is
fairly identical, with diagonal values being close to 1. The first 45 columns
are those relevant to the attenuation coefficients ai. There
is only a weak smearing of each
j along the
attenuation coefficients, since the off-diagonal values are close to
10–3. Therefore, the resolution matrix indicates that each
model parameter can be satisfactorily resolved, and the mutual dependence
between the term including the source and the term describing the attenuation is
weak. The columns of the unit covariance matrix [C] in
Figure 3 relevant to
j (parameter index > 45) are close to being
identical, with standard deviations (for unit data variance) between 0.3 and 1.
The bottom frame of Figure 3
shows an example of columns of the unit covariance matrix relevant to
ai. The standard deviations are smaller than 0.3 (times the
data uncertainty). The standard deviations are greater for the longest (>70
km) and shortest (<20 km) distances, depending on the lower sampling of the
corresponding bins. In the distance range well constrained by data (20–70
km), the standard deviations of the model parameters are smaller than 0.1, and
the spreading of the off-diagonal elements is narrowed.
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| Nonparametric Attenuation A(f,r) |
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The attenuation is significant in the distance range between 60 and 80 km, but it is weaker than those in the first 40 km. Beyond 80 km, the attenuation-distance curves become flattened and then sloped upward after 100 km, in particular at low frequencies. The difference in the amount of attenuation for P and S waves decreases with frequency, and the P-wave amplitude is always less attenuated than the S- wave one. Moreover, the logarithm of attenuation, logA(f,r), decreases with frequency, and the difference between P- and S-wave attenuation increases with distance, being larger at low frequencies. In Figure 6, the estimated log(attenuation)- distance curves for P and S waves at three different frequencies (2, 5, and 10 Hz) are compared with the spectral amplitudes of events having 2.5 < ML < 3, which is well sampled by the analyzed earthquakes. In this figure, an arbitrary offset was added to amplitude to make the comparison easier. The general features of the inversion results are consistent with the data, in particular the slope of the decay at short distances, the change in slope between 30 and 40 km, and again between 80 and 90 km. Since the attenuation curves for distances larger than 100 km are weakly constrained by data, the upward slope of the curves could mainly be controlled by the smoothing applied. In any case, the consistency of this result with earlier studies (e.g., Boztepe- Güney and Horasan, 2002; Baumbach et al., 2003) suggests that this behavior of the attenuation-distance curves is a characteristic feature of crustal propagation in northwestern Turkey due to critical Moho reflections. Finally, the scatter affecting the data is mainly related to difference in magnitudes among the events, and to site amplification effects.
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| Parametrization of A(f,r) |
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| (4) |

is related to the quality factor
Q
(f) (i.e., 
=
f/Q
(f)v
,
where v
is the velocity of the considered phase
). We assume vS = 3.5 km/sec
(Table 2) and
|
Distance 10–38 km
Figure 7 (left frames) shows
n and Q(f) versus frequency for both S and
P waves. For both phases, the average value of n is
close to 1. QP(f) shows a weak frequency
dependency, while the frequency dependence of the S-wave quality factor
QS(f) is remarkable. If the power function
Q(f) =
Q0f
is fitted to
Q(f), the following relations are obtained:
|
| (5) |
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| (6) |
being close to 1 is in agreement with that observed in
seismically active regions. The value of QP(f)
confirms that P-wave propagation is more efficient than for
S waves. In
Figure 7 (top-left panel), the
estimated QS(f) and
QP(f), given in equations
(5) and
(6), are plotted for
comparison.
|
Distance 60–80 km
The propagation characteristics of P and S waves are
more complex over this range than those observed in the range from 10 to 38 km
(Fig. 7, right frames). In
particular, the geometrical spreading n is frequency dependent, for
both S and P waves. The mean values vary between 0.95
and 1.35 for S waves and from 0.75 to 1.28 for
P waves.
| QS/QP versus Distance |
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| (7) |
In Figure 8, the ratios of
QS(f) to QP(f)
computed from equation (7) for
the selected distances (16, 28, and 38 km in the left panel, 61, 70, and 79 km
in the right panel) are shown. We used the average geometrical spreading for
P and S waves previously obtained
(Fig. 7) and assumed a constant
ratio
. In the same
figure, the
QS(f)/QP(f) ratios
computed from equation (7) are
compared to the ratio (thick line) between the same quantities but computed
considering, for each distance range, the average quality factors that we
obtained in the previous section and are shown in
Figure 7. For distances between
10 and 38 km,
QS(f)/QP(f) values
computed from equation (7)
increase with frequency, reaching values close to one at 10 Hz. Moreover, it
varies with distance. In the range 60–80 km, the ratio oscillates from 0.5
to 1.5, and it shows a negligible dependency on distance. In both cases, the
ratio between the average QS and QP is
consistent with the distance-dependent ratios computed by equation
(7).
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In Figure 8, the dotted
horizontal lines correspond to
, and the
theoretical anelastic QP versus QS
relation given by Anderson and Hart
(1978):
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| (8) |
For zero bulk loss (i.e.,
), we obtain
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| (9) |
| MLTWA Analysis for S Waves |
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| (10) |
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| (11) |
(Qscv)–1 is the scattering
coefficient, h =
(Qlv)–1 is the absorption
coefficient,
= 2
f is the angular
frequency, and v is the S-wave velocity.
The seismic energy is integrated in three consecutive time windows, each 15
sec wide, starting 1 sec before the S arrival tS.
For each frequency, the integrals are evaluated from the square of the amplitude
spectrum at the selected frequency. The amplitude spectrum for each time window
is smoothed by applying the Konno–Ohmachi window, b = 60
(Konno and Ohmachi, 1998). The
correction for the geometrical spreading is applied by multiplying the integrals
for 4
r2, while the effects of a nonspherical radiation
pattern are not accounted for in the present study. The energy in each window is
then divided by the coda energy integrated in a fixed reference time window
(from 45 to 50 sec) in order to normalize all the different records to a common
source and site (Aki, 1980). In
the following, we refer to E1(r, f),
E2(r, f), and E3(r, f)
to indicate the results obtained from integrating the energy in the time windows
from ts to ts + 15, from
ts + 15 to ts + 30, and from
ts + 30 to ts + 45,
respectively. Figure 9 shows
E1, E2, and E3 for
the frequencies 1.6, 3.2, and 8 Hz. We computed the average of
E1(r, f),
E2(r, f), and
E3(r, f) over a window 5 km wide (black
lines), –1 standard deviation (gray area). The strategy of
the MLTWA method is to simultaneously minimize the discrepancy
between the computed integrals and those predicted
by theory. Assuming a spatially uniform medium, we
computed the synthetic integrals for a set of B0 and
pairs
using the Monte Carlo method. A grid search algorithm is
then applied to find the best fit to the data, that is, the solution
that minimizes the residual in a least-squares sense. The total
residual is computed by summing the relative residual over
each time window. Figure 10
shows the total residuals normalized
to their minimum value, for two frequencies. In the
bottom panels of Figure 10, the
pairs (B0,
) corresponding
to a residual within 10% from the minimum are also
displayed for estimating the uncertainties.
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In Figure 9, the synthetic
curves corresponding to the
minimum residual are compared to the integrated energy
against distance. In the bottom-right panel, the
,
,
and
corresponding
to the solutions of minimum residual
are plotted against frequency. At 1 Hz, the albedo B0 is 0.5
and the scattering loss and the intrinsic absorption equally
contribute to total attenuation. The value of QT at 1 Hz is
56. The albedo decreases with frequency, and it becomes 0.3
at 10 Hz. It follows that the influence of scattering loss on
total attenuation decreases with frequency with respect to
the intrinsic absorption. At 10 Hz, QT becomes 408. At
1 Hz,
QT is intermediate between the values of
QS obtained in the
previous sections for distances in the range 10–38 km and
60–80 km. The comparison at 1.6 Hz between synthetic and
actual integrals for the first time window E1 shows that the
theoretical curve only approximates the trend of the observed
data over the distance range considered. In particular,
at distances less than 40 km, E1 computed from observed
data decreases with distance more rapidly than E1 for the
synthetics. Since in the MLTWA method the decay of
E1 with
distance constrains the total attenuation, the obtained value
of
underestimates
the actual attenuation at short distances.
We attribute this underestimation to an inadequacy
in the assumed uniformity of the propagation medium, that
is, the decreases in the rate of decay for distances over 40 km
may reflect increases of propagation efficiency with depth.
Moreover, for distances between 40 and 60 km, the integrals
over the first window show a bump, similar to the behavior
observed for the spectral amplitude versus distance in
Figure 5. The bump could be a
consequence of reflected arrivals
whose energy adds to the energy of the direct arrival. The
presence of secondary arrivals in the range 40–60 km that
cannot be accounted for using a uniform model introduces
a further underestimation of the total attenuation at distances
less than 40 km.
Figure 11 shows the
synthetic SH velocity seismograms
computed by applying the method of Wang
(1999) to the
1D model shown in Table 2 and
derived from Karahan et
al. (2001). The source
depth is 10 km, typical for the considered
earthquakes. For distances larger than 30 km, the
results for this simplified model show that secondary arrivals
can contribute significantly to the total energy in the first
time window. For example, the maximum amplitude of synthetic
seismograms in Figure 11 is
almost constant for distances
between 60 and 80 km, and the peak value corresponds
to secondary arrivals for distances larger than 70 km.
This result suggests that vertical stratification is necessary to
obtain an accurate description of attenuation in northwestern
Turkey. The Monte Carlo method can also be used to synthesize
the energy integrals for a stratified medium
(Hoshiba,
1997). However, the computational burden strongly increases
with increasing number of layers and limits the grid
search procedure to only a coarse grid of Le and
B0 values
for each layer. In Figure 9
(top-left panel, dotted lines) we
also show the best-fit synthetic curves obtained by applying
the Hoshiba (1997) method to the
model given in Table 2.
The synthetic integrals are computed only for 1.6 Hz. The
values of Le and B0 are fixed for the
half-space and the second
layer, and the grid search is applied only to the first
layer. In particular, we set g = 0.001 and h =
0.003 for the
half-space, and g = 0.002 and h = 0.006 for the
second
layer. The attenuation coefficients of the uppermost layer for
the best-fit solution are g = 0.02 and h = 0.10
(i.e., B0 =
0.15 and
. The
value of
corresponds to QT = 45. The results for the layered
model do not increase the quality of the fit with respect to the results for the
uniform model. This is not surprising since a better description of the data
would require a less simplified vertical model, and to set up a multigrid
analysis for investigating the attenuation and velocity properties of all the
layers is beyond the aims of the present work. However, the results for the
stratified model can be used to stress the importance of considering vertical
layering. The theoretical E1 integral decreases till
50 km, from which it flattens and then slopes upward after 60 km. Even
if the upward trend is delayed toward larger distances, this resembles the
behavior of the observed E1. Moreover, the slope of
E1 computed for the layered model at short distances better
describes the observed energy decay, even if the values of the integrals are
slightly overestimated. The overestimation, considered together with the
observed underestimation of E2, suggests that the seismic
albedo has been underestimated.
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| Discussions and Conclusions |
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For 10
r
38 km, the waves propagate through a low
Q-volume. We obtained fairly constant values for n being close
to 1, suggesting that the selected windows are mainly dominated by direct
S or P waves. For f < 10 Hz,
QS(f) = 17f0.80 has a
behavior similar to that observed in previous studies along the NAF,
but with a smaller Q-value at 1 Hz. Gündüz et al.
(1998) found
QS(f) = 50f1.09 in the
Marmara region, Akyol et al.
(2002) found
QS(f) = 46.59f0.67 in
the Bursa region, and Akinci and Eyidogan
(1996) found
QS(f) = 35f0.83 in the
Erzincan region. Recently, Horasan and Boztepe-Güney
(2004) estimated the
QS values ranging from 13f1.22 to
94f0.83 in the Sea of Marmara using the earthquakes over the
distance range 15–70 km and in the frequency range 1.5–12 Hz. Our
QP(f) shows a weak frequency dependence in the
range 2–10 Hz, and is in good agreement with the mean value of 40 found by
Akinci et al. (2004) at
a distance of 30 km. The
QS(f)/QP(f) ranges
from 0.5 to 1.3 (Fig. 8).
Assuming a frequency-independent Q,
Liu et al. (1991)
suggested that the QS/QP in the New
Madrid seismic zone lies between 0.53 and 1.79, in agreement with
Chen et al. (1994). In
the Central Rio Grande rift,
Carpenter and Sanford (1985)
observed a ratio of between 0.72 and 2.94, and assumed it to be frequency
independent, whereas
Clouser and Langstone (1991)
found a ratio between 0.38 and 1.87 for a basin 1.4 km thick in the Gazli region
(Uzbekistan). Exploiting the results achieved in laboratory experiments and
extrapolating them to in situ analysis, the QS/
QP in sedimentary rocks is known to be affected by several
factors, including pore fluids, pore-fluid saturation levels, confining
pressure, crack distribution, and rock type. In particular, many laboratory
studies (Spencer, 1979;
Toksöz et al., 1979;
Johnston and Toksöz, 1980;
Winkler and Nur, 1982; etc.)
suggest that a QP greater than QS is
expected for fully saturated or dry rocks, and less than QS
for partially saturated rocks. Whatever the causes controlling the
QS/QP ratio are, a distance dependency
of this ratio is clear in the range from 10 to 38 km. This confirms that there
is a strong heterogeneous structure of upper crust in northwestern Turkey.
For 38 < r
60 km, two factors can be considered to describe
the behavior of spectral attenuation with distance: (a) the dependence of
Q with depth, which may cause a change in the slope of the attenuation
curve, and (b) the arrival of reflected waves. Several studies show that the
boundary between the fall-off of the direct waves and the emergence of lower
crustal or Moho reflections can lead to fairly constant amplitudes over distance
ranges that depend on several factors, such focal depth, crustal thickness,
crustal-velocity gradient, and so on. For example,
Burger et al. (1987)
found high amplitudes in the range between 60 and 150 km using a model for the
central United States.
Somerville and Yoshimura (1990)
observed high amplitudes in the range 40–100 km using the Loma Prieta
earthquake recorded in the San Francisco and Oakland areas, while
Hartzell (1992) found high
amplitudes in the range 30–40 km while analyzing the 1989 Loma Prieta
earthquake to estimate site response along the San Francisco Peninsula. Within
the framework of magnitude calibration studies,
Bakun and Joyner (1984) found
large amplitudes at distance ranges of 75–125 km for central California,
while Hutton and Boore (1987)
found similar results at around 60 km for southern California.
Mori and Helmberger (1996) noted
that these enhanced amplitudes might be attributed to SmS. Atkinson and
Mereu (1992) showed that the
contemporary arrivals of direct waves and postcritical reflections from the Moho
produce spectral amplitudes that are approximately constant between 70 and 130
km in southeastern Canada. In Turkey, Boztepe-Güney and Horasan
(2002) observed large- amplitude
SmS phases around 100 km for the data recorded toward the west in the
Sea of Marmara.
For 60 < r
80 km, the waves propagate through a volume
having an average higher Q than in the first 38 km, indicating an
increasing propagation efficiency with depth. Studies that applied the coda-wave
method to estimate the coda-quality factor Qc along the
NAF found an increase of Qc with lapse time. This
evidence has been interpreted as the presence of a more attenuating shallow
crust with respect to the deeper one. The ratio
QS/QP does not depend on distance,
suggesting a higher homogeneity of the properties that control this ratio. The
geometrical spreading for S waves is between 0.9 and 1.2 for
frequencies lower than 4 Hz. For higher frequencies, it ranges between 1.2 and
1.4. The geometrical spreading for P waves is about 0.9 for
frequencies less than 7 Hz, and increases up to about 1.2 at 10 Hz. The values
of geometrical spreading greater than one were found in vertically layered
medium by Frankel et al.
(1990). For
r > 80 km, first the slope of attenuation decay
decreases, then fairly constant values are obtained, until finally, the curves
slope upward for distances larger than 100 km.
The time integrals of energy against distance also confirm the depth
dependence of attenuation properties in the analyzed area and the presence of
secondary arrivals that significantly contribute to spectral amplitude in the
range 40–60 km. Since the application of the MLTWA to a medium
that is not spatially uniform requires both a large computational effort and the
availability of a realistic model for the area, we interpreted the observations
by generating synthetic integrals for a homogeneous medium, being aware that the
results can provide only an average description of the attenuation properties in
the range from 10 to 80 km. The results of MLTWA analysis indicate
that the albedo for the area is fairly low, assuming a value of 0.5 at 1 Hz and
decreasing to 0.3 at 10 Hz. Then, the intrinsic absorption contributes equally
to scattering loss in determining the total attenuation at low frequencies, but
it becomes the dominant mechanism at high frequencies, suggesting that the coda
could be mainly generated by a back-scattering mechanism
(Menke and Chen, 1984). The
decrease in albedo with frequency has been previously observed in other
seismogenic regions, such as Japan
(Hoshiba, 1993), northern Chile
(Hoshiba et al., 2001),
southern central Alaska
(Dutta et al., 2004),
and southern Spain
(Akinci, Del Pezzo, and Ibanez 1995).
The total attenuation
over the range
10–80 km varies from about 0.018 at 1 Hz to 0.0024 at 10 Hz. For
frequencies less than 2 Hz,
is intermediate
between the values of
obtained for the
ranges 10–40 km and 60–80 km, while for higher frequencies,
is close to
obtained for the
range 60–80 km. The result of this comparison confirms that the total
attenuation obtained via the MLTWA analysis applied to a homogeneous
medium provides an average estimate underestimating the attenuation at shallow
depths. A first attempt to compare the observations with the results obtained by
applying the MLTWA method to a layered model have also been
performed. Even if the results suffer from the limits imposed by the
computational effort required, they confirm that some peculiarities are present
in the observations that can be ascribed to the variation of attenuation and
velocity with depth. Since several variables play a role in determining the
results of the MLTWA analysis, such as the number of layers and their
thickness, the velocity and attenuation of each layers, and so on, producing a
detailed regional model for the investigated area is a matter that deserves
future work, and the features appearing in the attenuation-with-distance curves
could be helpful in constraining such a model for the area. In conclusion, the
obtained spectral model for attenuation can be exploited to calibrate synthetic
attenuation relationships regressing ground-motion parameters predicted by
applying, for example, stochastic techniques.
| Appendix |
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|
|
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Manuscript received March 4, 2005
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