David Boore has written many papers related to strong ground
motion and also developed a set of
computer programs to support his research. His home page giving publications, computer
codes and lectures is https://www.daveboore.com/ore.com/. The SMSIM (stochastic-method simulation) package is widely used.
Originally included in this package was a program to estimate
site-amplification through the use of the quarter-wavelength
approximation
[Boore, D.M. and L.T. Brown (1998).
Comparing shear-wave velocity profiles from inversion of
surface-wave phase velocities with downhole measurements:
Systematic differences between the CXW method and downhole
measurements at six USC strong-motion sites, Seismol.
Research Letters 69, 222-229. (778 Kb)]
Although the SiteAmp code is distributed separately from the current SMSIM package, the site_amp.for (dated Aug 13, 2001) is used here to check the CPS sacampl program.
This program uses a velocity model in the MDOEL96 format of
Computer Programs in Seismology and command line arguments.
For the current version the response is computed at frequencies
between 0.1 and 20Hz at increments of 0.1Hz. The command sequence
is
Usage: sacamp -M model [-P | -S ] [-A angdeg | -AYPay_parameter] [-TXT] [-?] [-h]
-M model (default none ) Earth model file
-P (default false ) P response
-S (default true ) S response
-A angdeg (default none ) S angle incidence at base
-RAYP ray_parameter (default none) (s/km) if model in km
NOTE: Either the angle or the ray parameter is required
-TXT (default false) Output in file sacamp.txt
-? (default none ) this help message
-h (default none ) this help message
The default output will be two Sac binary amplitude spectra files named AMP.sac.am and KAMP.sac.am. The first file contains the quarter-wavelength site effect. The second is the first multiplied by the site attenuation factor [ -
The table gives the data files and command sequence to run the
two programs. SITE_AMP has a interactive input while sacampl
is controlled form the command line.
site_amp |
sacampl |
Model |
|
t_amp.dat:Sample input file to site_amp |
soil.mod:MODEL.01 |
Execution | |
SITE_AMP |
sacampl -M soil.mod -S -A 10 -TXT |
The site_amp creates the file t.txt while sacampl
creates the Sac files AMP.sac.am and KAMP.sac.am
and the text file sacampl.txt. Here we
compare selected columns (13,14,16) of the site_amp output
to the sacampl.txt. Note for this comparison the sacampl.txt
has been sorted in terms of decreasing frequency. The columns
display the frequency, site site amplification without Q
attenuation, and the effective amplification that includes
the Q effect of the entire column, e.g., column 2 multiplied
by ( -
.
Incident
angle of 10 degrees |
|
site_amp |
sacampl |
t_amp-f t_amp-a t_ampak |
Freq(Hz) Amp Amp(kappa) |
The site amplification is based on the velocity density model.
The kappa effect is for the entire column from the base of the
model upward. The comparison for an S-wave incident at an
angle of 10 degrees is quite good. For an incidence angle of 45
degrees, the comparison is now
Incident
angle of 45 degrees |
|
site_amp |
sac_amp |
t_amp-f t_amp-a t_ampak |
Freq(Hz) Amp Amp(kappa) |
Here there are slight differences at frequencies less than
5Hz.
The comparison give confidence in the sacampl program.
The reason for writing this program was to be able to have the
site amplification in the format of a Sac file and to use the
same velocity model format as used in the execution of
synthetic seismogram codes of Computer Programs in
Seismology. In the examples that follow this site
amplification is compared to plane-wave synthetics and complete
wavenumber integration synthetics. To emulate the site
amplification response, the computations are based on two set of
models: a halfspace to represent the hard rock site, and the same
model with a thin veneer of low velocity materials to represent a
soil site. The procedure will be to compute Green's functions at
the surface of the two models, compute the Fourier amplitude
spectra, and then to form the ratio of spectra at the soil site to
the hard rock site. These will be compared to the sacampl prediction.
The computations that follow require the March, 2024 release of
Computer Programs in Seismology which now better supports the
Amplitude spectra format of Sac files by gsac.
This program was written very quickly. As such there may be some
differences with respect to the results of site_amp. For
the simple comparison made above, these differences do not seem
significant.
The comparison of the site response estimation using synthetics
shows that the SH response is similar to that given by sacampl.
The surprising results is the large radial component
amplification.
As remarked in the plane-wave study for large angles of incidence, and as seen in the time domain study at large distances, for which the angle of incidence is large, the site effect of the radial component because very large. As a matter of fact at an epicentral distance of 20 km, angle of incidence of 63o the radial ratio is very large at a frequency of 3 Hz. The surface wave approach show a large resonance at about 4 Hz. The surface-wave study indicates the importance of the radial ellipticity, but cannot include the tempering factors of attenuation which will reduce the level at high frequencies.
The output of
sacampl may be useful as a first approximation of site amplification. Since it is run from the command line, it would be easy to loop through different velocity models in a bath processing environment.
The only caveat here is that the site response of the Fourier amplification and not the Response Spectra amplification
.