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Chapter 4

Interpretation of raw seismic
records

In this chapter some typical records as obtained on land and at sea are analysed. On land,
typically, events such as direct waves, refracted/head waves, surface waves and reflections
can directly be observed in records. From these events velocities and estimates of depths
can be obtained. At sea, typically, events such as direct waves, refracted/head waves,
reflections and multiple reflections can directly be observed in raw records. For both these
cases on land an at sea, a first model for the subsurface is estimated (where the model
is here seen as the first interpretation of the data). Using the Fourier transformation, a
filtering example is shown with the aim to separate different events in these raw records.



4.1     Introduction

As said in the last chapter, the goal of exploration seismics is obtaining structural subsur-
face information from seismic data. In the last chapter we discussed the elements which
do NOT say anything about the earth itself. Seismic processing concerns itself with re-
moving or compensating for the effects of waves that propagate through the earth such
that an image is obtained from the subsurface. In this chapter, we will concern ourselves
with what is ”signal” and what is ”noise”, with the interpretations of these two on seismic
records as recorded in the field. Next we discuss the possibilities to separate ”signal” and
”noise” and the possibilities to remove the ”noise”.



4.2     Seismic processing and imaging

Wave propagation versus signal to noise ratio
   In seismic processing we are going to manipulate our measured data, such that we




                                             66
obtain an accurate image of the subsurface. We can consider two ways of introducing
seismic processing to a newcomer.
    One is in terms of wave theory. We have to understand the physical processes that
are involved all the way from the seismic source, through the subsurface, to the seismic
recording instrument. We have to try to obtain only those features which are due to the
structure of the subsurface and not related to other features. For instance, we want to
know the source signal we put into the earth such that we can compensate for it from our
data later: the structure of the subsurface does not depend on the source we use. In this
way we can remove or suppress certain unwanted features in the image.
    Another way of introducing seismic processing to a newcomer is more in terms of the
image we obtain: signal-to-noise ratio and resolution. In order to see the image we need
to have at least a moderate signal-to-noise ratio. We would like this ratio to be as large as
possible by trying to suppress unwanted features in the final image. The other aspect of the
final seismic image is the resolution: we would like the image to be as crisp as possible. As
you may know, these two aspects cannot be seen separately. Usually, given a certain data
set, an increase in signal-to-noise ratio decreases the resolution (as information is stacked
together), and also an increase in resolution (by correctly incorporating wave theory) has
normally the consequence that the signal-to-noise ratio gets worse. In seismic processing
we would like to obtain the optimum between the two: a good, although not perfect,
signal-to-noise ratio with a good resolution.
    In these notes we take the view of trying to understand each process in the wave
problem, and try to find ways to cope with them. In this way we hope at least to increase
the signal-to-noise ratio, perhaps at some costs with respect to resolution. This is a very
important characteristic of raw seismic data: it has a very poor signal-to-noise ratio, and
it needs a lot of cleaning up before the image of the subsurface can be made visible. It is
along this line that we will discuss seismic processing: trying to understand the physical
processes. Sometimes, we will refer to the effect it can have on the total signal in terms
of signal-to-noise ratio and resolution.
    With seismic processing, we have many physical processes we have to take into account.
Actually, there are too many and this means that we must make simplifying assumptions.
First, we only look at reflected energy, not at critically refracted waves, direct body waves,
surface waves, etc. Of course, these types of waves contain much information of the
subsurface (e.g. the surface waves contain information of the upper layers) but these
waves are treated as noise. Also critically refracted waves contain useful information
about the subsurface. That information is indeed used indirectly in reflection seismics
via determining static corrections, but in the seismic processing itself, this information
is thrown away and thus treated as noise. Another important assumption in processing
is that the earth is not elastic, but acoustic. In conventional processing, we mostly look
at P-wave arrivals, and neglect any mode-conversion to S-waves, and even if we consider
S-waves, we do not include any conversions to P-waves. Some elastic-wave processing
is done in research environments, but are still very rarely used in production. Money is
better spent on 3-D ”P-wave” seismics, rather than on 2-D ”elastic” seismics; 3-D seismics




                                             67
with three-component sources and receivers are still prohibitively expensive in seismic data
acquisition.
    As said previously, the conventional way of processing is to obtain an image of the
primary P-wave reflectivity, so the image could be called the ”primary P-wave reflectivity
image”. All other arrivals/signals are treated as noise. As the name ”primary P-wave
reflectivity” suggests, multiples are treated as noise (as opposed to ”primaries”); S-wave
are treated as noise (as opposed to P-waves); refractions are treated as noise (as opposed
to reflectivity). Therefore, we can define the signal-to-noise ratio as:

      S   Signal       Primary P-wave Reflection Energy
        =        =                                                                      (4.1)
      N   Noise    All but Primary P-wave Reflection Energy

It can be seen now that processing of seismic data is to cancel out and/or remove all
the energy which is not primary P-wave reflectivity energy, and ”map” the reflectivity in
depth from the time-recordings made at the surface. In terms of total impulse response
of the earth G(x, y, t), we want to obtain that part of the impulse response of the earth
which is due to primary P-wave reflections:

                   Processing
      G(x, y, t)      →       Gprimary,P-wave,reflectivity (x, y, z)                     (4.2)

   In this chapter, we will look at the interpretation of raw seismic data as recorded in
the field, but then mainly to see which ”event” is interpreted as what, and therefore can
be categorized as being ”signal” (desired) or ”noise” (undesired).



4.3      Interpretation of some field seismic records

Land record
    Let us consider first a record, which has been recorded on land. In Figure 4.1 a field
recording is shown. The first event we are considering, is the ”first arrival”. It shows itself
by giving a pulse after a quiet period. This arrival is interpreted as a refraction which
we already discussed in a previous chapter. The velocity with which it propagates along
the surface is: 2400 meters in 500 ms = 4800 m/s. This is a relatively high velocity so is
probably some very hard rock. Below the record in figure 4.1, a simple model is shown
that explains this first arrival; the synthetic record belonging to this model, is given on
the top right of the figure.
    The next events we consider are the strong events which crosses 2400 meter at some
1.3 seconds. This event is interpreted as ground-roll or surface waves (they propagate
along the surface). Calculating the velocity, we come to 1850 m/s. Again, the simple
model below the record explains this ground roll; the synthetic record on the top right of
the figure also shows this arrival.




                                                68
offset (m)                                                                                             offset (m)
                 0   500     1000 1500               2000                                                            500           1000 1500 2000 2500
            0                                                               0
                                                                                                                                                   refrac
                                                                                                                                                         tion
           0.5                                                             0.5


           1.0                                                             1.0                                               reflection su
                                                                                                                                            rfa
                                                                                                                                                ce
                                                                                                                                                   wa
           1.5                                                             1.5                                                                        ve
                                                                                                                                 reflection




                                                                time (s)
time (s)




           2.0                                                             2.0


           2.5                                                             2.5


           3.0                                                             3.0




                                                                                                                                air w
                                                                                                                                   ave
           3.5                                                             3.5


           4.0

                                               offset
                       Source       air wave                                                                           velocity 340 m/s
                                                                            Detector
                                           surface wave
                                                                                                            thickness 10 m




                                           (velocity 1850 m/s)
                                                                                                                             velocity 2800 m/s
                                                                                                                             (P waves)




                                                refraction                                                                   velocity 4800 m/s


                                                offset
                           Source                                            Detector
                                                                                 thickness 2000 m thickness 1800 m




                                                                                                                              velocity 4800 m/s
                                                re
                                                  fle
                                                     ct
                                                        io
                                                          n




                                                                                                                               velocity 5000 m/s
                                                     re
                                                     fle
                                                        ct
                                                          io
                                                            n




Figure 4.1: Field seismic shot record from land survey (top left), its synthetic seismogram
(top right) using model of near surface (middle) and model at larger depths (bottom).




                                                                  69
Also in this field record, a ”high-frequency” event can be observed which goes through
the 4-seconds mark at about 1300 meters distance. Calculating the velocity from this, we
come to some 325 m/s. It may be clear that this is a wave that goes through the air. This
event is also synthesized in the top right figure, using the model as given below it.
    Last, but not least, are ”high-frequency” events which are slightly curved, e.g. the ones
at 0.9 and 1.6 seconds. These events are interpreted as reflections from layer boundaries
in the deep subsurface. Those are usually the events we are interested in, when we want
to obtain an image of the subsurface. Using a simple model as given at the bottom of the
figure (which explains the deeper part of the earth), the synthetic record for these events
is also shown in the top right of the figure.
    In the above, we have interpreted four types of events, which can be captured in one
combined model and are shown in one combined synthetic seismogram. These synthetics
explain the most important events in the raw seismic record. Still, when looking at the
resulting synthetic seismogram, we see that we are very over-simplifying the situation
since the synthetic and field record are only resembling in the arrival times of the most
important events. When looking at the general characteristics, they are very different
indeed.
    The field record we discussed so far, was recorded on some hard rocks where the
velocities are relatively high. However, when shooting data on land with some loose top
soil, the characteristics are much different. In Figure 4.2, a field record of such a situation
is given. Again, we can determine the main events in this record. Let us first consider the
”first arrival”, i.e. the arrival that is coming in first after a quiet period. As usual, this is
interpreted as a refraction as shown in the figure below the record. The velocity can be
determined: we come to some 1600 m/s. This velocity is very near the velocity of water,
so this refraction may be due to the water table. In the right figure, the synthetic shows
this arrival.
    The next event is the most prominent one, namely the event which goes through the
1-second mark at some 180m, so its velocity is around 180 m/s. This arrival is interpreted
as ”ground-roll”/surface waves, which travel along the surface. The model which explains
this arrival, is given again below the record, and its synthetic shown on the top right.
   The most important events for this record, are the ”high-frequency” events which are
the sightly curved arrivals, which can all be interpreted as reflections from deep layers.
The number of reflections are too many; only a few are synthesized in the record on the
top right, using the model as given at the bottom of the figure.
    Again, when comparing the synthetic to the field seismogram, it is obvious that we
have very over-simplified the earth; the positive side is that we have probably been able
to understand most of the events in the field record.




                                              70
offset (m)                                                                 offset (m)
                 100          200         300                                               100          200                 300
            0                                                            0


                                                                                                                     refracti
                                                                                                                             on


           0.5                                                          0.5
                                                                                                                  reflections
time (s)




                                                             time (s)
           1.0                                                          1.0




                                                                                                                  su
                                                                                                                     r
                                                                                                                   fac
                                                                                                                      ew
                                                                                                                        av
                                                                                                                         e
           1.5                                                          1.5




                                     offset
                   Source                                                     Detector
                                    direct surface wave
                                    (velocity 180 m/s)
                                                                                            velocity 600 m/s
                                                                                  5m




                                                                                            (P waves)




                                       refraction                                          velocity 1600 m/s


                                       offset
                       Source                                                  Detector
                                                                                   400 m




                                                                                              velocity 1600 m/s
                                         re
                                           fle
                                                ct
                                                    io
                                                      n



                                                                                               velocity 2000 m/s
                                                                                   180 m
                                        re
                                          fle
                                              ct
                                                io
                                                    n




                                          re
                                                                                   100 m




                                              fle
                                                 ct
                                                     io                                        velocity 2500 m/s
                                                         n




   Figure 4.2: Field seismic shot record from land survey with loose top soil (top left), its
   synthetic seismogram (top right) using model of near surface (middle) and model at larger
   depths (bottom).




                                                                    71
Marine record
   Figure 4.3 shows a raw seismic recordings, made at sea. This record is much ”cleaner”
than the land record, as we measure in a water layer, which is a good conductor for sound.
    Let us analyze some separate events again. The first event in the marine record is the
faint one, going nearly through the origin. It crosses the 500 meter at some 340 ms; this
means a velocity of some 1470 m/s. It may be clear that this is the direct arrival from
the source to the receivers through the water, as explained in the model below the record.
This direct arrival is thus a body wave, since it travels with the velocity of water.
    The next event is the first arrival at farther offsets; this arrival is interpreted as a
refractive event. When analyzing the distance travelled over time, i.e. the apparent
velocity, a velocity of roughly 2000 m/s is obtained. Using the results for a refraction in
the first chapter, a depth of 300 meter is obtained. This is quantified in the model below
the figure, and its associated synthetic seismogram in the figure on the top right.
    The third event we analyze is the first strong event that looks hyperbolic: starting
at some 0.4 seconds and bending down to some 2.2 seconds at 3200 m offset. Clearly,
because of its hyperbolic behaviour, it is interpreted as a reflection. When looking at later
times, we some more strong hyperbolic events, such as at 0.8 seconds (bending downward
toward some 2.3 seconds), and at 1.2 seconds (bending downwards toward 2.4 seconds),
and even more. These events are interpreted as so-called multiply reflected waves, i.e.,
waves that bounce up and down in the water layer. In fact almost all events we see below
0.8 seconds are due to multiply reflected waves, or short-hand: multiples. The times at
which the multiply reflected waves arrive, seem to be periodic; this is indeed the case. A
simple model explaining these events, is shown in the figure below the record, with a water
layer of 300 meter. The resulting synthetic seismogram is shown on the top right of the
figure. It may be clear that the multiply reflected waves come from the same reflective
boundary in the subsurface, namely the sea bottom (and the sea surface, of course), and
are therefore superfluous. They are considered as noise, the only one being ”signal” is the
one at around 0.4 seconds.




                                            72
offset (m)                                            offset (m)
                 500 1000 1500 2000 2500 3000                          500 1000 1500 2000 2500 3000
            0                                                     0
                                                                       di
                                                                         re
                                                                             ct

           0.5                                                   0.5
                                                                        re
                                                                            fle
                                                                                  cti
                                                                                     on
           1.0                                                   1.0          mu
                                                                                    ltip
                                                                                          le
                                                                                               re
                                                                                                 fle
                                                                                                      cti                  re
                                                                                                           on                fra
           1.5                                                   1.5                       mu                                   cti
                                                                                                                                   on
                                                                                                    ltip
                                                                                                        le
                                                                                                             re
                                                                                                                fle




                                                      time (s)
time (s)




                                                                                                                   cti
           2.0                                                   2.0                                                  on



           2.5                                                   2.5


           3.0                                                   3.0


           3.5                                                   3.5


           4.0




                                        offset
 Source                                                                                    Detector
                  direct body wave
                                              m
                                                 ul
                                                 tip




                                                                                                             velocity 1470 m/s
                                                  le




                                                                                                300 m
                                                      re
                                                        fle




                               ref
                                  lec
                                                            ct




                                     tio
                                                               io




                                          n
                                                                  n




                                              refraction                                                        velocity 2000 m/s



Figure 4.3: Seismic shot record from marine survey (top left), its synthetic seismogram
(top right) using model of water layer and sea-water bottom, where only the path of one
multiple reflection is drawn (bottom).




                                                        73
4.4     Spectral analysis and filtering of field seismic records


In the previous section, we analyzed the data as they are recorded in the field. However, we
only looked at the data as a function of time, not of frequency. When we look at the data of
the previous section in more detail, we see that the events have a wavelength which differs
for the type of event. In particular, let us consider the data from figure 4.2. The surface
wave has a longer waveshape (lower-frequency) than the reflections and refractions; in the
modelling we already took account of this, as can be seen in the synthetic seismogram on
the top right of the figure. Also in the other land record, figure 4.1, a difference in length
of waveshape can be observed. The surface wave has also here a longer waveshape than
the reflections. The event with even another length of waveshape is the air wave. It has
a very ”high-frequency” shape.
    It may now be clear that when we make spectra of these data, i.e., transform the time-
axis to a frequency axis using the Fourier transformation, that different arrivals will give
different peaks in the Fourier spectra. What we achieve is that we can analyze and interpret
different frequencies in terms of different events. Moreover, we can start thinking about
using the Fourier-transformed data for filtering purposes, i.e., removing certain frequency
bands with the aim to remove undesired signal, like, e.g. the surface wave. Let us look at
some spectra.
    In figure 4.4, we have selected only 3 traces to illustrate our points. On the left of the
figure, we plotted the 3 traces as a function of time; we can still observe the first arrival
and the surface wave, which is characterized by its long waveshape. In the plot next to it,
we have plotted the amplitude spectra of these 3 traces. First of all, notice that we obtain
frequencies up to 500 Hz, which is the Nyquist frequency f N = 1/(2∆t), associated with
the sampling interval: ∆t = 1 ms. Next, it is evident that the largest amplitudes occur
at the low frequencies, i.e., around 10 to 15 Hz. It may be clear that these frequencies
are associated with the surface wave. Finally, it is not clear from the amplitude spectra
where the reflection information is; when we look at the whole record we would expect it
to be at higher frequencies.
    Let us now filter the data, i.e., make the amplitudes zero at certain frequencies. Since
we are not interested in the surface waves, we can make the amplitudes zero at the low
frequencies. This is done in the next plot; notice that the plot is scaled to the maximum
of the spectrum, so now other amplitudes become visible. When we transform this data
back to the time domain, we obtain the rightmost plot. We see that we have effectively
removed the surface wave.
    From this plot, we cannot see whether we have changed the character of the whole
record. To that end, all the traces of the original field record have been filtered with the
same filter as we did for the 3 traces, and the result before and after filtering is shown in
figure 4.5. What we can now see is that the surface wave is indeed pretty well removed,
although not completely, and that the reflection are hardly affected. We can now even see
the reflections that were masked by the surface wave before we did any filtering.




                                             74
It may now be clear that we have removed the most important ”noise” in the field
record. Before we did the filtering, we had a signal-to-noise ration which was well below
1; after filtering the signal-to-noise ratio is larger than 1 since the highest amplitudes now
seem to be the reflections themselves. What is important to realize is that, using the
Fourier transformation, we have obtained a method to separate the surface waves from the
reflections. In the time-domain, the surface waves crossed the reflections and therefore we
could not make the ”time”-amplitudes of the surface wave zero: we would then also have
removed part of the reflections.
    In this example, we have shown the power of filtering via analysis of Fourier-transformed
data. This has solved one problem, namely the one of surface waves. However, many cases
exist where such a filtering is partly successfull, and other types of filters are necessary. In
the case of multiple reflections, as seen in the marine record (figure 4.3), transforming the
time axis to a frequency axis does not solve anything since the multiple reflections have
the same frequency contents as the primary reflections: we cannot achieve a separation
between ”signal” (primaries) and ”noise” (multiples), so filtering cannot help us here.




                                             75
distance (m)                           distance (m)                          distance (m)                    distance (m)
                  100 300                                100 300                               100 300                         100 300
            0                                      0                                     0                               0


                                                   50                                    50


                                                  100                                   100
           0.5                                                                                                          0.5
                                                  150                                   150


                                                  200                                   200
                                 frequency (Hz)




                                                                       frequency (Hz)
time (s)




                                                                                                             time (s)
           1.0                                    250                                   250                             1.0


                                                  300                                   300


                                                  350                                   350
           1.5                                                                                                          1.5
                                                  400                                   400


                                                  450                                   450


                                                  500                                   500



                   Figure 4.4: 3 seismic traces from raw seismic field record for analysis. From left to right:
                   3 original traces; amplitude spectra from Fourier-transformed traces; amplitude spectra
                   from Fourier-transformed filtered traces; filtered traces.




                                                                           76
offset (m)                                       offset (m)
                 100          200   300                           100          200   300
            0                                                0




           0.5                                              0.5
time (s)




           1.0                                   time (s)   1.0




           1.5                                              1.5




Figure 4.5: Seismic shot record from land survey with loose top soil. Original record (left)
and record after removing low frequencies (right).




                                            77

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Seismic Data Interpretation

  • 1. Chapter 4 Interpretation of raw seismic records In this chapter some typical records as obtained on land and at sea are analysed. On land, typically, events such as direct waves, refracted/head waves, surface waves and reflections can directly be observed in records. From these events velocities and estimates of depths can be obtained. At sea, typically, events such as direct waves, refracted/head waves, reflections and multiple reflections can directly be observed in raw records. For both these cases on land an at sea, a first model for the subsurface is estimated (where the model is here seen as the first interpretation of the data). Using the Fourier transformation, a filtering example is shown with the aim to separate different events in these raw records. 4.1 Introduction As said in the last chapter, the goal of exploration seismics is obtaining structural subsur- face information from seismic data. In the last chapter we discussed the elements which do NOT say anything about the earth itself. Seismic processing concerns itself with re- moving or compensating for the effects of waves that propagate through the earth such that an image is obtained from the subsurface. In this chapter, we will concern ourselves with what is ”signal” and what is ”noise”, with the interpretations of these two on seismic records as recorded in the field. Next we discuss the possibilities to separate ”signal” and ”noise” and the possibilities to remove the ”noise”. 4.2 Seismic processing and imaging Wave propagation versus signal to noise ratio In seismic processing we are going to manipulate our measured data, such that we 66
  • 2. obtain an accurate image of the subsurface. We can consider two ways of introducing seismic processing to a newcomer. One is in terms of wave theory. We have to understand the physical processes that are involved all the way from the seismic source, through the subsurface, to the seismic recording instrument. We have to try to obtain only those features which are due to the structure of the subsurface and not related to other features. For instance, we want to know the source signal we put into the earth such that we can compensate for it from our data later: the structure of the subsurface does not depend on the source we use. In this way we can remove or suppress certain unwanted features in the image. Another way of introducing seismic processing to a newcomer is more in terms of the image we obtain: signal-to-noise ratio and resolution. In order to see the image we need to have at least a moderate signal-to-noise ratio. We would like this ratio to be as large as possible by trying to suppress unwanted features in the final image. The other aspect of the final seismic image is the resolution: we would like the image to be as crisp as possible. As you may know, these two aspects cannot be seen separately. Usually, given a certain data set, an increase in signal-to-noise ratio decreases the resolution (as information is stacked together), and also an increase in resolution (by correctly incorporating wave theory) has normally the consequence that the signal-to-noise ratio gets worse. In seismic processing we would like to obtain the optimum between the two: a good, although not perfect, signal-to-noise ratio with a good resolution. In these notes we take the view of trying to understand each process in the wave problem, and try to find ways to cope with them. In this way we hope at least to increase the signal-to-noise ratio, perhaps at some costs with respect to resolution. This is a very important characteristic of raw seismic data: it has a very poor signal-to-noise ratio, and it needs a lot of cleaning up before the image of the subsurface can be made visible. It is along this line that we will discuss seismic processing: trying to understand the physical processes. Sometimes, we will refer to the effect it can have on the total signal in terms of signal-to-noise ratio and resolution. With seismic processing, we have many physical processes we have to take into account. Actually, there are too many and this means that we must make simplifying assumptions. First, we only look at reflected energy, not at critically refracted waves, direct body waves, surface waves, etc. Of course, these types of waves contain much information of the subsurface (e.g. the surface waves contain information of the upper layers) but these waves are treated as noise. Also critically refracted waves contain useful information about the subsurface. That information is indeed used indirectly in reflection seismics via determining static corrections, but in the seismic processing itself, this information is thrown away and thus treated as noise. Another important assumption in processing is that the earth is not elastic, but acoustic. In conventional processing, we mostly look at P-wave arrivals, and neglect any mode-conversion to S-waves, and even if we consider S-waves, we do not include any conversions to P-waves. Some elastic-wave processing is done in research environments, but are still very rarely used in production. Money is better spent on 3-D ”P-wave” seismics, rather than on 2-D ”elastic” seismics; 3-D seismics 67
  • 3. with three-component sources and receivers are still prohibitively expensive in seismic data acquisition. As said previously, the conventional way of processing is to obtain an image of the primary P-wave reflectivity, so the image could be called the ”primary P-wave reflectivity image”. All other arrivals/signals are treated as noise. As the name ”primary P-wave reflectivity” suggests, multiples are treated as noise (as opposed to ”primaries”); S-wave are treated as noise (as opposed to P-waves); refractions are treated as noise (as opposed to reflectivity). Therefore, we can define the signal-to-noise ratio as: S Signal Primary P-wave Reflection Energy = = (4.1) N Noise All but Primary P-wave Reflection Energy It can be seen now that processing of seismic data is to cancel out and/or remove all the energy which is not primary P-wave reflectivity energy, and ”map” the reflectivity in depth from the time-recordings made at the surface. In terms of total impulse response of the earth G(x, y, t), we want to obtain that part of the impulse response of the earth which is due to primary P-wave reflections: Processing G(x, y, t) → Gprimary,P-wave,reflectivity (x, y, z) (4.2) In this chapter, we will look at the interpretation of raw seismic data as recorded in the field, but then mainly to see which ”event” is interpreted as what, and therefore can be categorized as being ”signal” (desired) or ”noise” (undesired). 4.3 Interpretation of some field seismic records Land record Let us consider first a record, which has been recorded on land. In Figure 4.1 a field recording is shown. The first event we are considering, is the ”first arrival”. It shows itself by giving a pulse after a quiet period. This arrival is interpreted as a refraction which we already discussed in a previous chapter. The velocity with which it propagates along the surface is: 2400 meters in 500 ms = 4800 m/s. This is a relatively high velocity so is probably some very hard rock. Below the record in figure 4.1, a simple model is shown that explains this first arrival; the synthetic record belonging to this model, is given on the top right of the figure. The next events we consider are the strong events which crosses 2400 meter at some 1.3 seconds. This event is interpreted as ground-roll or surface waves (they propagate along the surface). Calculating the velocity, we come to 1850 m/s. Again, the simple model below the record explains this ground roll; the synthetic record on the top right of the figure also shows this arrival. 68
  • 4. offset (m) offset (m) 0 500 1000 1500 2000 500 1000 1500 2000 2500 0 0 refrac tion 0.5 0.5 1.0 1.0 reflection su rfa ce wa 1.5 1.5 ve reflection time (s) time (s) 2.0 2.0 2.5 2.5 3.0 3.0 air w ave 3.5 3.5 4.0 offset Source air wave velocity 340 m/s Detector surface wave thickness 10 m (velocity 1850 m/s) velocity 2800 m/s (P waves) refraction velocity 4800 m/s offset Source Detector thickness 2000 m thickness 1800 m velocity 4800 m/s re fle ct io n velocity 5000 m/s re fle ct io n Figure 4.1: Field seismic shot record from land survey (top left), its synthetic seismogram (top right) using model of near surface (middle) and model at larger depths (bottom). 69
  • 5. Also in this field record, a ”high-frequency” event can be observed which goes through the 4-seconds mark at about 1300 meters distance. Calculating the velocity from this, we come to some 325 m/s. It may be clear that this is a wave that goes through the air. This event is also synthesized in the top right figure, using the model as given below it. Last, but not least, are ”high-frequency” events which are slightly curved, e.g. the ones at 0.9 and 1.6 seconds. These events are interpreted as reflections from layer boundaries in the deep subsurface. Those are usually the events we are interested in, when we want to obtain an image of the subsurface. Using a simple model as given at the bottom of the figure (which explains the deeper part of the earth), the synthetic record for these events is also shown in the top right of the figure. In the above, we have interpreted four types of events, which can be captured in one combined model and are shown in one combined synthetic seismogram. These synthetics explain the most important events in the raw seismic record. Still, when looking at the resulting synthetic seismogram, we see that we are very over-simplifying the situation since the synthetic and field record are only resembling in the arrival times of the most important events. When looking at the general characteristics, they are very different indeed. The field record we discussed so far, was recorded on some hard rocks where the velocities are relatively high. However, when shooting data on land with some loose top soil, the characteristics are much different. In Figure 4.2, a field record of such a situation is given. Again, we can determine the main events in this record. Let us first consider the ”first arrival”, i.e. the arrival that is coming in first after a quiet period. As usual, this is interpreted as a refraction as shown in the figure below the record. The velocity can be determined: we come to some 1600 m/s. This velocity is very near the velocity of water, so this refraction may be due to the water table. In the right figure, the synthetic shows this arrival. The next event is the most prominent one, namely the event which goes through the 1-second mark at some 180m, so its velocity is around 180 m/s. This arrival is interpreted as ”ground-roll”/surface waves, which travel along the surface. The model which explains this arrival, is given again below the record, and its synthetic shown on the top right. The most important events for this record, are the ”high-frequency” events which are the sightly curved arrivals, which can all be interpreted as reflections from deep layers. The number of reflections are too many; only a few are synthesized in the record on the top right, using the model as given at the bottom of the figure. Again, when comparing the synthetic to the field seismogram, it is obvious that we have very over-simplified the earth; the positive side is that we have probably been able to understand most of the events in the field record. 70
  • 6. offset (m) offset (m) 100 200 300 100 200 300 0 0 refracti on 0.5 0.5 reflections time (s) time (s) 1.0 1.0 su r fac ew av e 1.5 1.5 offset Source Detector direct surface wave (velocity 180 m/s) velocity 600 m/s 5m (P waves) refraction velocity 1600 m/s offset Source Detector 400 m velocity 1600 m/s re fle ct io n velocity 2000 m/s 180 m re fle ct io n re 100 m fle ct io velocity 2500 m/s n Figure 4.2: Field seismic shot record from land survey with loose top soil (top left), its synthetic seismogram (top right) using model of near surface (middle) and model at larger depths (bottom). 71
  • 7. Marine record Figure 4.3 shows a raw seismic recordings, made at sea. This record is much ”cleaner” than the land record, as we measure in a water layer, which is a good conductor for sound. Let us analyze some separate events again. The first event in the marine record is the faint one, going nearly through the origin. It crosses the 500 meter at some 340 ms; this means a velocity of some 1470 m/s. It may be clear that this is the direct arrival from the source to the receivers through the water, as explained in the model below the record. This direct arrival is thus a body wave, since it travels with the velocity of water. The next event is the first arrival at farther offsets; this arrival is interpreted as a refractive event. When analyzing the distance travelled over time, i.e. the apparent velocity, a velocity of roughly 2000 m/s is obtained. Using the results for a refraction in the first chapter, a depth of 300 meter is obtained. This is quantified in the model below the figure, and its associated synthetic seismogram in the figure on the top right. The third event we analyze is the first strong event that looks hyperbolic: starting at some 0.4 seconds and bending down to some 2.2 seconds at 3200 m offset. Clearly, because of its hyperbolic behaviour, it is interpreted as a reflection. When looking at later times, we some more strong hyperbolic events, such as at 0.8 seconds (bending downward toward some 2.3 seconds), and at 1.2 seconds (bending downwards toward 2.4 seconds), and even more. These events are interpreted as so-called multiply reflected waves, i.e., waves that bounce up and down in the water layer. In fact almost all events we see below 0.8 seconds are due to multiply reflected waves, or short-hand: multiples. The times at which the multiply reflected waves arrive, seem to be periodic; this is indeed the case. A simple model explaining these events, is shown in the figure below the record, with a water layer of 300 meter. The resulting synthetic seismogram is shown on the top right of the figure. It may be clear that the multiply reflected waves come from the same reflective boundary in the subsurface, namely the sea bottom (and the sea surface, of course), and are therefore superfluous. They are considered as noise, the only one being ”signal” is the one at around 0.4 seconds. 72
  • 8. offset (m) offset (m) 500 1000 1500 2000 2500 3000 500 1000 1500 2000 2500 3000 0 0 di re ct 0.5 0.5 re fle cti on 1.0 1.0 mu ltip le re fle cti re on fra 1.5 1.5 mu cti on ltip le re fle time (s) time (s) cti 2.0 2.0 on 2.5 2.5 3.0 3.0 3.5 3.5 4.0 offset Source Detector direct body wave m ul tip velocity 1470 m/s le 300 m re fle ref lec ct tio io n n refraction velocity 2000 m/s Figure 4.3: Seismic shot record from marine survey (top left), its synthetic seismogram (top right) using model of water layer and sea-water bottom, where only the path of one multiple reflection is drawn (bottom). 73
  • 9. 4.4 Spectral analysis and filtering of field seismic records In the previous section, we analyzed the data as they are recorded in the field. However, we only looked at the data as a function of time, not of frequency. When we look at the data of the previous section in more detail, we see that the events have a wavelength which differs for the type of event. In particular, let us consider the data from figure 4.2. The surface wave has a longer waveshape (lower-frequency) than the reflections and refractions; in the modelling we already took account of this, as can be seen in the synthetic seismogram on the top right of the figure. Also in the other land record, figure 4.1, a difference in length of waveshape can be observed. The surface wave has also here a longer waveshape than the reflections. The event with even another length of waveshape is the air wave. It has a very ”high-frequency” shape. It may now be clear that when we make spectra of these data, i.e., transform the time- axis to a frequency axis using the Fourier transformation, that different arrivals will give different peaks in the Fourier spectra. What we achieve is that we can analyze and interpret different frequencies in terms of different events. Moreover, we can start thinking about using the Fourier-transformed data for filtering purposes, i.e., removing certain frequency bands with the aim to remove undesired signal, like, e.g. the surface wave. Let us look at some spectra. In figure 4.4, we have selected only 3 traces to illustrate our points. On the left of the figure, we plotted the 3 traces as a function of time; we can still observe the first arrival and the surface wave, which is characterized by its long waveshape. In the plot next to it, we have plotted the amplitude spectra of these 3 traces. First of all, notice that we obtain frequencies up to 500 Hz, which is the Nyquist frequency f N = 1/(2∆t), associated with the sampling interval: ∆t = 1 ms. Next, it is evident that the largest amplitudes occur at the low frequencies, i.e., around 10 to 15 Hz. It may be clear that these frequencies are associated with the surface wave. Finally, it is not clear from the amplitude spectra where the reflection information is; when we look at the whole record we would expect it to be at higher frequencies. Let us now filter the data, i.e., make the amplitudes zero at certain frequencies. Since we are not interested in the surface waves, we can make the amplitudes zero at the low frequencies. This is done in the next plot; notice that the plot is scaled to the maximum of the spectrum, so now other amplitudes become visible. When we transform this data back to the time domain, we obtain the rightmost plot. We see that we have effectively removed the surface wave. From this plot, we cannot see whether we have changed the character of the whole record. To that end, all the traces of the original field record have been filtered with the same filter as we did for the 3 traces, and the result before and after filtering is shown in figure 4.5. What we can now see is that the surface wave is indeed pretty well removed, although not completely, and that the reflection are hardly affected. We can now even see the reflections that were masked by the surface wave before we did any filtering. 74
  • 10. It may now be clear that we have removed the most important ”noise” in the field record. Before we did the filtering, we had a signal-to-noise ration which was well below 1; after filtering the signal-to-noise ratio is larger than 1 since the highest amplitudes now seem to be the reflections themselves. What is important to realize is that, using the Fourier transformation, we have obtained a method to separate the surface waves from the reflections. In the time-domain, the surface waves crossed the reflections and therefore we could not make the ”time”-amplitudes of the surface wave zero: we would then also have removed part of the reflections. In this example, we have shown the power of filtering via analysis of Fourier-transformed data. This has solved one problem, namely the one of surface waves. However, many cases exist where such a filtering is partly successfull, and other types of filters are necessary. In the case of multiple reflections, as seen in the marine record (figure 4.3), transforming the time axis to a frequency axis does not solve anything since the multiple reflections have the same frequency contents as the primary reflections: we cannot achieve a separation between ”signal” (primaries) and ”noise” (multiples), so filtering cannot help us here. 75
  • 11. distance (m) distance (m) distance (m) distance (m) 100 300 100 300 100 300 100 300 0 0 0 0 50 50 100 100 0.5 0.5 150 150 200 200 frequency (Hz) frequency (Hz) time (s) time (s) 1.0 250 250 1.0 300 300 350 350 1.5 1.5 400 400 450 450 500 500 Figure 4.4: 3 seismic traces from raw seismic field record for analysis. From left to right: 3 original traces; amplitude spectra from Fourier-transformed traces; amplitude spectra from Fourier-transformed filtered traces; filtered traces. 76
  • 12. offset (m) offset (m) 100 200 300 100 200 300 0 0 0.5 0.5 time (s) 1.0 time (s) 1.0 1.5 1.5 Figure 4.5: Seismic shot record from land survey with loose top soil. Original record (left) and record after removing low frequencies (right). 77