Seismic data acquisition
Acquisition of seismic exploration data involves the synthetic generation of
seismic waves, and their subsequent detection after passing through or reflecting
off the region of interest (i.e., the "target"). The most frequently practiced
form of seismic acquisition is the reflection seismic survey. A reflection
seismic survey typically involves generating hundreds to tens of thousands of
seismic source events, or shots, at different locations in the survey area. The
seismic energy generated by each shot is detected and recorded at a variety of
distances from the source location (Figure 3). The detectors used to transform
ground movement into an electrical voltage that can be recorded are geophones
and hydrophones, generically referred to as receivers. For every source event,
each receiver generates a seismogram or trace, which is a time series
representing the earth movement at the receiver location. Each trace has a
reference time zero corresponding to the time of its source event. A record of
all traces for each shot is usually written to a medium such as magnetic tape for
subsequent study, including processing, display and interpretation.
Figure 3: Geophones record the movement of the ground due to the propagation
of seismic energy as seismograms or seismic traces. Seismograms are freqently
displayed as "wiggle traces." (Click for larger figure.)
Precise relative and absolute positioning information must also be collected and
recorded for all source and receiver locations. This task has been greatly
simplified since the deployment of the Global Positioning Satellite (GPS)
constellation. Absolute source and receiver positions are usually known to
within five meters thanks to the availability of differential GPS techniques.
The relative distance between the source and receiver for each trace is its
offset.
Seismic reflection surveys are acquired in both land and marine environments.
Although the fundamental principles of the two survey types are the same, the
acquisition equipment and procedures differ by necessity. Moving-coil
electromagnetic geophones that sense vertical velocity are usually used as
receivers in land acquisition. The seismic source on land is usually either
dynamite planted in a borehole or Vibroseis, a vibrating mechanism mounted on
large trucks. Unlike dynamite, the Vibroseis signal is not impulsive, but rather
lasts from 7 to 40 seconds. To emit its signal, the
Vibroseis source sweeps through a range of frequencies from about 10 Hz to 60 Hz.
Because seismic reflectors in the earth are more closely spaced than the
length of the Vibroseis signal, the reflections in raw Vibroseis records
overlap, making raw Vibroseis data uninterpretable. A Vibroseis trace must be
processed to produce a replacement trace with a signal equivalent to that of an
impulsive source. This is accomplished by cross-correlating the raw seismogram
with the Vibroseis sweep.
Marine acquisition of seismic reflection data is generally accomplished using
large ships with multiple airgun arrays for sources. Airguns are deployed behind
the seismic vessel and generate a seismic signal by forcing highly pressurized
air into the water. Receivers are towed behind the ship in long streamers that
are several kilometers in length. Marine receivers are composed of piezoelectric
hydrophones, which respond to changes in water pressure. Being pressure
sensitive, hydrophones measure the acceleration of the medium as a seismic wave
passes through it, unlike geophones, which respond to the velocity of the
medium. Because of sensitivity and noise issues, responses from a group of 5 to
50 hydrophones are summed to produce a single seismogram, and the group is
considered a single receiver. Note that the equipment just described is generally
intended for probing subsurface depths of a few hundred meters to 10 kilometers.
Marine seismic acquisition is also performed for shallow hazard surveys using
smaller ships, higher frequency sources and much shorter hydrophone streamers,
frequently with only a single receiver group.
Until the 1980's, reflection seismic acquisition was carried out by arranging the
source and receivers in a line for a shot, then advancing the equipment along a
linear transit as necessary to complete the survey. Geographic and cultural
obstacles on the earth's surface frequently forced some deviation from this
idealize acquisition pattern, but the end result was usually the acquisition of
a 2-D seismic profile along a nearly linear transit. Since the mid-1980's,
improvements in computational power have made the acquisition and processing of
3-D seismic surveys a practical, though expensive, endeavor. Because geological
structures are three dimensional in nature, 3-D acquisition and processing are
usually desirable, or even necessary, to produce a proper representation of the
subsurface. As a result, most seismic surveys and the vast majority of seismic
data are now collected as 3-D surveys. The shift from 2-D acquisition to 3-D
acquisition has had operational consequences that have greatly changed the nature
of the seismic exploration industry. Because the facilities and equipment
necessary for modern acquisition are very expensive, most seismic surveying is
now carried out by a handful of large contracting companies. Because terabytes of
data are acquired in medium size surveys, most data processing is also performed
by contractors, and the client frequently only receives a processed and greatly
compressed seismic image volume as a product for use in interpretation.
Recent advances in acquisition technology are improving the quality and economics
of 3-D acquisition. In land acquisition, the logistics of deploying receiver
stations and cables are a significant expense, severely limiting the number of
receivers that can be deployed per shot. Thanks to advances in electronics, the
receiver signal is now commonly digitized at or near the receiver, and the data
are either recorded near the receiver stations during a survey, or transmitted to
a base station by radio or by fiber-optic cables. This improvement in data handling
makes it economical to deploy more receivers during a survey. In marine surveys,
the streamer mode of acquisition has traditionally allowed only nearly "in-line"
source-receiver azimuths and provided only limited angular raypath coverage of
the subsurface. Today, seismic vessels can deploy a number of streamers behind
the ship in parallel -- as many as 20 -- allowing the acquisition of a wider
azimuth of source-receiver offsets and making it possible to acquire more data in
a fixed amount of time. Another new development in marine acquisition is the
deployment of multiple vertical cables, each anchored at the seafloor bottom and
containing multiple receivers. As the source ship shoots around and over the
vertical cable deployment, data are acquired with multiple source-receiver offsets
and receivers at multiple depths. The variety of receiver depths beneath the water
surface makes the elimination of water surface multiples a simple task during
subsequent data processing.
An important subset of reflection seismology is multi-component seismology.
Multi-component seismic acquisition has recently been transformed by new
technological developments that have improved the practicality of marine
acquisition. In the solid earth, the
complete elastic wavefield is composed of both P-waves and S-waves and is a
vector quantity. Multi-component receivers that measure particle displacements in
three perpendicular orientations are necessary, therefore, to detect the full
elastic wavefield. In a marine environment, however, water cannot transmit shear
wave energy, so direct recording of multi-component information is not possible
using towed streamers. Marine multi-component acquisition is feasible using ocean
bottom seismograms (OBS's), but placing individual multi-component receivers on
the sea floor is time consuming and expensive. These practical constraints on
ocean bottom acquisition have recently been addressed by the development of
cables containing multi-component arrays that can be deployed on the sea floor
more economically. This advance in acquisition technique has been matched by the
recent appreciation of the importance of converted mode energy in reflection
seismology. Although marine seismic airguns generate only P-wave energy, some
portion of the P-wave energy is converted into S-wave energy as the direct wave
travels downward into the subsurface and encounters impedance boundaries. The
converted mode corresponding to conversion upon reflection from
down-going P-wave to up-going S-wave is sometimes referred to as the C-wave, and
is now known to have practical applications in exploration. Multi-component
seismic data are discussed further in the section on seismic interpretation.
In addition to reflection seismology, there are a number of other important
methods in seismic exploration. In refraction seismology, for each source event,
only the initial ground movement that arrives at each receiver is significant in
later analysis. This results in a data set of time versus source-receiver offset
for each shot. These first arrivals or head waves followed travel paths that were
refracted at the critical angle upon entering a high velocity layer. These travel
paths are predominately horizontal, and these data can be interpreted to reveal
the depths and seismic velocities of layers that support critical angle
refraction paths. (A refraction experiment can only observe a layer if its
seismic velocity is higher than all the velocities above the layer.) Because
refraction seismology only uses seismic energy that propagates through critical
angle travel paths, relatively large source-receiver offsets are required, and
the data analysis usually assumes a layered geology without structural
complications. In spite of these limitations, seismic refraction experiments are
useful for shallow engineering studies and for large scale crustal studies
-- depths that are generally too shallow or too deep for seismic reflection
surveys.
Another subset of exploration seismology is downhole seismology. Vertical seismic
profile (or VSP) surveying involves recording the responses of geophones in a
borehole or well for sources at the earth's surface. Likewise, a reverse VSP is
collected using a source in the borehole and receivers at the surface. A
crosshole survey measures the seismic responses of geophones in one borehole to a
source in another borehole. Downhole methods are especially useful for accurately
determining seismic P-wave and S-wave velocities since the distance of equipment
down the hole is a known value. (In the crosshole case, this implies analysis
using crosshole tomography.) Additionally, either the sources or receivers, or
both, are much closer to the target than in surface reflection acquisition, and
the seismic travel paths avoid at least one of two passes through the near
surface weathering zone. As a result, downhole data can be used to construct very
high-resolution images of the subsurface target region.
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