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3D Resistivity Imaging
Technique
By:
Zaidoon Taha Abdulrazzaq
Introduction to 3-D surveys
The earth often shows three-dimensional characteristics, which can limit a 2D
interpretation. As multi-electrode systems were developing rapidly, e.g., by the use of
multichannel recorders, it became more and more interesting to carry out
measurements allowing for a three-dimensional reconstruction. There are two current
developments that should make 3D surveys more cost-effective option in the near future.
One is the development of multi-channel resistivity meters that enable more than one
reading to be taken at a single time. This is important to reduce the survey time.
The second development is faster microcomputers to enable the inversion of very large
data sets (with more than 8,000 data points and survey grids of greater than 30 by 30) to
be completed within a reasonable time (Loke, 2014).
Theory of 3D Electrical Resistivity
Tomography
The theory of 3D electrical resistivity tomography is consistent with the common
electrical method that conductive of underground material differences as the
prerequisite, make underground is full of electricity and observe of subsurface electric
field distribution, so as to solve different geological problems.
Compared with 3D electrical resistivity tomography the 2D high-density electrical
resistivity tomography still exist some problems: when the survey line doesn’t layout in
the hidden the underground objects cannot be reflected, which brought difficulty in
field test and there is more difficult to detect complex leakage channels especially;
Accuracy also have difference by using several 2D cross sections at the same time in an
interface to open for forming a quasi 3D images between obtained true 3D images after
3D inversion
The 3D inversion divided the subsurface into a number of small
rectangular to build geoelectric model [8], and give the initial value of each
small rectangle, the resistivity value of each small rectangular volume is
obtained by forward calculation, then use the least square method to
compare the theoretical value and the measured value to adjust the
resistivity of each sub block [9] [10]. Establish objective function F:
Where: ρm is the measured resistivity value of the profile; ρt is the theoretical
resistivity value of the initial model.
Comparing the accuracy between the measured resistivity value and the theoretical
value to determine the results of the inversion calculation if it meets the requirements.
When the requirements don’t meet, it is required to recalculate the theoretical value
until the difference is in the proper range.
Array types for 3-D surveys
The pole-pole, pole-dipole and dipole-
dipole arrays are frequently used for 3-D
surveys. Because of other arrays have poorer
data coverage near the edges of the survey grid.
1. The pole-pole array
In the figure, one possible arrangement of the
electrodes for a 3-D survey using a multi-electrode
system with 25 nodes. For convenience the
electrodes are usually arranged in a square grid
with the same unit electrode spacing in the x and y
directions. To map slightly elongated bodies, a
rectangular grid with different numbers of
electrodes and spacings in the x and y directions
could be used. The pole-pole electrode
configuration was commonly used for 3-D surveys,
such as the E-SCAN method (Li and Oldenburg,
1992; Ellis and Oldenburg, 1994b). The maximum
number of independent measurements, nmax, that
can be made with ne electrodes is given by
nmax = ne (ne -1) / 2
Two possible measurement sequences for a 3-D survey. The location of potential electrodes corresponding to a
single current electrode in the arrangement used by (a) a survey to measure the complete data set and (b) a cross-
diagonal survey.
This array is an attractive alternative to the pole-pole array
for surveys with medium and large survey grids (12 by 12 and
above). It has a better resolving power than the pole-pole array
(Sasaki, 1992), and is less susceptible to telluric noise since
both potential electrodes are kept within the survey grid.
Compared to the dipole-dipole array, it has a significantly
stronger signal strength. Although it has one “remote”
electrode (the C2 electrode), the effect of this electrode on the
measurements is much smaller compared to the pole-pole
array.
2.The pole-dipole array
3.The dipole-dipole
The dipole-dipole array can be recommended only
for grids that are larger than 12 by 12 due to the poorer
horizontal data coverage at the sides. The main problem
that is likely to be faced with this array is the
comparatively low signal strength. Similar to 2-D surveys,
this problem can be overcome by increasing the “a”
spacing between the P1-P2 dipole to get a deeper depth of
investigation as the distance between the C1-C2 and P1-P2
dipoles is increased. Also, the use of overlapping data
levels is recommended.
Summary of array types
• For relatively small grids of less than 12 by 12 electrodes, the pole-pole array has a substantially
larger number of possible independent measurements compared to other arrays. The loss of data
points near the sides of the grid is kept to a minimum, and it provides better horizontal data coverage
compared to other arrays. This is an attractive array for small survey grids with relatively small spacings
(less than 5 meters) between the electrodes. However, it has the disadvantage of requiring two
“remote” electrodes that must be placed at a sufficiently large distance from the survey grid.
• The pole-dipole array is an attractive option for medium size grids. It has a higher resolution than
the pole-pole array and it requires only one remote electrode and is much less sensitive to telluric
noise. For surveys with large grids, particularly when there is no convenient location for a remote
electrode, the dipole-dipole array can be used. The electrodes for 3-D surveys are frequently
arranged in a rectangular grid. However, the RES3DINV resistivity and I.P. inversion program can
also handle survey layouts with an arbitrary distribution of the electrodes.
In large 3-D I.P. surveys, it has become popular to use the offset version of the pole-dipole and
dipole-dipole arrays to cover a large area rapidly. The C1 current electrode (or C1-C2 current dipole) is
placed on a separate line parallel to the line with the potential receivers.
Sensitivity
Dipole-dipole : The sensitivity values have small but negative values
outside the immediate vicinity of the array. Another interesting feature
is that the sensitivity contours tend to be elongated in the y-direction,
particularly for the larger “n” value. The 4 unit sensitivity contour
extends to about 0.6 times the array length in the y-direction, or about
1.8 times the unit electrode spacing. This means that the array is more
sensitive to structures off the array axis compared to the pole-pole and
pole-dipole arrays. This feature is troublesome in 2-D surveys, but
might be advantageous in 3-D surveys.
The off-axis elongation of the sensitivity contours agrees with the
observation by Dahlin and Loke (1997) that the dipole-dipole array is
more sensitive to 3-D effects compared to other common arrays. This
factor is important when the dipole-dipole array is used in 2-D imaging
surveys where it is assumed that the subsurface geology is 2-D. In many
cases, 3-D data sets for the dipole-dipole arrays are constructed from a
number of parallel 2-D survey lines, particularly from previous surveys.
Due to the elongated sensitivity pattern, the dipole-dipole array can
probably tolerated a larger spacing between the survey lines (to about three
times the inline unit electrode spacing) and still contain significant 3-D
information.
The sensitivity contours for the Wenner alpha array, outside of the
immediate vicinity of the electrodes, are elongated in the direction of the
line of electrodes. This means that the Wenner alpha array is less
sensitive to off-line structures than the dipole-dipole array, i.e. it is less
sensitive to 3-D. This agrees with empirical observations by Dahlin and
Loke (1997).
The sensitivity pattern for the Wenner-Schlumberger array is similar to
that for the Wenner alpha array except for a slight bulge near the center
of the array. The sensitivity patterns for the Wenner gamma array show
characteristic bulges near the C1 and C2 electrodes that were observed
earlier in the 2-D sensitivity sections. Thus it is expected to be more
sensitive to 3-D structures near the C1 and C2 electrodes.
Field Measurement Procedures.
The field measurement procedures were described by
Loke and Barker (1996b). The initial suggestion
involved the deployment of one multi - core cable in
snakelines across a regular grid of electrodes, as in
figure.
However, such a procedure is only viable for small grids
of the order of 10 × 10 electrodes. For larger (or more
detailed) 3D surveys, data are usually acquired along a
sequence of parallel lines which involves the installation
of multiple cables or the use of roll-along techniques
(Dahlin and Bernstone, 1997) in order to increase
efficiency.
3D Imaging by Means of a Number of 2D
Layouts
A simple way of carrying out a 3D survey is to measure a number of parallel, and
optionally orthogonal, 2D sections, and afterwards merge the 2D data sets into a
3D data set before inverting the data. A condensed step-by-step description is given
below, in which it is assumed that the (first) electrode cable layout direction is called
X and the perpendicular direction is called Y . In this case, according to the
nomenclature of Res2dinv collate tool, all lines have the same X location of first the
electrode along this line, but different Y locations. The line direction is zero in all cases
(0=X, 1=Y), and the line direction/sign is also zero (0=positive, 1=negative). The
description assumes that Res3dinv is to be used for the inversion, but the procedure
should also be applicable to alternative inversion software.
According to Loke, (2012), for larger coverage and
more depths by 3D surveys, measurements are
made only in two perpendicular or parallel 2D
survey lines (X and Y). The 3D data set consists of
a number of parallel 2D lines, (Rucker et al., 2009).
The data from each 2D survey line is initially inverted independently to
give a series of 2D cross-sections. In this case, the spacing between the
electrodes must be equaled or smaller than the spacing between the 2D
lines to reduce banding effects ,(Loke, 2010). Al-Zubedi (2015) indicated
that the 3D imaging technique that carried out through parallel 2D
imaging lines not give a good image about subsurface structures, whether
the (Y- spacing) equaled electrode spacing (a) or larger than 4a, especially
if the survey is carried out for deep investigation . This is agreed with
previously mentioned by (Loke, 2014), the model will be constructed from
the series of 2D inversions along parallel lines is not a true 3D inversion
model.
The parallel 2D lines are used because it is useful for
surveys with any electrode arrays, (Loke, 2012). However,
some authors such as (Pavlova and Shevnin , 2013) consider
the cross 2D imaging lines (perpendicular lines) that used
to construct 3D model is the 2D azimuthal resistivity
imaging survey. The cross 2D imaging lines do not
represent the 2D azimuthal resistivity imaging survey
because the principles of this survey based on measuring
the variation of the resistivity values in different directions
and not only in two directions (Taylor and Fleming, 1988).
Figure : Dense 2D measurements. a) parallel to the X-axis (X-lines), b) parallel
to the Y-axis (Y-lines) and c) combined XY-lines from (Tsourlos, 2004) .
This approach of
combining dense 2-D
measurement with 3D inversion
is considered practical for
routine data treatment since the
extra computational time/power
required by 3D inversion
schemes is compensated by the
reduced amount (50% less) of
field data required when
compared with the 2D approach
(Tsourlos, 2004).
3D Imaging by Electrode Grid Layouts
In some cases a roll-along procedure as described above is
not sufficient for 3D surveys, in which case a grid of
electrodes can be used. Since the built-in relay switch of a
single Terrameter LS can switch 64 electrodes the maximum
layout size is 8 x 8 electrodes. For larger electrode layouts
external relay switches can be connected to Terrameter LS.
A variety of survey
configurations are supported,
from simple rectangular grids
(Figures a and b), to non-
rectangular grids (Figure c), to
even data sets collated from
survey lines in different
directions (Figure d, in
RES3DINVx64 only).
Some possible layouts for 3-D surveys.
3-D roll-along techniques
Most commercial 3-D surveys will probably involve grids of at
least 16 by 16 in order to cover a reasonably large area. A 16 by 16
grid will require 256 electrodes which is more than that available
on many multi-electrode resistivity meter systems. One method
to survey such large grids with a limited number of electrodes is
to extend the roll-along technique used in 2-D surveys to 3-D
surveys (Dahlin and Bernstone, 1997).
One method to survey such large grids with a
limited number of electrodes is to extend the
roll-along technique used in 2D surveys to 3D
surveys (Dahlin and Bemstone 1997). This
Figure shows an example of a survey using a
multi-electrode resistivity-meter system with
50 electrodes to survey a 10 by 10 grid,
(Loke, 2014). However, numerous authors
have been noted several suggestions to help
migrate 2D imaging data to 3D acquisition
(Loke and barker, 1996b; Dahlin and
Bemstone, 1997; Dahlin et al., 2002; Bentley
and charibi, 2004; Gunther et al., 2006; Loke
and Dahlin 2010).
A 3-D forward modeling program
In the interpretation of data from 2-D resistivity imaging surveys, it is
assumed that the subsurface geology does not change significantly in
the direction that is perpendicular to the survey line. In areas with very
complex geology, there are could be significant variations in the
subsurface resistivity in this direction (i.e. the geology is 3-D), which could
cause distortions in the lower sections of the 2-D model obtained.
The 3-D resistivity forward modeling program, RES3DMOD.EXE, enables
you to calculate the apparent resistivity values for a survey with a rectangular
grid of electrodes over a 3-D structure.
Three dimensional grids used for dc resistivity forward modeling. (a) Structured grid,
(b) block–oriented grid, and (c) unstructured tetrahedral grid. From Rücker et al.
(2006).
Inversion Method
For 3D resistivity imaging, the
inversion program divides the
subsurface into a number of small
rectangular prisms, and attempts to
determine the resistivity values of the
prisms so as to minimize the difference
between the calculated and observed
apparent resistivity values. One possible
arrangement used by Loke and Barker
(1996b) is shown in figure (2.26).
Figure (2.26) The model blocks arrangement used by (Loke and Barker, 1996b).
The optimization method tries to reduce the difference
between the calculated and measured apparent resistivity
values by adjusting the resistivity of the model blocks.
The inversion routine is based on the smoothness
constrained least-squares method (deGroot-Hedlin and
Constable, 1990; Sasaki, 1992; Loke and Barker, 1996a).
One of the challenges of the inverse problem is to efficiently transform
between the forward problem, which requires a fine discretization of the
subsurface, and the resistivity structure, which is defined on a coarser mesh.
Accordingly, there are three different meshes associated with the inversion, as
indicated in Figure.
The three meshes used in the inversion algorithm. (a) The model parameter mesh; (b) the secondary field
mesh; (c) the primary field mesh. The arrows indicate electrode locations. From Günther et al. (2006).
Interpretation of 3D Imaging Data.
Research and development on forward and inverse
modeling methods for 3D resistivity imaging technique are
underway. The principles are the same as those for the
2D case, but the demand on computational power is
much higher and the practical application of 3D techniques
is still in its infancy (Li, 1992; Oldenburg and Li, 1994;
Loke and Barker, 1996b(.
One model used to interpret the 3D data set is shown in figure (3-
14a). The subsurface is divided into several layers and each layer is
further subdivided into a number of rectangular blocks. A 3D
resistivity inversion program, RES3DINV, is used to interpret the data
from 3D surveys. This program attempts to determine the resistivity of
the blocks in the inversion model that will most closely reproduce the
measured apparent resistivity values from the field survey. Within the
RES3DINV program, the thickness of the layers can be modified by the
user. Two other alternative models which can be used with this program
are shown in (Figures 3-14b and c).
The second inversion model subdivides the top few layers vertically
as well as horizontally by half. Another alternative is to subdivide the top
few layers by half only in the horizontal directions figure (3-14c). Since
the resolution of the resistivity method decreases rapidly with
depth, it has been found that subdividing the blocks is only beneficial
for the top two layers only. In many cases, subdividing the top layer only
is enough. By subdividing the blocks, the number of model parameters
and thus the computer time required to invert the data set can increase
dramatically, (Loke, 2012).
The following figures shows the output from the RES3DINVsoftware. However, there are many programs can be
used to display the 3D imaging data as 3D view.
Arrangement of electrodes in the Birmingham 3-D field survey, (b) Horizontal and (c) vertical cross-sections of
the model obtained from the inversion of the Birmingham field survey data set. The locations of observed tree
roots on the ground surface are also shown, (Loke, 2014).
A 3-D view of the
model obtained from the
inversion of the
Lernacken Sludge
deposit survey data set
displayed with the
Slicer/Dicer program. A
vertical exaggeration
factor of 2 is used in the
display to highlight the
sludge ponds. Note that
the color contour
intervals are arranged in
a logarithmic manner
with respect to the
resistivity, (Loke, 2014).
References
• [8] Li, J.M. (2005) Electric Field and Electric Prospecting. Geological
Publishing House, Beijing.
• [9] Yang, J.F., Deng, J.Z., Chen, H. and K, H.Y. (2012) 3D Direct Resistivity
Forward Modeling by the Precondition Conjugate Gradient Method.
Geophysical Geochemical Exploration, 34, 303-309.
• [10] Liu, B., Nie, L.C., Li, S.C. Xu, L., Liu, Z.Y., Song, J., et al. (2012) 3D
electrical Resistivity Inversion Tomography with Spatial Constraint. Chinese
Journal of Rock Mechanics and Engineering, 31, 2258-2268.

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3d resistivity imaging technique

  • 2. Introduction to 3-D surveys The earth often shows three-dimensional characteristics, which can limit a 2D interpretation. As multi-electrode systems were developing rapidly, e.g., by the use of multichannel recorders, it became more and more interesting to carry out measurements allowing for a three-dimensional reconstruction. There are two current developments that should make 3D surveys more cost-effective option in the near future. One is the development of multi-channel resistivity meters that enable more than one reading to be taken at a single time. This is important to reduce the survey time. The second development is faster microcomputers to enable the inversion of very large data sets (with more than 8,000 data points and survey grids of greater than 30 by 30) to be completed within a reasonable time (Loke, 2014).
  • 3. Theory of 3D Electrical Resistivity Tomography The theory of 3D electrical resistivity tomography is consistent with the common electrical method that conductive of underground material differences as the prerequisite, make underground is full of electricity and observe of subsurface electric field distribution, so as to solve different geological problems. Compared with 3D electrical resistivity tomography the 2D high-density electrical resistivity tomography still exist some problems: when the survey line doesn’t layout in the hidden the underground objects cannot be reflected, which brought difficulty in field test and there is more difficult to detect complex leakage channels especially; Accuracy also have difference by using several 2D cross sections at the same time in an interface to open for forming a quasi 3D images between obtained true 3D images after 3D inversion
  • 4. The 3D inversion divided the subsurface into a number of small rectangular to build geoelectric model [8], and give the initial value of each small rectangle, the resistivity value of each small rectangular volume is obtained by forward calculation, then use the least square method to compare the theoretical value and the measured value to adjust the resistivity of each sub block [9] [10]. Establish objective function F: Where: ρm is the measured resistivity value of the profile; ρt is the theoretical resistivity value of the initial model. Comparing the accuracy between the measured resistivity value and the theoretical value to determine the results of the inversion calculation if it meets the requirements. When the requirements don’t meet, it is required to recalculate the theoretical value until the difference is in the proper range.
  • 5. Array types for 3-D surveys The pole-pole, pole-dipole and dipole- dipole arrays are frequently used for 3-D surveys. Because of other arrays have poorer data coverage near the edges of the survey grid.
  • 6. 1. The pole-pole array In the figure, one possible arrangement of the electrodes for a 3-D survey using a multi-electrode system with 25 nodes. For convenience the electrodes are usually arranged in a square grid with the same unit electrode spacing in the x and y directions. To map slightly elongated bodies, a rectangular grid with different numbers of electrodes and spacings in the x and y directions could be used. The pole-pole electrode configuration was commonly used for 3-D surveys, such as the E-SCAN method (Li and Oldenburg, 1992; Ellis and Oldenburg, 1994b). The maximum number of independent measurements, nmax, that can be made with ne electrodes is given by nmax = ne (ne -1) / 2
  • 7. Two possible measurement sequences for a 3-D survey. The location of potential electrodes corresponding to a single current electrode in the arrangement used by (a) a survey to measure the complete data set and (b) a cross- diagonal survey.
  • 8. This array is an attractive alternative to the pole-pole array for surveys with medium and large survey grids (12 by 12 and above). It has a better resolving power than the pole-pole array (Sasaki, 1992), and is less susceptible to telluric noise since both potential electrodes are kept within the survey grid. Compared to the dipole-dipole array, it has a significantly stronger signal strength. Although it has one “remote” electrode (the C2 electrode), the effect of this electrode on the measurements is much smaller compared to the pole-pole array. 2.The pole-dipole array
  • 9. 3.The dipole-dipole The dipole-dipole array can be recommended only for grids that are larger than 12 by 12 due to the poorer horizontal data coverage at the sides. The main problem that is likely to be faced with this array is the comparatively low signal strength. Similar to 2-D surveys, this problem can be overcome by increasing the “a” spacing between the P1-P2 dipole to get a deeper depth of investigation as the distance between the C1-C2 and P1-P2 dipoles is increased. Also, the use of overlapping data levels is recommended.
  • 10. Summary of array types • For relatively small grids of less than 12 by 12 electrodes, the pole-pole array has a substantially larger number of possible independent measurements compared to other arrays. The loss of data points near the sides of the grid is kept to a minimum, and it provides better horizontal data coverage compared to other arrays. This is an attractive array for small survey grids with relatively small spacings (less than 5 meters) between the electrodes. However, it has the disadvantage of requiring two “remote” electrodes that must be placed at a sufficiently large distance from the survey grid. • The pole-dipole array is an attractive option for medium size grids. It has a higher resolution than the pole-pole array and it requires only one remote electrode and is much less sensitive to telluric noise. For surveys with large grids, particularly when there is no convenient location for a remote electrode, the dipole-dipole array can be used. The electrodes for 3-D surveys are frequently arranged in a rectangular grid. However, the RES3DINV resistivity and I.P. inversion program can also handle survey layouts with an arbitrary distribution of the electrodes. In large 3-D I.P. surveys, it has become popular to use the offset version of the pole-dipole and dipole-dipole arrays to cover a large area rapidly. The C1 current electrode (or C1-C2 current dipole) is placed on a separate line parallel to the line with the potential receivers.
  • 11. Sensitivity Dipole-dipole : The sensitivity values have small but negative values outside the immediate vicinity of the array. Another interesting feature is that the sensitivity contours tend to be elongated in the y-direction, particularly for the larger “n” value. The 4 unit sensitivity contour extends to about 0.6 times the array length in the y-direction, or about 1.8 times the unit electrode spacing. This means that the array is more sensitive to structures off the array axis compared to the pole-pole and pole-dipole arrays. This feature is troublesome in 2-D surveys, but might be advantageous in 3-D surveys.
  • 12. The off-axis elongation of the sensitivity contours agrees with the observation by Dahlin and Loke (1997) that the dipole-dipole array is more sensitive to 3-D effects compared to other common arrays. This factor is important when the dipole-dipole array is used in 2-D imaging surveys where it is assumed that the subsurface geology is 2-D. In many cases, 3-D data sets for the dipole-dipole arrays are constructed from a number of parallel 2-D survey lines, particularly from previous surveys. Due to the elongated sensitivity pattern, the dipole-dipole array can probably tolerated a larger spacing between the survey lines (to about three times the inline unit electrode spacing) and still contain significant 3-D information.
  • 13. The sensitivity contours for the Wenner alpha array, outside of the immediate vicinity of the electrodes, are elongated in the direction of the line of electrodes. This means that the Wenner alpha array is less sensitive to off-line structures than the dipole-dipole array, i.e. it is less sensitive to 3-D. This agrees with empirical observations by Dahlin and Loke (1997). The sensitivity pattern for the Wenner-Schlumberger array is similar to that for the Wenner alpha array except for a slight bulge near the center of the array. The sensitivity patterns for the Wenner gamma array show characteristic bulges near the C1 and C2 electrodes that were observed earlier in the 2-D sensitivity sections. Thus it is expected to be more sensitive to 3-D structures near the C1 and C2 electrodes.
  • 14. Field Measurement Procedures. The field measurement procedures were described by Loke and Barker (1996b). The initial suggestion involved the deployment of one multi - core cable in snakelines across a regular grid of electrodes, as in figure. However, such a procedure is only viable for small grids of the order of 10 × 10 electrodes. For larger (or more detailed) 3D surveys, data are usually acquired along a sequence of parallel lines which involves the installation of multiple cables or the use of roll-along techniques (Dahlin and Bernstone, 1997) in order to increase efficiency.
  • 15. 3D Imaging by Means of a Number of 2D Layouts A simple way of carrying out a 3D survey is to measure a number of parallel, and optionally orthogonal, 2D sections, and afterwards merge the 2D data sets into a 3D data set before inverting the data. A condensed step-by-step description is given below, in which it is assumed that the (first) electrode cable layout direction is called X and the perpendicular direction is called Y . In this case, according to the nomenclature of Res2dinv collate tool, all lines have the same X location of first the electrode along this line, but different Y locations. The line direction is zero in all cases (0=X, 1=Y), and the line direction/sign is also zero (0=positive, 1=negative). The description assumes that Res3dinv is to be used for the inversion, but the procedure should also be applicable to alternative inversion software.
  • 16.
  • 17. According to Loke, (2012), for larger coverage and more depths by 3D surveys, measurements are made only in two perpendicular or parallel 2D survey lines (X and Y). The 3D data set consists of a number of parallel 2D lines, (Rucker et al., 2009).
  • 18. The data from each 2D survey line is initially inverted independently to give a series of 2D cross-sections. In this case, the spacing between the electrodes must be equaled or smaller than the spacing between the 2D lines to reduce banding effects ,(Loke, 2010). Al-Zubedi (2015) indicated that the 3D imaging technique that carried out through parallel 2D imaging lines not give a good image about subsurface structures, whether the (Y- spacing) equaled electrode spacing (a) or larger than 4a, especially if the survey is carried out for deep investigation . This is agreed with previously mentioned by (Loke, 2014), the model will be constructed from the series of 2D inversions along parallel lines is not a true 3D inversion model.
  • 19. The parallel 2D lines are used because it is useful for surveys with any electrode arrays, (Loke, 2012). However, some authors such as (Pavlova and Shevnin , 2013) consider the cross 2D imaging lines (perpendicular lines) that used to construct 3D model is the 2D azimuthal resistivity imaging survey. The cross 2D imaging lines do not represent the 2D azimuthal resistivity imaging survey because the principles of this survey based on measuring the variation of the resistivity values in different directions and not only in two directions (Taylor and Fleming, 1988).
  • 20. Figure : Dense 2D measurements. a) parallel to the X-axis (X-lines), b) parallel to the Y-axis (Y-lines) and c) combined XY-lines from (Tsourlos, 2004) . This approach of combining dense 2-D measurement with 3D inversion is considered practical for routine data treatment since the extra computational time/power required by 3D inversion schemes is compensated by the reduced amount (50% less) of field data required when compared with the 2D approach (Tsourlos, 2004).
  • 21. 3D Imaging by Electrode Grid Layouts In some cases a roll-along procedure as described above is not sufficient for 3D surveys, in which case a grid of electrodes can be used. Since the built-in relay switch of a single Terrameter LS can switch 64 electrodes the maximum layout size is 8 x 8 electrodes. For larger electrode layouts external relay switches can be connected to Terrameter LS.
  • 22. A variety of survey configurations are supported, from simple rectangular grids (Figures a and b), to non- rectangular grids (Figure c), to even data sets collated from survey lines in different directions (Figure d, in RES3DINVx64 only). Some possible layouts for 3-D surveys.
  • 23. 3-D roll-along techniques Most commercial 3-D surveys will probably involve grids of at least 16 by 16 in order to cover a reasonably large area. A 16 by 16 grid will require 256 electrodes which is more than that available on many multi-electrode resistivity meter systems. One method to survey such large grids with a limited number of electrodes is to extend the roll-along technique used in 2-D surveys to 3-D surveys (Dahlin and Bernstone, 1997).
  • 24. One method to survey such large grids with a limited number of electrodes is to extend the roll-along technique used in 2D surveys to 3D surveys (Dahlin and Bemstone 1997). This Figure shows an example of a survey using a multi-electrode resistivity-meter system with 50 electrodes to survey a 10 by 10 grid, (Loke, 2014). However, numerous authors have been noted several suggestions to help migrate 2D imaging data to 3D acquisition (Loke and barker, 1996b; Dahlin and Bemstone, 1997; Dahlin et al., 2002; Bentley and charibi, 2004; Gunther et al., 2006; Loke and Dahlin 2010).
  • 25. A 3-D forward modeling program In the interpretation of data from 2-D resistivity imaging surveys, it is assumed that the subsurface geology does not change significantly in the direction that is perpendicular to the survey line. In areas with very complex geology, there are could be significant variations in the subsurface resistivity in this direction (i.e. the geology is 3-D), which could cause distortions in the lower sections of the 2-D model obtained. The 3-D resistivity forward modeling program, RES3DMOD.EXE, enables you to calculate the apparent resistivity values for a survey with a rectangular grid of electrodes over a 3-D structure.
  • 26. Three dimensional grids used for dc resistivity forward modeling. (a) Structured grid, (b) block–oriented grid, and (c) unstructured tetrahedral grid. From Rücker et al. (2006).
  • 27. Inversion Method For 3D resistivity imaging, the inversion program divides the subsurface into a number of small rectangular prisms, and attempts to determine the resistivity values of the prisms so as to minimize the difference between the calculated and observed apparent resistivity values. One possible arrangement used by Loke and Barker (1996b) is shown in figure (2.26). Figure (2.26) The model blocks arrangement used by (Loke and Barker, 1996b).
  • 28. The optimization method tries to reduce the difference between the calculated and measured apparent resistivity values by adjusting the resistivity of the model blocks. The inversion routine is based on the smoothness constrained least-squares method (deGroot-Hedlin and Constable, 1990; Sasaki, 1992; Loke and Barker, 1996a).
  • 29. One of the challenges of the inverse problem is to efficiently transform between the forward problem, which requires a fine discretization of the subsurface, and the resistivity structure, which is defined on a coarser mesh. Accordingly, there are three different meshes associated with the inversion, as indicated in Figure. The three meshes used in the inversion algorithm. (a) The model parameter mesh; (b) the secondary field mesh; (c) the primary field mesh. The arrows indicate electrode locations. From Günther et al. (2006).
  • 30. Interpretation of 3D Imaging Data. Research and development on forward and inverse modeling methods for 3D resistivity imaging technique are underway. The principles are the same as those for the 2D case, but the demand on computational power is much higher and the practical application of 3D techniques is still in its infancy (Li, 1992; Oldenburg and Li, 1994; Loke and Barker, 1996b(.
  • 31. One model used to interpret the 3D data set is shown in figure (3- 14a). The subsurface is divided into several layers and each layer is further subdivided into a number of rectangular blocks. A 3D resistivity inversion program, RES3DINV, is used to interpret the data from 3D surveys. This program attempts to determine the resistivity of the blocks in the inversion model that will most closely reproduce the measured apparent resistivity values from the field survey. Within the RES3DINV program, the thickness of the layers can be modified by the user. Two other alternative models which can be used with this program are shown in (Figures 3-14b and c). The second inversion model subdivides the top few layers vertically as well as horizontally by half. Another alternative is to subdivide the top few layers by half only in the horizontal directions figure (3-14c). Since the resolution of the resistivity method decreases rapidly with depth, it has been found that subdividing the blocks is only beneficial for the top two layers only. In many cases, subdividing the top layer only is enough. By subdividing the blocks, the number of model parameters and thus the computer time required to invert the data set can increase dramatically, (Loke, 2012).
  • 32. The following figures shows the output from the RES3DINVsoftware. However, there are many programs can be used to display the 3D imaging data as 3D view. Arrangement of electrodes in the Birmingham 3-D field survey, (b) Horizontal and (c) vertical cross-sections of the model obtained from the inversion of the Birmingham field survey data set. The locations of observed tree roots on the ground surface are also shown, (Loke, 2014).
  • 33. A 3-D view of the model obtained from the inversion of the Lernacken Sludge deposit survey data set displayed with the Slicer/Dicer program. A vertical exaggeration factor of 2 is used in the display to highlight the sludge ponds. Note that the color contour intervals are arranged in a logarithmic manner with respect to the resistivity, (Loke, 2014).
  • 34. References • [8] Li, J.M. (2005) Electric Field and Electric Prospecting. Geological Publishing House, Beijing. • [9] Yang, J.F., Deng, J.Z., Chen, H. and K, H.Y. (2012) 3D Direct Resistivity Forward Modeling by the Precondition Conjugate Gradient Method. Geophysical Geochemical Exploration, 34, 303-309. • [10] Liu, B., Nie, L.C., Li, S.C. Xu, L., Liu, Z.Y., Song, J., et al. (2012) 3D electrical Resistivity Inversion Tomography with Spatial Constraint. Chinese Journal of Rock Mechanics and Engineering, 31, 2258-2268.