Slide 1 Induced Polarization (IP) n Basic principles n Data Acquistion n Pseudosection n Inversion n Case Histories
Slide 1
Induced Polarization (IP)
n Basic principles
n Data Acquistion
n Pseudosection
n Inversion
n Case Histories
Induced Polarization
n Current injected into ground and the voltage continues to increase.
n Recognized in 1950’s: it was termed Over-voltage. n Understand the effect in terms of charge accumulation.n The phenomenon is called induced polarization.
I source V potentialNot chargeable Chargeable
Source(Amps)
Potential(Volts)
Chargeability is a microscopic phenomenon
Thoroughly understanding what is happening at the microscopic levelis scientifically challenging. In practice we work with the concept of “chargeability”
Chargeability
pyritechalcocite
copper
graphite
chalcopyrite
bornite
galena
magnetitemalachite
hematite
13.4 ms
13.3 ms
12.3 ms
11.2 ms
9.4 ms
6.3 ms
3.7 ms2.2 ms
0.2 ms0.0 ms
Minerals at 1% Concentration in Samples
Chargeability: rocks and minerals
Earth materials are “chargeable”
Initial situationNeutrality
Apply an electric fieldBuild up of charges
Net effectCharge PolarizationElectric dipole
Induced Polarization: Over-voltage
Not chargeable Chargeable
Source(Amps)
Potential(Volts)
Chargeability Data: Time domain IP
Intrinsic chargeability0<n<1 (dimensionless)
Integrate over the decay
Sample a channel
(msec) mV/V
IP data: frequency domainn Percent frequency effect:
n Phase:
low freq. f2high freq. f1
Sourcecurrent
Measuredpotential
V1 V2
I I
⎟⎟⎠
⎞⎜⎜⎝
⎛ −=
1
12100a
aaPFEρρρ
Sourcecurrent
Measuredpotential
Phase (mrad)
phase (mrad)
Data acquisition
n Data are acquired along with DC resistivity data (just sample a different part of the waveform)
n Data are plotted as pseudosections (exactly the same as DC resistivity)
n For IP the data plotted in the pseudosections will have units (mV/V, msec, mrad, PFE).
Earth
Energy Source In Measured signalsOut = “Data”
Plotting plane
~ v
Plotting plane
~ v
Plotting plane
~ v
Plotting plane
~ v
IGV
aΔ
=π
ρ2
Each data point is an apparent resistivity:
~ v~v
(Click for animation)
DC resistivity and IP data
Example IP pseudosection
2) A chargeable block.
2) A chargeable block and geologic noise.
Example IP pseudosection
3) The “UBC-GIF model”
Example IP pseudosection
Pseudosections … conclusions
n Except for very simple structures, geologic interpretations can not be clearly made directly from pseudosections.
n Interpretation is even more difficult in 3D
Given:- Field observations- Error estimates- Ability to forward model- Prior knowledge
Choose a suitable misfit criterion
Design modelobjective function
Discretize the Earth
Perform inversion
Evaluate results Iterate
Interpret preferred model(s)
Summary: what is needed to invert a data set?
( )∫ −= dxmmsm2
0αφ
∫ ⎟⎠
⎞⎜⎝
⎛ −+ dxmmdxd
x
2
0 )(α
∫ ⎟⎠
⎞⎜⎝
⎛ −+ dzmmdzd
z
2
0 )(α
Summary of IP data types:
n Time domain:q Theoretical chargeability (dimensionless).q Integrated decay time (msec).
n Frequency domain:q PFE (dimensionless)q Phase (mrad)
n For all data types, Jη = d .
n where J is a sensitivity matrix that requires that the electrical conductivity σ is known. We find σ by inverting the DC resisitivity data.
DC / IP datagathered together
Use σ model forforward mapping of
chargeability
IPData
Invert potentialsfor conductivity
model
Potential (i.e. voltage) dataConductivity model
Invert for chargeability models
Chargeability model
IP Inversion
Inversion of IP data
Step 1: Invert Vm to obtain σ.
Step 2: Generate sensitivities
Step 3: Invert the IP data (any form) by solving:
j
i
ijJ σφ
lnln
∂
∂−=
obsdJ =η subject to η > 0.
Example 1: buried prism.
Chargeability model
Data with 5% Gaussian noise
• Pole-dipole; n=1,8; a=10m; N=316; (αs, αx, αz)=(.001, 1.0, 1.0)
Recovered chargeability
Predicted data
Example 2: prism with geologic noise.
Chargeability model
Data with 5% Gaussian noise
• Pole-dipole; n=1,8; a=10m; N=316; (αs, αx, αz)=(.001, 1.0, 1.0)
Recovered chargeability
Predicted data
Example 3: UBC-GIF model.
Chargeability model Recovered chargeability
Data with 5% Gaussian noise Predicted data
• Pole-dipole; n=1,8; a=10m; N=316; (αs, αx, αz)=(.001, 1.0, 1.0)
Field Case History
n Cluny deposit, Australia
n 10 lines of DCIP data acquired
n Inversion carried out in 3D
Data set #1:
Apparent resistivity,dipole - pole.
Cluny: 3D resistivityn Eight survey linesn Two survey configurations.
Easting (m) Easting (m)
mS/m
10500 11500 12500
13000
14000
15000
16000
400
450
500
Easting (m)
North
ing
(m)
Surface topography:ElevationMeters
10 lines surveyed
Easting (m) Easting (m)
mS/m
Data set #2:
Apparent resistivity,pole - dipole.
Data set #1:
Apparent resistivity,dipole - pole.
Cluny: 3D resistivityn Eight survey linesn Two survey configurations.
Easting (m) Easting (m)
mS/m
10500 11500 12500
13000
14000
15000
16000
400
450
500
Easting (m)
North
ing
(m)
Surface topography:ElevationMeters
10 lines surveyed
Easting (m) Easting (m)
mS/m
Data set #2:
Apparent resistivity,pole - dipole.
Conductivity model from 3D inversion of DC
Conductivity model from 3D inversion of DC
Apparent chargeability,dipole - pole.
10500 11500 12500
13000
14000
15000
16000
400
450
500
Easting (m)
North
ing
(m)
Surface topography:ElevationMeters
10 lines surveyed
3D Induced polarization (IP)
Click image to see the AVI movie
Chargeability model from 3D inversion of IP
Click image to see the AVI movie
Chargeability model from 3D inversion of IP
Volume rendered resistivity model Volume rendered chargeability model
3D conductivity and chargeability models
Coming Up
n TBL DC resistivity and IP
n Quiz