sintef petroleum research 1 seismic angle migration: an adaptive limitation of the operator aperture...
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1SINTEF Petroleum Research
Seismic angle migration: an adaptive limitation of the operator aperture
Mathias Alerini
Gemini kollokvium
28 02 2008
2SINTEF Petroleum Research
PostDoc work...
With Pr. Bjørn Ursin
Sponsored by NFR
(grants 159117/I30 and 162612/S30 and the ROSE project)
July 2005 to December 2007... in parallel to many other things...
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Seismic Data
time
Amplitude
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Seismic Data
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Imaging process
Seismic survey
Seismic processing
Subsurface Data
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Seismic migration
From seismic trace to image position (& dynamic information)
x
+ Velocity of seismic waves
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Seismic migration
Kirchhoff type
+ Velocity
Recorded energy comes from somewhere along the curve!
For all M points along the curve, the travel times T(s,M,r) are equal
M
s r
T
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Seismic migration
Kirchhoff type
+ VelocityRecorded energy is somewhere along the curve!
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Seismic migration
Common Image gather
s rs r r r r r r rrssssssss
x
z
z0
offset
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Seismic migration
Common Image gather
s rs r r r r r r rrssssssss
x
z
z0
angle
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Angle Migration: Advantages
Complex geological setting (Strong lateral velocity variations)
Triplications: 1 offset, 2 (e.g.) angles
Artifacts
1
2
hs r
AVO/AVA:Reflection coefficients depends on the angle and not the offset !
AVO/AVA:Reflection coefficients depends on the angle and not the offset !
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Limitation of the migration operator
The traveltime tells us that the recorded energy comes from somewhere along the curves but the migration result tells us the energy comes from the envelop
The traveltime tells us that the recorded energy comes from somewhere along the curves but the migration result tells us the energy comes from the envelop
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Limitation of the migration operator
We just need this information. The rest :- increases the computation time- adds noise
We just need this information. The rest :- increases the computation time- adds noise
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Limitation of the migration operator
The noise is not completely destroyed by the summation process
The noise is not completely destroyed by the summation process
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Limitation of the migration operator
We want to keep only constructive interferences between the specular ray (respects Snell-Descartes) and the migrated ray
s r
migrated ray vs
specular ray
migrated ray vs
specular ray
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Limitation of the migration operator
at the image point
s rrs
Difference in traveltime between the specular ray and the migrated ray
relation to the migration operator aperture
Difference in traveltime between the specular ray and the migrated ray
relation to the migration operator aperture
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Limitation of the migration operator
at the image point, looking at one side
T
isochrone = same traveltime
but...
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Limitation of the migration operator
sub-horizontal rays...
T
isochrone = same traveltime
a small angles produces a large traveltime difference
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Limitation of the migration operator
sub-horizontal rays...
T
isochrone = same traveltime
tangent to the isochrone
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Limitation of the migration operator
sub-horizontal rays...
T
isochrone = same traveltime
tangent to the isochrone
... it is equivalent to the Young’s experiment
Signals in phase
Observed interferences
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Limitation of the migration operator
results: 25m between srcs and recs
No LAM LAM
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Limitation of the migration operator
results: 100m between srcs and 100m between recs
No LAM LAM
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Conclusion
Our Limitation of the migration aperture is easy to implement in an existing code easy to use can handle multi-orientations (faults) can include easily a local error on the geological dip
gave very good results !
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... finally codes have been written, rewritten in a coherent way with
new tools and then ported to the cluster...
... or how to do 3 times the same work...
25SINTEF Petroleum Research
... finally codes have been written, rewritten in a coherent way with
new tools and then ported to the cluster...
... or how to do 3 times the same work...
“Through continuous efforts we succeed eventually. Thus, the more it fails, the greater chance that it succeeds”
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