“exploring” spherical-wave reflection coefficients
DESCRIPTION
“Exploring” spherical-wave reflection coefficients. Chuck Ursenbach Arnim Haase. Research Report: Ursenbach & Haase, “An efficient method for calculating spherical-wave reflection coefficients”. Outline. Motivation : Why spherical waves? Theory : How to calculate efficiently - PowerPoint PPT PresentationTRANSCRIPT
“Exploring” spherical-wave reflection
coefficientsChuck Ursenbach
Arnim Haase
Research Report: Ursenbach & Haase, “An efficient method for calculating spherical-wave reflection
coefficients”
Outline
• Motivation: Why spherical waves?• Theory: How to calculate efficiently• Application: Testing exponential
wavelet• Analysis: What does the calculation
“look” like?• Deliverable: The Explorer• Future Work: Possible directions
Motivation
• Spherical wave effects have been shown to be significant near critical angles, even at considerable depth
• Spherical-wave AVO is thus important for long-offset AVO, and for extraction of density information
See poster: Haase & Ursenbach, “Spherical wave AVO-modelling in elastic isotropic media”
Outline
• Motivation: Why spherical waves?• Theory: How to calculate efficiently• Application: Testing exponential
wavelet• Analysis: What does the calculation
“look” like?• Deliverable: The Explorer• Future Work: Possible directions
Spherical Wave Theory• One obtains the potential from integral over all p:
• Computing the gradient yields displacements
00( ) exp( ) ( ) ( ) exp[ ( )]PP PP
pAi i t R p J pr i h z dp
• Integrate over all frequencies to obtain trace
• Extract AVO information: RPPspherical
( ) ( ) ( )u t f u d
( ) ( )u
Hilbert transform → envelope; Max. amplitude; Normalize
Alternative calculation routePP
max
PP
( )
gradient
( )
-integration
[{ }]
inverse FFT
( )
Hilbert transform
| ( ) [ ( )] |
locate maximum
envelope[ ( )]
normalize
i
u
p
u
u t
u t iH u t
u t t
R
( )PP 00 0
PP0
PP0
PP
PP0
( ) e ( ) e
analytic for ( ) exp( | |)
( , )
gradient
( , )
/ ; normalize with 1
( )
nume
i t i h z
n
n
pR f i J pr d dp
f s
pR I p t dp
I p t pR dp
R
t R R
pR W p dp
sphericalPP
rical integration
R
Outline
• Motivation: Why spherical waves?• Theory: How to calculate efficiently• Application: Testing exponential
wavelet• Analysis: What does the calculation
“look” like?• Deliverable: The Explorer• Future Work: Possible directions
Class I AVO application
• Values given by Haase (CSEG, 2004; SEG, 2004)• Possesses critical point at ~ 43
Upper Layer
Lower Layer
VP (m/s) 2000 2933.33
VS (m/s) 879.88
1882.29
(kg/m3)
2400 2000
Test of method for f () = 4 exp([.173 Hz-1])
Wavelet comparison
Spherical RPP for differing wavelets
Outline
• Motivation: Why spherical waves?• Theory: How to calculate efficiently• Application: Testing exponential
wavelet• Analysis: What does the calculation
“look” like?• Deliverable: The Explorer• Future Work: Possible directions
Behavior of Wn
sphericalPP
PP0( ) ,
sin
n
R
pR W p dp
p
i = 0
i = 85
i = 45
i = 15
Outline
• Motivation: Why spherical waves?• Theory: How to calculate efficiently• Application: Testing exponential
wavelet• Analysis: What does the calculation
“look” like?• Deliverable: The Explorer• Future Work: Possible directions
Waveform
inversion
Joint
inversion
Spherical effects
EO gather
s Pseudo-linear
methods
Conclusions• RPP
sph can be calculated semi-analytically with appropriate choice of wavelet
• Spherical effects are qualitatively similar for wavelets with similar lower bounds
• New method emphasizes that RPPsph is a
weighted integral of nearby RPPpw
• Calculations are efficient enough for incorporation into interactive explorer
• May help to extract density information from AVO
Possible Future Work
• Include n > 4
• Use multi-term wavelet: n An n exp(-|sn
• Layered overburden (effective depth, non-sphericity)
• Include cylindrical wave reflection coefficients• Extend to PS reflections
Acknowledgments
The authors wish to thank the sponsors of CREWES for financial support of this research, and Dr. E. Krebes for careful review of the manuscript.