Presentation is loading. Please wait.

Presentation is loading. Please wait.

John C. Bancroft and grad students

Similar presentations


Presentation on theme: "John C. Bancroft and grad students"— Presentation transcript:

1 John C. Bancroft and grad students
AVO, migration apertures Fresnel zones, stacking, Q, anisotropy, and fast inversions John C. Bancroft and grad students University of Calgary CREWES 2003 NSERC

2 Grad students Shuang Sun Pavan Elapavuluri Kun Liu (and Hugh Geiger)
John Millar Xiang Du Zhihong (Nancy) Cao Chunyan (Mary) Xiao

3 Outline Differentiators Fresnel zones AVO migration apertures Q
Wavefield extrapolators Multiples and radon transforms Inversion

4 Digital differentiator
Accuracy Speed Beauty (1, -1) 1, 0, -1) better Theoretical shape?

5 Inverse FFT of (j)

6 Derivative assumes: Maximum bandwidth Ideal interpolator
Sinx/x operator Derivative of sinx/x SincFn.m

7 What is the basic unit of laryngitis?
Shuang Sun Stacking specula energy Fresnel zone for offset and dipping reflectors Balanced AVO in areas of poor geometry Caution: model based migration One hoarsepower What is the basic unit of laryngitis?

8 What size hole can we see with seismic?

9 What happens at the edge of a reflector?

10 Fresnel zone Fresnel Size: frequency depth velocity Claerbout

11 Depends on the size of the Fresnel radius
Only for stacked data!!!

12 Analytic function for zero-offset case (no wavelet)
Solution to the acoustic wave equation for zero-offset, the diffraction response can be written as: Diffraction operator D0: te : minimum two-way travel time to the edge of the reflector; t’=t-te: time measured after onset time te ; e : angle between the normal to the reflector and raypath of the minimum travel time to the edge of the reflector. Berryhill, 1977

13 Diffraction amplitude
Time Angle

14 Diffraction amplitude

15 Scaled amplitude (evaluate phase)

16 Fresnel zone with Ricker wavelet source
Source signature with dominant frequency 50hz Reflected signal amplitude

17 Fresnel zone with fixed bandwidth
Frequency from hz Frequency from hz

18 Reflector smaller than Fresnel zone: width 50m

19 Reflector width: 1000m

20 Amplitude (no wavelet)

21 Diffraction modelling

22 Valid area for AVO ?

23 Comments Locations for AVO analysis before migration should be at least a Fresnel radius away from the target edge. The amplitudes will be in error if the target size is smaller than or equal to the Fresnel zone. Wavelet will contribute to the size of contamination area. Only zero offset was considered Should consider a prestack migration to perform AVO analysis.

24 Offset traveltime 2h DSR eqn.

25 Cheop’s pyramid - DSR eqn.
Hyperbola CMP at T0 Zero off. DSR eqn. Const. Off CMP gath.

26 Prestack data, flat… 7 Cheop’s .
Specula energy

27 Reflections from dipping event
Reflecting element

28 Prestack data, dipping... Cheop’s p.
Defines exact shape of surface, specula energy

29 Cheop’s summation: specula energy
Fresnel zones

30 Prestack Fresnel zone horizontal layers

31 P. S. Fresnel zone for dipping event

32 Contours : equal angle of incidence
Offset increases with x Angle 1

33 Constant offset migration

34 What about dipping specula energy?
Smear of dips Still OK ???

35 CMP gather

36 Limited aperture EO gather

37 Comments … Prestack specula energy can be identified, Limited aperture
horizontal and dipping Limited aperture faster, better SNR, may preserve amplitudes Optimum size of a super-CMP gather can be defined using Fresnel zones Should use prestack migration gathers for AVO Use model based migration with caution

38 Comments Constant offset migration EOM
smears AVO energy (OK) requires velocity information EOM also smears AVO energy (OK) Stacking within the Fresnel zone may reduce acquisition geometry artifacts

39 What is one millionth of a mouth wash?
Pavan Elapavuluri Q What is one millionth of a mouth wash? One microscope

40 Wavelets with varying Q and Time
Build Q wavelet table: [Q, time] Q: 30, 50, 70, 90, 110, … T: 0 to 6.0 sec Cross-correlate (coherence) trace with all wavelets At a given time, peak corresponds to Q

41 9 wavelets T=1000 T=3000 T=5000 Q=90 Q=70 Q=50

42 3 Spikes on trace Q = 70 T=1000 T=3000 T=5000 Q=90 Q=70 Q=50

43 Noise on trace Q = 70 T=1000 T=3000 T=5000 Q=90 Q=70 Q=50

44 Kun Liu (and Hugh Geiger)
Wavefield extrapolation What is 2000 pounds of Chinese soup? Won ton

45 Input

46 200m depth extrapolation …with adaptive taper

47 What is half a large intestine?
Xiang Du Finite element method integrated with Finite difference migration A semicolon What is half a large intestine?

48 Comparison: FE-FDM with FX-FDM
Result of FE-FDM Result of FX-FDM (SU)

49 Trace comparisons

50 Steep oblique model Velocity model Seismic section

51 Comparison of methods Result of FE-FDM Result of FX-FDM (SU)

52 Runtime and memory requirements
FE-FD 26 secs 2.2 meg FK-FD 31 secs 1.3 meg.

53 What is one thousand aches?
Zhihong (Nancy) Cao Chunyan (Mary) Xiao Tutorials Review of Multiple suppression techniques Multiple attenuation using the Radon transform What is one thousand aches? A kilohurtz

54 after Kabir and Marfurt, 1999

55 Semblance plot is a Radon transform

56 Lorraine Bloom David Henley Larry Lines The model and inverse

57 Modelling process Inversion expert

58 The Model (Not the inverse)

59 The Inverse

60 The artifacts (of inversion)
Before modelling After inversion

61 Of course, … some things are easier to model and invert.

62 Inversion Mathematical process Geophysical terminology
Used in many geophysical applications: decon., statics, tomography, tau-p, … Geophysical terminology Estimation of rock properties Modelling <-> Inversion

63 What is the ratio of an igloo’s circumference to its diameter?
Millar time Multigrid inversion Borrowed from fluid dynamics Recursive Variable grid size Solutions are frequency dependent Fast What is the ratio of an igloo’s circumference to its diameter? Eskimo pi

64

65 Iterative solution

66 Laplace’s equation

67 Variable grid size

68 Analogous to FFT ???

69 Sorting a 2-D array into a vector

70

71 Extractions, smoothings and interpolations
S = Solution with one iterative step 33x33 17x17 3x3 9x9 5x5 3x3 9x9 5x5 Pass defects down and errors up

72 Performance

73 Conclusions: Migration apertures speed, SNR, balanced amplitudes
CMP AVO: consider Fresnel zones Finite element / Finite difference migration Multiples and Radon transforms Q and differential operators Multi grid inversions

74 The end

75


Download ppt "John C. Bancroft and grad students"

Similar presentations


Ads by Google