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EXTENDED SEISMIC DATA
PROCESSING-DMO
SEISMIC DATA PROCESSING
Last lecture we discussed the f-k domain filtering. Today
we make swift review and then move to dip move out
DMO. F-K domain is a transformation from t-x domain.
The transformation is done using Fourier transform for
both frequency and wavenumber. The subject seems
complex but let’s start with the mathematical formula:
𝑢 𝑘, 𝜔 =
−∞
∞
𝑈 𝑥, 𝑡 𝑒−𝑖 𝜔𝑡+𝑘𝑥 𝑑𝑥 𝑑𝑡
As we are recording the wavefield at geophones distributed at
the earth’s surface with certain intervals, we are actually
sampling that wavefield in both space and time. Hence, all
considerations pertinent to time are also valid for space ‘x’.
Terminology changes only, for space domain, transform moves
me to the wavenumber domain. Mathematically:
𝑘 =
2𝜋
𝐿
Where L is the wavelength
Now back to yesterday example
From the figure it is visible also that the CMP points do not lie at the
mid-distance between the source and the receiver, the midpoints are
smeared in the up-dip direction. The intention here is find that extra
term that corrects for the dipping of the reflector.
The distance between the source and receiver can be derived using
the following equation:
To get rid of dR we use :
Substituting
The travel time then becomes:
The true velocity is related with the apparent
velocity (dip-dependent) with the relation
Cdip can give good nmo correction although that the velocity is
not true. The problem arise more when we deal with the so
called conflicting dip case as in the next figure.
Now correction for DMO using the
formula
Where
The time correction is thus given
by
DMO flowchart
Extended seismic data processing dmo

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Extended seismic data processing dmo

  • 2. Last lecture we discussed the f-k domain filtering. Today we make swift review and then move to dip move out DMO. F-K domain is a transformation from t-x domain. The transformation is done using Fourier transform for both frequency and wavenumber. The subject seems complex but let’s start with the mathematical formula: 𝑢 𝑘, 𝜔 = −∞ ∞ 𝑈 𝑥, 𝑡 𝑒−𝑖 𝜔𝑡+𝑘𝑥 𝑑𝑥 𝑑𝑡
  • 3.
  • 4.
  • 5. As we are recording the wavefield at geophones distributed at the earth’s surface with certain intervals, we are actually sampling that wavefield in both space and time. Hence, all considerations pertinent to time are also valid for space ‘x’. Terminology changes only, for space domain, transform moves me to the wavenumber domain. Mathematically: 𝑘 = 2𝜋 𝐿 Where L is the wavelength
  • 6. Now back to yesterday example
  • 7.
  • 8. From the figure it is visible also that the CMP points do not lie at the mid-distance between the source and the receiver, the midpoints are smeared in the up-dip direction. The intention here is find that extra term that corrects for the dipping of the reflector. The distance between the source and receiver can be derived using the following equation:
  • 9. To get rid of dR we use : Substituting
  • 10. The travel time then becomes:
  • 11.
  • 12. The true velocity is related with the apparent velocity (dip-dependent) with the relation Cdip can give good nmo correction although that the velocity is not true. The problem arise more when we deal with the so called conflicting dip case as in the next figure.
  • 13.
  • 14. Now correction for DMO using the formula Where The time correction is thus given by