A.Nassir Saeed, Gary Margrave, David Henley, Helen Isaac ...
Transcript of A.Nassir Saeed, Gary Margrave, David Henley, Helen Isaac ...
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A.Nassir Saeed,
Gary Margrave, David Henley, Helen Isaac & Larry Lines
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Introduction Seismic processing flow PSTM algorithms Band signal analysis Well to seismic tie Post stack & Prestack inversion Conclusion Acknowledgments
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Outline
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Note residual noise left in the CIG and pose as step ladder across the CIG. Max Offset bin: 1980m
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Processing flow: Hussar 2D line
Reformat & Geometry assignment Trace and shot edit
Amplitude recovery
Apply datum and refraction statics
Noise suppression: Radial filter , air blast
Surface Consistent Gabor Deconvolution
Two passes of velocity analysis |Surface Consistent Residual Statics
PSTM gathers preparation
Pre Stack Time Migration
Post migration Gabor Deconvolution
FX noise attenuation
Mute & Stack
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middle bottom arrow refers to noise from ground roll while two side arrows are for pump noise
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• Noise are noticeably attenuated.
• Reflectors at the
middle of the shot gather are now visible after they were masking by ground roll and pump jack noise.
• Energy is now
distributed better across the shot gather after they were mostly taken by ground roll and pump noise
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Some low frequency noise left at the lower side of the shot gather. The amplitude spectrum is broadened
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Noise are further cleaned up. Amplitude spectrum is improved and broadened at -10db
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STRUCTURE STACK POST STACK MIGRATION
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Over all, Reflections are sharpened and improved the high frequency content. More details are now seen at reflections from 100-500ms.
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Weak reflection signals at the near offset of CIG gather.
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PSTM-KIRCHHOFF: CONTRACTOR PSTM-KIRCHHOFF: CREWES
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Contractor used a different datum & replacement velocity than us (Bulk shift is needed for comparison). Contractor applied zero-phase decon after migration whereas we applied minimum phase decon.
Contractor PSTM CREWES PSTM
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Phase-Shift : Pre- & Post– stack migration
Stack section of Pre-stack phase shift migration used CIGs of live traces only.
Output CIG gathers form pre-stack phase-shift migration
populate noisy traces for the padded traces compared to PSTM Kirchhoff.
If we ask to re-kill dead traces inside phase-shift module, then the CIG does not populate full regular offsets for each bin for the CIG gather.
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POST-STACK PHASE-SHIFT PRE-STACK PHASE-SHIFT
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More detailed are shown and better continuity of reflectors at the top of PSTM.
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Zone of interest
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Zone of interest
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Zone of interest
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Inversion Seismic data conditioning – Trim static and super gathers. Offset to angle conversion - angle gather & angle stacks Well to seismic tie and Wavelet extraction for each angle stack AVO Analysis Building low frequency model Post stack analysis and inversion Pre-stack analysis and inversion
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Contractor CREWES
Zone of interest from 1000-1100ms. Note the smooth and continuity of interval velocity across section compared to CGG interval velocity section
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*Negative values (orange in color) shows top of sand reservoir of Glauco more clear compared to Ellerslie FM. * Bright yellow is the base of the reservoir where shale layers manifests.
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Zone of interests are Glauco sand channel overlain by Medicine River coal marker. The second zone of interest is Ellersli Fm above Pekisko. From literature this oil bearing formation.
Horizon colors: Midicne-River coal: green Glauco horizon: red Pekisko Horizon: Cyan
Medicine River coal
Gluaco sand
Ellerslie
Pekisko
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Medicine River coal
Gluaco sand
Ellerslie
Pekisko
Horizon colors: Medicine-River coal: green Glauco horizon: red Pekisko Horizon: Cyan
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Medicine River coal
Gluaco sand
Ellerslie
Pekisko
Hard shale top of Ellerslie is clearly showing
Horizon colors: Medicine-River coal: green Glauco horizon: red Pekisko Horizon: Cyan
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Medicine River coal
Gluaco sand
Ellerslie
Pekisko
Horizon colors: Medicine-River coal: green Glauco horizon: red Pekisko Horizon: Cyan
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Conclusions
Re-processing of 2D lines show more details at the zone of interests. Reflection signal is down to 3Hz.
Noise attenuation by Radial dip filter successfully attenuate ground roll and pump jack noise.
Maximum offset of CIG gathers is good to approximately 3440m compared to 1980m of CGG processing.
PSTM migration focuses reflected energy, collapses diffraction and improve image section.
Elastic rock sections delineate lateral extensions of Glauconitic and Ellerslie prospects. All impedance and elastic sections were inverted to 3Hz as low frequency cutoff (1-3Hz).
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Further work
Improve pre-stack imaging using PSPI. Will use CREWES PSPI code for Hussar data.
To gain more reflection signals from 100-500ms that we were seeing in
phase-shift migration and were missing from Kirchhoff migrations.
Investigate the CIG gather to see if reflection and S/N would be improved at near offset by using wave equation migration (PSPI).
Enhance lateral extension at the east side of inverted sections at
Medicine Rive coal and Glauco formations for better correlation with the dipole sonic well 12-27.
Rock physics modeling and analysis work to be done pending providing further logs and other info from Husky.
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Acknowledgments
CREWES sponsors, staff and students
Husky Energy
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