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Marine 3D Survey Design Marine 3D Survey Design LDEO 3D Seismic - PowerPoint PPT Presentation

Marine 3D Survey Design Marine 3D Survey Design LDEO 3D Seismic Workshop : September 10, 2005 LDEO 3D Seismic Workshop : September 10, 2005 Phil Fontana - Veritas DGC, Inc. Phil Fontana - Veritas DGC, Inc. Geologic Interpretation Survey


  1. Sample spreadsheet for spatial sampling Frequency vs dX 3D Survey Parameterisation RMS velocity (ft/sec or m/sec)= 2500 No. of samples per wavelength= 2 2-way time (in msecs)= 2700 Minimum dip (in degrees)= 20 Dip increment= 5 Minimum frequency= 30 Frequency increment= 5 --------------------------------------------------------------------------------------------------------------------------------- Dip-----> 20 25 30 35 40 45 50 -------------------------------------------------------------------------------------------------------------------------------- Frequency <------------------Sampling required at 2 samples per wavelength--------------> 30 61 49 42 36 32 29 27 35 52 42 36 31 28 25 23 40 46 37 31 27 24 22 20 45 41 33 28 24 22 20 18 50 37 30 25 22 19 18 16 55 33 27 23 20 18 16 15 60 30 25 21 18 16 15 14 65 28 23 19 17 15 14 13 70 26 21 18 16 14 13 12 75 24 20 17 15 13 12 11 80 23 18 16 14 12 11 10 85 21 17 15 13 11 10 10

  2. Spatial Sampling - 3D Grid Definition P1 3D Grid P3 Inline Crossline � Bin or grid cell: seismic traces with midpoints that fall within the bin boundaries are gathered for CMP P2 stacking

  3. Spatial Sampling – Source / Streamer Geometry � Inline Sampling = ½ of the Group Interval � Most streamers have 12.5 m interval = 6.25m CMP � Crossline Sampling = ½ of Streamer Separation per Source � Conventional CMP Line Spacing = 25m to 50m � “High” Resolution CMP Line Spacing = 12.5m to 18.75m The cost of the survey is greatly influenced by the required crossline sampling

  4. Multiple Source and Multiple Streamer Acquisition Configurations � For almost all current marine 3D surveys multiple subsurface lines are routinely recorded for each vessel traverse � Three factors have been major incentives: � Requirements for reduced overall survey costs � Requirements for reduced survey turnaround time � Requirements for denser spatial sampling � Technological advancements: � Larger seismic vessels (so-called "super ships") � Increased compressor capacity � Better airgun arrays � Larger channel capacity recording systems � Navigation and positioning improvements (networks) � High efficiency diverters (paravanes, etc.)

  5. LAYOUT Plan View / Port-side only (not to scale) Tow point 160 m. ‘kevlar’ rope bend restrictors ‘live’ streamer section(s) 160 m. armored lead-in cables ‘vimm’ sections (2 per streamer) ropes gun array(s) 2000 liter floats 1050 liter floats barovane Veritas Viking - I : generic layout (Keathley Canyon 2001)

  6. Multiple Source and Streamer Acquisition Relative Production Rates Acquisition Subsurface Lines Boat Track Subsurface Configuration per Vessel Pass Km/Month Km/Month 1C - 1S 1 4800 4800 2C - 1S 2 4050 8100 2C - 2S 4 3750 15000 3C - 2S 6 3000 18000 4C - 2S 8 2750 22000 6C - 2S 12 2500 30000 12C - 1S 12 2250 27000 Source and streamer spacing can be varied to achieve required subsurface line spacing

  7. MARINE LAYOUT Alternating sources: Six streamers: 25 meters downline 6000meters length @ 10 sec. interval @ 480 channels S1 S2 Streamer 1 Streamer 6 file ‘x’ 1 3 5 7 9 11 cmp- lines file ‘x+1’ 2 4 6 8 10 12 Dual Source + 6 Streamers = 12 cmp lines

  8. Marine 3D CMP Lines 11 9 7 5 3 1 6 5 4 3 2 1 x x x x x x S1 Source 1 Streamers Nominal Program Bin-Line Nominal down-going energy (port source S1) x Source-near offset midpoint Nominal up-coming energy Dual Source + 6 Streamers

  9. Marine 3D CMP Lines 11 9 7 5 3 1 12 10 8 6 4 2 6 5 4 3 2 1 x x x x x x Source S2 1 Streamers Nominal Program Bin-Line Nominal down-going energy (port source S1) x Source-near offset midpoint Nominal Program Bin-Line (starboard source S2) Nominal up-coming energy Dual Source + 6 Streamers

  10. LAYOUT Vessel Sail-Lines Sail-Line separation X-Line spread “Flip-Flop” Source Subsurface coverage Dual Source + 8 Streamers

  11. LAYOUT Vessel Sail-Lines Sail-Line separation X-Line spread “Flip-Flop” Source Subsurface coverage Dual Source + 8 Streamers

  12. LAYOUT Vessel Sail-Lines Sail-Line separation X-Line spread “Flip-Flop” Source Subsurface coverage Dual Source + 8 Streamers

  13. Survey Area

  14. Image Apertures Area to be imaged Dip migration aperture Minimum or Fresnel CMP fold aperture CMP fold taper taper CMP fold

  15. Migration aperture defined by dips Constant velocity / straight raypaths θ V * T 2 Migration aperture X = V * T * sin θ 2 X θ

  16. Migration aperture defined by dips Straight raypath example For typical Gulf of Mexico velocity function V = 1500 + 0.6 Z V rms T 0 15 30 45 60 75 90 (<--------------- dip in degrees-------------------->) (<--------migration aperture in metres----------->) 1756 1.000 227 439 621 760 848 878 1910 1.500 371 716 1013 1241 1384 1433 2086 2.000 540 1043 1475 1807 2015 2086 2285 2.500 739 1428 2020 2474 2759 2856 2512 3.000 975 1884 2664 3263 3640 3768

  17. Diffraction energy � According to Claerbout (Imaging the Earth's Interior) � Approximately 70% of diffraction energy is within the Fresnel Zone � Migration is focussing/collapsing data within the Fresnel Zone � Diffraction energy within the Fresnel Zone must be adequately sampled � Dip of diffraction energy at edge of Fresnel Zone is approximately 15 degrees � For adequate spatial sampling � Always consider minimum dip to be not less than 15 degrees � Some people consider minimum dip to be not less than 30 degrees � Approximately 95% of diffraction energy is within 30 degree range

  18. Fold Taper * * 0-6000m 0-6000m Fold taper = ½ maximum offset

  19. Taper On and Taper Off: Impact on Survey Size Full Operational Area Taper off Taper on

  20. Survey Surface Area basic program area 15 deg. dip 15 deg. dip 30 deg. dip 30 deg. dip “full-fold” program area incorporating migration apertures complete program surface area Migration - 9: Migration Aperture/ “fringe” - 3D case

  21. The Concept of Fold “Fold” refers to the number of traces collected at each CMP location. In the strictest sense “Full Fold” refers to a CMP containing a trace from each receiver group in the streamer cable. In order to achieve full fold the shot point interval has to be ½ the group interval. Therefore if the shot point interval equals: Multiple of Group Interval Effective Fold 1 1/2 2 1/4 3 1/6 4 1/8 n 1/(2*n)

  22. Bin Fold source movement X-line Inline Planar View - expanded inline axis bin Binfold Increase

  23. Pre-stack sampling Common offset x s Dual source Single source x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x Common shot x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x Common midpoint x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x x dx r = 12.5m dx r = 12.5m x x x x x x x x x x x x x x x x x x x x x x x dx s = 25m dx s = 50m Common receiver x x x x x x x x x x x x x x x x x x x x x x x x r

  24. Vessel Speed and Record Length � Computation for record length is: R = (SI / V) - O � R is the maximum record length in seconds � SI is the shot interval in meters � V is the OTG vessel speed in meters/second � O is the recording system overhead in seconds Example SI = 25m V= 2.5 m/s O = 0.75 s R= (25m / 2.5m/s)-0.75s = 9.25s 9250 ms / 1024 samples /binary sec = 9.03 s > 9.0 sec record

  25. Temporal Sampling = Vertical Resolution The bandwidth of marine seismic data is primarily related to the depth of tow of the sources and receivers.

  26. Surface Reflections = Ghosting Air Reflection Coefficient = -1 D= depth of source or receiver Water dT= Time delay between primary and ghost = 2D/V

  27. Impulse Response P r i m a r y I m p u l s e 1 . 2 1 0 . 8 0 . 6 Amplitude n o g h o s t 0 . 4 0 . 2 0 0 5 0 1 0 0 1 5 0 2 0 0 2 5 0 3 0 0 - 0 . 2 T i m e ( m s ) I m p u l s e A m p l i t u d e S p e c t r u m 0 - 1 0 - 2 0 - 3 0 - 4 0 Amplitude (dB) - 5 0 - 6 0 - 7 0 - 8 0 - 9 0 - 1 0 0 0 5 0 1 0 0 1 5 0 2 0 0 2 5 0 F r e q u e n c y ( H z )

  28. Ghosted Impulse Response G h o s t e d I m p u l s e G h o s t e d I m p u l s e P r i m a r y I m p u l s e P r i m a r y I m p u l s e 1 . 2 1 . 5 1 . 5 1 . 2 t p t p 1 1 1 1 0 . 8 0 . 8 0 . 5 0 . 5 0 . 6 0 . 6 Amplitude Amplitude Amplitude Amplitude 0 0 n o g h o s t n o g h o s t 0 0 5 0 5 0 1 0 0 1 0 0 1 5 0 1 5 0 2 0 0 2 0 0 2 5 0 2 5 0 3 0 0 3 0 0 0 . 4 0 . 4 - 0 . 5 - 0 . 5 t g t g 0 . 2 0 . 2 - 1 - 1 0 0 dt g = t g – t p dt g = t g – t p 0 0 5 0 5 0 1 0 0 1 0 0 1 5 0 1 5 0 2 0 0 2 0 0 2 5 0 2 5 0 3 0 0 3 0 0 - 0 . 2 - 1 . 5 - 1 . 5 - 0 . 2 T i m e ( m s ) T i m e ( m s ) T i m e ( m s ) T i m e ( m s ) I m p u l s e A m p l i t u d e S p e c t r a 2 0 f p =1/2dt g 0 - 2 0 Amplitude (dB) n o g h o s t _ s p e c - 4 0 g h o s t _ s p e c - 6 0 f g =1/dt g - 8 0 - 1 0 0 0 5 0 1 0 0 1 5 0 2 0 0 2 5 0 F r e q u e n c y ( H z )

  29. Source Ghost Response 4 4 5 0 in 3 A r r a y S ig n a t u r e 6 m D e p t h 3 - 1 2 8 H z 8 0 3 0 Amplitude ( bar-m) - 2 0 - 7 0 - 1 2 0 0 5 0 1 0 0 1 5 0 2 0 0 2 5 0 3 0 0 T i m e ( m s ) N o R x G h o s t 6 m S o u r c e D e p th S p e c tr a 2 2 0 Amplitude ( dB re 1 uPa-m) 2 0 0 1 8 0 1 6 0 0 2 0 4 0 6 0 8 0 1 0 0 1 2 0 1 4 0 1 6 0 1 8 0 2 0 0 F r e q u e n c y ( H z )

  30. Source and Receiver Ghost Responses 4 4 5 0 in 3 A r r a y S ig n a t u r e 6 m D e p t h 3 - 1 2 8 H z 8 0 3 0 Amplitude ( bar-m) - 2 0 - 7 0 - 1 2 0 0 5 0 1 0 0 1 5 0 2 0 0 2 5 0 3 0 0 N o R x T i m e ( m s ) G h o s t 8 m G h o s t 6 m S o u r c e D e p th S p e c tr a 2 2 0 Amplitude ( dB re 1 uPa-m) 2 0 0 1 8 0 1 6 0 0 2 0 4 0 6 0 8 0 1 0 0 1 2 0 1 4 0 1 6 0 1 8 0 2 0 0 F r e q u e n c y ( H z ) N o R x G h o s t 8 m G h o s t

  31. Source / Streamer Ghost Responses 6m Source/ 9m Streamer vs 6m Source / 7m Streamer 220 15 dB Amplitude ( dB re 1 uPa-m) 200 180 160 0 20 40 60 80 100 120 140 160 180 200 Frequency (Hz) 6m/7m 6m / 9m

  32. 80 Hz Signal Amplitude: Weather Risks 80 Hz Amplitude vs Source and Streamer Depth 220 65% Wx 50% Wx 214 Amplitude ( dB re 1 uPa-m) 2 dB increase from 7 to 6-m 208 4 dB increase from 8 to 7-m 202 Estimated weather risks using conventional fluid filled streamers 30% Wx 196 5 6 7 8 9 Streamer Depth (m) 5m 6m 7m

  33. In-Water Positioning Networks Center of Center of Last Active G roup Last Active G roup RG PS RG PS RG PS STREAM ER 8 STREAM ER 8 Center of 100 m Last Active G roup Center of 100 m Last Active G roup RG PS RG PS RG PS STREAM ER 7 STREAM ER 7 Center of 100 m Last Active G roup Center of 100 m Last Active G roup RG PS RG PS RG PS STREAM ER 6 v STREAM ER 6 Center of v Last Active G roup RG PS RG PS Center of 100 m Last Active G roup RG PS 100 m 52.16 m 52.16 m STREAM ER 5 DG PS DG PS 52.16 m STREAM ER 5 Fanbeam 50 m RG PS RG PS Fanbeam DG PS 50 m Fanbeam RG PS 50 m 50 m Center of Last Active G roup 50 m NRP NRP Fanbeam Fanbeam 50 m Center of RG PS Last Active G roup NRP Fanbeam RG PS 50 m STREAM ER 4 Center of STREAM ER 4 Center of Last Active G roup RG PS First Active G roup Center of 100 m Center of Last Active G roup RG PS First Active G roup 100 m STREAM ER 3 v Center of STREAM ER 3 Last Active G roup Center of v First Active G roup Center of RG PS RG PS 100 m Last Active G roup Center of First Active G roup RG PS 100 m STREAM ER 2 Center of Last Active G roup RG PS RG PS Center of STREAM ER 2 First Active G roup Center of 100 m Last Active G roup Center of RG PS First Active G roup STREAM ER 1 100 m STREAM ER 1 Center of First Active G roup Center of First Active G roup Source to near trace offset Center of the nearest active group to the center of the farthest active group 5985.84m 233.5 m Source to near trace offset Center of the nearest active group to the center of the farthest active group 5985.84m 233.5 m

  34. Positioning Network Design – Past to Present Network design and implementation has improved dramatically over the last decade. The main factors for this are: � Improved reliability in navigation recording system and streamer telemetry. � Improved data quality and reliability from compass and acoustic providers. � Increased towing capacities provide a wider baseline that improves the geometry for positioning networks.

  35. Segmented In-Water Positioning Network Head Acoustic Net Tail Acoustic Net Mid Acoustic Net

  36. Forward Network Design This is the forward network configuration used in the current survey conducted by the Veritas Vantage. Green arrows indicate observation direction from rGPS antenna to surface located buoy nodes on source sub-arrays and cable heads. Black circles indicate acoustic sub-surface nodes, except for gun centers and streamer reference points (Near Trace Location).

  37. Mid-Network / In-Line Distance 300m in-line

  38. Tail-Network Design With rGPS Range/Bearing on all Tail Buoys, Ellipse error ellipse at far traces are all less than 2.5meters at 95% confidence.

  39. Front & Tail Network – Early 1990’s Early networks utilized a front network that positioned the guns and cable heads consisting of acoustics, laser & rGPS. A separate tail network of acoustics and rGPS positioned the far traces. This also provided inline and cross-line (rotation) adjustments for the streamer shape. Compasses situated every 300m along the streamer provided readings with which to model the streamer shape.

  40. Front, Mid & Tail Network (1996-present) Current Veritas method utilizes an additional mid-acoustic network. This creates a precise grid of locations for nodes defined within the middle portion of the streamers. The front and tail networks determine the geodetic controls used as anchor points to start the iterative process of calculating the best fit of the streamer shape through this mid-net. The total network solution also provides inline and cross-line (rotation) adjustments for the streamer shape.

  41. Full-Braced Network / 150m separation (6-cables)

  42. Full-Braced Network Capability Veritas has the capability to provide a fully braced acoustic network. This would consist of the current front and tail network geometry. An array of acoustic pods located every 600m along the streamers would provide a connected, or fully braced network along the entire streamer length. Compasses located every 300m would provide additional observations to support the modeling of the receiver positions.

  43. Node Precision Comparison As can be seen below, there is an improvement in the estimated precision of a fully braced network. When compared to the current mid-net configuration, maximum improvement is observed at the far-mid portion of the streamers and is on the order of 3 to 3.5 meters.

  44. HMP Precision Comparison Horizontal Mid-Point (HMP), is the reflection point for each source/receiver pair. The HMP positioning precision can be seen below. The improvement in the estimated precision of the HMP using a fully braced network can again be seen in this comparison of Mid-net versus a fully braced network. When compared to the current mid-net configuration, maximum improvement is on the order of 0.5 to 1.7 meters.

  45. Forward Network Design (Drop-Out Analysis) In order to predict the effects of data loss within the network, a set of “worst case” scenarios are calculated. This test shows an acoustic loss of hull and gun acoustics to the outer port near-trace pod.

  46. Least Squares Calculation

  47. Least Squares Calculation

  48. Least Squares Calculation

  49. Streamer Shaping View

  50. Streamer Shaping View

  51. Streamer Shaping View

  52. Marine 3D Survey Quality Control Marine 3D Survey Quality Control

  53. Project QC Stages Pre-Mobilization On Board QC On-Line QC Project Plan Document Off-line QC Geodetics Database population Navigation Post Survey Seismic Operating Specifications Data Archiving Final Report Support Mobilization Systems’ Set-up Initial Parameter Checks

  54. Onboard Survey QC � Assurance and verification of seismic survey coverage � Assurance and verification of seismic data quality. � Assurance and verification of positioning data quality.

  55. Real Time QC On Line Seismic S / N Observers Bin Coverage Recording System Guns Streamers Navigators GPS Spectra In-Water Network

  56. Off-Line QC Navigation Processing Final Seismic QC P 1/90 Accept (Green) HMP Precision Reject (Red) Seismic Processing - QC Hold for further analysis (Yellow) Noise Analysis Time Limit (48 hrs?) Swell Strum Seismic Pre- Processing Seismic Interference nav merge, resample, filter, etc.. Low Fold Cube Generate SEG-Y LMO Fast Track Cube Areal Attributes examples

  57. Marine Survey QC � Assurance and verification of seismic survey coverage � Assurance and verification of seismic data quality. � Assurance and verification of positioning data quality.

  58. Mid-point Scatter and “Bin” Definition Survey Source Vessel Shot line X X X X X X X s X p Midpoints u X o r g X r e v i e c X e R X Cable "Bins" or "cells"

  59. 3D Subsurface Coverage 3D Grid P1 P3 Inline Crossline Subsurface (midpoint) coverage P2

  60. 3D Offset Binning: All Offsets

  61. 3D Offset Binning: Zone 1 (Nears)

  62. 3D Offset Binning: Zone 2 (Near-Mids)

  63. 3D Offset Binning: Zone 3 (Far-Mids)

  64. 3D Offset Binning: Zone 4 (Fars)

  65. Binning Streamer x-line bin Offset >25m< 0 1 600m 2 2400m 3 4200m 4 6000m ‘fixed’ binfold ‘flexed’ binfold <------ 125m-------> Effect of flexed-binning on fold displays

  66. All Offsets – Racetrack 1 Flexed low In Progress Complete – May have some remaining coverage low low Complete Complete Complete low Complete Complete Complete

  67. Zone 1 – Racetrack 1 Flexed low low low low

  68. Zone 2 – Racetrack 1 Flexed low low low low

  69. Zone 3 – Racetrack 1 Flexed low low low low

  70. Zone 4 – Racetrack 1 Flexed low low low low

  71. Zone 5 – Racetrack 1 Flexed low low low low

  72. Infill Planning Summary Images include up to sequence 158 � Time estimates from Sequence 159 SOL (03:04 15/Jan/2002) � Time to record all remaining passes 42 hrs � Time to line change all remaining passes 24 hrs � Total time to record and line change 66 hrs � Regional Downtime to date 40.0% � Technical Downtime to date 0.01% � Total time including all Downtime 92 hrs � Final Infill Percentage 18% � 19 th Jan Completion Date �

  73. How Much Fill is Required? � Fill requirements are obvious related to the survey objectives, geologic setting, the frequency bandwidth of the seismic data, spatial sampling requirements, and so forth, so it impossible to make blanket statements concerning fill requirements � Fold decimation studies conducted on 2D data during the survey pre-planning stage can play a vital role in establishing objective offset distribution and fill requirements � Onboard seismic processing can obviously play a major role here if 3D bin stacks, rather than just bin attribute plots, are available to guide fill decisions � Fill can always be reduced by bin expansion (overlapping or flex), but this expansion can attenuate high frequency components of dipping events during stacking

  74. Marine Survey QC � Assurance and verification of seismic survey coverage � Assurance and verification of seismic data quality. � Assurance and verification of positioning data quality.

  75. RMS Evaluation – SOL / EOL

  76. Raw Shots – Noise Evaluation

  77. Shot Gather Availability � Images stored to disk and accessed by QC View � View 2 streamers for each image combing every 9 th shot. � Utility and Images are freely available to all on the ship’s network Lauch QC View

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