KEGS- EXPLORATION 07 SYMPOSIUM GEOPHYSICAL CONTRIBUTIONS TO NEW DISCOVERIES 1 Synthetic Model...
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Transcript of KEGS- EXPLORATION 07 SYMPOSIUM GEOPHYSICAL CONTRIBUTIONS TO NEW DISCOVERIES 1 Synthetic Model...
1
KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
CONTRIBUTIONS TO NEW
DISCOVERIES
Synthetic Model Testing and Titan-24 DC Resistivity Results at Wheeler River
An Athabasca-type Unconformity Uranium Target in Northwestern Saskatchewan, Canada
By: Jean M. Legault*, Quantec Geoscience Ltd., Toronto, ONDon Carriere, Carriere Process Management Ltd., Mississauga, ON
Larry Petrie, Denison Mines Corporation, Saskatoon, SK
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
CONTRIBUTIONS TO NEW
DISCOVERIES
Wheeler River Case History
• Survey design based on initial synthetic model testing (best approach)
• Comparison of several array configurations(modeling and field application)
• Presence of major powerline impacts geophysics(choice of methods)
• Compare 2-D and 3-D Inversion results(improve understanding)
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
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DISCOVERIES
Titan 24 DCIP & MT
Overview
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
CONTRIBUTIONS TO NEW
DISCOVERIES
Common DCIP Electrode Arrays
Titan PldpdpCombinesPldp-left + Pldp-right
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
CONTRIBUTIONS TO NEW
DISCOVERIES
Standard Titan spreadN=0.5 to 23.5, a= 100m(552 data points)
Line Length 2.4 kmCurrent Injectionsinside Rx Array
N=0.5
N=23.5
Extended Titan spread(adding current extensionsbeyond end of receiver array)N=0.5-33.5, a=100m(approx. 1032 points)
Line Length approx. 4.4 kmCurrent Injections inside
& outside Rx Array
N=0.5
N=23.5
N=10.5
N=33.5
Titan-24 Pole-Dipole-Dipole Pseudosections
TITAN DCIP ARRAY CONFIGURATIONS
Note: Combinespldp & dppl data
Note: Combinespldp & dppl data
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
CONTRIBUTIONS TO NEW
DISCOVERIES
Case History: M-zone at Wheeler River
Commissioned byDenison Mines Corporation
in JV with Cameco Corporationand Japan-Canada Uranium Ltd.
April-May, 2007
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KEGS-EXPLORATION 07
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DISCOVERIES
• Define DC (+/- IP) signatures associated with:a) Uranium-bearing graphitic conductor at M-Zoneb) Granitic gneiss to the south-east of M-Zonec) Alteration chimney in sandstones above M-Zone
• Wheeler River mineralization occurs in 400m thick Athabasca Sandstone along the Unconformity, below alteration zone that is associated with underlying basement Graphitic metapelites known as the M-Zone conductive trend.
• Test Titan multi-parameter capability, with emphasis onGalvanic DC Resistivity (possibly also IP) using Pole-Dipole Array, in direct comparison with Dipole-Dipole and more widely used Pole-Pole Array.
Titan Survey Objectives
• Field Surveys were preceded by 2-D synthetic modeling study that tested for optimal array parameters (dipole size) and configurations (Pldp vs Plpl vs Dpdp array).
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
CONTRIBUTIONS TO NEW
DISCOVERIES
Introduction
Wheeler River Project
Key Lake
Moore Lake
WheelerRiverLocation:
HISTORIC NOTES
Since 1980’s, major powerline through property (along BL) – impacts EM follow-up.
Originally discovered in 1980’s (UTEM follow-up of Airborne) but remained unexplored until recently.
35km NE of Key Lake & 10km W of Moore Lake.
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
CONTRIBUTIONS TO NEW
DISCOVERIES
BASEMENT AND UNCONFORMITY HOSTED URANIUM DEPOSIT STYLES
ALTERATION ASSOCIATED WITH UNCONFORMITY-HOSTED URANIUM DEPOSITS
M-ZoneDepositStyle:
Possible Targets:
1) Alteration Zone2) Unconformity3) Basement Graphite
Mineralization occurs: a) at unconformity,b) above graphite, c) with basement elevation change.
Silicification Clay-Alteration
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
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DISCOVERIES
WHEELER M-ZONE – AIRBORNE TOTAL FIELD MAGNETICS
0 200m
Road
M-Z
ONE
M-Z
ONE
Power
line
Drillh
oles
Grani
tic G
neiss
in B
asem
ent
Pelit
ic M
etas
edim
ents
in B
asem
ent
L100S
L100S
ZM
-06
ZM
-10
ZM
-11
VR
-20
5
- Ground SurfaceOverburden (<10m) ->
Manitou Falls C ->Sandstone(80-90m thick)
Manitou Falls B ->Sandstone(100-120m thick)
Manitou Falls A ->Sandstone(70-100m thick)
Manitou Falls D ->(10-20m thick)
- Unconformity
380-400m
WHEELER M-ZONE – GEOLOGIC SECTION ACROSS L100S
Basement Rocks ->Arkose-Anatexite (blues) Pegmatite-Granite (pink)Pelite-Graphites (grey-black)
UraniumMineralizedZone
0 50m
View Looking NE
GEOLOGIC NOTES
L 100S
BL
0E
M-ZONE DRILLING
0 200m
Plan View
M-zone consists of DDH Intersections along Graphitic Conductor and Elevation Change in Basement Topography.
Basement Dips Uncertain – possibly Steep Southeast
Known Geology is based on drilling Along a Narrow Corridor, with Little Known Outside that line.
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
CONTRIBUTIONS TO NEW
DISCOVERIES
Case History: Wheeler River
2-D Synthetic Modeling
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KEGS-EXPLORATION 07
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CONTRIBUTIONS TO NEW
DISCOVERIES
Water 100 – 2 000 m
Alteration 50 -20 000 m
Graphitic Metapelite <1 -50 m
Psammitic (Felsic) Gneiss 5 - 100 k m
Fault
Unconformity
Lake seds 100 - 500 m
Sandstone 2 000 – 5 000 m
Granite 10 - 100 k m
Overburden 10 - 100 k m
Metapelite 50 -1 000 m
Contact
UC
(from Witherly, 2005)
GEOPHYSICAL PROPERTY MODEL for ATHABASCA-TYPE URANIUM DEPOSITS
300m -
1000m -
UBC 2d SyntheticForward Model Data
2d Reference Model
Note: 1500m (n=10)Current extensions
C) Extended TitanPole-dipole Arraya=150m / n=0.5-33.5
6.75 km Total array length
150m A-spacing
10-10kohm-metres
0 500m
300m -
1000m -
UBC 2d SyntheticForward Model Data
2d Reference Model
B) Extended TitanPole-dipole Arraya=100m / n=0.5-29.5
Note: 600m (n=6)Current extensions
3.7 km Total array length
100m A-spacing
10-10k ohm-metres
0 500m
3000 ohm-m
300m -
1000m -
UBC 2d Synthetic Forward Model Data
2d Reference Model
Note: 500m (n=10)Current extensions
A) Extended TitanPole-dipole Arraya=50m / n=0.5-33.5
2.2 km Total array length
50m A-spacing
10-10k ohm-metres
0 500m
1000 ohm-m
3000 ohm-m
5 ohm-m100m
1000 ohm-m
3000 ohm-m
5 ohm-m100m
1000 ohm-m 5 ohm-m
100m
3000 ohm-m
Titan Multi-Array DC Survey 2D DC Forward Models
Note: Gp response onlyat base of pseudosection, i.e.,50m a-spacing likely providesinsufficient penetration
Note: Gp response in middle,i.e., 100m a-spacing likely providessufficient penetration and focuswithin Sandstone and Gp
Note: Gp response in upper 1/3,i.e., 150m a-spacing possiblyexceeds required penetrationlacks and focus within Sandstone
2d DC ResistivityPole-pole Array
Range
10 to 10kohm-metres
500m -
1000m -
0m -
C)
0 500m
1500m -Loke 2d Inversions using Res2dInv (Loke and Barker, 1996)
2d DC ResistivityDipole-dipole Array 500m -
1000m -
Range
10 to 10kohm-metres0m -
A)
-300m Unconformity
-300m Unconformity
2d DC ResistivityPole-dipole Array
500m -
1000m -
0m -
B)
Range
10k to 10ohm-metres
Multi-Array Survey 2D Synthetic DC Inversions
-300m Unconformity
Note: Dpdp provideshigh resolution but possibly lacks depth penetration
Note: Pldp providesgood balance between resolution and depth penetration
Note: Pldp providesbest depth penetrationbut possibly lacks deep resolution
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
CONTRIBUTIONS TO NEW
DISCOVERIES
Case History: Wheeler River
DC/IP Field Tests along L100S
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
CONTRIBUTIONS TO NEW
DISCOVERIESROAD
M-Z
ONE
M-Z
ONE
0 1km
POW
ERLINE
L100S
L100S
Range
10 to 10k
ohm-metres
Pole-Pole Array Pole-pole Array
Range
0 to 30
milliradians
(a=100m / n=0.5-27.5 / 0.73A avg) (a=100m / n=0.5-17.5 / 0.73A avg)
N=27.5 -
- N=17.5
Range
10 to 10kohm-metres
Pole-dipole Array Pole-dipole Array
Range
0 to 30
milliradians
(a=100m / n=0.5-33.5 / 0.51A avg) (a=100m / n=0.5-19.5 / 0.51A avg)
N=33.5 -
- N=19.5
Line 100S Titan DC Survey 2D DC/IP Pseudosections
0 500m
1160 of 1166 total pts(>99%) retained for Inversion
785 of 1166 total pts(68%) retained for Inversion
1089 of 1150 total pts(95%) retained for Inversion
571 of 1150 total pts (50%) retained for Inversion
Apparent Resistivity Pseudosections(Max 10% Vp error shown)
IP Phase Pseudosections(Max 3mrad error shown)
Dipole-dipole Array Dipole-dipole Array(a=100m / n=0.5-28.5 / 0.55A avg) (a=100m / n=0.5-17.5 / 0.55A avg)
Range
10 to 10kohm-metres
Range
0 to 30
milliradians
N=28.5 -
- N=17.5
887 of 1091 total pts(81%) retained for Inversion
431 of 1091 total pts(40%) retained for Inversion
?
?
Note: Coincident DCLow + IP High over Gp
Note: Weaker DC Lowand No IP high over GP
Note: Strong but Wide DC Low + No IP
high over GP
2d DC ResistivityPole-dipole Array
500m -
1000m -
0m -
B)
Range
10k to 10ohm-metres
-400m Unconformity
2d DC ResistivityDipole-dipole Array
500m -
1000m -
Range
10 to 10kohm-metres
0m -
A)
2d DC ResistivityPole-pole Array
Range
10 to 10kohm-metres
500m -
1000m -
0m -
Loke 2d Inversions using Res2dInv (Loke and Barker, 1996)
C)
-400m Unconformity
-400m Unconformity
0 500m
Line 100S Titan DC Survey 2D DC Inversions
Note: Dpdp provides high resolution but lacks depth penetration
Note: Pldp provides best balance between resolution and penetration
Note: Plpl provides most depth penetration but possibly lacks resolution
Range
10 to 10kohm-metres
2d DC Resistivity 500m -
1000m -
0m -
Range
0 to 50milliradians
2d IP Chargeability 500m -
1000m -
0m -
2d PW MT TM-TE Resistivity
Range
10 to 10kohm-metres
500m -
1000m -
0m -
1500m -Quantec PW2dia Inversions based on algorithm by de Lugao and Wannamaker (1996)
Loke 2d Inversions using Res2dInv (Loke and Barker, 1996a)
Loke 2d Inversions using Res2dInv (Loke and Barker, 1996a)
Line 100S DC, IP & MT2D & 3D Inversions
0 500m
Alteration Zone
Alteration Zone
Gra
phite
Gra
phite
Alteration Zone?
-400m Unconformity
-400m Unconformity
-400m Unconformity
Gra
phite
?
Granite-Metasedim
ent Contact?
Granite Contact?
Granite Contact?
3d DC Resistivity
3d IP Chargeability
Loke 3d Inversions using Res2dInv (Loke and Barker, 1996b)
Loke 3d Inversions using Res2dInv (Loke and Barker, 1996b)
Alteration Zone
Gra
phite
Alteration Zone?
500m -
1000m -
0m -
500m -
1000m -
0m -
Gra
phite
Granite Contact?
Granite Contact?Note: 2d DC suggests W-dipfor M-zone
Note: M-zone poorly resolved
Note: M-zone alteration appears well resolved but conductor dip andcontrast differs w DC
Note: 3d DC indicates steeper dip
Note: 3d IP resolves M-zone
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
CONTRIBUTIONS TO NEW
DISCOVERIES
A) Z=20mZ=50mZ=100m
Note: Powerline Visiblein Near Surface
Z=150mZ=200mZ=250mZ=300m
Note: Alteration Visible100m above UC
Z=350mZ=400mZ=450mZ=500m
Note: Graphite Visiblein Basement
Z=550mZ=600mZ=650mZ=700mZ=750mZ=800mZ=850mZ=900mZ=950mZ=1000mZ=1050mZ=1100mZ=1150mZ=1200mZ=1250m
Note: Migration of GraphiteConductive Zone to NW
Z=1300m
WHEELER M-ZONE – 3-D VOLUME of 2-D SMOOTH DC RESISTIVITY
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
CONTRIBUTIONS TO NEW
DISCOVERIES
Z=20mZ=100m
Note: PL+Road+NoiseVisible in Near Surface
Z=300m
Note: Alteration in IP low above UC?
WHEELER M-ZONE – 3-D VOLUME of 2-D SMOOTH CHARGEABILITY
Z=500m
Note: Graphite IP High?
Z=700m
Note: Graphite IP High?
Z=900m
Note: Graphite IP High?
Z=1100m
Note: Graphite IP High?
Z=1400m
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
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DISCOVERIES
WHEELER M-ZONE – 3-D VOLUME of 3-D SMOOTH RESISTIVITY
Z=20mZ=100m
Note: Powerline correlateswith near surface DC low
Z=300m
Note focused DC resistivitylow 100m above UC
Z=500m
Note: Graphite wellresolved in basement
Z=900m
Note: Absence of NWmigration in Gp signature
Z=1300m
Note: Absence of NWmigration in Gp signature
Z=1400m
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KEGS-EXPLORATION 07
SYMPOSIUMGEOPHYSICAL
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DISCOVERIES
WHEELER M-ZONE – 3-D VOLUME of 3-D SMOOTH CHARGEABILITY
Z=200mZ=100m
Note: Layer-like IP-High zone in sandstone?
Z=300m
Note widespreadpresence of IP highlayer in sandstone
Z=500m
Note: Well definedIP high along DC low
(except on north lines)
Z=900m
Note: Well definedIP high along DC low(also on north lines)
Z=1300m
Note: Well definedIP high along DC low(also on north lines)
Z=1400m
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KEGS-EXPLORATION 07
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DISCOVERIES
Study Findings
• Field surveys corroborated our initial 2-D DC synthetic modeling studies, i.e., Dpdp offered best resolution but poorest penetration; Plpl had greatest penetration but poorer resolution; Pldp had better combination of resolution, penetration and economy.
• MT data quality excellent – not hindered by ground contacts or Powerline effects – confirms all season capability.
• DC resistivity data quality and survey productivity greatly improved current injections (>0.5A avg), thanks to more powerful GDD Tx – suggests >2-3 season capability for DC/IP.
• Multi-parameter DC-IP-MT results show remarkable similarities and contrasting behaviour (i.e., DC vs MT; 2D vs 3D).
• DC resistivity results do not appear to be significantly hindered by powerline effects, but IP significantly more affected (acceptable).
• Coincident DC+MT resistivity low and IP high confirmed over graphite > additional tool for geologic mapping & discrimination.
• 3-D inversions simplify, improve understanding of responses.
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KEGS-EXPLORATION 07
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CONTRIBUTIONS TO NEW
DISCOVERIES
Titan-24 DC Resistivity Results at Wheeler River
Thank You
CAMECO CorporationSaskatoon, SK
DENISON MINES CorporationToronto, ON
Japan-Canada UraniumTokyo, Japan
Toronto, ON