i 2.40276 i received znog · vlf-em survey survey results magnetic survey results vlf-em survey...

I I I I I I I I I I I I I I I I I I I -

- -2.40276

PHASE ONE GEOPHYSICAL REPORT

FOR SAN GOLD CORPORATION

ON THE BIG MARSH LAKE PROPERTY

CARS CALLEN & BRISTOL TOWNSHIPS PORCUPfNE MINfNG DIVISION

NORTHEASTERN, ONTARIO

RECEIveD

JAt 2 1 znog GEOSCIENCE ASSESSMENT

OFFICE

Prepared by: John C. Grant, CET, FGAC November, 2008


TABLE OF CONTENTS

INTRODUCTION

PROPERTY LOCATION AND ACCESS

CLAIM BLOCK

PERSONNEL

GROUND PROGRAM

MAGNETIC SURVEY

VLF-EM SURVEY

SURVEY RESULTS

MAGNETIC SURVEY RESULTS

VLF-EM SURVEY RESULTS

FOLLOW -UP PROGRAM

IP SURVEY

IP SURVEY RESULTS

CONCLUSIONS AND RECOMMENDATIONS

AUTHOR'S NOTE

CERTIFICATE

LIST OF FIGURES FIGURE 1: FIGURE 2: FIGURE 3:

LOCATION MAP PROPERTY LOCATION MAP CLAIM MAP/GRID MAP

PAGE

2

2

2,3

3

3

4

4,5,6

6

6

6,7

7TO 16

18

LIST OF APPENDICIES APPENDIX A: SCINTREX ENVI MAG SYSTEM APPENDIX B: G.D.D. IP RECEIVER, GRx8-32

G.D.D. TRANSMITTER,TXII 3600W


LIST OF INSERTS:

POCKET MAPS:

COMPILATION OF THE TOTAL FIELD MAGNETIC SURVEY WITH THE VLF-EM CONDUCTORS AND CHARGEABILITY ANNOMAL Y TRENDS. GEOPHYSICAL AND GEOLOGICAL COMPILATION VLF-EM SURVEY WITH CONDUCTOR AXIS.

TOTAL FIELD MAGNETIC SURVEY WITH IP AND VLF ANOMALIES IN COLOR, 1 :5000 VLF-EM SURVEY WITH CONDUCTOR AXIS, 1:5000 INDIVIDUAL IP LINE PSEUDO-SECTIONS FOR LINES 900MW TO 2300MW INCLUSIVE IN COLOR, SCLAE 1 :2500

I I I I I I I I I I I I I I I I I I I •

Page 1

INTRODUCTION:

The services of Exsics Exploration Limited were retained by Mr. J. Boissonneault 011 behalf of the Company, San Gold Corporation to complete a detailed ground geophysical program across a portion of their claim holdings in Bristol and Carscallen Township. Both townships are part of the Porcupine Mining Division in Northeastern Ontario.

This property covers a felsic intrusive unit that lie just to the north of the Destor·· Porcupine fault that cuts across the Porcupine mining camp and is and has been the host of most of the gold deposits in the camp. The property is also just to the west and along strike of the gold deposit that is currently being drilled and developed by Lake Shore Gold located in the southwest section of Bristol Township.

There are several airborne conductors present within the grid area that are striking northwest to southeast that will be covered by the ground program.

The present program consisted of a detailed, total field magnetic survey that was done in conjunction with a VLF-EM survey. These survey methods are excellent mapping tools to define the geological characteristics of the property as well as to define potential electromagneti(; horizons that may relate to sulphide minearlization.

This report will detail the results of this present program as well as all conclusions and recommendations.

PROPERTY LOCATION AND ACCESS:

The Bigmarsh Lake property is located in the east central portion of Carscallen Township and the western section of Bristol Township of the Porcupine Mining Division in Northeastern Ontario. More specifically the property is located approximately 18 kilometers west of the City of Timmins and just to the immediate east of Bigrnarsh Lake. The survey area is located approximately 9 kilometers north of Highway 101 west.

Access to the grid during the survey period was ideal. Highway 101 runs just to the south of the property and a series of ingress gravel roads and A TV trails allowed for good ground access to the grid area and throughout the cut lines. Traveling time from the City of Timmins to the property is approximately 45 minutes. Figures 1 and 2.

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LEGEND / LfGENDE 8 National capital / • Capitale nationale

o Provincial capital / Capitale provinciale

• Other populated places / Autres lieux habites

_ .;.. _ Trans-Canada Highway / - La Transcanadlenne

Major road I Route principale

_._. International boundary / Frontiere internationale

_ .. _ Provincial boundary / Limite provinciale

Hudson Bay Baie d'Hudson

James Bay

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L PO Box IBBO, P4N-7J(1 m EXSICS EXPLORATION LTD. Suite 13, Hollinger Bldg, Timmlls Ont. ~-::-:c--=-_ _ T_e_Ie~phone: 705-267-4151. 267-2424 CUF..NT: SAN GOW CORPORATION

PROPERTY: B1GMARSH LAKE PROPERTY TITLE: CARSCALLEN TOWNSHIP

LOCATION MAP


Page 2

CLAIM BLOCK:

The claim numbers that represent the holdings of San Gold in the area and that were covered by the current ground program are as follows:

P-4212529 12 units P-4202663 16 units P-4202662 9 units P-4212522 3 units P-4210999 4 units P-4211013 16 units P-4213856 4 units P-4202665 4 units P-4204384 14 units P-4213855 9 units P-3019638 6 units P-3019639 11 units P-3019640 2 units P-4213856 4 units

Refer to Figure 3 that has been copied from the MNDM Plan Map G-3040 of Carscallen Township and MNDM Plan Map G-3998 of Bristol Township.

PERSONNEL:

The field crew directly responsible for the collection of the raw Magnetic and VLF-EM, data were as follows.

E. Jaakkola Timmins, Ontario R. Bradshaw Timmins, Ontario

The field crew directly responsible for collecting and completing the IP survey were as follows.

M. Cayen Timmins, Ontario P. Lemire Timmins, Ontario J. Hamlin Timmins, Ontario D. Poirier Timmins, Ontario J. Francoeur Timmins, Ontario

The ground program was completed under the direct supervision of J.c.Grant and all of the plotting and compilation was completed by in-house staff.

GROUND PROGRAM:

The ground program was completed in three phases. The first phase was to establish a detailed metric grid across the property. This was done by first cutting a base line across the grid from the west boundary to the east boundary of the claim block. Lines were then turned off of this base line at 100 meter intervals from line 900MW to and including 2300ME. Lines 900MW to 700MW were cut and chained from 800MS to 800MN. Lines 600MW to 500ME were cut and chained from 800MS to 2400MN. Lines 600ME to 1100ME were cut and chained from 2400MN to 2000MS with lines 1200ME to 1900ME were cut from the base line to 1600MS. Lines 2000ME to 2300ME were cut from the base line to 1600MS A tie line was cut parallel to the base line at 800MN to control the cross lines. All of these cut lines were then chained with 25 meter station intervals. In all, a total of 94.50 kilometers of grid lines were established across the property from the 20th of May to the 30th of November 2008.

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4201


PORCUPINE Mining Division - 136071 - GERVAIS, LARRY NOEL I

Township/ Area Claim Recording Claim

Status Percent Work Total Total Claim

Number Date Due Date Option Required Applied Reserve Bank BOND 1218962 1996-Nov-07 2009-Nov-09 A 75 % $ 3,200 $ 16,000 , $ 356 $0

BOND 4215956 2008-Mar-27 201O-Mar-27 A 90% $ 4,000 $ 0 I $0 $0 BRISTOL 3012035 2004-Mar-24 2010-Mar-24 A 100% $ 6,400 $ 25,600 $0 $0

BRISTOL 3012036 2004-Mar-24 20 1 0-Mar-24 A 100% $ 6,400 $ 25,600 $0 $0 BRISTOL 3015806 2007-Sep-12 2009-Sep-12 A 25% $ 800 $ 0 I $0 $0 BRISTOL 3016554 2004-Mar-26 20 1 O-Mar-26 A 100% $ 6,000 $ 24,000 . $0 $0

BRISTOL 3016555 2004-Mar-26 20 1 0-Mar-26 A 100% $ 1,600 $ 6,400 $0 $0

BRISTOL v 3019639 2007-May- 2009-May- A 50% $ 4,400 $0 $0 $0 07 07

BRISTOL 3QI9640 2007-May- 2009-May- A 50% $ 800 $0 $0 $0 07 07

BRISTOL 4200738 2005-0ct-12 2009-0ct-12 A 100% $400 $ 800 I $ 1,866 $0 BRISTOL 4202662 2006-0ct-1O 2009-0ct-l0 A 34 % $ 3,600 $ 3,600 , $0 SO BRISTOL 4212414 2007-Mar-23 2009-Mar-23 A 67% $ 3,200 $0 1 $0 $0 BRISTOL 4212415 2007-May- 2009-May- A 67% $ 4,800 $ 0 i $0 $0

18 18

BRISTOL 4212424 2007-May- 2009-May- A 67% $ 1,600 $0 $0 $0 18 18 I

BRISTOL 4212522 2006-0ct-16 2009-0ct-16 A 34% $ 1,200 $ 1,200 $0 $0 BRISTOL 4213~58 2007 -Oct-17 2009-0ct -17 A 67% $ 800 $0 $0 $0 BRISTOL 4215519 2007-Sep-27 2009-Sep-27 A 67% $ 800 $0 I $0 $0 BRISTOL 4224265 2008-Jan-25 2010-Jan-25 A 67% $ 1,600 SO I $0 $0 CARSCALLEN v 3019618 2007-May- 2009-May- A 50% $ 2,400 $0 $0 $0

07 07

CARSCALLEN 420266,J 2006-0ct -10 2009-0ct -10 A 34% $ 6,400 $ 6,400 $0 $0

CARS CALLEN 4202665 2006-0ct-I I 20II-Oct-1 1 A 34% $ 1,600 $ 4,800 $0 $0

CARSCALLEN 42Q4384 2006-Aug- I I 201O-Aug- 11 A 50% $ 5,600 $ 11,200 $0 $0

CARSCALLEN 4210999 2006-0ct-16 2009-0ct-16 A 34% $ 1,600 $ 1,600 $0 $0

CARSCALLEN 42 11013 2006-Jun- I 9 2010-Jun-1 9 A 100% $ 6,400 $ 12,800 $ 26,933 $ 0

CARSCALLEN 4212498 2007-Jan-15 2009-Jan-15 A 67% $ 1,600 $0 I $0 $0

CARSCALLEN 4212529 2006-0ct- I 1 2009-0ct- 11 A 34 % $ 4,800 $ 4,800 I $0 $0

CARS CALLEN 4213799 2007-Feb-20 2009-Feb-20 A 50% $ 4,800 $0 ! $0 $0

CARS CALLEN 4213854 2007-Feb-07 2009-Feb-07 A 50% $ 2,000 $0 $0 $0

CARSCALLEN 42 13855 2007-Feb-07 2009-Feb-07 A 50% $ 3,600 $0 $0 $0

CARSCALLEN 4213856 2007-Feb-07 2009-Feb-07 A 50% $ 1,600 $0 $0 $0

CARS CALLEN 4226028 2007-Dec-07 2009-Dec-07 A 100 % $ 1,200 $0 $0 $0

CARSCALLEN 4226029 2007-Dec-07 2009-Dec-07 A 100% $ 1,600 $0 $0 $0

CARS CALLEN 4243Q75 2008-Jun-l1 2010-Jun-l1 A 50% $ 2,800 $0 $0 $0 , .. - . . .. .. . . . .

The colored claim numbers represent the San Gold optioned claims in Bristol and Carscallen Townships some of which were covered by the Phase one program.


Page 3

Upon the completion of the line cutting the second phase of the program consisted of a detailed Total Field Magnetic and a VLF-EM survey that was completed across all of the cut lines. This survey was done using the Scintrex, Envi Mag system for both the field unit and for the magnetic base station recorder. Specification for this unit can be found as A£pendix A of this report. Thte entire program was completed between May 20th and November 30 2008

The following parameters were kept constant throughout the survey.

MAGNETIC SURVEY: Line spacing Station spacing Reading Interval Diurnal Monitoring Record interval Reference field Datum subtracted Unit accuracy Parameters measured

100 meters 25 meters 12.5 meters base station recorder 30 seconds 57,000 nT 56,500 nT +/- 0.1 Nt Systematic measurements of the earth's total field in (nT)

Upon the completion of the magnetic survey, the collected magnetic data was corrected through the base station data to eliminate diurnal variances and the data had a background of 56,500 nT removed from each corrected reading for ease in plotting purposes only. The corrected and leveled data was then plotted directly onto a base map at a scale of 1 :5000 and then contoured at 10 gamma intervals wherever possible. A copy of this contoured base map is included in the back pocket of this report.

VLF-EM SURVEY:

Line spacing: Station spacing: Reading intervals: Transmitter station/frequency: Transmitter direction: Parameters measured:

Parameters plotted:

100 meter intervals 25 meters 12.5 meters Cutler Maine, 24.0 kHz Azimuth 115 degrees Inphase and quadrature components, Field strength In phase component, in percent

Upon the completion of the surveys, the collected in phase data was then plotted directly onto a base map at a scale of 1:5000 and then profiled at lcm to +/- 10 percent. Any and all conductor axis were then interpreted and placed on this base map. The Government Airborne survey that was issued in 1988 showed a number of conductors scattered across the grid area and these conductors have also been added to the VLF-EM base map for correlation.


Page 4

A copy of this profiled base map with full interpretation of all VLF-EM conductor axis is included in the back pocket of this report.

SURVEY RESULTS:

The results of the geophysical program will be discussed in detail in the following text. The magnetic and VLF·EM surveys are excellent methods for outlining the geological structures across the survey area.

MAGNETIC SURVEY RESULTS:

The magnetic survey was very successful in locating and outlining the geological structures underlying the grid area. The most predominant structures outlined by the magnetic survey are a series of north-south striking magnetic highs that generally parallel the grid lines. The first structure was noted between lines 800MW and 900MW. This unit has been cross cut by at least 3 to 4 northwest to southeast striking highs and lows. The second north-south striking zone is a well defined high paralleling line 100MW from 200MN to the north end of the grid line and it continues off of the grid to the north. The southern extension of this dike like magnetic: high appears to have run into a probable fault like cross structure that generally cuts across the entire grid in a northwest to southeast direction and can be traced from line 900ME at 300MS to at least line 900MW at 600MN. The southern extension of this north-south zone has been offset by the cross faulting and generally parallels line 100ME from the base line to at least 400MS were it appears to have been cross cut by a magnetic low that can be traced from line 100ME to 900MW at 300MS where it continues off of the grid to the west.

There is a third magnetic high that generally parallels lines 900ME and 1000ME from the south ends of the line to the base line where it also seems to be faulted and or distorted by the same magnetic low that interrupted the dike to the immediate east. This north striking high has then been shifted to the east and parallels lines 11 OOME and 1200ME and continues off of the grid to the north. The cross structure that offset the high to the west also distorts the shape of this high in the vicinity ofline 1000ME at 300MS.

Another interpretation might suggest that this dike like unit has offset the northwest to southeast cross structure at IOOOME and 300MS and shifted it to the north and east where it appears as a good magnetic high with and associated VLF-EM zone striking east across lines 1300ME to 1700ME at lOOMS to 200MS.

This zone may have offset the next dike like unit that is paralleling lines 1900ME. This dike like unit has been offset to the northeast and continues off of the grid along line 2000ME.

The southern extension of the fourth dike continues along 1800ME but it has been cross cut by at least 4 southeast striking structures at Tie line 800MS, lOOMS, 1300MS and 1650MS. Each of these cross structures were noted by the VLF-EM survey as well.

The last north-south striking zone seems to parallel line 2300ME from 1000MS to the base line and appears to continue off of the grid to the north and east.


Page 5

There are at least 5 northwest to southeast cross structures that cut across the entire cut grid. Three of these structures have had major effects on the strike directions of the dike like units discussed earlier in this report. There are two parallel structures that generally cross cut all of the dikes and strike across the entire cut grid and continue off of the grid area in both directions.

The first of these units can be followed from line 900MW to 200MW from 700MN to 350MN. This zone has tenninated the most westerly dike like unit at it's northern end and runs into the next dike at 200MW at 350MN. The zone then appears top continue to the southeast as a weak to modest and narrow high from lOOME at 300MN to line 1000ME at the base line. The zone them runs into another north striking dike, possibly pinching it and the continues as a good strong magnetic high from 1300ME to at least 2100ME where it appears to have folded the fourth dike at the northern end before stopping at the most easterly dike. There is good correlation between the magnetic and VLF-EM survey with this high. The VLF survey shows a good conductive zone that is either directly associated with this narrow high or runs along the north and or south shoulders of the high. In most cases, the VLF trends have been cut off by the dikes.

The second northwest to southeast striking magnetic trend closely parallels the above trend and it can be traced from line 900MW at 325MN to 1000ME at 275 to 300MS. The dike at this point appears to be shifted to the east by this cross structure. The narrow high then continues southeast across lines 1300ME!550MS to 1800ME1750MS where it again appears to offset the dike along Tie line 800MS and then it continues into the dike to the immediate east.

Again the VLF zones are either directly associated with this unit and or parallel the flanks of the high.

There is a well dermed and narrow magnetic low striking northwest to southeast across the entire grid. This zone can be followed from line 900MW at 300MS to line 2300ME at 1300MS and it either distorts, terminates or interrupts the north-south striking dikes. The fault is a major structural trend and it may represent a splay striking off of the Porcupine-Destor fault to the southeast. The trend of this fault structure should it continue to the southeast would put it in line with Lakeshores Gold deposit to the southeast of this property.

This fault structure appears to continue off of the San Gold property to the southeast and the assumption is that if it did continue on it's present strike direction it would run into the junction of the Porcupine-Des tor Fault and the Lakeshore Gold deposit.

Another parallel magnetic trend that is striking northwest to southeast lies between line 1300ME at 1400MS to line 1900ME at 1650MS that continues off of the grid to the southeast. This structure has folded and or faulted the dike paralleling lines 1700ME and 1800ME. This zone has good correlation with the VLF zones that strike across lines 1600ME to 1900ME.

A similar looking magnetic trend parallels this zone and it lies between line 1700ME at 1300MS to 2300ME at 1425MS. This zone also parallels the fault structure to the immediate north. This zone also cuts off the dike and continues off of the grid to the southeast.


Page 6

A final northwest to southeast magnetic trend was noted at the southern ends of line 600ME at 1800MS to line 1500ME at 1900MS. This zone is represented by a moderate magnetic high that is evident on both sides of the dike. The zone correlates directly with a good VLF-EM zone for most of it's strike length.

VLF-EM SURVEY RESULTS:

The VLF-EM survey was successful in locating a number of conductive horizons across the grid area. At least 3 or 4 of these zones lie within the swann of airborne targets that had been identified in the 1988 release. These zones are the features that strike across lines 800MW to 900ME between 750MN and 300MN and the broken zone between 900MW at 700MS to 200ME at 750MS north of Tie line 800MS.

Generally the VLF-EM zones parallel the northwest to southeast magnetic trends that were noted on the grid. The VLF zones either directly correlate with these features or lie along the north and or south flanks of the highs. These VLF zones are well defined and in most cases they either stop at the dikes or are distorted by the dikes.

The major fault zone was also detected by the VLF survey with conductive axis either directly associated with the fault or lying along the edges of the fault. The zones also appear to cut through the dikes instead of being offset or distorted by the dikes.

FOLLOW-UP GROUND PROGRAM:

The IP program was done to follow up on the magnetic and VLF-EM results that had been completed earlier across the grid area. The IP survey commenced on line 900MW of the grid and was read from this line to line 2300ME. In all, a total of 72.60 kilometers of grid lines have been covered by the IP survey currently and the survey is to continue to the northeast and north of the existing coverage.

This survey was done using the G.D.D. Receiver and the G.D.D. 3.6 kilowatt transmitter. Specification for these units can be found as Appendix A of this report. This phase of the IP program began on the 7th of July and was completed on the 21 st of October 2008 and is ongoing at the time of this report. The following parameters were kept constant throughout the survey.

IPSURVEY:

Line spacing Station spacing Reading Interval IP method: IP array: IP mode: Delay time Transmitter time: Number of electrodes & spacing: Parameters measured:

100 meters 25 meters 25 meters Time domain Pole-dipole Arithmetic 240ms 2 seconds on, 2 seconds off 6 stainless steel, 25 meters Apparent resistivity and chargeability

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Page 7

Upon the completion of the IP survey, the collected data was the plotted onto individual line pseudo-sections, one such section for each of the lines read, at a scale of 1 :2500. These sections show the contoured results of the chargeability and resistivity as well as a calculated Metal Factor. A copy of these contoured sections are included in the back pocket of this report.

IP SURVEY RESULTS:

The IP results for each of the grid lines will be discussed in detail as well as any correlation to the Magnetic and VLF-EM surveys. The IP survey results will be completed in a west to east direction.

LINE900MW:

There is a strong IP anomaly lying between 450MS and 300MS that correlates to a good resistivity low as well as a modest magnetic low that lies to the immediate west of a dike like unit. This zone also correlates to an airborne target. The zone probably relates to a graphitic zone. There may be two zone combined here that are too close together for the present survey to separate.

Another broad IP anomaly lies between the baseline and 150MN that correlates to a broad weak resistivity high and it also lies just to the west of the dike like unit.

A third zone is a well-defined target lying between 450MN and 550MN that correlates to a broad resistivity high. This zone lies along the southern edge of a magnetic unit that appears to strike northwest to southeast across the entire grid.

LINE 800MW:

The IP results show the same graphitic horizon lying between 550MS and 350MS that again correlates to a good resistivity low unit and a magnetic high that appears to lie within the dike like unit. Again there may be two parallel zones situated here that are too close for the survey to separate.

A second zone lies between lOOMS and 100MN that correlates to a broad resistivity high unit that in-tum appears to have been cross cut by a narrow resistivity low which may be indicative of the eastern edge of the dike like unit.

A final zone lies between 375MN and 525MN that correlates to a broad weak resistivity high and the southern edge of the magnetic unit striking across the grid.


Page 8

LINE700MW:

There is a good IP anomaly situated between 550MS and 300MS that correlates to a known graphitic horizon and it is well represented in the IP survey results. The second zone is now becoming a bit more defined as the two zones appear to be separating more as they head east across the grid. Again the zone correlates to a resistivity low as well as a weak magnetic high and a VLF zone that lies just to the east of the dike like unit. The zone also correlates to the airborne target. The second zone lies between the base line and 200IVIN and this zone also correlates to a broad and deep resistivity high as well as a modest magnetic high.

The last zone is a weak zone lying between 350MN and 500MN that correlates to a broad resistivity high as well as the southern limb of the magnetic structure striking across the grid area.

LINE 600MW:

The graphitic horizon is still well defined between 600MS and 350MS as well as the parallel zone that lies just to the north of the zone. The anomaly is a textbook IP response to this sort of conductor which is a well defined IP anomaly with an associated resistivity low. The zone also correlates to a narrow magnetic low and the airborne targets.

The second zone is a well defined IP anomaly between the base line and 150MN that correlates to a broad and deep resistivity high and a broad magnetic high and a VLF zone just to the east of the dike.

A third zone lies between 300MN and 400MN that correlates to the same deep resistivity high and again lies along the southern edge of the northwest to southeast magnetic structure.

A final zone is between 525MN and 650MN and it appears to be a broad weak zone at depth that correlates to a modest resistivity high and it lies along the north edge of the magnetic high unit that strikes northwest to southeast across the grid.

LINE500MW:

The southern graphitic horizon is still present between 600MS and 400MS however it now correlates to a shallow resistivity low that is flanked by a resistivity high to the south. The zone generally correlates to a magnetic low.

The second zone lies between lOOMS and 50MN and it correlates to a moderate and deep resistivity high and a modest magnetic high. The zone also correlates directly with a VLF zone.

The third zone lies between 200MN and 300MN and correlates to a deep rooted resistively high and the southern limb of a good magnetic unit.

A final zone lies between 500MN and 575IVIN and correlates to a moderate and deep resistivity high and the north limb of the same magnetic trend that host the IP anomaly to the immediate south.


Page 9

LINE400MW:

The southern zone is still well defined on this line and it correlates to a well-defined resistivity low and magnetic low. The second zone is a well defined IP anomaly situated between 50MS and 75MN and it correlates to a deep rooted resistivity high and the southern edge of a modest magnetic trend that is striking northwest to southeast between the two dike like units. The third zone lies between 250Mn and 350MN and it is a weak zone with a broad resistivity high at depth. This zone lies at the southeast tip of the magnetic unit striking northwest to southeast across the grid, just to the west of a second dike like unit.

The final zone lies between 550MN and 650MN and it correlates to a deep and broad resistivity high and a narrow magnetic high striking east off of the dike.

LINE300MW:

The southern graphitic zone is still well defined on this line but it appears to be migrating southward. The zone correlates to a shallow resistivity low that is flanked by highs on both sides. The magnetics show a low association with this target.

The second zone lies between 150MS and the base line and it too appears to be migrating to the south. It correlates to the northern edge of a deep-rooted resistivity high and a broad magnetic high just to the west of the second dike.

Another zone lies between 175MN and 250MN that correlates to a modest resistivity high and a magnetic low situated between the two dikes.

The final zone lies between 450MN and 600MN and correlates to a deep-seated resistivity high and a broad modest magnetic high.

LINE 200MW:

The southern zone appears to be migrating off of the grid to the south. It still correlates to a resistivity low as well as a magnetic low that also seems to be striking off of the grid to the south.

The second zone lies between 200MS and lOOMS and it is still moving southward on the grid. It correlates to a deep-seated resistivity high and possibly the western edge of the second dike like unit paralleling lines 200MW and line 0+00.

The third zone lies between 50MN and 200MN and it correlates to a moderate resistively High and a bulging mag high located on the western edge of the dike.

The final zone lies between 375MN and 525MN and it lies on the northern edge of a moderate resisti vity high and a magnetic low located on the western edge of the dike.

LINE lOOMW:

The southern zone has almost disappeared off the southern edge of the grid line as it continues southward. The second zone lies between 200MS and 50MS and it correlates to a modest resistivity high and the western edge of the dike. The third zone lies between 100MN and


Page 10

225MN and it lies along the southern edge of a moderate resistivity high and is associated with the dike.

The fourth zone lies between 400MN and 550MN and correlates to a moderate resistivity low as well as the center of the dike.

The last zone is a deep zone between 650MN and 750MN that correlates to a deep resistively high and it also is within the center of the dike.

LINE 0+00:

The southern zone is still present between 700MS and the south end of the line and it correlates to a modest resistivity low and a broad magnetic high which may be the southern end of the dike.

The second zone lies between 150MS and the base line and it is a broad zone with a deep-seated resistivity high that lies within the dike like unit and corresponds to a modest VLF zone.

A third zone lies between 150MN and 250M1'J" and it correlates to a resistivity low and the magnetic structure that is striking across the dike in a southeast direction.

The fourth zone is a broad strong response between 500MN and the north end of the grid line that correlates to a good resistivity low and a budging on the east side of the dike.

LINE 100ME:

A good broad zone lies between 300MS and lOOMS that lies on the southern edge of a resistivity high and correlates to the southern extension of a dike like mag unit.

The zone that lies between 50MN and 200MN lies on the northern flank of the same resistivity high and it appears to be getting stronger at depth. It correlates to a narrow magnetic high that strikes northwest to southeast across the entire grid and it is this feature that has offset the dike.

The last zone is a broad anomaly that lies between 375MN and 700Mn and seems to parallel the eastern edge of the dike. This zone has a good resistivity low associated with it.

LINE 200ME:

There is a good strong zone building up on the southern end of the grid that has an associated resistivity low as well as a magnetic low. This zone lies just to the south of the main fault zone on the grid.

There is a text book style anomaly between 200MS and 50MS that lies on the southern flank of a good resistivity high and this correlates to the eastern edge of the dike and lies just to the south of one of the major northwest to southeast striking mag trends.

A weak and deep zone is situated between 75MN and 150MN that correlates to a broad magnetic low and lies on the northern edge of the resistivity high. A final broad and strong zone lies between 350MN and 650MN that correlates to a resistivity low and represents the known airborne string of targets outlined in the 1989 survey. Several VLF zones lie within this zone.


Page 11

LINE 300ME:

There is a good zone between 350MS and 150MS that correlates to a modest magnetic low to the east of the dike and it also correlates to a VLF zone. The zone lies on the southern edge of a broad resistivity high.

A weak deep zone was noted between 50MN and 150Mn that lies on the northern flank of the same resistivity high and this target lies just to the north of the main cross structure.

A final broad zone lies between 300MN and 650Mn that correlates to a good broad resistivity low. The zone is also host to at least two VLF zones and correlates to the government airborne targets.

LINE400ME:

A good and broad strong zone lies between 1550MS and the southern end of the line and this zone appears to continue off of the grid to the south. The zone lies on the contact between a resistivity high and good broad low and also correlates to a suspected fault zone that strikes southeast across the grid lines.

Another target lies between 1400MS and 1250MS that also correlates to the same low as well as to a broad magnetic low.

A third zone lies between 850MS and 700MS that correlates to a narrow resistivity low. This zone lies just to the south of the main fault zone and it appears to strengthen at depth.

A good zone lies between 350MS and 150MS that lies on the southern edge of a resistivity high. The zone is host to a good VLF zone and it lies on the extreme southern edge of the main cross structure.

The final zone lies between 350MN and 650MN and it correlates to the airborne targets in the area. The zone has good resistivity low association.

LINE 500ME:

The strong southern zone was also well defined on this line and it correlates to a resistivity low and a good VLF zone. This zone lies to the immediate north of a good magnetic high.

The next zone lies between 950MS and 750MS and correlates to a modest resistivity low and a broad magnetic low. Another broad and deep zone lies between 600MS and 200MS that is host to two VLF zones and correlates to a broad resistivity high.

A weak and or deep zone was noted between the baseline and 50MN correlates to a good VLF zone.

The final zone is a broad deep and strong zone between 250MN and 600MN that correlates to a good resistivity low as well as the airborne targets.


Page 12

LINE 600ME:

The southern zone that is being followed across the southern ends of lines 200ME to 500ME was noted on this line but it is migrating to the north as the grid proceeds to the east. This zone lies between 1850MS and 1550MS and correlates to the contact between a resistively high to the south and a low to the north. This zone is host to a least two VLF zones

Another somewhat distorted zone lies between 800MS and 500MS an it correlates to a resistivity low to the south and a high to the north. The resistivity low represents the fault zone. A weak zone lies between 75MS and 50MN that correlates to a good VLF zone and a deep resisti vity high.

A final zone lies between 200MN and 550MN that correlates to a good resistivity low. This zone host a VLF zone and correlates to a broad and weak magnetic low.

LINE 700ME:

There is a good zone between 1800MS and 1550MS that represents the southern zone at the ends of the grid lines. This zone is host to two VLF zones and lies to the immediate west of a dike like unit.

A good zone lies between 850MS and 600MS that correlates to a good resistivity low and it correlates directly with the main fault zone in the area. A weak and or deep zone lies between 150MS and 25MN that is deep and being over shadowed by the stronger zone to the north. This zone correlates to a good VLF zone and lies just to the north of a main cross structure. The stronger zone between 150MN and 450MN correlates to a good resistivity low and it host a good VLF zone.

LINE 800ME:

A strong zone lies between 1650MS and 1400MS and it seems to correlate to the western edge of a dike like unit. The zone lies on the northern flank of a resistivity high. Another good zone lies between 900MS and 650MS and it too correlates to a good resistivity low which represents the major fault zone in the area.

Another good zone lies between IOOMN and 425MN that correlates to a good resistivity low and a very weak magnetic low. This zone is host to a good VLF target.

LINE 900ME:

A zone lies between 1700MS and 1400MS that correlates to a modest resistivity high and the entire zone lies within the dike like unit. Another good zone is between 1000MS and 800MS that lies on the southern edge of a modest resistivity high. This zone lies just to the immediate south of the main fault cross structure that cuts the dike.


Page 13

A deep zone lies between 400MS and 250MS that lies between two modest a deep resistivity highs. This zone correlates to a main southeast striking cross structure and it is also host to a good VLF zone.

The final zone lies between the base line and 350MN and it is associated with a good broad resistivity low as well as a broad magnetic low. The zone is also host a good VLP zone.

The next set of lines that run from 1000ME to 2300ME and they were all read from the base line to their southern limits. The previous set of lines were read from 800MN to their southern limits.

LINE lOOOME:

A good zone lies between 1450MS and l300MS and correlates to a broad resistivity low that north flanks a weak high. This zone lies within the dike like unit. A second zone was noted to the immediate north of this first zone and it lies between 1150MS and 900MS. It generally is associated with a broad resistivity high and it is also contained within the dike.

The last zone lies between 400MS and 250MS and it represents a deep zone that is building at depth. The zone correlates to a resistivity low and it host a good VLF zone. The zone also correlates to a main southeast striking cross structure.

LINE llOOME:

There is a well defined zone between 1500MS and 1250MS that correlates to a modest resistivity low. The zone is also host to a good VLF zone and appears to lie within the dike. A modest and deep zone lies between lOOMS and 950MS and it lies along the southern edge of a modest resistivity high. The zone seems to be within the dike.

Another zone lies between 500MS and 350MS that correlates to the northern edge of a resistivity high and seems to correlate to the cross unit that has offset the dike in the vicinity. A final zone is building up at the northern end of the line and it is associated with a resistivity low and may also relate to the cross structure that has offset the northern section of the dike.

LINE 1200ME:

There is a good zone building up at the southern tip of the line that is associated with a resistivity low. This zone correlates to a good VLP zone as well as one of the main southeast striking cross structures. There is a narrow zone between 1400MS and 1350MS that correlates to a good VLF zone and it lies on the northern flank of a deep resistivity high. A strong zone lies between1250MS and 800MS that correlates to a resistivity low and appears to lie along the eastern edge of the dike.

A weak zone lies between 500MS and 400MS that correlates to the northern edge of a resistivity high a good VLP zone and an offset in the dike which seems to have been caused by a main southeast striking cross structure. A final zone is building up on the northern tip of the line and it correlates to a good resistivity low and to one of the main southeast striking cross units.


Page 14

LINE 1300ME:

The zone between 1900MS and 1775MS correlates to the magnetic high that is associated with the southeast cross structure noted in this vicinity.

Another broad zone lies between 1400MS and lOOOMS that is stronger on it's northern extension. The northern extension of this zone is cut off by the main fault zone that strikes southeast across this section of the grid and id visible in the resistivity low associated with the target. There is a broad and deep zone between 650MS and 500MS that correlates to a deep rooted resistivity high and this zone correlates directly with a main southeast striking cross structure. This zone is also host to a good VLF zone.

LINE 1400ME:

There is a broad zone between 1600MS and the end of the line that is associated with a resistivity low. This zone is host to two VLF zones and correlates directly with a good magnetic high that represents one of the main southeast striking zones. Another broad zone lies between 1400MS and 1050MS with the strongest portion of the zone lying between 1350MS and 1250MS. This portion of the zone correlates to a good VLF zone as well as a resistivity low and weak magnetic low.

The moderate to weak zone at 550MS correlates to a VLF zone and the main southeast striking structures that has disrupted the dike's strikes. The zone is also associated with a deep resistivity high.

The zones between 350MS and 150MS correlates to a good magnetic unit that represents another of the southeast striking magnetic trends that has a good direct VLF zone association.

LINE 1500ME:

There is a well detined zone between 1750MS and 1625MS that lies on the southern edge of a resistivity high. The zone itself correlates to a resistivity low and it is host to a modest VLF zone. The zone lies to the immediate south of a main southeast striking structure.

There is another well defined zone situated between 1350MS and 1100MS that is host to two good VLF zones and appears to lie across one of the main cross structures. This zone lies along the northern edge of a good resistivity high. A deep weak zone lies at 850MS which correlates to the fault structure and a VLF zone. Another zone is at 650MS to 600MS which also correlates to a southeast striking magnetic high unit and correlates to a good VLF zone.

The strong zone between 475MS and 350MS correlates to the southern limb of a good magnetic trend. The zone between 250MS and 150MS correlates to a weak resistivity Iowa good VLF zone and a good magnetic high trend that represents one of the main cross structures that has offset the dikes.

LINE 1600ME:

The weak zone at 1900MS to 1850MS is associated with a bulging in the dike that also host a VLF zone. A second zone between 1600MS and 1400MS lies on the southern edge of a


Page 15

resistivity high but correlates directly with a resistivity low. This zone is directly associated with one of the main cross structures and a VLF zone.

A large zone possibly comprised of two parallel zones lies between 1 t 50MS and 750MS with concentrations between 1150MS and 1100MS and l050MS and 950MS. The southern portion of this target correlates with a resistivity high and a magnetic low as well as to one of the main southeast striking structures. The northern section of the zone correlates to a deep-rooted resistivity high as well as the suspected main fault zone.

Another zone lies between 550MS and 400MS and it lies to the immediate south of a modest resistivity high and a broad and weak magnetic low.

A final zone lies between 250MS and lOOMS and correlates directly with a good magnetic high trend that represents one of the main cross structures. It also correlates directly with a good VLF zone. The entire zone is associated with a resistivity low unit.

LINE 1700ME:

There is a well defined zone between 1600MS and 1450MS that correlates to a good resistivity low and a weak magnetic low. The zone is also host to a good VLF zone and is directly associated with the main cross structures striking southeast. This zone appears to offset the dike.

There is a broad strong zone between 1150MS and 700MS that is associated with a broad resistivity low that represents the main fault zone that has offset the dike. A good VLF zone is also associated with this zone. Another zone closely parallels this zone and lies between 650MS and 500MS. The zone lies to the immediate north of a main cross structure and it is associated with a modest magnetic low unit.

The last zone lies between 300MS and 200MS and it is associated with a low resistivity lying between two highs. This zone correlates to the eastern tip of a good magnetic unit that represents on of the main southeast striking units.

LINE 1800ME:

There is a good conductive zone between 1450MS and 1200MS that correlates to a good resistivity low that is situated between to highs. This zone is directly associated with the major fault zone that has offset the dikes as well as a cross structure that closely parallels this fault. Several VLF zone are also hosted in this IP zone.

The second zone lies between 950MS and 750MS and again correlates to a resistivity low on the north edge of a resistivity high. This zone is also associated with a major southeast striking cross structure as well as a good VLF zone. The last zone is a weak and deep zone between 250MS and lOOMS that is associated with a modest resistivity high. The zone also correlates to one of the main cross structures.


Page 16

LINE 1900ME:

A weak zone was noted at the south end of the line that correlates to a moderate resistivity high and a modest magnetic low. A good zone lies between 1450MS and 1250MS that is associated with a moderate resistivity low and this zone correlates to the main fault zone and a parallel cross structure that also host at least two VLF zones. The remainder of the line appears to relate to the dike that the majority of the north section of the line is covered by.

LINE 2000ME:

A broad and weak zone is situated between 1350MS and 1100MS that correlates to the fault and parallel cross structure. The fault can be seen by the weak low at 1300MS between the two highs. A weak zone was noted at 800MS to 750MS that correlates to one of the main cross structures. This zone lies at the contact between a resistivity high and low unit.

LINE 2100ME:

A weak zone at 1300MS correlates to the suspected cross structure and this zone has an associated resistivity high and a modest magnetic high. Another weak zone was noted between 825MS and 700MS that correlates to a good resistivity low and it is associated with a break in the dike and a main cross structure with a correlating VLF zone.

The weak zone at 250MS correlates to a cross structure that strikes southeast across the grid.

LINE 2200ME:

The two cross structures at 1300MS and 800MS to 700MS were noted weakly by this survey line. The southern zone lies along a broad resistivity high. The northern zone lies at the contact between the resistivity high and low. The remainder of the line was non descriptive.

LINE 2300ME:

This line represents the last line of the grid and the most easterly line read by the IP and magnetic surveys. The line weakly located the cross structures but suggest that they may be deepening and or petering out as they strike to the southeast. The magnetics suggest that there is a dike like unit paralleling the northern half of the grid line but the southern section has been folded and or faulted off to the south and east.


Page 17

CONCLUSIONS AND RECOMMENDATIONS:

The surveys were successful in locating and outlining several major cross structures that strike northwest to southeast across the grid area. There is a major fault zone that generally strikes across the central section of the grid and it has offset by faulting and or folding all of the north-south striking dikes. The VLF -EM survey and the IP survey reacted well to this fault and was able to map it successfully across the entire grid as well. This fault zone should be considered as a priority target for drilling as it may represent a significant horizon for mineral deposition.

The cross structure that parallels the strike of the fault and lies well north of the base line on the western section of the grid and just to the south of the base line on the eastern section of the grid has also offset all of the dikes. This may suggest that it is a fault controlled zone which would make it a high priority target for follow up drilling as it may suggest a plumbing system for metal deposition.

Another cross structure that cuts across the grid in a northwest to southeast direction runs from 900MW just north of the base line to at least line 2100ME at tie line 800MS should also be considered as a prime drill target. There are numerous VLF-EM zones associated with the structure and the IP survey reacted well to it.

The three southeast striking zones between lines 1300ME and 2100ME south of the suspect fault zone are all good targets that reacted well to the VLF and IP surveys and all of the zones have either offset the dikes and or distorted their strikes.

The San Gold property is situated to the northwest of the Lake Shore Gold Mine that will be in production by the first quarter of 2009. The main structures of the San Gold property that were outlined by this summer ground program would suggest that the property is underlain by several well defined cross structures that strike northwest to southeast At least one and possibly two of these cross structures may represent a major fault structure that could represent a splay off of the Porcupine-Destor Fault that represents the main conduit for the gold mineralization in the Timmins Camp. The Lake Shore Gold Mine will be the first gold mine west of the Mattagami River which represents a major north-south trending fault and it had offset the Porcupine-Destor to the south and west Geophysics has proven that there are numerous north-south striking dikes in Bristol and Carscallen townships that have been faulted, folded and distorted by major cross structures generally striking west to east and or northwest to southeast These faulted and or folded areas in and around the dikes may become potential trap zones for mineral deposition. Thus any such area on the San Gold property should be considered as a priority area for diamond drilling. Also, several holes should be done across the northwest to southeast striking cross structures to better define them for mineral deposition.

Priority should be given to the VLF and IP zones between lines 800MW and 200MW to the immediate north and south of the base line. Another area of high priority would be the VLF and IP zone between 1200ME and 1700ME just to the south of the base line that has a good magnetic high association.

I I I I I I I I I I I I I I I I I I I I

Page 18

Another area of priority would be the VLF and IP zones between lines 1300ME and 1900ME from 11 OOMS to I600MS that correlate to the fault zone and parallel cross structures.

A final priority target would be the magnetic high with the associated VLF zone and IP target that lies across the southern ends of lines 1200ME to 1500ME. This could represent a blowout along the eastern edge of one of the dikes and could represent a potential trap zone for minearlization.

Should any of the drilling return encouraging numbers and or results then the VLF and IP targets would have to be re-evaluated according to determine a second round of follow-up drilling.

AUTHOR'S NOTE:

At the time of this report the grid has been extended to the northwest and north from lines 600MW to 1100ME and from 800ME to 2400ME and it is being covered by the total field magnetic and VLF-EM surveys. The total to be cut and read for this portion of the grid would be about 32 kilometers. Surveys should be completed by the 21 st of November 2008.

Respectfully submitted

John C. Grant C.E.T., FGAC November 17t\ 2008

. ~~"' ...• :'.:' ... ," .. ':;::;;',:':.... . ..... ....,...--... ~. " '


CERTIFICATION

I, John Charles Grant, of 108 Kay Crescent, in the City of Timmins, Province of Ontario, hereby certify that:

1). I am a graduate of Cambrian College of Applied Arts and Technology, 1975, Sudbury Ontario Campus, with a 3 year Honors Diploma in Geological and Geophysical Technology.

2). I have worked subsequently as an Exploration Geophysicist for Teck Exploration Limited, (5 years, 1975 to 1980), and currently as Exploration Manager and Chief Geophysicist for Exsics Exploration Limited, since May, 1980.

3). I am a member in good standing of the Certified Engineering Technologist Association, (CET), since 1984.

4). I am in good standing as a Fellow of the Geological Association of Canada, (FGAC), since 1986.

5). I have been actively engaged in my profession since the 15th day of May, 1975, in all aspects of ground exploration programs including the planning and execution of field programs, project supervision, data compilation, interpretations and reports.

6). I have no specific or special interest nor do I expect to receive any such interest in the herein described property. I have been retained by the property holders and or their Agents as a Geological and Oeo.physical Consultant and Contract Manager.

John Charles Grant, CET., FGAC.

I I I I APPENDIX A I I I I I I I I I I I I I I I •

I I I I I I I I I I I

Locating Buried Drums and Tanks?

The ENVI-MAG is the solution to this environmental problem. ENVI-MAG is an inexpensive, lightweight, portable "WALKMAG" which enables you to survey large areas quickly and accurately.

EN VI-MAG is a portable, proton precession magnetometer and/or gradiometer, for geotechnical, archaeological and environ-mental applications where high produc-tion , fast count rate and high sensitivity are required. It may also be used for other applications, such as mineral exploration, and may be configured as a total-field magnetometer, a vertical gradiometer or as a base station .

The ENVI-MAG

• easily detects buried drums to depths of 10 feet or more

• more sensitive to the steel of a buried drum than EM or radar

• much less expensive than EM or radar

• survey productivity much higher than with EM or radar

I Features and Benefits "WALKMAG"

I I I I I I I -

Magnetometer/Gradlometer

The "WALKMAG" mode of operation (sometimes known as "Walking Mag") is user-selectable from the keyboard. In this mode, data is acquired and recorded at the rate of 2 readings per second as the operator walks at a steady pace along a line. At desired intervals, the operator "triggers" an event marker by a single key stroke, assigning coordinates to the recorded data.

True Simultaneous Gradlometer

An optional upgrade kit is available to configure ENVI-MAG as a gradiometer to make true, simultaneous gradiometer measurements. Gradiometry is useful for geotechnical and archaeological surveys where small near surface magnetic targets are the object of the survey.

Selectable Sampling Rates

0 .5 second, 1 second and 2 second reading rates user selectable from the keyboard .

Main features Include:

• select sampling rates as fast as 2 times per second

• 'WALKMAG" mode for rapid acquisition of data

• large internal, expandable memory

• easy to read, large LCD screen displays data both numerically and graphically

• ENVIMAP software for processi"g and mapping data

ENVI-MAG comprises several basic modules; a lightweight console with a large screen alphanumeric display and high capacity memory, a staff mounted sensor and sensor cable, rechargeable battery and battery charger, gS-232 cable and ENVIMAP processing and mapping software . For gradiometry applications an upgrade kit is available, compriSing an additiona' processor module for installation in the console, and a second sensor with a staff ex1ender.

Large-Key Keypad

The large-key keypad allows easy access for gloved-hands in cold-weather opera·· tions. Each key has a multi-purpose function .

Front panel of ENVI -MAG showing a graphic profile of data and large-key keypad

Large Capacity Memory

ENVI-MAG with standard memory stores up to 28,000 readings of total field meas-urements, 21,000 readings of gradiometry data or 151,000 readings as a base station. An expanded memory option is available which increases this standard capacity by a factor of 5.

ENV/-MAG Proton Magnetometer in operation

For base station applications a Base Station Accessory Kit is available so that the sensor and staff may be converted into a base station sensor.

Easy Review of Data

For quality of data and for a rapid analysis of the magnetic characteristics of the survey line, several modes of review are possible. These include the measure-ments at the last four stations, the ability to scroll through any or all previous readings in memory, and a graphic display of the previous data as profiles, line by line. This feature is very useful for environ-mental and archaeological surveys.

Highly Productive

The 'WALKMAG" mode of operation acquires data rapidly at close station intervals, ensuring high-definition results. This increases survey productivity by a factor of 5 when compared to a conven-tional magnetometer survey.

"Datacheck" Quality Control of Data

"Datacheck" provides a feature wherein at the end of each survey line, data may be reviewed as a profile on ENVI-MAG's screen. Oatacheck confirms that the instrument is functioning correctly and

allows the user to note the magnetic relief (anomaly) on the line.

large Screen Display

"Super-Twist" 64 x 240 dot (8 lines x 40 characters), LCD graphic screen provides good visibility in all light conditions . A display heater is optionally available for low-temperature operations below O°C.

I , , •

It I • !~ • _ • . , .

I ' .

I ; . I - •

Close-up of the ENVI-MAG screen showing data presented after each reading

Interactive Menus

The set-up of ENVI-MAG is menu-driven, and minimizes the operator's learning time, and on-going tasks.

:~'-~~-li~~'~~;; I ; '.... ,'r'~. '~.t~! . . I" .

- « . , . .. . .

Close-up of display of EN V/-MAG showing interactive set-up menu

Total FIeld OperatIng Range 20,000 to 100,000 nT (gammas)

Total FIeld Absolute Accuracy +/- tnT

Sensitivity

Q.1 nT at 2 second sampling rate

Tuning

Fully solid state. Manual or automatic, key-board selectable

Cycling (ReadIng) Rates

0.5, 1 or 2 seconds, up to 9999 seconds for base station applications, keyboard selectable

Gradlometer Option Includes a second sensor, 20 inch (Y2m) staff extender and processor module

"WALKMAG" Mode

0.5 second for walking surveys, variable rates for hilly terrain

DIgital Olsp/ay

LCD "Super Twisf' , 240 x 64 dots graphics. 8 line x 40 characters alphanumerics

Display Heater

Thermostatically controlled , for cold weather operations

Keyboard Input

17 keys, dual function . membrane type

Notebook Function 32 characters, 5 user-defined MACRO's for quick entry

Rechargeable Battery and Battery Charger

An "off-the-shelf' lead-acid battery and charger are provided as standard. The low-cost "Camcorder" type battery is available from electronic parts distributors everywhere.

HELP-LIne Available

Purchasers of ENVI-MAG are provided with a HELP-Line telephone number to call in the event assistance is needed with an application or instrumentation problem .

ENVIMAP Processing and Mapping Software

Supplied with ENVI-MAG, and custom designed for this purpose, is easy-to-use, very user-friendly, menu driven data processing and mapping software called ENVIMAP. This unique software appears to the user to be a single program, but is in fact a sequence of separate programs, each performing a specific task. Under the menu system, there are separate programs to do the following : a) read the ENVI-MAG data and reformat it into

a standard compatible with the ENVIMAP software

b) grid the data into a standard grid format

c) create a vector file of posted values

Standard Memory

Total Field Measurements: 28.000 readings Gradiometer Measurements: 21,000 readings Base Station Measurements: 151 ,000 readings

Expanded Memory

Total Field Measurements: 140,000 readings Gradiometer Measurements: 109,000 readings Base Station Measurements: 750,000 readings

Real-Time Clock

Records full date, hours, minutes and seconds with 1 second resolution , +/- 1 second stability over 12 hours

DigItal Data Output

RS-232C interlace, 600 to 57,600 Baud, 7 or 8 data bits, 1 start, 1 stop bit, no parity format. Selectable carriage return delay (0-999 ms) to accommodate slow peripherals . Handshaking is done by X-onlX-off

Analog Output

o - 999 mV full scale output voltage with keyboard selectable range of 1. 10, 100, 1,000 or 10,000 nT full scale

Power Supply

Rechargeable "Camcorder" type, 2.3 Ah. Lead-acid battery.

12 Volts at 0.65 Amp for magnetometer, 1.2 Amp for gradiometer,

External 12 Volt input for base station operations

Optional external battery pouch for cold weather operations

Battery Charger

110 Volt - 230 Volt , 50/60 Hz

with line and baseline identification that allows the user to add some title information and build a suitable surround

d) contour the gridded data

e) autoscale the combined results of the posting/surround step and the contouring step to fit on a standard 8.5 ins. wide dot-matrix printer

f) rasterize and output the results of step e) to the printer

ENVIMAP is designed to be as Simple as possible . The user is required to answer a few basic questions asked by ENVIMAP, and then simply toggles "GO" to let ENVIMAP provide default parameters for the making of the contour map. The user can modify certain characteristics of the output plot. ENVIMAP'S menu system is both keyboard and mouse operable. HELP screens are integrated with the menu system so that HELP is displayed when-ever the user requests it.

Options Available

• True simultaneous gradiometer upgrade

• Base station upgrade

• Display heater for low temperature operations

• External battery pouch

Operating Temperature Range Standard 0° to 60°C Optional -400C to 60°C

Dlmensfons Console - 10 x 6 x 2.25 inches

(250 mm x 152 mm x 55 mm)

T,F. sensor - 2.75 inches dia. x 7 inches (70 mm x 175 mm)

Grad. sensor and staff extender - 2.75 inches dia. x 26.5 inches (70 mm x 675 mm)

T.F. staff - 1 inch dia. x 76 inches (25 mm x 2 m)

Weight

Console - 5.4 Ibs (2.45 kg) with rechargeable battery

T, F. sensor - 2.2 Ibs (1 .15 kg)

Grad. sensor - 2.51bs (1 .15 kg)

Staff - 1.75 Ibs (0.8 kg)

SCINTREX Head Office 222 Snidercroft Road Concord, Ontario, Canada L4K 195 Telephone: (905) 669-2280 Fax: (905) 669-6403 or 669-5132 Telex: 06-964570

In the USA: Scintrex Inc. 85 River Rock Drive Unit 202 BuHalo, NY 14207 Telephone: (716) 298-1219 Fax: (716) 298-1317

I I I I APPENDIX B I I I I I I I I I I I I I I I

I INSTRUMENTATION

SPECIFICATIONS Number of channels: 8, expandable to 16, 24 or 32 Survey capabilities: Resistivity and Time domain IP Twenty chargeability windows: Arithmetic, logarithmic, semi-

logarithmic, IPR-12 and user defined Synchronization: Automatic re-synchronization process on primary

voltage signal Noise reduction: Automatic stacking number Computation: Apparent resistivity, chargeability,

standard deviation, and % of symetrical Vp Size: 41 X 33 X 18 em (16 X 13 X 7 in) Weight (32 channels): 8.9 kg (19.6Ib) Enclosure: Heavy-duty Pelican case, environmentally sealed Serial ports: RS-232 and Sluetooth to communicate with a PDA Temperature range: -45 to +60oC (-49 to +14QoF) Humidity range: Waterproof

POWER Power: -12 V rechargeable batteries.

-Standard plug for external battery. ,.....---

POA included with GRx8-32 Standard Juniper - Allegro CX mobile PDA computer provided with the GOD receiver with all accessories. Operating system: Windows CE

Comes with Sluetooth and RS-232 r\ ELECTRICAL CHARACTERISTICS Ground Resistance: Up to 1.5 MO Signal waveform: Time domain (ON+, OFF, ON-, OFF) Time base: 0.5, 1, 2, 4 and 8 seconds Input impedance: 104 Go Primary voltage: ±10 uV to ±15 V for any channel Input: True differential for common-mode

rejection in dipole configuration Voltage measurement: Resolution 1 jJV SP offset adjustment: ± 5 V, automatic compensation throug~

linear drift correction per steps of 150 ~\ Filter: Eight-pole Sessellow-pass 15 Hz,

notch filter 50 Hz and 60 Hz

32 channels GOD GRx8-32 IP Receiver

8 Channels --->

+8 = 16 Ch. --->

+8 = 24 Ch. --->

+8 -=0 32 Ch.-->

t Components included with GOD IP Receiver GRx8-32

A B C o E F G H I K

PURCHASE

1 x Not shown but included: Receiver L lx Not shown but included: Transportation box M lx GRx8-321P receiver wall charger (120-240V) N

Red cable banana/alligator (8 chll0x, 16 chl19x, 24 chl28x, 32 chl37x) 0 2x Black cable banana/alligator P 1 x Allegro Cx field computer Q lx Allegro Cx wall charger (120-240V) R lx Serial communication cable 9 pos. O-SUB female - 9 pos. O-SUB female S 2x Serial communication cable 9 pas. D-SUB female - 5 pas. Amphenol male T 1 x Allegro Cx shoulder strap U

Can be shipped anywhere in the world. RENTAL - available in Canada and USA only Starts on the day the instrument leaves GOD office in Quebec to the day of its retum in

GOD offICe. 50% of the rental fees up to a maximum of 4 months can be credited towards

the purchased of the rented instrument.

WARRANTY All GOD instruments are covered by a one-year warranty. All repairs will be done free of charge at our office in Quebec, Quebec, Canada.

INSTRU MENTATION

GOO INC .

3700, boul. de la Chaudiere, suite 200 Quebec (Quebec), Canada G1X 4B7 Phone: +1 (418) 877-4249 Fax: +1 (418) 877-4054 E-Mail: [email protected] Web Site: www.gddinstrumentation.com

1 x Alleg ro Cx hand strap 2x Allegro Cx NIMH battery pack 3000mAh 3.6V 1x Allegro Cx external NIMH 3000mAh 3.6V battery charger (120-240V) 1 x Allegro Cx ut~ity CD 1 x Allegro Cx AA alkaline battery holder lx Charger with 4 AA 2400mAh 1.2V NIMH batteries 1 x Allegro Cx USB power dock 1x Allegro Cx USB cable for USB power dock IX Not shown but included: Instnuction manual (Receiver) Ix Not shown but included: Instruction manual (Allegro Cx mobile POA)

SERVICE If an instrument manufactured by GOO breaks down while under warranty or service contract, it will be replaced free of charge during repairs (upon request and subject to instruments availability). OTHER COSTS Shipping, insurances, customs and taxes are extra if applicable. PAyr-,iENT Checks, credit cards, bank transfer, etc.

SpeCifications are subject to change without notice Printed in Quebec, Canada, 2008

I I I I I I I I I I

Canadian Man ufacture r of Geophysica l Instrumentation since 1976 Sales , Rental, Customer Service, R&D and Field tra in ing

Induced Polarization Transmitter Txlll-1800W-2400V-10A Model Txll-3600W-2400V-10A Model

I New feature: link two GOD 1800W or 3600W IP TX together and double the voltage (4800V) and power . Its high power combined with its light weight and a Honda generator

I makes it particular1y suitable for dipole-dipole Induced Polarization surveys. I • •

•

I • •

Protection against short circuits even at zero (0) ohm Output voltage range: 150 V - 2400 V 114 steps Power source: 120 V - Optional: 220 V, 50/60 liz Displays electrode contact, transmitting power and current One-year warranty on parts and labour

I This backpackable 1800 watts Induced Polarization (JP.) transmitter works from a standard 120 V source and is well adapted to rocky environments where a high output voltage of up to 2400 volts is needed. Moreover, in highly conductive overburden, at 150 V, the highly efficient

I Txll-1800W transmitter is able to send current up to 10 A. By using this IP. transmitter, you obtain fast and high-quality I.P. readings even in the worst conditions. Link two GOO 1800 W IP TX together and transmit up to 3600 watts - 4800 volts - 10 amps.

Its high power combined with a Honda generator makes it particularly sUitable for pole-{lipole Induced Polarization surveys

• • • • •

Protection against short circuits even at zero (0) ohm Output voltage range: 150 V - 2400 V /14 steps Power source: 220 V, 50/ 60 Hz - standard 220 V generator Displays electrode contact, transmitting power and current One-year warranty on parts and labour

This 3600 watts Induced Polarization (J.P.) transmitter works from a standard 220 V source and is well adapted to rocky environments where a high output voltage of up to 2400 volts is needed. Moreover, in highly conductive overburden , at 350 V, the highly efficient Txll-3600W transmitter is able to send current up to 10 A. By using this JP. transmitter, you obtain fast and high-qualily JP. readings even in the most difficult conditions. link two GOO 3600 W IP TX together and transmit up to 7200 watts - 4800 volts - 10 amps.

I I I

Face plate o f the +--1800W

-and 3600W-> IP Tx

S PE CIFICA TlONS Txll-1800W

• Size: 50cm x 30.5cm x 45.7 em • Weight: approximately 28 kg • Operating temperature: -40 °C to 65°C

ELECTRICAL CHARACTERISTICS Txll-1800W and Txll-3600W

Txll-3600W Size: 51 X 41.5 X 21 .5 cm - built in transportation box from Pelican

• Weight: approximately 32 kg Operating temperature: -40 °C to 65 °C

• Standard time base of 2 seconds for time-domain: 2 seconds ON, 2 seconds OFF

• Optional time base: DC, 0.5, 1, 2, 4 or DC, 1, 2,4, 8 seconds • Output current range: 0.030 to 10 A (normal operation)

0.000 to 10 A (cancel open loop) • Output voltage range: 150 to 2400 V / 14 steps • Ability to link 2 GOD Tx to double power using optional Master / Slave cable

CONTROLS Txll-1800W and Txll-3600W

• Power ON/OFF • Output voltage range switch: 150 V, 180 V, 350 V, 420 V, 500 V,

600 V, 700 V, 840 V, 1000 V, 1200 V, 1400 V, 1680 V, 2000 V, 2400 V

DISPLAYS Txll-1800W and Txll-3600W - now 2 displays

• Output current LCD: reads to ± 0.0010 A. • Electrode contact displayed when not transmitting. • Output power displayed when transmitting. • Automatic thermostat controlled LCD heater for read-out. • Total protection against short circuits even at zero (0) ohm. • Indicator lamps in case of overload:

-High voltage ON/OFF -Output overcurrent -Generator over or undervoltage -Overheating -Logic fail -Open Loop Protection

POWER Txll-1800W Recommended generator

• Standard 120 V / 60 Hz backpackable Honda generator • Suggested models: Honda EU1000iC, 1000 W, 13.5 kg or

Honda EU2000iC, 2000 W, 21 .0 kg

DESCRIPTION Txll-1800W

• Includes shipping box, instruction manual and 110 V plug • Optional backpackable Tx frame, Master / Slave optional cable

PURCHASE Can be shipped anywhere in the world. RENT AL - available in Canada and USA only

Txll-3600W Recommended generator :

• Standard 220 V, 50/60 Hz Honda generator • Suggested models: EM3500XK1C, 3500 W, 62 kg or

EM5000XK1C, 5000 W, 77 kg

Txll-3600W • Includes built-in shipping box, instruction manual and 220 V plug • Optional 220 V extension, Master / Slave optional cable

OTHER COSTS Shipping, insurances, customs and taxes are extra if applicable. PAY MENT

Starts on the day the instrument leaves GOO office in Quebec to the day of its retum in GOO office. 50% of the rental fees up to a maximum of 4 months can be credited towards the purchased of the rented instrument.

Checks, credit cards, bank transfer, etc SERVICE If an instrument manufactured by GOO breaks down while under warranty or service contract, it will be replaced free of charge during repairs (upon request and subject to instruments availability).

WARRANTY All GOO instruments are covered by a one-year warranty. All repairs will be done free of charge at our office in Quebec, Quebec, Canada.

IN STRurvl ENTATION

~DP 3700, boul. de la Chaudiere, suite 200 Quebec (Quebec) Canada G1X 4B7 Phone: +1 (418) 8774249 Fax: +1 (418) 8774054 E-Mail: gdd@gddinstrumentation .com Web Site: www.gddinstrumentation.com

Specifications are subject to change without notice Printed in Quebec, Canada, 2008

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