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<strong>MAGNETIC</strong> <strong>SUPERGRIDS</strong><br />

<strong>Ontario</strong> <strong>Airborne</strong> Geophysical Surveys<br />

Magnetic Data<br />

Geophysical Data Set 1037<br />

<strong>Ontario</strong> Geological Survey<br />

Ministry of Northern Development and Mines<br />

Willet Green Miller Centre<br />

933 Ramsey Lake Road<br />

Sudbury, <strong>Ontario</strong>, P3E 6B5<br />

Canada<br />

Report on Magnetic Supergrids<br />

Geophysical Data Set 1037


TABLE OF CONTENTS<br />

CREDITS .....................................................................................................................................................................3<br />

DISCLAIMER .............................................................................................................................................................3<br />

CITATION...................................................................................................................................................................3<br />

1) INTRODUCTION..............................................................................................................................................4<br />

2) PREPARATION OF <strong>MAGNETIC</strong> <strong>SUPERGRIDS</strong>........................................................................................9<br />

3) SPECIFIC DETAILS: <strong>MAGNETIC</strong> <strong>SUPERGRIDS</strong> ...................................................................................14<br />

APPENDIX A<br />

ARCHIVE DEFINITION........................................................................................................19<br />

APPENDIX B MERGING OF GRIDS BY GRIDKNIT TM METHOD ........................................................23<br />

Report on Magnetic Supergrids<br />

Geophysical Data Set 1037Rev.<br />

2


CREDITS<br />

The following is a list of the organizations that have participated in this project, and their various<br />

responsibilities:<br />

• The overall project management, scientific authority and quality control was provided by<br />

Desmond Rainsford, <strong>Ontario</strong> Geological Survey, Sudbury.<br />

• Paterson, Grant & Watson Limited, Toronto - Prime contractor<br />

- project management<br />

- magnetic data processing<br />

DISCLAIMER<br />

To enable the rapid dissemination of information, this digital data has not received a technical<br />

edit. Every possible effort has been made to ensure the accuracy of the information provided;<br />

however, the <strong>Ontario</strong> Ministry of Northern Development and Mines does not assume any<br />

liability or responsibility for errors that may occur. Users may wish to verify critical<br />

information.<br />

CITATION<br />

Information from this publication may be quoted if credit is given. It is recommended that<br />

reference be made in the following form:<br />

<strong>Ontario</strong> Geological Survey 2003. Magnetic Supergrids, <strong>Ontario</strong> <strong>Airborne</strong> Geophysical Surveys;<br />

magnetic data, grid data; <strong>Ontario</strong> Geological Survey, Geophysical Data Set 1037.<br />

Report on Magnetic Supergrids<br />

Geophysical Data Set 1037<br />

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1) INTRODUCTION<br />

Aeromagnetic Surveys Acquired Before 1999<br />

High resolution airborne magnetic and electromagnetic surveys, over major greenstone belts,<br />

were initiated in 1975 by the <strong>Ontario</strong> Department of Mines (currently known as the <strong>Ontario</strong><br />

Geological Survey) to aid geological mapping and mineral exploration. Between the period<br />

1975 to 1992, thirty-two airborne surveys were flown and processed by different survey<br />

contractors and subcontractors. The two earlier surveys, Matachewan and Bamaji-Fry Lakes,<br />

were acquired in analog form and the remaining thirty surveys were recorded digitally. The<br />

surveys were flown at a nominal flight line spacing of 200 metres with the exception of James<br />

Bay Cretaceous Basin survey, which was flown at a flight line spacing of 1000 metres. The<br />

flight directions for the surveys, including individual survey blocks, were chosen to transect the<br />

predominant regional structural trends of the underlying rocks. The results of the surveys were<br />

published on 1:20,000 semi-controlled photo mosaic paper maps, showing total magnetic field<br />

contours onto which picked electromagnetic conductor anomalies were superimposed in symbol<br />

form.<br />

There are significant differences in quality of data acquisition, and original processing, of older<br />

and newer surveys. The surveys flown recently were designed and flown based on the state-ofthe-art<br />

specifications, equipment and technology, while some of the older surveys, though<br />

conducted to the then industry prevailing standards, were poorly processed. In many cases, on<br />

older surveys, the local map coordinates were registered in map inches of uncontrolled to semicontrolled<br />

photo mosaics. The vast amount of digital data, collected by the survey contractors,<br />

was archived on 9-track tapes of different sizes and densities, in numerous incompatible data<br />

formats and file structures, many of which were difficult to access. For this reason the archival<br />

digital data largely remained inaccessible to the mining industry.<br />

To alleviate many of these problems, and to bring the archival data set of all thirty-two airborne<br />

magnetic and electromagnetic (AMEM) surveys to modern data storage, digital processing and<br />

interpretation standards, the present recompilation and reprocessing project was initiated under<br />

the Northern <strong>Ontario</strong> Development Agreement (NODA). This includes approximately 450 000<br />

line-km of AMEM data, which was recompiled and reprocessed to correct any errors in the<br />

original data sets, to compute new derived products and to produce a revised electromagnetic<br />

anomaly database, using state-of-the-art geophysical data processing and imaging techniques.<br />

The major objectives of this project were to:<br />

1) Provide a single, well-defined, common data format for all thirty-two AMEM survey data<br />

sets on CD-ROM, allowing easy access to the data on a PC platform.<br />

2) Digitize survey data acquired in analog form, obtain missing or bad data from digital or<br />

paper archives, and check the validity of all data including units, conversion factors, etc.<br />

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Geophysical Data Set 1037<br />

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3) Analyze and correct errors in the flight path to account for distortions in the<br />

photomosaics and provide a digital flight path referenced to Universal Transverse<br />

Mercator (UTM) coordinates.<br />

4) Link and level all thirty-two surveys total magnetic field data to the Single Master<br />

Aeromagnetic Grid for <strong>Ontario</strong>, which was prepared from the Geological Survey of<br />

Canada's magnetic database under an earlier project.<br />

5) Reprocess the magnetic data to provide image quality total magnetic field grids and<br />

profiles for each survey.<br />

6) Create image quality second vertical derivative grids of the total magnetic field.<br />

7) Compute image quality apparent resistivities from a selected single frequency of the<br />

frequency-domain electromagnetic data, which have been fully corrected for signal to<br />

noise enhancement and accurately levelled.<br />

8) Compute image quality decay constant and resistivity values from the corrected and<br />

levelled data channels of time-domain electromagnetic data (INPUT, GEOTEM I and<br />

GEOTEM II systems). Provide de-herringboned (i.e. correct for directional effect) decay<br />

constant and resistivity grids for all time-domain surveys.<br />

9) Re-pick electromagnetic anomalies from the surveys in a consistent manner, and store<br />

anomaly parameters, including a unique identifier, in a new digital anomaly database.<br />

10) Prepare seamless supergrids of total magnetic field and its second vertical derivative, for<br />

all surveys that share a common boundary or overlap.<br />

The resulting profile and grid data in digital form, along with the second vertical derivative of<br />

the total magnetic field, the apparent resistivity and decay constant values, and a comprehensive<br />

EM anomaly database, will become valuable tools for orebody detection, and enhanced<br />

lithological and structural mapping of the geology. The original profile data are also included in<br />

the profile database for reference.<br />

A complete description of the magnetic processing techniques applied for all AMEM surveys,<br />

and the specific details concerning each individual survey, are provided in the survey report<br />

included on the CD-ROM issued for each survey (e.g. Geophysical Data Set CD-ROM 1027,<br />

Armstrong-Caribou Lake Area).<br />

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Geophysical Data Set 1037<br />

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Aeromagnetic Surveys Acquired After 1999<br />

Recognising the value of geoscience data in reducing private sector exploration risk and<br />

investment attraction, the <strong>Ontario</strong> Government embarked on “Operation Treasure Hunt” (OTH).<br />

The OTH initiative comprises a three-year, $29 million program that commenced April 1, 1999.<br />

It incorporates:<br />

• airborne geophysics (high-resolution magnetic/electromagnetic surveys, including the<br />

purchase of proprietary data sets)<br />

• surficial geochemistry (lake sediments and indicator minerals)<br />

• bedrock map compilation<br />

• methods development (e.g. electro-geochemical modelling applied to exploration and 3-<br />

D geological/geophysical modelling)<br />

• delivery of digital data products.<br />

The OGS was charged with the responsibility to manage OTH. The OGS sought advice about the<br />

mineral industry needs and priorities from its OGS Advisory Board – a stakeholder board<br />

including representatives from the <strong>Ontario</strong> Mining Association, <strong>Ontario</strong> Prospectors Association,<br />

Prospectors and Developers Association, Aggregate Producers Association of <strong>Ontario</strong>, Chairs of<br />

<strong>Ontario</strong> University <strong>Geology</strong> Departments, Canadian Mining Industry Research Organisation and<br />

Geological Survey of Canada. The OGS Advisory Board mandated a Technical Committee to<br />

advise the OGS on geographic areas of interest within <strong>Ontario</strong> where collection of new data<br />

would make the greatest impact on reducing exploration risk. Various criteria were assessed,<br />

including:<br />

• commodities and deposit types sought<br />

• prospectivity of the geology<br />

• state of the local mining industry and infrastructure<br />

• existing, available data<br />

• mineral property status.<br />

The geophysical component of the OTH program involved:<br />

• acquiring from the private sector existing proprietary airborne geophysical data that met<br />

<strong>Ontario</strong> Geological Survey (OGS) quality standards and objectives of Operation Treasure<br />

Hunt;<br />

• flying new airborne magnetic and electromagnetic surveys over various greenstone belts;<br />

• disseminating these geophysical data sets and their daughter products to clients in digital<br />

and hardcopy formats.<br />

In late 1999, MNDM commenced an ambitious program of airborne magnetic and<br />

electromagnetic surveys as part of OTH geoscience initiative. The project involved four survey<br />

contractors, five different electromagnetic systems and more than 105,000 line-km of data<br />

acquisition.<br />

The airborne survey contracts were awarded through a Request for Proposal and Contractor<br />

Selection process. The system and contractor selected for each survey area were judged on many<br />

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Geophysical Data Set 1037<br />

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criteria, including the following:<br />

• applicability of the proposed system to the local geology and potential deposit types<br />

• aircraft capabilities and safety plan<br />

• experience with similar surveys<br />

• QA/QC plan<br />

• capacity to acquire the data and prepare final products in the allotted time<br />

• price-performance.<br />

In August 1999, Paterson, Grant & Watson Limited (PGW) was retained by MNDM to provide<br />

Geophysicist Project Management and quality assurance (QA)/quality control (QC) inspection<br />

services for the airborne geophysical survey component of OTH. One of PGW’s roles as the<br />

OTH Geophysicist was to seek out, and recommend for purchase by MNDM, proprietary<br />

airborne geophysical data that would complement the acquisition of new data being undertaken<br />

by OTH. PGW commenced the search process in September 1999.<br />

Ranking and valuation of submitted airborne geophysical survey data sets were based on the<br />

following criteria:<br />

• date of survey – recent surveys were favoured over older surveys because of improved<br />

acquisition technology, greater data density and improved final products.<br />

• survey method – magnetometer surveys, without supplementary radiometrics or VLF,<br />

were given the lowest rating in this category; AEM and magnetometer were given the<br />

highest; the objective was to acquire data that complements what is already available in<br />

the public domain, with emphasis on exploration rather than mapping.<br />

• location of area<br />

• highest value was accorded to data sets lying within areas identified by the <strong>Ontario</strong><br />

Geological Survey Advisory Board as being of special commodity interest and<br />

worthy of airborne geophysical coverage (Figure 1).<br />

• data sets occurring within areas already surveyed or scheduled for survey under<br />

Operation Treasure Hunt were only selected if they added significantly to the<br />

acquired data sets,<br />

• proximity or coincidence of the survey block with areas having restricted land use<br />

designations affected the value assigned to that survey,<br />

• consideration was given to data sets that were collected in remote areas where<br />

logistical costs are very high.<br />

• line spacing - not normally a significant factor in the valuation of an airborne<br />

geophysical survey; however, in the case of OTH, points were assigned according to<br />

how well the line spacing met the desired exploration requirements; detailed surveys<br />

were normally accorded a higher rating than reconnaissance surveys.<br />

• quality of data - data quality, processed products, and adherence to correct survey<br />

specifications had to be up to normal industry standards.<br />

• survey size - data sets comprising less than 1000 line-km were selected only if they<br />

fell in very strategic locations.<br />

• other criteria - factors such as apparent mineral significance, previous exploration<br />

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Geophysical Data Set 1037<br />

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activity and land availability were also considered in making the final selection.<br />

Figure 1<br />

In February 2002, Paterson, Grant & Watson Limited (PGW) was retained by MNDM to<br />

microlevel and level to a common datum the aeromagnetic surveys of OTH. Adjacent surveys<br />

were also to be merged together with existing AMEM surveys into supergrids. PGW<br />

commenced this project in March 2002.<br />

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Geophysical Data Set 1037<br />

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2) PREPARATION OF <strong>MAGNETIC</strong> <strong>SUPERGRIDS</strong><br />

Six supergrids were produced in 1999 using 22 of the 32 AMEM high resolution grids flown<br />

during the period 1975 to 1992. Aeromagnetic data acquired since 1999 through Operation<br />

Treasure Hunt were microlevelled, levelled to a common datum and added to the existing<br />

supergrids. Where large overlaps existed between surveys, the survey with the higher quality<br />

data took precedence.<br />

The following table lists the final supergrids and the grids used in their construction:<br />

Table 1<br />

Supergrid<br />

Abitibi Supergrid<br />

Bamaji - Vickers Supergrid<br />

Stormy Supergrid<br />

Schreiber Supergrid<br />

Red Lake Supergrid<br />

Fort Hope - James Bay –<br />

Attawapiskat Supergrid<br />

Component Grids<br />

Abitibi (previous supergrid), Wawa (previous supergrid),<br />

Temagami, Matheson, Kirkland Lake, Cochrane, Oba -<br />

Kapuskasing, Kapuskasing - Chapleau, Tyrell, Amyot -<br />

Browning, Gowan - Evelyn, Cobalt, Temagami South,<br />

Temiskaming, Robb - Jamieson, Turnbull - Godfrey,<br />

Kenabeek, Latchford, Redwater<br />

Pickle Lake (previous supergrid), Vickers, Gitche Lake<br />

Dryden (previous supergrid), Stormy Lake, Docker,<br />

Kakagi Lake<br />

Schreiber, GECO Manitouwadge, Hemlo<br />

Red Lake (previous supergrid), Troutlake River, Pakwash<br />

Lake<br />

Fort Hope, Albany River-James Bay, Attawapiskat,<br />

Albany – Atikameg - Attawapiskat Rivers, Nagagami –<br />

Squirrel -Wakashi Rivers, Kenogami River, Kapiskau<br />

River East<br />

Creation of Supergrids from Aeromagnetic Surveys Acquired Before 1999<br />

Six magnetic supergrids were constructed for the AMEM project, in areas where two or more<br />

individual surveys share a common boundary and/or survey data overlap. This applies to 22 of<br />

the 32 magnetic surveys that were reprocessed. The goal was to provide, wherever possible, a<br />

regional picture of the total magnetic field and its second vertical derivative that encompasses a<br />

number of individual surveys, where geological trends can be reliably followed across survey<br />

boundaries. The transition between individual aeromagnetic surveys is seamless on the total<br />

magnetic and its second vertical derivative supergrids. The integrity of the individual grids has<br />

been maintained (except occasionally in the overlapping areas – see below “Preparation of the<br />

Magnetic Supergrids”) and therefore detailed magnetic interpretation can be undertaken, and is<br />

Report on Magnetic Supergrids<br />

Geophysical Data Set 1037<br />

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considered to be as reliable as on the individual magnetic grids.<br />

Each individual grid was constructed with a grid cell size of 40 metres, and the resulting<br />

supergrids have the same grid cell size of 40 metres. The grids of the total magnetic field<br />

supplied on the Geophysical Data Set (GDS) CD-ROMs were utilised as the starting point for<br />

preparation of the magnetic supergrids. These are:<br />

I. The Abitibi Supergrid (9 individual surveys merged) GDS CD-ROM #<br />

1. Black River - Matheson 1001<br />

2. Blake River Syncline 1006<br />

3. Detour – Burntbush - Abitibi 1007-1008<br />

4. Kirkland Lake 1022<br />

5. Matachewan 1014<br />

6. North Swayze - Montcalm 1005<br />

7. Shining Tree 1003<br />

8. Swayze 1015<br />

9. Timmins 1004<br />

II. The Dryden supergrid (4 individual surveys merged) GDS CD-ROM #<br />

1. Dryden 1016<br />

2. Manitou-Stormy Lakes 1019<br />

3. Sioux Lookout 1023<br />

4. Sturgeon Savant Lake 1033<br />

III. The Geraldton supergrid (2 individual surveys merged) GDS CD-ROM #<br />

1. Armstrong - Caribou Lake 1027<br />

2. Geraldton - Tashota (north-west and south-east) 1031, 1032<br />

IV. The Pickle Lake supergrid (2 individual surveys merged) GDS CD-ROM #<br />

1. Bamaji - Fry Lakes 1013<br />

2. Pickle Lake 1012<br />

V. The Red Lake supergrid (3 individual surveys merged) GDS CD-ROM #<br />

1. Birch - Confederation Lakes 1025<br />

2. Red Lake 1028<br />

3. Uchi - Bruce Lakes 1026<br />

VI. The Wawa supergrid (2 individual surveys merged) GDS CD-ROM #<br />

1. Micipicoten 1010<br />

2. Wawa 1009<br />

If aeromagnetic measurements were perfect, there would be no need for any further adjustments<br />

to data or grids in order to get a seamless fit between survey boundaries. In theory, one should be<br />

able to measure the magnetic field at the same location above the earth, but at different times,<br />

Report on Magnetic Supergrids<br />

Geophysical Data Set 1037<br />

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and obtain the same magnetic value after all corrections have been applied. In aeromagnetic<br />

survey practice, it is common that data mismatches occur where surveys overlap. The possible<br />

contributing factors include:<br />

• accuracy of survey navigation and flightpath recovery;<br />

• type and noise envelope of the magnetometer;<br />

• differing flightline directions;<br />

• variations in magnetic sensor height and orientation;<br />

• magnetometer sampling rate;<br />

• techniques used to measure errors and correct the data (e.g. diurnal, IGRF, levelling);<br />

• variations in the diurnal activity; and<br />

• changes in the ground conditions between surveys (e.g. cultural effects)<br />

All AMEM surveys were levelled to a common magnetic datum provided by the Single Master<br />

Aeromagnetic Grid for <strong>Ontario</strong>. One effect of this procedure is that any medium to long<br />

wavelength mismatch (i.e. > ~1000 metres) between surveys is removed. In fact, one QC/QA<br />

check employed during the AMEM project was to verify that the total magnetic field grids<br />

matched well along common boundaries.<br />

There are two typical magnetic sensor elevations for the AMEM project: 120 metres for fixed<br />

wing surveys, and 45 metres for helicopter surveys. All magnetic surveys have been brought to a<br />

common altitude (level of observation) prior to the creation of the supergrids. They were either<br />

downward or upward continued (data mathematically projected to a level surface above or<br />

below the original datum). In general, surveys flown at a higher altitude were downward<br />

continued to the level of the lower altitude surveys. This has the effect that every detail in the<br />

grid flown at a lesser height was preserved and the details on the grid flown at a greater height<br />

were enhanced.<br />

Of the 22 surveys incorporated in the supergrids, four required downward continuation and one<br />

required upward continuation (see Table 2: the continuation value represents the number of<br />

meters the grid was upward (cf. 75 metres) or downward (cf. –75 metres) continued; where no<br />

continuation was applied, the value is 0). The continuation process was applied using standard<br />

2-D Fourier-domain filtering. Downward continuation may result in amplification of any noise<br />

contained in a grid, as well as of geological signal. Consequently, the survey-specific optimum<br />

Wiener filter, originally designed for computation of the second vertical derivative (see<br />

individual survey reports on Geophysical Data Set CD ROM’s), was incorporated in the<br />

downward continuation. This resulted in the enhancement of the geological signal in preference<br />

to the noise (by the very design of the Wiener optimum filter; see any individual report: e.g.<br />

Armstrong-Caribou Lake Area Geophysical Data Set CD-ROM # 1027).<br />

The suture method of the Geosoft GridKnit TM routine was used to merge the grids, since it<br />

offers more flexibility and control in the process of merging grids than the blending routine. The<br />

suture method defines a line at which to join the two grids, which lies completely within the<br />

overlapping area (see Appendix B). The automatic option of the suture path definition was<br />

GridKnit TM : Trademark of Geosoft Inc.<br />

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Geophysical Data Set 1037<br />

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usually chosen. The automatic option produces smoother paths, by using the edges from both<br />

grids simultaneously and finding the midpoints between them (see Appendix B – Locating a<br />

Suture Path). When values in the grids differ along the suture path, they must be corrected by<br />

adjusting the grids on either side of the path (see Appendix B – Multi-Frequency Suturing<br />

Algorithm).<br />

Table 2<br />

SURVEY<br />

GEOPHYSICAL<br />

DATA SET #<br />

SURVEY HEIGHT<br />

(metres)<br />

Armstrong - Caribou Lake 1027 45 0<br />

Bamaji - Fry Lakes 1013 120 0<br />

Black River - Matheson 1001 120 0<br />

Blake River Syncline 1006 45 75<br />

Birch - Confederation Lakes 1025 120 -75<br />

Detour - Burntbush - Abitibi 1007-1008 120 0<br />

Dryden 1016 120 -75<br />

Geraldton - Tashota 1031-1032 45 0<br />

Kirkland Lake 1022 120 0<br />

Manitou - Stormy Lakes 1019 45 0<br />

Matachewan 1014 120 0<br />

Micipicoten 1010 30 0<br />

North Swayze - Montcalm 1005 120 0<br />

Pickle Lake 1012 120 0<br />

Red Lake 1028 120 -75<br />

Shining Tree 1003 120 0<br />

Sioux Lookout 1023 45 0<br />

Sturgeon Savant Lake 1033 45 0<br />

Swayze 1015 120 0<br />

Timmins 1004 120 0<br />

Uchi Bruce Lakes 1026 45 0<br />

Wawa 1009 45 -15<br />

Thus, for the six supergrids the final continuation height was, as follows:<br />

Table 3<br />

Supergrid<br />

Abitibi Supergrid<br />

Dryden Supergrid<br />

Geraldton Supergrid<br />

Pickle Lake Supergrid<br />

Red Lake Supergrid<br />

Final Continuation Height<br />

120 metres<br />

45 metres<br />

45 metres<br />

120 metres<br />

45 metres<br />

CONTINUATION<br />

(metres)<br />

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Wawa Supergrid<br />

30 metres<br />

As all grids were already levelled to the <strong>Ontario</strong> Master Grid, no trend removal or base level shift<br />

was required. The only adjustments to grid values were made in the overlapping areas in order<br />

to achieve a seamless link, affected the short wavelength features. The adjustments may reach<br />

several hundred nanoTeslas in areas of high amplitude, high gradient anomalies. Wherever the<br />

overlapping area between two surveys was reasonable in extent (a couple of kilometres), and the<br />

quality of the data was at a similar level, both grids were adjusted equally (see Appendix B –<br />

Suture Weighting). Wherever there were large overlaps and/or different levels of data quality,<br />

the lower quality grid (usually the older dataset) was adjusted to the higher quality one (usually<br />

the most recent dataset) which remained unmodified. The adjustments were made only within<br />

the overlapping areas. In all other areas, the grids have not been modified at all.<br />

Creation of Supergrids from Aeromagnetic Surveys Acquired After 1999<br />

Five of the six supergrids created in 1999 were incorporated within the final supergrids as part of<br />

Geophysical Data Set 1037. The procedure to link the individual surveys into one contiguous<br />

supergrid is similar that that of the previous phase of supergrid creation.<br />

To summarize:<br />

• all grids to be included within the supergrid are reprojected to the same UTM projection.<br />

The chosen UTM zone is the zone for the majority of the surveys.<br />

• all grids are upward or downward continued to their final continuation height. The value<br />

of the final continuation height is chosen to be that of the most recent survey. This<br />

usually refers a survey flown for “Operation Treasure Hunt”.<br />

• all grids are regridded to a 40 metre grid cell size, however grids used to construct the<br />

Fort Hope - James Bay - Attawapiskat supergrid were regridded to 80 metres.<br />

• all supergrids were created using Geosoft’s GridKnit TM routine. The total magnetic<br />

field grids were merged using the suturing method, while the 2vd grids were merged<br />

using the blending method.<br />

The residual magnetic field supergrids were created from the individual residual magnetic field<br />

grids. The second vertical derivative supergrids were created from the individual second vertical<br />

derivative grids.<br />

Two different grid stitching methods were used for the total magnetic field and the second<br />

vertical derivative grids. The total magnetic field grids have been levelled to the <strong>Ontario</strong> Master<br />

Grid but there still may be a static shift or trend between neighbouring grids. The suture method<br />

is effective at removing these differences. By definition, the second vertical derivative grids<br />

have had a trend and static shift removed so that the mean value of the grid is approximately<br />

zero. Thus, further static shifts and trends would not be applied by using the blending method.<br />

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3) SPECIFIC DETAILS: <strong>MAGNETIC</strong> <strong>SUPERGRIDS</strong><br />

Thirty-two airborne magnetic surveys, in five geographical regions, containing 40 metre by 40<br />

metre cell size grids of the total magnetic field and its second vertical derivative were merged to<br />

create five 40 metre by 40 metre cell size supergrids of the total magnetic field and five<br />

supergrids of the second vertical derivative of the total magnetic field. Ten airborne magnetic<br />

surveys, in one geographical region, containing a 80 metre by 80 metre cell size grid of the total<br />

magnetic field and its second vertical derivative were merged to create a 80 metre by 80 metre<br />

cell size supergrid of the total magnetic field and a supergrid of the second vertical derivative of<br />

the total magnetic field. The supergrids were merged using the suture method of the Geosoft<br />

GridKnit TM software.<br />

Table 4 Final Continuation and grid cell size of the supergrids<br />

Survey<br />

Final<br />

Continuation<br />

Height (metres)<br />

Final Grid Cell Size<br />

(metres)<br />

Abitibi Supergrid 70 40 UTM 17N<br />

Bamaji - Vickers 30 40 UTM 15N<br />

Supergrid<br />

Stormy Supergrid 75 40 UTM 15N<br />

Schreiber Supergrid 45 40 UTM 16N<br />

Red Lake Supergrid 45 40 UTM 15N<br />

Fort Hope - James Bay -<br />

Attawapiskat Supergrid<br />

80 80 UTM 16N<br />

Final Projection<br />

(NAD27 NTv2)<br />

I. The Abitibi magnetic supergrid<br />

The magnetic sensor heights of the OTH surveys in the Abitibi area varied from 70 to 75 metres.<br />

As well, many of the proprietary surveys were at 70 metres, so that a final continuation height<br />

was chosen to be 70 metres.<br />

Table 5 Abitibi Supergrid<br />

Survey<br />

Magnetic<br />

Sensor Height<br />

(metres)<br />

Continuation<br />

(metres)<br />

Original Grid<br />

Cell Size<br />

(metres)<br />

Projection<br />

(NAD27<br />

NTv2)<br />

Kirkland Lake 75 -5 40 UTM 17N 1<br />

Matheson 72 -2 40 UTM 17N 2<br />

Temiskaming 100 -30 25 UTM 17N 3<br />

Temagami 70 0 40 UTM 17N 4<br />

Order of<br />

Merging<br />

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Temagami 70 0 40 UTM 17N 5<br />

South<br />

Gowan - Evelyn 45 +25 20 UTM 17N 6<br />

Cobalt 70 0 60 UTM 17N 7<br />

Abitibi 120 -50 40 UTM 17N 8<br />

Supergrid<br />

Robb - Jamieson 70 0 20 UTM 17N 9<br />

Turnbull – 75 -5 40 UTM 17N 10<br />

Godfrey<br />

Cochrane 70 0 40 UTM 17N 11<br />

Tyrell 90 -20 30 UTM 17N 12<br />

Amyot - 122 -52 30 UTM 17N 13<br />

Browning<br />

Kapuskasing - 100 -30 40 UTM 17N 14<br />

Chapleau<br />

Wawa Supergrid 30 +40 40 UTM 16N 15<br />

Latchford - 100 -30 50 UTM 17N 16<br />

Redwater<br />

Kenabeek 100 -30 40 UTM 17N 17<br />

Oba -<br />

Kapuskasing<br />

45 +25 40 UTM 17N 18<br />

The OTH surveys Kirkland Lake and Matheson and the OTH proprietary surveys Gowan –<br />

Evelyn, Turnbull – Godfrey, and Robb - Jamieson almost entirely overlaps the older Abitibi<br />

supergrid. Since the quality and resolution of the newer magnetic data is superior to that of the<br />

older Abitibi supergrid data, only the Kirkland Lake, Matheson, Gowan – Evelyn, Turnbull –<br />

Godfrey, and Robb - Jamieson data were used in the overlapping area.<br />

The Latchford-Redwater survey was originally one contiguous survey, but it overlapped with the<br />

Temagami survey. Thus the survey was windowed into two separate surveys with approximately<br />

1 kilometre of overlap with the Temagami survey.<br />

II.<br />

The Bamaji – Vickers magnetic supergrid<br />

The magnetic sensor height of the OTH survey Vickers was flown at 30 metres. Since the<br />

downward continuation of the Bamaji supergrid and Gitche Lake grids did not increase its noise<br />

significantly, the final continuation height was chosen to be at 30 metres.<br />

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Table 6 Bamaji - Vickers Supergrid<br />

Survey<br />

Magnetic<br />

Sensor Height<br />

(metres)<br />

Continuation<br />

(metres)<br />

Original Grid<br />

Cell Size<br />

(metres)<br />

Projection<br />

(NAD27<br />

NTv2)<br />

Bamaji 120 -90 40 UTM 15N 1<br />

Supergrid<br />

Vickers 30 0 40 UTM 15N 2<br />

Gitche Lake 45 -15 20 UTM 15N 3<br />

Order of<br />

Merging<br />

III.<br />

The Stormy magnetic supergrid<br />

The magnetic sensor height of the OTH survey Stormy Lake was flown at 75 metres. Since the<br />

upward continuation of the Dryden supergrid, Docker and Kakagi Lake grids does not increase<br />

the noise, the final continuation height was chosen to be at 75 metres.<br />

Table 7 Stormy Supergrid<br />

Survey<br />

Magnetic<br />

Sensor Height<br />

(metres)<br />

Continuation<br />

(metres)<br />

Original Grid<br />

Cell Size<br />

(metres)<br />

Projection<br />

(NAD27<br />

NTv2)<br />

Stormy Lake 75 0 40 UTM 15N 1<br />

Supergrid<br />

Dryden 45 +30 40 UTM 15N 2<br />

Supergrid<br />

Docker 45 +30 25 UTM 15N 3<br />

Kakagi Lake 73 +2 40 UTM 15N 4<br />

Order of<br />

Merging<br />

The OTH survey Stormy Lake overlaps the Dryden supergrid. As the quality and resolution of<br />

the Stormy Lake magnetic data is superior to that of the Dryden supergrid data, only the Stormy<br />

Lake data were used in the overlapping area.<br />

IV.<br />

The Schreiber magnetic supergrid<br />

The magnetic sensor height of the OTH grid Schreiber was not chosen as the final continuation<br />

height. The three surveys that make up the Schreiber supergrid (Schreiber, Manitouwadge and<br />

Hemlo) were all flown at low terrain clearances. If the Schreiber height of 30 metres was chosen<br />

as the final continuation height, the Hemlo survey needed to be downward continued by 25<br />

metres. Such a large downward continuation of the Hemlo data increased the amount of noise to<br />

an unacceptable degree. A compromise height was chosen so that intermediate height of 45<br />

metres of the Manitouwadge survey was used as the final continuation height.<br />

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Table 8 Schreiber Supergrid<br />

Survey<br />

Magnetic<br />

Sensor Height<br />

(metres)<br />

Continuation<br />

(metres)<br />

Original Grid<br />

Cell Size<br />

(metres)<br />

Projection<br />

(NAD27<br />

NTv2)<br />

Schreiber 30 +15 40 UTM 16N 1<br />

GECO<br />

45 0 30 UTM 16N 2<br />

Manitouwadge<br />

Hemlo 55 -10 20 UTM 16N 3<br />

Order of<br />

Merging<br />

The OTH survey Schreiber overlaps the GECO Manitouwadge grid. As the quality and<br />

resolution of the Schreiber magnetic data is superior to that of the GECO Manitouwadge data,<br />

only the Schreiber data were used in the overlapping area.<br />

V. The Red Lake magnetic supergrid<br />

There were no OTH surveys flown in the Red Lake supergrid area. Thus the final continuation<br />

height was chosen to be the same as the existing Red Lake supergrid, i.e., a final continuation<br />

height of 45 metres. The downward continuation of the Troutlake River and Pakwash Lake<br />

surveys did not increase its noise significantly.<br />

Table 9 Red Lake Supergrid<br />

Survey<br />

Magnetic<br />

Sensor Height<br />

(metres)<br />

Continuation<br />

(metres)<br />

Original Grid<br />

Cell Size<br />

(metres)<br />

Projection<br />

(NAD27<br />

NTv2)<br />

Red Lake 45 0 40 UTM 15N 1<br />

Supergrid<br />

Troutlake River 73 -28 40 UTM 15N 2<br />

Pakwash Lake 65 -20 50 UTM 15N 3<br />

Order of<br />

Merging<br />

The OTH proprietary surveys Troutlake River, and Pakwash Lake overlap the Red Lake<br />

supergrid. As the quality and resolution of the Troutlake River, and Pakwash Lake magnetic<br />

data is much superior to those of the Red Lake supergrid data, only the Troutlake River, and<br />

Pakwash Lake data were used in the overlapping area.<br />

VI.<br />

The Fort Hope - James Bay – Attawapiskat magnetic supergrid<br />

Fort Hope, Albany River – James Bay and Attawapiskat are the three large grids that comprise<br />

most of the Fort Hope - James Bay – Attawapiskat supergrid. The James Bay and Attawapiskat<br />

surveys were flown with a sensor height of 80 metres and this height was chosen as the final<br />

continuation height. Only one grid, the Kapiskau River East survey, had to be downward<br />

continued, but did not increase its noise significantly.<br />

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Table 10 Fort Hope - James Bay - Attawapiskat Supergrid<br />

Survey<br />

Magnetic<br />

Sensor Height<br />

(metres)<br />

Continuation<br />

(metres)<br />

Original Grid<br />

Cell Size<br />

(metres)<br />

Projection<br />

(NAD27<br />

NTv2)<br />

Attawapiskat 80 0 40 and 80 UTM 16N 1<br />

Albany River - 80 0 80 UTM 16N 2<br />

James Bay<br />

Kenogami River 65 +15 50 UTM 16N 3<br />

Nagagami –<br />

Squirrel -<br />

Wakashi Rivers<br />

56 +24 40 UTM 16N 4<br />

Albany –<br />

Atikameg -<br />

Attawapiskat<br />

Rivers<br />

80 0 40 and 80 UTM 16N 5<br />

Kapiskau River 100 -20 50 UTM 17N 6<br />

East<br />

Fort Hope 75 +5 40 UTM 16N 7<br />

The Nagagami – Squirrel - Wakashi Rivers survey consisted of three separate aeromagnetic<br />

surveys. The Albany – Atikameg - Attawapiskat Rivers survey consisted of two separate<br />

aeromagnetic surveys.<br />

Order of<br />

Merging<br />

Grids that had a grid cell size less than 80 metres were regridded to 80 metres in the GridKnit TM<br />

process.<br />

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APPENDIX A<br />

ARCHIVE DEFINITION<br />

Data File Layout<br />

The files are archived on two Geophysical Data Set CD’s 1037a and 1037b which contain ASCII<br />

and Geosoft ® binary formatted data respectively. The content of the ASCII and binary products<br />

is identical. They are provided in both forms to suit the user’s available software.<br />

Coordinate Systems<br />

The gridded data are provided in the two UTM coordinate systems:<br />

Abitibi Supergrid<br />

• Universal Transverse Mercator (UTM) projection, Zone 17N, NAD27 datum, Canada<br />

NTv2 (20 min) local datum<br />

• Universal Transverse Mercator (UTM) projection, Zone 17N, NAD83 datum, North<br />

American local datum<br />

Bamaji - Vickers Supergrid<br />

• Universal Transverse Mercator (UTM) projection, Zone 15N, NAD27 datum, Canada<br />

NTv2 (20 min) local datum<br />

• Universal Transverse Mercator (UTM) projection, Zone 15N, NAD83 datum, North<br />

American local datum<br />

Stormy Supergrid<br />

• Universal Transverse Mercator (UTM) projection, Zone 15N, NAD27 datum, Canada<br />

NTv2 (20 min) local datum<br />

• Universal Transverse Mercator (UTM) projection, Zone 15N, NAD83 datum, North<br />

American local datum<br />

Schreiber Supergrid<br />

• Universal Transverse Mercator (UTM) projection, Zone 16N, NAD27 datum, Canada<br />

NTv2 (20 min) local datum<br />

• Universal Transverse Mercator (UTM) projection, Zone 16N, NAD83 datum, North<br />

American local datum<br />

Red Lake Supergrid<br />

• Universal Transverse Mercator (UTM) projection, Zone 15N, NAD27 datum, Canada<br />

NTv2 (20 min) local datum<br />

• Universal Transverse Mercator (UTM) projection, Zone 15N, NAD83 datum, North<br />

American local datum<br />

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Fort Hope - James Bay - Attawapiskat Supergrid<br />

• Universal Transverse Mercator (UTM) projection, Zone 16N, NAD27 datum, Canada<br />

NTv2 (20 min) local datum<br />

• Universal Transverse Mercator (UTM) projection, Zone 16N, NAD83 datum, North<br />

American local datum<br />

The original profile, electromagnetic and gridded data were compiled in UTM NAD27<br />

projection. No documentation could be found that specified a local datum. A local datum of<br />

Canada NTv2 (20 min) was assumed and used to create the reprojected data in UTM NAD83,<br />

North American local datum.<br />

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Gridded Data<br />

The gridded data are provided in two formats, one ASCII and one binary:<br />

• *.gxf - ASCII Grid eXchange Format (revision 3.0)<br />

• *.grd - Geosoft OASIS montaj binary grid file (no compression)<br />

• *.gi - binary file that defines the coordinate system for the *.grd file<br />

The grids are summarized as follows:<br />

thabmagsup27.grd/.gxf<br />

thabmagsup83.grd/.gxf<br />

thab2vdsup27.grd/.gxf<br />

thab2vdsup83.grd/.gxf<br />

thbamagsup27.grd/.gxf<br />

thbamagsup83.grd/.gxf<br />

thba2vdsup27.grd/.gxf<br />

thba2vdsup83.grd/.gxf<br />

thjafhmagsup27.grd/.gxf<br />

thjafhmagsup83.grd/.gxf<br />

thjafh2vdsup27.grd/.gxf<br />

thjafh2vdsup83.grd/.gxf<br />

thrlmagsup27.grd/.gxf<br />

thrlmagsup83.grd/.gxf<br />

thrl2vdsup27.grd/.gxf<br />

thrl2vdsup83.grd/.gxf<br />

thshmagsup27.grd/.gxf<br />

thshmagsup83.grd/.gxf<br />

thsh2vdsup27.grd/.gxf<br />

Abitibi supergrid of the GSC levelled magnetic field in nanoteslas<br />

(UTM coordinates, NAD27 datum)<br />

Abitibi supergrid of the GSC levelled magnetic field in nanoteslas<br />

(UTM coordinates, NAD83 datum)<br />

Abitibi supergrid of the calculated second vertical derivative of total magnetic field in<br />

nanoteslas per metre 2 (UTM coordinates, NAD27 datum)<br />

Abitibi supergrid of the calculated second vertical derivative of total magnetic field in<br />

nanoteslas per metre 2 (UTM coordinates, NAD83 datum)<br />

Bamaji – Vickers supergrid of the GSC levelled magnetic field in nanoteslas<br />

(UTM coordinates, NAD27 datum)<br />

Bamaji – Vickers supergrid of the GSC levelled magnetic field in nanoteslas<br />

(UTM coordinates, NAD83 datum)<br />

Bamaji – Vickers supergrid of the calculated second vertical derivative of total magnetic<br />

field in nanoteslas per metre 2 (UTM coordinates, NAD27 datum)<br />

Bamaji – Vickers supergrid of the calculated second vertical derivative of total magnetic<br />

field in nanoteslas per metre 2 (UTM coordinates, NAD83 datum)<br />

Fort Hope - James Bay - Attawapiskat supergrid of the GSC levelled magnetic field in<br />

nanoteslas (UTM coordinates, NAD27 datum)<br />

Fort Hope - James Bay - Attawapiskat supergrid of the GSC levelled magnetic field in<br />

nanoteslas (UTM coordinates, NAD83 datum)<br />

Fort Hope - James Bay - Attawapiskat supergrid of the calculated second vertical<br />

derivative of total magnetic field in nanoteslas per metre 2 (UTM coordinates, NAD27<br />

datum)<br />

Fort Hope - James Bay - Attawapiskat supergrid of the calculated second vertical<br />

derivative of total magnetic field in nanoteslas per metre 2 (UTM coordinates, NAD83<br />

datum)<br />

Red Lake supergrid of the GSC levelled magnetic field in nanoteslas<br />

(UTM coordinates, NAD27 datum)<br />

Red Lake supergrid of the GSC levelled magnetic field in nanoteslas<br />

(UTM coordinates, NAD83 datum)<br />

Red Lake supergrid of the calculated second vertical derivative of total magnetic field in<br />

nanoteslas per metre 2 (UTM coordinates, NAD27 datum)<br />

Red Lake supergrid of the calculated second vertical derivative of total magnetic field in<br />

nanoteslas per metre 2 (UTM coordinates, NAD83 datum)<br />

Schreiber supergrid of the GSC levelled magnetic field in nanoteslas<br />

(UTM coordinates, NAD27 datum)<br />

Schreiber supergrid of the GSC levelled magnetic field in nanoteslas<br />

(UTM coordinates, NAD83 datum)<br />

Schreiber supergrid of the calculated second vertical derivative of total magnetic field in<br />

nanoteslas per metre 2 (UTM coordinates, NAD27 datum)<br />

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thsh2vdsup83.grd/.gxf<br />

thskmagsup27.grd/.gxf<br />

thskmagsup83.grd/.gxf<br />

thsk2vdsup27.grd/.gxf<br />

thsk2vdsup83.grd/.gxf<br />

Schreiber supergrid of the calculated second vertical derivative of total magnetic field in<br />

nanoteslas per metre 2 (UTM coordinates, NAD83 datum)<br />

Stormy Lake supergrid of the GSC levelled magnetic field in nanoteslas<br />

(UTM coordinates, NAD27 datum)<br />

Stormy Lake supergrid of the GSC levelled magnetic field in nanoteslas<br />

(UTM coordinates, NAD83 datum)<br />

Stormy Lake supergrid of the calculated second vertical derivative of total magnetic field<br />

in nanoteslas per metre 2 (UTM coordinates, NAD27 datum)<br />

Stormy Lake supergrid of the calculated second vertical derivative of total magnetic field<br />

in nanoteslas per metre 2 (UTM coordinates, NAD83 datum)<br />

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APPENDIX B<br />

MERGING OF GRIDS BY GRIDKNIT TM METHOD<br />

(Documentation supplied by Geosoft Inc.)<br />

Stitch Method<br />

Geosoft’s GridKnit TM enables you to stitch together any two grids, even if the grids have<br />

different cell sizes and/or transforms. The GridKnit TM tool delivers two advanced methods that<br />

produce fast, high-quality results for virtually any type of geophysical grid. The blending<br />

method provides a quick way of merging two grids via standard smoothing functions. The<br />

suturing method enables you to automatically or manually define a suture path for estimating<br />

errors and then applies a proprietary multi-frequency correction along the path. This method is<br />

used for joining grids that have a narrow overlap area and relatively small anomalies. Suturing<br />

provides more accurate results and greater control than blending.<br />

Blending Method<br />

The Blending method uses a blending function over the area of overlap so that transition from<br />

one grid to the other is smooth. Except for the optional removal of a static offset or trend, the<br />

grids beyond the overlap regions remain unchanged.<br />

The blending function determines the<br />

weighting of one grid against the other inside<br />

the overlap region. The function works by<br />

calculating the distance to the edge of each<br />

grid for each data point. The diagram on the<br />

right shows the distance to the edge of Grid 1<br />

(from a single data point ) as D 1 and the<br />

distance to Grid 2 as D 2 . The blending<br />

function uses a “cosine” function which varies<br />

smoothly from 0 to 1 – the function takes on<br />

the value of 0.5 at positions midway between<br />

the two grids, and whose derivative approaches<br />

0 at both ends. If a position is equidistance<br />

between both edges, its value is the average of<br />

the grid values found at that point. The<br />

diagram (right) shows the value (on the cosine<br />

curve) for Grid 1 is around 0.7 and the value<br />

for Grid 2 is 0.3. This means that when the<br />

blending function calculates the value for the<br />

data point, it uses 0.7 of the value of the point<br />

on Grid 1 and 0.3 of the value of the point on<br />

Grid 2.<br />

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Note: Where the edges of Grid 1 and Grid 2 cross at any single point, the blending scheme<br />

breaks down, since by definition both grids are full owners of that point. In this case the<br />

average of the two grid values at that point will be used.<br />

Suture Method<br />

The suture method defines a suture line to determine where the grids will be joined. The line<br />

must lie completely within the overlapping area of the two grids. The area outside of the overlap<br />

remains unchanged.<br />

Along the suture line, a mismatch in the grid values is corrected by adjusting the grids on either<br />

side of the path. For instance, for a point on the suture path where the value for Grid #1 is larger<br />

than the value for Grid #2, the average value is used to eliminate discrepancies. Points adjacent<br />

to the path point might then be adjusted to produce a smooth transition between the two grids.<br />

The suture method uses a multi-frequency approach to spread corrections over the two grids in<br />

proportion to the wavelength of the mismatch found along the suture path. This ensures that the<br />

transition from one grid to the other remains smooth, regardless of the amplitude and wavelength<br />

of the features that the suture path crosses.<br />

Locating a Suture Path<br />

The suture line must be located inside the<br />

overlap area between the two grids.<br />

GridKnit provides four methods of<br />

determining the position of the suture line<br />

in the overlap area between the two grids.<br />

• Automatic<br />

• Interactive<br />

• Grid 1 edge<br />

• Grid 2 edge<br />

The diagram on the right illustrates where<br />

the suture path is located using each<br />

method. The automatic suture path is<br />

located equidistant between the two grid<br />

edges. The interactive suture line is<br />

defined by the user and can be located<br />

anywhere in the overlap area. The grid 1<br />

suture option uses the edge of Grid 1 as<br />

the suture path. Likewise, the Grid 2<br />

option uses the edge of grid 2 as the suture<br />

path.<br />

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Automatic Suture Path<br />

If the automatic option is selected, the suture line will bisect the overlap region; every point<br />

along the line will be at approximately equal distance from the borders (grid edges) of the<br />

overlap region. Use this method when you want to place the suture line in the middle of the two<br />

grids and use both grids equally to determine the values of the output grid.<br />

Interactive Suture Path Definition<br />

If the interactive option is selected, the user must define a path using the current map as a<br />

reference. (If there is no current map, one will be requested).<br />

All suture paths must, by definition, lie within regions of overlap. The start and end points of the<br />

path within these regions is pre-determined by the geometry of the overlap, and cannot be<br />

altered. Those parts of the user-path not intersecting the overlapping grid sections are ignored. If<br />

the "start" and/or "end" points are not present in the user-path, the user-path is automatically<br />

altered to include them. It does this by joining the first and last points of the user-path within the<br />

overlap to the fixed start and end points. The resulting path may not cross any dummy positions,<br />

or any non-overlapping region of the data, or an error occurs.<br />

A single user-path may be used to define the path through two or more separate overlap sections<br />

by including at least one "outside" point as a space indicator between each path section through<br />

an overlap area. (All "outside" points are ignored when calculating the suture path from a userpath.)<br />

Postage Stamp Stitching (Grid Edge Path)<br />

"Postage stamp" stitching is used to incorporate a smaller grid into a larger grid; this is<br />

accomplished using the Grid Edge path selections. Selecting the Grid Edge path corresponding<br />

to that grid may preserve the contents of the entire smaller grid – the suture path will entirely<br />

enclose the smaller grid.<br />

Note: The path creation algorithm may run into difficulty when the Grid Edge path is selected if<br />

the boundaries of the grid are not sufficiently smooth. It may be necessary to smooth<br />

jagged edges, remove "peninsulas" or fill in "bays" using interpolation (see Preprocessing<br />

Algorithms) in order for the path to be determined unambiguously. The<br />

automatic option produces smoother paths due to the averaging effects of using edges<br />

from both grids simultaneously, and finding the midpoints between them.<br />

Suture Weighting<br />

A value in the range 0 to 1 determines how corrections are apportioned between the grids. A<br />

cosine function is used to weight the grids. The figure below shows how the weight function<br />

works. The numbers of the side of the chart below represent the proportion of weighting for each<br />

grid. For example, to calculate the suture point referring to the grid value (dot) closest to the<br />

bottom, the weighting function would use 0.25 of grid 1 and 0.75 of grid 2. Similarly, if a value<br />

of the “Proportion of Grid 1” is 0, then all corrections are applied to Grid 1. A value of 0<br />

indicates that all corrections are applied to Grid 2, and value of 0.5 (dot in the centre) means<br />

corrections are shared equally between both grids.<br />

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By default, the weighting is even between the grids. However, by forcing all the corrections<br />

toward one grid or the other, the user can keep one grid unaltered up to and including the suture<br />

path.<br />

Suture Weighting<br />

1<br />

0<br />

0.75<br />

0.25<br />

Proportion<br />

of Grid 1<br />

0.5<br />

0.5<br />

Proportion<br />

of Grid 2<br />

0.25<br />

0.75<br />

0<br />

Multi-Frequency Suturing Algorithm (Fast Fourier Transform)<br />

1<br />

To ensure that the suturing process creates the smoothest possible transition between grids,<br />

GridKnit, uses a Multi-Frequency Fourier Transform (FFT) function. A Fourier transform<br />

breaks a single, complex curve into a family of 'sine' type curves, each with a unique frequency<br />

and amplitude.<br />

The diagram below illustrates how the function works in suturing. GridKnit first selects the<br />

grid values along the suture line for each grid. The grid values (frequency) for the points from<br />

each grid along the suture path are plotted. In the diagram below, Grid 1 values along the suture<br />

line are represented by the red line and Grid 2 values by the blue line. The system calculates the<br />

difference (purple line) between the values of Grid 1 and Grid 2.<br />

Grid<br />

Values<br />

(V )<br />

3<br />

2.5<br />

2<br />

1.5<br />

1<br />

0.5<br />

0<br />

-0.5<br />

Grid 2<br />

Grid 1<br />

Difference<br />

Distance<br />

(D)<br />

Grid 1<br />

Grid 2<br />

Difference<br />

The difference curve is split using a Fourier transform function, into many curves, each<br />

representing a unique frequency (or wavelength). Next, a cascading "smooth" correction surface<br />

is applied to each unique frequency (or wavelength) curve. The correction surface (grid) applied<br />

for each wavelength is proportional to the wavelength. This proportional correction means that<br />

narrow features on a grid are given a narrow correction and wider features are given a wider<br />

correction. The correction surface for each frequency is added to the existing overlapping grid<br />

area so that the grids join perfectly at the edges.<br />

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Pre-processing Tools<br />

Grid Cell Size<br />

If you have two grids with different cell sizes, the cell size and transform of the first grid have<br />

primacy. GridKnit will automatically convert the grid cell size of the second grid to match that<br />

of the first. Also, the offsets are adjusted (even to the primary grid) to ensure that grid lines in the<br />

output overlie the zero axes. If you wish to check or modify the cell size of one of your grids<br />

manually, follow the procedure below.<br />

TO CHECK GRID CELL SIZE<br />

1 To determine the cell size of a grid, select the Grid|Grid Info… menu.<br />

2 Specify the grid name and press the button. The system will display the grid information.<br />

3 The two numbers in the X Element Separation and Y Element Separation fields represent the grid cell size.<br />

These numbers must be the same for both grids.<br />

TO CHANGE GRID CELL SIZE<br />

1 To change the cell size of a grid, select the Grid|Gridding|Re-grid a grid… menu item.<br />

2 Specify the input and output name of the grid.<br />

3 Modify the cell size so that it matches the cell size of the other grid. Press the button.<br />

Trend Order<br />

The Trend Removal dialog box enables you to remove a static shift or trend from one or both<br />

grids before stitching. The static or zero-order correction adds or removes a single average value<br />

from the entire grid. Use this trend when you want to increase or decrease all the values on a grid<br />

by a constant amount. The slope or first-order correction removes the best-fitting plane. If none<br />

is specified for grid #1, and a trend is specified for grid #2, then grid #2 takes on the specified<br />

trend of grid #1 (i.e. grid #2 is brought to grid #1). However, if a trend is specified for both grids,<br />

the specified trends are removed individually from both grids.<br />

The trend options enable you to set a different trend order for each grid. This option is useful if<br />

you are connecting a small grid to a master grid and want to adjust the trend of the smaller grid<br />

to the master grid. In this case, you would select none for the master grid and another trending<br />

method (static or slope) for the smaller grid.<br />

Point Usage<br />

The calculation for the Trend Order correction may be done in one of three ways: using all the<br />

points in the grid, using the edge points, or using only the points that overlap with the other grid.<br />

It is not recommended to use the overlap point selection for the first-order (slope) correction in<br />

cases where the overlap region is small, or thin in one dimension. In these situations, the trend in<br />

a small region of the grid may be quite different from that found in the remainder, and removing<br />

it may seriously alter the appearance of the full grid.<br />

Note: If "edge points" is selected, and there is more than one data area in the grid data, then<br />

only the first section that the algorithm encounters is used in the calculation.<br />

Report on Magnetic Supergrids<br />

Geophysical Data Set 1037<br />

27


Interpolation Options<br />

The Interpolation Options dialog box in GridKnit enables the user to set the spline method to<br />

use during interpolation and the maximum gap to interpolate across. Interpolation is used to fill<br />

gaps between points in individual grids prior to grid stitching.<br />

Spline Method<br />

The spline method determines how values are predicted in areas without data. Three methods are<br />

available: Linear, Cubic, and Akima. The linear spline assumes a simple linear variation between<br />

the values bounding the gap. The cubic spline is a minimum-curvature method. In cases where<br />

the data contains rapid changes in the gradient, the minimum curvature spline may produce<br />

undesirable highs or lows in the gap. The Akima spline method does not suffer as much from this<br />

problem, although it does tend to produce sharper corners around actual data points and the<br />

resulting grid tends to be less smooth.<br />

Gap Size<br />

A gap refers to a hole in the gridded data or a nil or dummy value within the dataset. If the gap<br />

size is set to a value "x", then all gaps in the data smaller than size "x" will be interpolated prior<br />

to stitching. If the gap size is set to 0.0, all gaps will be interpolated. If the gap size is not<br />

specified, no interpolation is performed prior to stitching.<br />

Grids may have gaps or holes inside the overlap region. The presence of gaps will affect the<br />

behaviour of the stitching methods. If the blending method finds a gap in the overlapping area of<br />

a grid, it fills in the gap by using the values from the other grid.<br />

In the suture method the suture path will tend to avoid the gaps, because it chooses the path<br />

midway between the edges of the two grids. Furthermore, a long-wavelength feature lying along<br />

the suture path may be interpreted as two or more short-wavelength features, with less than<br />

optimal results. These effects may be reduced or eliminated by choosing to interpolate the gaps<br />

prior to the stitching process.<br />

The interpolated values are used only during stitching to alter or improve performance of the<br />

stitching algorithm. When the final stitched grid is constructed, it is done on the basis of the<br />

original, un-interpolated grids. For instance, if both grids have a gap in the same location in the<br />

overlap area, then the gap will remain in the combined grids. In the same manner, gaps outside<br />

the blending area always remain in the output grid. If you wish to remove gaps from the final<br />

combined grid, either interpolate the grids separately prior to running the grid stitching routine,<br />

or interpolate the resulting, combined grid afterwards.<br />

Report on Magnetic Supergrids<br />

Geophysical Data Set 1037<br />

28

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