MAGNETIC SUPERGRIDS Ontario Airborne ... - Geology Ontario
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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 />
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Geophysical Data Set 1037Rev.<br />
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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 />
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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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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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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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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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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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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 />
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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 />
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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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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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Geophysical Data Set 1037<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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Geophysical Data Set 1037<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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Geophysical Data Set 1037<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 />
Report on Magnetic Supergrids<br />
Geophysical Data Set 1037<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