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INTRODUCTION TO UTM COORDINATES AND MAP DATUMS
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UTM COORDINATES ZONE CENTRAL MERIDIAN = 500,000 m 300,000 700,000 500,000 108102 105
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TRANSVERSE MERCATOR
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UTM ZONES UNITED STATES NM
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UTM CARTISIAN COORDINATES
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USGS MAPS AND UTM
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COORDINATE SYSTEMS NAD 27 = North American Datum, 1927 NAV 29 = North American Vertical, 1929 NAD 83 = North American Datum, 1983 WGS 84 = World Geodetic System 1984 (ALL GPS) CORPSCON – CONVERSION PROGRAM
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INTRODUCTION TO MAGNETIC METHODS –Earth’s Magnetic Field –Rock Magnetism –Geologic Models Magnetic Anomaly Sources –Planning a Survey –Examples REFERENCE: Sheldon Breiner, Applications Manual for Portable Magnetometers www.georentals.co.uk/ampm-opt.pdf
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TOTAL FIELD MEASUREMENTS
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EARTH’S DIPOLE FIELD
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MAGNETIC ELEMENTS H = F cos I Z = F sin I = H tan I X = cos D Y = H sin D X² + Y² = H² X² + Y² + Z² = F² F = Total Field Intensity I = Inclination D = Declination H = Horizontal Component X = North Component Y = East Component Z = Vertical Component East North
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TOTAL INTENSITY 25 70 X 1000 nTeslas 50
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GEOMAGNETIC INCLINATION 60N 80N 0 80S 60S GEOMAGNETIC INCLINATION DEGREES OF ARC FROM HORIZONTAL
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CHANGES IN DECLINATION AND INCLINATION AT LONDON SINCE 1540 SECULAR VARIATIONS 2010 Declination Inclination
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SOLAR DIURNAL VARIATIONS MID NORTHERN AND MID SOUTHERN LATITUDES 50 nT EQUATORIAL LATITUDES
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MICRO PULSATIONS 10 nT 10 minutes
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TYPICAL MAGNETIC STORM 50 nT 1 day
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CORRECTING FOR TIME VARYING FIELDS F = f(x,y,z,t) –x = Easting (Longitude) –y = Northing (Latitude) –z = Elevation (very small effect) –t = time F B = Field at Base Station (time dependent) F R = Field at Rover (space/time dependent) F C = Time Correct Field at Rover = F B – F R GEOREF = Geomagnetic Reference Correction
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AVERAGE MAGNETIC SUSCEPTIBILITIES BASIC IGENOUS ACID IGNEOUS METAMORPHIC SEDIMENTARY Magnetic Susceptibility x 10 6 (c.g.s.)
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MEASURED SUSCEPTIBILITIES OF ROCK MATERIALS MaterialK x 10 6 cgsAt H, Oe Magnetite300,000-800,0000.6 Pyrrhotite125,0000.5 Ilmenite135,0001.0 Franklinite36,000 Granite28-27001.0 Diorite46.81.0 Gabbro68-23701.0 Basalt6801.0 Sandstone161.0
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INDUCED VS REMANENT MAGNETIZATION Induced Magnetization –Polarization in direction of Earth’s Field Remanent Magnetization –Thermoremanent (Curie Temperature) –Detrital (Depositional) –Chemical
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GEOLOGICAL MODEL REPRESENTATIONS OF COMMON MAGNETIC ANOMALY SOURCES
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Dipoles vs. Monopoles vs. Arrays of Poles
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ANOMALIES FOR GEOLOGICAL BODIES AT VARIOUS ORIENTATIONS AND FIELD INCLINATIONS ↓ F F →F T N-S T E-W T N-S T E-W 1234512345
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TOTAL INTENSITY INDUCED DIPOLE SIGNATURES AT VARIOUS INCLINATIONS OF THE FIELD Induced dipole Vertical Field (North or South Poles) Induced dipole (Inclination 60 º) Induced dipole Equatorial Field (Inclination 0 º)
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REMANENT DIPOLE SIGNATURES MOMENT NOT PARALLEL TO INDUCING FIELD
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EFFECT OF DEPTH ON ANOMALY WIDTH The amplitude of the anomaly is maintained constant By adjusting the size of the anomalous body.
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DEPTH/AMPLITUDE BEHAVIOR OF DIPOLE ANOMALIES M 8MM Note: Same Amplitude but Change in width
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F DISTANCE nT 500 100 1 10 20010Ft 1 ton iron
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ANOMALIES OF COMMON OBJECTS OBJECT Ft/nT Ft/nT Automobile (1 ton) 30/40 100/1 Ship (1000 ton) 100/300-700 1000/1 Aircraft (light) 20/10-30 50/1 Pipeline (12”) 25/50-200 50/12-50 Wellhead 50/200-500 500/2-5 Fenceline 10/15 25/1-2 Rifle 5/10-50 10/ 2-10 Revolver 5/10-20 10/1-2
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TYPICAL MAGNETIC ANOMALIES OF COMMON ARCHAEOLOGICAL FEATURES Kiln-baked brick wall Sandstone wall in more magnetic soil Shallow grave or pathway Humus-rich site of habitation Shallow tomb Deeply buried tomb Bricks in disarray Fire pit with bricks In original position
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PLANNING A SURVEY SIZE OF TARGET AERIAL EXTENT OF SEARCH GROUND OR AIRBORNE RESOLUTION OF SURVEY FIELD METHODS PITFALLS EXAMPLES
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TYPICAL SEQUENCES OF TRAVERSES DURING SEARCH PROCEDURES Secondary Traverse Primary Traverse Final Traverse Object location Total magnetic field contours (not known during search)
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ESTIMATION OF DEPTH TO TOP OF ANOMALOUS BODIES USING MAXIMUM SLOPE
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52490 nT 52195 nT 52280 nT Contour Interval 5 nT GNTN Maximum slope 5 m
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F DISTANCE nT 500 100 1 10 20010Ft 1 ton iron SOLUTION FOR BILLS CRATER
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MAGNETIC EFFECT OF LATERAL SUSCEPTIBILITY CHANGE VS STRUCTURE
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HIGH RESOLUTION AIRBORNE MAGNETIC MAP OF THE SAGE 2010 FIELD AREA SAGE 2005 SEISMIC PROFILE SAGE 2005 MT PROFILE SAGE 2010 ARCH SITE
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