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COORDINATE GEOMETRY Except for Geodetic Control Surveys, most surveys are referenced to plane rectangular coordinate systems. Frequently State Plane Coordinate Systems are used. The advantage of referencing surveys to defined coordinate systems are: Spatial relations are uniquely defined. Points can be easily plotted. Coordinates provide a strong record of absolute positions of physical features and can thus be used to re-construct and physically re-position points that may have been physically destroyed or lost. Coordinate systems facilitate efficient computations concerning spatial relationships. In many developed countries official coordinate systems are generally defined by a national network of suitably spaced control points to which virtually all surveys and maps are referenced. Such spatial reference networks form an important part of the national infrastructure. They provide a uniform standard for all positioning and mapping activities.
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THE TRIANGLE x = -b ± b2 – 4ac is also often used.
The geometry of triangles is extensively employed in survey calculations. B For any triangle ABC with sides a, b and c: a = b = c (LAW OF SINES) sin A sin B sin C AND a2 = b2 + c2 -2ab cosA b2 = a2 + c2 -2ac cosB (LAW OF COSINES) c2 = a2 + b2 -2ab cosC c a A b C A + B + C = 180° The solution of the quadratic equation ax2 + bx + c = 0 x = -b ± b2 – 4ac is also often used. 2a
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THE STRAIGHT LINE Y ∆XAB = XB-XA AND ∆YAB = YB-YA
∆XAB = XB-XA AND ∆YAB = YB-YA LAB = ∆XAB2 + ∆YAB2 AzAB = atan(∆XAB / ∆YAB ) + C C=0° for ∆XAB >0 and ∆YAB >0 C=180° for ∆YAB <0 and C=360° for ∆XAB <0 and ∆YAB >0 B(XB,YB) P(XP,YP) AzAB For P on line AB: YP = mXp + b where the slope m = ((∆yAB / ∆xAB ) = cot(AzAB ) AzAB = atan (1/m) + C A(XA,YA) b
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THE CIRCLE Y P(XP,YP) R R2 = ∆XOP2 + ∆YOP2 O(XO,YO)
P(XP,YP) R R2 = ∆XOP2 + ∆YOP2 XP2+YP2 – 2XOXP – 2YOYP + f = 0 R = XO2 + YO2 - f O(XO,YO) f
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THE PERPENDICULAR OFFSET
Y X Given known points A,B and P, compute distance PC (LPC) C=0° for ∆XAB >0 and ∆YAB >0 C=180° for ∆YAB <0 and C=360° for ∆XAB <0 and ∆YAB >0 P(XP,YP) B(XB,YB) AzAP = atan(∆XAP / ∆YAP ) + C LAP = ∆XAP2 + ∆YAP2 AzAB = atan(∆XAB / ∆YAB ) + C LAB = ∆XAB2 + ∆YAB2 AzAP C a AzAB A(XA,YA) a = AzAB – AzAP LPC = LAB sin LAC = LAB cos a b
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THE INTERSECTION Y X Given A(XA,YA), B(XB,YB), AzAP and AzBP compute P(XP,YP) AzAB = atan(∆XAB / ∆YAB ) + C LAB = ∆XAB2 + ∆YAB2 a = AzAB – AzAP β = AzBA – AzBP γ = 180° – a – β LAP = LAB (sin rule) sin β sin γ LAP = LAB (sin β / sin γ ) XP = XA + LAP sin AzAP YP = YA + LAP cos AzAP C=0° for ∆XAB >0 and ∆YAB >0 C=180° for ∆YAB <0 and C=360° for ∆XAB <0 and ∆YAB >0 B(XB,YB) AzBP AzAP β Outside Orientation AzBA Similarly (as a check on the calculations): LBP = LAB (sin rule) sin a sin γ LBP = LAB (sin β / sin γ ) XP = XA + LBP sin AzBP YP = YA + LBP cos AzBP AzAB a γ A(XA,YA) P(XP,YP) WARNING: USE A THIRD KNOWN POINT TO CHECK ORIENTATIONS
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INTERSECTION OF A LINE WITH A CIRCLE
Y X Given A,B and C and radius R, compute P1 and P2 Note a = AzAC – AzAB and LBP1 = LBP2 = R Apply the cos rule to triangle ABP1: LBP12 = LAB2+ LAP12-2(LAB)(LAP1)cos a or LAP12 –(2LABcos a) LAP1 + (LAB2 - LBP12) = 0 which is a quadratic equation with LAP1 as unknown C(XC,YC) B(XB,YB) R Note that since LBP1 = LBP2 = R the above equation also applies to triangle ABP2. Hence the two solutions of the quadratic equation are AP1 and AP2. P2(XP2,YP2) a P1(XP1,YP1) AP= 2LABcos a ± (2LABcos a)2-4(LAB2 - LBP12) 2 A(XA,YA) Now use AzAC and the solutions of AP to compute P1(XP1,YP1) and P2(XP2,YP2)
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INTERSECTION OF TWO CIRCLES
Y X Given A,B and C and radius R, compute P1 and P2 Note LAP1 = LAP2 = RA and LBP1 = LBP2 = RB Compute AzAB and LAB from given coordinates of A and B Apply the cos rule to triangle ABP1: a = acos ((LAB2+ LAP12-LBP12)/(2LABLAP1)) = acos ((LAB2+ RA2-RB2)/(2LABRA)) B(XB,YB) AzAP1 = AzAB – a and AzAP2 = AzAB + a P1(XP1,YP1) RB P2(XP2,YP2) a a XP1 = XA + RAsin (AzAP1) YP1 = YA + RAcos(AzAP1) and XP2 = XA + RAsin (AzAP2) YP2 = YA + RAcos(AzAP2) RA A(XA,YA) WARNING Trilatertion of a point with only two distances yields two positions!!!!!
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HOMEWORK: LECTURE 13 (CHAPTER 11 SEC 1-6)
11.1, 11.9, 11.13, 11.15, 11.17
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Types of Coordinate Systems
(1) Global Cartesian coordinates (x,y,z) for the whole earth (2) Geographic coordinates (f, l, z) (3) Projected coordinates (x, y, z) on a local area of the earth’s surface The z-coordinate in (1) and (3) is defined geometrically; in (2) the z-coordinate is defined gravitationally
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Global Cartesian Coordinates (x,y,z)
Greenwich Meridian Equator •
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Global Positioning System (GPS)
24 satellites in orbit around the earth Each satellite is continuously radiating a signal at speed of light, c GPS receiver measures time lapse, Dt, since signal left the satellite, Dr = cDt Position obtained by intersection of radial distances, Dr, from each satellite Differential correction improves accuracy
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Global Positioning using Satellites
Dr2 Dr3 Number of Satellites 1 2 3 4 Object Defined Sphere Circle Two Points Single Point Dr4 Dr1
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Geographic Coordinates (f, l, z)
Latitude (f) and Longitude (l) defined using an ellipsoid, an ellipse rotated about an axis Elevation (z) defined using geoid, a surface of constant gravitational potential Earth datums define standard values of the ellipsoid and geoid
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Shape of the Earth It is actually a spheroid, slightly larger in radius at the equator than at the poles We think of the earth as a sphere
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Ellipse Z b O a X F1 F2 P An ellipse is defined by:
Focal length = Distance (F1, P, F2) is constant for all points on ellipse When = 0, ellipse = circle Z b O a X F1 F2 For the earth: Major axis, a = 6378 km Minor axis, b = 6357 km Flattening ratio, f = (a-b)/a ~ 1/300 P
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Ellipsoid or Spheroid Rotate an ellipse around an axis
Z b O a a Y X Rotational axis
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Standard Ellipsoids Ref: Snyder, Map Projections, A working manual, USGS Professional Paper 1395, p.12
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Horizontal Earth Datums
An earth datum is defined by an ellipse and an axis of rotation NAD27 (North American Datum of 1927) uses the Clarke (1866) ellipsoid on a non geocentric axis of rotation NAD83 (NAD,1983) uses the GRS80 ellipsoid on a geocentric axis of rotation WGS84 (World Geodetic System of 1984) uses GRS80, almost the same as NAD83
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Definition of Latitude, f
m S p n O f q r (1) Take a point S on the surface of the ellipsoid and define there the tangent plane, mn (2) Define the line pq through S and normal to the tangent plane (3) Angle pqr which this line makes with the equatorial plane is the latitude f, of point S
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Cutting Plane of a Meridian
Equator plane Prime Meridian
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Definition of Longitude, l
l = the angle between a cutting plane on the prime meridian and the cutting plane on the meridian through the point, P 180°E, W -150° 150° -120° 120° 90°W (-90 °) 90°E (+90 °) -60° P l -60° -30° 30° 0°E, W
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Latitude and Longitude on a Sphere
Z Meridian of longitude Greenwich meridian N Parallel of latitude =0° P • =0-90°N - Geographic longitude - Geographic latitude W O E • Y R R - Mean earth radius • =0-180°W Equator =0° • O - Geocenter =0-180°E X =0-90°S
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Length on Meridians and Parallels
(Lat, Long) = (f, l) Length on a Meridian: AB = Re Df (same for all latitudes) R Dl 30 N R D C Re Df B 0 N Re Length on a Parallel: CD = R Dl = Re Dl Cos f (varies with latitude) A
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Example: What is the length of a 1º increment along
on a meridian and on a parallel at 30N, 90W? Radius of the earth = 6370 km. Solution: A 1º angle has first to be converted to radians p radians = 180 º, so 1º = p/180 = /180 = radians For the meridian, DL = Re Df = 6370 * = 111 km For the parallel, DL = Re Dl Cos f = 6370 * * Cos 30 = 96.5 km Parallels converge as poles are approached
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Representations of the Earth
Mean Sea Level is a surface of constant gravitational potential called the Geoid Earth surface Ellipsoid Sea surface Geoid
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Geoid and Ellipsoid Gravity Anomaly
Earth surface Ellipsoid Ocean Geoid Gravity Anomaly Gravity anomaly is the elevation difference between a standard shape of the earth (ellipsoid) and a surface of constant gravitational potential (geoid)
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Definition of Elevation
Elevation Z P z = zp • z = 0 Land Surface Mean Sea level = Geoid Elevation is measured from the Geoid
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Vertical Earth Datums A vertical datum defines elevation, z
NGVD29 (National Geodetic Vertical Datum of 1929) NAVD88 (North American Vertical Datum of 1988) takes into account a map of gravity anomalies between the ellipsoid and the geoid
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Converting Vertical Datums
Corps program Corpscon (not in ArcInfo) Point file attributed with the elevation difference between NGVD 29 and NAVD 88 NGVD 29 terrain + adjustment = NAVD 88 terrain elevation
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Geodesy and Map Projections
Geodesy - the shape of the earth and definition of earth datums Map Projection - the transformation of a curved earth to a flat map Coordinate systems - (x,y) coordinate systems for map data
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Earth to Globe to Map Map Projection: Map Scale: Scale Factor
Representative Fraction Globe distance Earth distance = Scale Factor Map distance Globe distance = (e.g. 1:24,000) (e.g )
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Geographic and Projected Coordinates
(f, l) (x, y) Map Projection
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Projection onto a Flat Surface
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Types of Projections Conic (Albers Equal Area, Lambert Conformal Conic) - good for East-West land areas Cylindrical (Transverse Mercator) - good for North-South land areas Azimuthal (Lambert Azimuthal Equal Area) - good for global views
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Conic Projections (Albers, Lambert)
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Cylindrical Projections (Mercator)
Transverse Oblique
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Azimuthal (Lambert)
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Albers Equal Area Conic Projection
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Lambert Conformal Conic Projection
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Universal Transverse Mercator Projection
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Lambert Azimuthal Equal Area Projection
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Projections Preserve Some Earth Properties
Area - correct earth surface area (Albers Equal Area) important for mass balances Shape - local angles are shown correctly (Lambert Conformal Conic) Direction - all directions are shown correctly relative to the center (Lambert Azimuthal Equal Area) Distance - preserved along particular lines Some projections preserve two properties
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Geodesy and Map Projections
Geodesy - the shape of the earth and definition of earth datums Map Projection - the transformation of a curved earth to a flat map Coordinate systems - (x,y) coordinate systems for map data
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Coordinate Systems Universal Transverse Mercator (UTM) - a global system developed by the US Military Services State Plane Coordinate System - civilian system for defining legal boundaries California State Mapping System - a statewide coordinate system for California
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Coordinate System A planar coordinate system is defined by a pair
of orthogonal (x,y) axes drawn through an origin Y X Origin (xo,yo) (fo,lo)
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Universal Transverse Mercator
Uses the Transverse Mercator projection Each zone has a Central Meridian (lo), zones are 6° wide, and go from pole to pole 60 zones cover the earth from East to West Reference Latitude (fo), is the equator (Xshift, Yshift) = (xo,yo) = (500000, 0) in the Northern Hemisphere, units are meters
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UTM Zone 21 &22 -123° -102° -96° 6° Origin Equator -120° -90 ° -60 °
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State Plane Coordinate System
Defined for each State in the United States East-West States (e.g. Texas) use Lambert Conformal Conic, North-South States (e.g. California) use Transverse Mercator Texas has five zones (North, North Central, Central, South Central, South) to give accurate representation Greatest accuracy for local measurements
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California Mapping System
Designed to give State-wide coverage of Texas without gaps Lambert Conformal Conic projection with standard parallels 1/6 from the top and 1/6 from bottom of the State Adapted to Albers equal area projection for working in hydrology
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Standard Hydrologic Grid (SHG)
Developed by Hydrologic Engineering Center, US Army Corps of Engineers Uses USGS National Albers Projection Parameters Used for defining a grid over the US with cells of equal area and correct earth surface area everywhere in the country
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Coordinate Systems Geographic coordinates (decimal degrees)
Projected coordinates (length units, ft or meters)
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Summary Concepts Two basic locational systems: geometric or Cartesian (x, y, z) and geographic or gravitational (f, l, z) Mean sea level surface or geoid is approximated by an ellipsoid to define an earth datum which gives (f, l) and distance above geoid gives (z)
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Summary Concepts (Cont.)
To prepare a map, the earth is first reduced to a globe and then projected onto a flat surface Three basic types of map projections: conic, cylindrical and azimuthal A particular projection is defined by a datum, a projection type and a set of projection parameters
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Summary Concepts (Cont.)
Standard coordinate systems use particular projections over zones of the earth’s surface Types of standard coordinate systems: UTM, State Plane, California State Mapping System, Standard Hydrologic Grid Reference Frame in ArcInfo 8,& Geomedia requires projection and map extent
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Cartesian Coordinate System
Satellite Locations Cartesian Coordinate System Three dimensional right coordinate system with an origin at the center of the earth and the X axis oriented at at the Prime Meridian and the Z at the North Pole X Axis Coordinate Distance in meters from the the prime meridian at the origin; positive from 90º E Long to 90º W Long Y Axis Coordinate Distance in meters from 90º E longitude at the origin; positive in the eastern hemisphere and negative in the western Z Axis Coordinate Distance in meters from the plane of the equator; positive in the northern Hemisphere negative in the southern Z (X,Y,Z) Like the moon, which has reliably spun around the earth for millions of years without any significant change, the GPS satellites are orbiting the earth very predictably as well. The orbits are known in advance and in fact, some GPS receivers have an “almanac” programmed in them to tell where in the sky each satellite will be at any given moment. Each satellite is known where it is in space via Cartesian Coordinates. These known coordiantes are used to triangulate the position of the receiver. GPS satellites are consistently monitored by the Department of Defense to ensure that each satellite is travelling along its mathematically modeled orbit. This is the reason that the satellites are put in a non geo-synchronous orbit. This allows each satellite to pass over the monitoring station twice a day. This gives the DoD the chance to precisely measure their altitude, position and speed. Any variations are called ephemeris errors. These are typically minor and are caused from anomolies such as gravitational pulls from the moon and sun, and from pressure of solar radiation on the satellite.Once any ephemeris errors are detected, the correction is relayed to the satellite and the corrected information or ephemeris is then incorporated onto the timing information sent from the satellite. Y 90°E X 0º Long Prime Meridian
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