1 | #!/usr/bin/env python |
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2 | |
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3 | # Lat Long - UTM, UTM - Lat Long conversions |
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4 | # |
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5 | # see http://www.pygps.org |
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6 | # |
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7 | |
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8 | from math import pi, sin, cos, tan, sqrt |
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9 | |
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10 | #LatLong- UTM conversion..h |
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11 | #definitions for lat/long to UTM and UTM to lat/lng conversions |
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12 | #include <string.h> |
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13 | |
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14 | _deg2rad = pi / 180.0 |
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15 | _rad2deg = 180.0 / pi |
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16 | |
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17 | _EquatorialRadius = 2 |
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18 | _eccentricitySquared = 3 |
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19 | |
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20 | _ellipsoid = [ |
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21 | # id, Ellipsoid name, Equatorial Radius, square of eccentricity |
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22 | # first once is a placeholder only, To allow array indices to match id numbers |
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23 | [ -1, "Placeholder", 0, 0], |
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24 | [ 1, "Airy", 6377563, 0.00667054], |
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25 | [ 2, "Australian National", 6378160, 0.006694542], |
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26 | [ 3, "Bessel 1841", 6377397, 0.006674372], |
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27 | [ 4, "Bessel 1841 (Nambia] ", 6377484, 0.006674372], |
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28 | [ 5, "Clarke 1866", 6378206, 0.006768658], |
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29 | [ 6, "Clarke 1880", 6378249, 0.006803511], |
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30 | [ 7, "Everest", 6377276, 0.006637847], |
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31 | [ 8, "Fischer 1960 (Mercury] ", 6378166, 0.006693422], |
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32 | [ 9, "Fischer 1968", 6378150, 0.006693422], |
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33 | [ 10, "GRS 1967", 6378160, 0.006694605], |
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34 | [ 11, "GRS 1980", 6378137, 0.00669438], |
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35 | [ 12, "Helmert 1906", 6378200, 0.006693422], |
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36 | [ 13, "Hough", 6378270, 0.00672267], |
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37 | [ 14, "International", 6378388, 0.00672267], |
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38 | [ 15, "Krassovsky", 6378245, 0.006693422], |
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39 | [ 16, "Modified Airy", 6377340, 0.00667054], |
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40 | [ 17, "Modified Everest", 6377304, 0.006637847], |
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41 | [ 18, "Modified Fischer 1960", 6378155, 0.006693422], |
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42 | [ 19, "South American 1969", 6378160, 0.006694542], |
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43 | [ 20, "WGS 60", 6378165, 0.006693422], |
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44 | [ 21, "WGS 66", 6378145, 0.006694542], |
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45 | [ 22, "WGS-72", 6378135, 0.006694318], |
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46 | [ 23, "WGS-84", 6378137, 0.00669438] |
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47 | ] |
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48 | |
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49 | #Reference ellipsoids derived from Peter H. Dana's website- |
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50 | #http://www.utexas.edu/depts/grg/gcraft/notes/datum/elist.html |
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51 | #Department of Geography, University of Texas at Austin |
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52 | #Internet: pdana@mail.utexas.edu |
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53 | #3/22/95 |
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54 | |
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55 | #Source |
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56 | #Defense Mapping Agency. 1987b. DMA Technical Report: Supplement to Department of Defense World Geodetic System |
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57 | #1984 Technical Report. Part I and II. Washington, DC: Defense Mapping Agency |
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58 | |
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59 | #def LLtoUTM(int ReferenceEllipsoid, const double Lat, const double Long, |
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60 | # double &UTMNorthing, double &UTMEasting, char* UTMZone) |
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61 | |
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62 | def LLtoUTM( Lat, Long, ReferenceEllipsoid=23): |
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63 | """ |
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64 | converts lat/long to UTM coords. Equations from USGS Bulletin 1532 |
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65 | East Longitudes are positive, West longitudes are negative. |
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66 | North latitudes are positive, South latitudes are negative |
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67 | Lat and Long are in decimal degrees |
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68 | Written by Chuck Gantz- chuck.gantz@globalstar.com |
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69 | """ |
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70 | a = _ellipsoid[ReferenceEllipsoid][_EquatorialRadius] |
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71 | eccSquared = _ellipsoid[ReferenceEllipsoid][_eccentricitySquared] |
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72 | k0 = 0.9996 |
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73 | |
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74 | #Make sure the longitude is between -180.00 .. 179.9 |
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75 | LongTemp = (Long+180)-int((Long+180)/360)*360-180 # -180.00 .. 179.9 |
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76 | |
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77 | LatRad = Lat*_deg2rad |
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78 | LongRad = LongTemp*_deg2rad |
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79 | |
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80 | ZoneNumber = int((LongTemp + 180)/6) + 1 |
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81 | |
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82 | if Lat >= 56.0 and Lat < 64.0 and LongTemp >= 3.0 and LongTemp < 12.0: |
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83 | ZoneNumber = 32 |
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84 | |
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85 | # Special zones for Svalbard |
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86 | if Lat >= 72.0 and Lat < 84.0: |
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87 | if LongTemp >= 0.0 and LongTemp < 9.0:ZoneNumber = 31 |
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88 | elif LongTemp >= 9.0 and LongTemp < 21.0: ZoneNumber = 33 |
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89 | elif LongTemp >= 21.0 and LongTemp < 33.0: ZoneNumber = 35 |
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90 | elif LongTemp >= 33.0 and LongTemp < 42.0: ZoneNumber = 37 |
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91 | |
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92 | LongOrigin = (ZoneNumber - 1)*6 - 180 + 3 #+3 puts origin in middle of zone |
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93 | LongOriginRad = LongOrigin * _deg2rad |
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94 | |
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95 | #compute the UTM Zone from the latitude and longitude |
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96 | UTMZone = "%d%c" % (ZoneNumber, _UTMLetterDesignator(Lat)) |
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97 | |
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98 | eccPrimeSquared = (eccSquared)/(1-eccSquared) |
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99 | N = a/sqrt(1-eccSquared*sin(LatRad)*sin(LatRad)) |
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100 | T = tan(LatRad)*tan(LatRad) |
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101 | C = eccPrimeSquared*cos(LatRad)*cos(LatRad) |
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102 | A = cos(LatRad)*(LongRad-LongOriginRad) |
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103 | |
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104 | M = a*((1 |
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105 | - eccSquared/4 |
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106 | - 3*eccSquared*eccSquared/64 |
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107 | - 5*eccSquared*eccSquared*eccSquared/256)*LatRad |
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108 | - (3*eccSquared/8 |
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109 | + 3*eccSquared*eccSquared/32 |
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110 | + 45*eccSquared*eccSquared*eccSquared/1024)*sin(2*LatRad) |
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111 | + (15*eccSquared*eccSquared/256 + 45*eccSquared*eccSquared*eccSquared/1024)*sin(4*LatRad) |
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112 | - (35*eccSquared*eccSquared*eccSquared/3072)*sin(6*LatRad)) |
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113 | |
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114 | UTMEasting = (k0*N*(A+(1-T+C)*A*A*A/6 |
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115 | + (5-18*T+T*T+72*C-58*eccPrimeSquared)*A*A*A*A*A/120) |
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116 | + 500000.0) |
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117 | |
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118 | UTMNorthing = (k0*(M+N*tan(LatRad)*(A*A/2+(5-T+9*C+4*C*C)*A*A*A*A/24 |
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119 | + (61 |
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120 | -58*T |
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121 | +T*T |
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122 | +600*C |
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123 | -330*eccPrimeSquared)*A*A*A*A*A*A/720))) |
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124 | |
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125 | if Lat < 0: |
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126 | UTMNorthing = UTMNorthing + 10000000.0; #10000000 meter offset for southern hemisphere |
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127 | #UTMZone was originally returned here. I don't know what the |
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128 | #letter at the end was for. |
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129 | #print "UTMZone", UTMZone |
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130 | return (ZoneNumber, UTMEasting, UTMNorthing) |
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131 | |
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132 | |
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133 | def _UTMLetterDesignator(Lat): |
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134 | #This routine determines the correct UTM letter designator for the given latitude |
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135 | #returns 'Z' if latitude is outside the UTM limits of 84N to 80S |
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136 | #Written by Chuck Gantz- chuck.gantz@globalstar.com |
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137 | |
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138 | if 84 >= Lat >= 72: return 'X' |
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139 | elif 72 > Lat >= 64: return 'W' |
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140 | elif 64 > Lat >= 56: return 'V' |
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141 | elif 56 > Lat >= 48: return 'U' |
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142 | elif 48 > Lat >= 40: return 'T' |
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143 | elif 40 > Lat >= 32: return 'S' |
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144 | elif 32 > Lat >= 24: return 'R' |
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145 | elif 24 > Lat >= 16: return 'Q' |
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146 | elif 16 > Lat >= 8: return 'P' |
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147 | elif 8 > Lat >= 0: return 'N' |
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148 | elif 0 > Lat >= -8: return 'M' |
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149 | elif -8> Lat >= -16: return 'L' |
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150 | elif -16 > Lat >= -24: return 'K' |
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151 | elif -24 > Lat >= -32: return 'J' |
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152 | elif -32 > Lat >= -40: return 'H' |
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153 | elif -40 > Lat >= -48: return 'G' |
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154 | elif -48 > Lat >= -56: return 'F' |
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155 | elif -56 > Lat >= -64: return 'E' |
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156 | elif -64 > Lat >= -72: return 'D' |
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157 | elif -72 > Lat >= -80: return 'C' |
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158 | else: return 'Z' # if the Latitude is outside the UTM limits |
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159 | |
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160 | #void UTMtoLL(int ReferenceEllipsoid, const double UTMNorthing, const double UTMEasting, const char* UTMZone, |
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161 | # double& Lat, double& Long ) |
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162 | |
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163 | def UTMtoLL(northing, easting, zone, isSouthernHemisphere=True, |
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164 | ReferenceEllipsoid=23): |
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165 | """ |
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166 | converts UTM coords to lat/long. Equations from USGS Bulletin 1532 |
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167 | East Longitudes are positive, West longitudes are negative. |
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168 | North latitudes are positive, South latitudes are negative |
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169 | Lat and Long are in decimal degrees. |
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170 | Written by Chuck Gantz- chuck.gantz@globalstar.com |
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171 | Converted to Python by Russ Nelson <nelson@crynwr.com> |
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172 | |
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173 | FIXME: This is set up to work for the Southern Hemisphere. |
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174 | |
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175 | Using |
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176 | http://www.ga.gov.au/geodesy/datums/redfearn_geo_to_grid.jsp |
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177 | |
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178 | Site Name: GDA-MGA: (UTM with GRS80 ellipsoid) |
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179 | Zone: 36 |
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180 | Easting: 511669.521 Northing: 19328195.112 |
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181 | Latitude: 84 0 ' 0.00000 '' Longitude: 34 0 ' 0.00000 '' |
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182 | Grid Convergence: 0 -59 ' 40.28 '' Point Scale: 0.99960166 |
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183 | |
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184 | ____________ |
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185 | Site Name: GDA-MGA: (UTM with GRS80 ellipsoid) |
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186 | Zone: 36 |
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187 | Easting: 519384.803 Northing: 1118247.585 |
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188 | Latitude: -80 0 ' 0.00000 '' Longitude: 34 0 ' 0.00000 '' |
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189 | Grid Convergence: 0 59 ' 5.32 '' Point Scale: 0.99960459 |
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190 | ___________ |
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191 | Site Name: GDA-MGA: (UTM with GRS80 ellipsoid) |
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192 | Zone: 36 |
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193 | Easting: 611263.812 Northing: 10110547.106 |
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194 | Latitude: 1 0 ' 0.00000 '' Longitude: 34 0 ' 0.00000 '' |
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195 | Grid Convergence: 0 -1 ' 2.84 '' Point Scale: 0.99975325 |
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196 | ______________ |
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197 | Site Name: GDA-MGA: (UTM with GRS80 ellipsoid) |
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198 | Zone: 36 |
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199 | Easting: 611263.812 Northing: 9889452.894 |
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200 | Latitude: -1 0 ' 0.00000 '' Longitude: 34 0 ' 0.00000 '' |
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201 | Grid Convergence: 0 1 ' 2.84 '' Point Scale: 0.99975325 |
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202 | |
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203 | So this uses a false northing of 10000000 in the both hemispheres. |
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204 | ArcGIS used a false northing of 0 in the northern hem though. |
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205 | Therefore it is difficult to actually know what hemisphere you are in. |
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206 | """ |
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207 | k0 = 0.9996 |
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208 | a = _ellipsoid[ReferenceEllipsoid][_EquatorialRadius] |
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209 | eccSquared = _ellipsoid[ReferenceEllipsoid][_eccentricitySquared] |
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210 | e1 = (1-sqrt(1-eccSquared))/(1+sqrt(1-eccSquared)) |
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211 | |
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212 | x = easting - 500000.0 #remove 500,000 meter offset for longitude |
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213 | y = northing |
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214 | |
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215 | ZoneNumber = int(zone) |
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216 | if isSouthernHemisphere: |
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217 | y -= 10000000.0 # remove 10,000,000 meter offset used |
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218 | # for southern hemisphere |
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219 | |
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220 | LongOrigin = (ZoneNumber - 1)*6 - 180 + 3 # +3 puts origin in middle of zone |
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221 | |
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222 | eccPrimeSquared = (eccSquared)/(1-eccSquared) |
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223 | |
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224 | M = y / k0 |
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225 | mu = M/(a*(1-eccSquared/4-3*eccSquared*eccSquared/64-5*eccSquared*eccSquared*eccSquared/256)) |
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226 | |
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227 | phi1Rad = (mu + (3*e1/2-27*e1*e1*e1/32)*sin(2*mu) |
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228 | + (21*e1*e1/16-55*e1*e1*e1*e1/32)*sin(4*mu) |
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229 | +(151*e1*e1*e1/96)*sin(6*mu)) |
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230 | phi1 = phi1Rad*_rad2deg; |
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231 | |
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232 | N1 = a/sqrt(1-eccSquared*sin(phi1Rad)*sin(phi1Rad)) |
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233 | T1 = tan(phi1Rad)*tan(phi1Rad) |
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234 | C1 = eccPrimeSquared*cos(phi1Rad)*cos(phi1Rad) |
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235 | R1 = a*(1-eccSquared)/pow(1-eccSquared*sin(phi1Rad)*sin(phi1Rad), 1.5) |
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236 | D = x/(N1*k0) |
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237 | |
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238 | Lat = phi1Rad - (N1*tan(phi1Rad)/R1)*(D*D/2-(5+3*T1+10*C1-4*C1*C1-9*eccPrimeSquared)*D*D*D*D/24 |
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239 | +(61+90*T1+298*C1+45*T1*T1-252*eccPrimeSquared-3*C1*C1)*D*D*D*D*D*D/720) |
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240 | Lat = Lat * _rad2deg |
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241 | |
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242 | Long = (D-(1+2*T1+C1)*D*D*D/6+(5-2*C1+28*T1-3*C1*C1+8*eccPrimeSquared+24*T1*T1) |
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243 | *D*D*D*D*D/120)/cos(phi1Rad) |
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244 | Long = LongOrigin + Long * _rad2deg |
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245 | return (Lat, Long) |
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246 | |
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247 | if __name__ == '__main__': |
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248 | (z, e, n) = LLtoUTM(45.00, -75.00, 23) |
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249 | print z, e, n |
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250 | (lat, lon) = UTMtoLL(n, e, z, 23) |
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251 | print lat, lon |
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