| 1 | /*!\file Xy2llx.cpp
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| 2 | */
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| 3 |
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| 4 | #include "./Xy2llx.h"
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| 5 | #include "../../include/include.h"
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| 6 | #include "../../shared/shared.h"
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| 7 | #include <math.h>
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| 8 |
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| 9 | int Xy2llx(double* lat, double* lon, double* x, double* y, int ncoord, int sgn){
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| 10 | /* This is a cpp conversion of the following:
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| 11 | %XY2LL - converts xy to lat long
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| 12 | %
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| 13 | % Converts Polar Stereographic (X,Y) coordinates for the polar regions to
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| 14 | % latitude and longitude Stereographic (X,Y) coordinates for the polar
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| 15 | % regions.
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| 16 | % Author: Michael P. Schodlok, December 2003 (map2xy.m)
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| 17 | %
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| 18 | % Usage:
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| 19 | % [lat,lon] = xy2ll(x,y,sgn);
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| 20 | % [lat,lon] = xy2ll(x,y,sgn,central_meridian,standard_parallel);
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| 21 | %
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| 22 | % - sgn = Sign of latitude +1 : north latitude (default is mer=45 lat=70)
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| 23 | % -1 : south latitude (default is mer=0 lat=71)
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| 24 | */
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| 25 |
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| 26 | double delta,slat;
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| 27 | bool flag=true;
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| 28 |
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| 29 | /* Get central_meridian and standard_parallel depending on hemisphere */
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| 30 | if (sgn == 1) {
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| 31 | delta= 45;
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| 32 | slat = 70;
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| 33 | _printf_(flag,"Warning: expecting coordinates in polar stereographic (Std Latitude: 70N Meridian: 45).\n");
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| 34 | }
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| 35 | else if (sgn == -1) {
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| 36 | delta= 0;
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| 37 | slat = 71;
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| 38 | _printf_(flag,"Warning: expecting coordinates in polar stereographic (Std Latitude: 71S Meridian: 0).\n");
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| 39 | }
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| 40 | else _error_("Sign should be either +1 or -1.\n");
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| 41 |
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| 42 | return(Xy2llx(lat,lon,x,y,ncoord,sgn,delta,slat));
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| 43 | }
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| 44 |
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| 45 | int Xy2llx(double* lat, double* lon, double* x, double* y, int ncoord, int sgn, double central_meridian, double standard_parallel){
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| 46 | /* This is a cpp conversion of the following:
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| 47 | %XY2LL - converts xy to lat long
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| 48 | %
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| 49 | % Converts Polar Stereographic (X,Y) coordinates for the polar regions to
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| 50 | % latitude and longitude Stereographic (X,Y) coordinates for the polar
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| 51 | % regions.
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| 52 | % Author: Michael P. Schodlok, December 2003 (map2xy.m)
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| 53 | %
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| 54 | % Usage:
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| 55 | % [lat,lon] = xy2ll(x,y,sgn);
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| 56 | % [lat,lon] = xy2ll(x,y,sgn,central_meridian,standard_parallel);
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| 57 | %
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| 58 | % - sgn = Sign of latitude +1 : north latitude (default is mer=45 lat=70)
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| 59 | % -1 : south latitude (default is mer=0 lat=71)
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| 60 | */
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| 61 |
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| 62 | int i,iret=0;
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| 63 | double delta,slat;
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| 64 | double cde,re,ex2,ex,pi;
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| 65 | double sl,rho,cm,T,chi;
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| 66 |
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| 67 | if((sgn!=1) && (sgn!=-1)) _error_("Sign should be either +1 or -1.\n");
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| 68 |
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| 69 | delta = central_meridian;
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| 70 | slat = standard_parallel;
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| 71 |
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| 72 | /* Conversion constant from degrees to radians */
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| 73 | cde = 57.29577951;
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| 74 | /* Radius of the earth in meters */
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| 75 | re = 6378.273*pow(10.,3.);
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| 76 | /* Eccentricity of the Hughes ellipsoid squared */
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| 77 | ex2 = 0.006693883;
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| 78 | /* Eccentricity of the Hughes ellipsoid */
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| 79 | ex = sqrt(ex2);
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| 80 |
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| 81 | /* loop over all the coordinate pairs */
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| 82 | for(i=0; i<ncoord; i++){
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| 83 | sl = slat*PI/180.;
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| 84 | cm = cos(sl)/sqrt(1.0-ex2*(pow(sin(sl),2.)));
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| 85 | rho= sqrt(pow(x[i],2.) + pow(y[i],2.));
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| 86 | T = tan((PI/4.0) - (sl/2.0))/pow(((1.0-ex*sin(sl))/(1.0+ex*sin(sl))),(ex/2.0));
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| 87 |
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| 88 | if(fabs(slat-90.) < 1.e-5)
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| 89 | T =rho*sqrt(pow((1.+ex),(1.+ex))*pow((1.-ex),(1.-ex)))/2./re;
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| 90 | else
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| 91 | T =rho*T/(re*cm);
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| 92 |
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| 93 | chi = (PI / 2.0) - 2.0 * atan(T);
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| 94 | lat[i] = chi + ((ex2 / 2.0) + (5.0 * pow(ex2,2.0) / 24.0) + (pow(ex2,3.0) / 12.0)) *
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| 95 | sin(2.0 * chi) + ((7.0 * pow(ex2,2.0) / 48.0) + (29.0 * pow(ex2,3.0) / 240.0)) *
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| 96 | sin(4.0 * chi) + (7.0 * pow(ex2,3.0) / 120.0) * sin(6.0 * chi) ;
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| 97 |
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| 98 | lat[i] = (double)sgn * lat[i];
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| 99 | lon[i] = atan2((double)sgn * x[i],-(double)sgn * y[i]);
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| 100 | lon[i] = (double)sgn * lon[i];
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| 101 |
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| 102 | if(rho <= 0.1){
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| 103 | lat[i] = 90. * (double)sgn;
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| 104 | lon[i] = 0.0;
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| 105 | iret=1;
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| 106 | }
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| 107 |
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| 108 | lon[i] = lon[i] * 180. / pi;
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| 109 | lat[i] = lat[i] * 180. / pi;
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| 110 | lon[i] = lon[i] - delta;
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| 111 | }
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| 112 |
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| 113 | return(iret);
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| 114 | }
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