1 |
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2 | // Part of BNC, a utility for retrieving decoding and
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3 | // converting GNSS data streams from NTRIP broadcasters.
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4 | //
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5 | // Copyright (C) 2007
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6 | // German Federal Agency for Cartography and Geodesy (BKG)
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7 | // http://www.bkg.bund.de
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8 | // Czech Technical University Prague, Department of Geodesy
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9 | // http://www.fsv.cvut.cz
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10 | //
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11 | // Email: euref-ip@bkg.bund.de
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12 | //
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13 | // This program is free software; you can redistribute it and/or
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14 | // modify it under the terms of the GNU General Public License
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15 | // as published by the Free Software Foundation, version 2.
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16 | //
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17 | // This program is distributed in the hope that it will be useful,
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18 | // but WITHOUT ANY WARRANTY; without even the implied warranty of
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19 | // MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
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20 | // GNU General Public License for more details.
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21 | //
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22 | // You should have received a copy of the GNU General Public License
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23 | // along with this program; if not, write to the Free Software
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24 | // Foundation, Inc., 59 Temple Place - Suite 330, Boston, MA 02111-1307, USA.
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25 |
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26 | /* -------------------------------------------------------------------------
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27 | * BKG NTRIP Client
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28 | * -------------------------------------------------------------------------
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29 | *
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30 | * Class: t_astro, t_tides, t_tropo
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31 | *
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32 | * Purpose: Observation model
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33 | *
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34 | * Author: L. Mervart
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35 | *
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36 | * Created: 29-Jul-2014
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37 | *
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38 | * Changes:
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39 | *
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40 | * -----------------------------------------------------------------------*/
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41 |
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42 |
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43 | #include <cmath>
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44 |
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45 | #include "pppModel.h"
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46 |
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47 | using namespace BNC_PPP;
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48 | using namespace std;
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49 |
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50 | const double t_astro::RHO_DEG = 180.0 / M_PI;
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51 | const double t_astro::RHO_SEC = 3600.0 * 180.0 / M_PI;
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52 | const double t_astro::MJD_J2000 = 51544.5;
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53 |
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54 | Matrix t_astro::rotX(double Angle) {
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55 | const double C = cos(Angle);
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56 | const double S = sin(Angle);
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57 | Matrix UU(3,3);
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58 | UU[0][0] = 1.0; UU[0][1] = 0.0; UU[0][2] = 0.0;
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59 | UU[1][0] = 0.0; UU[1][1] = +C; UU[1][2] = +S;
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60 | UU[2][0] = 0.0; UU[2][1] = -S; UU[2][2] = +C;
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61 | return UU;
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62 | }
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63 |
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64 | Matrix t_astro::rotY(double Angle) {
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65 | const double C = cos(Angle);
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66 | const double S = sin(Angle);
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67 | Matrix UU(3,3);
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68 | UU[0][0] = +C; UU[0][1] = 0.0; UU[0][2] = -S;
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69 | UU[1][0] = 0.0; UU[1][1] = 1.0; UU[1][2] = 0.0;
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70 | UU[2][0] = +S; UU[2][1] = 0.0; UU[2][2] = +C;
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71 | return UU;
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72 | }
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73 |
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74 | Matrix t_astro::rotZ(double Angle) {
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75 | const double C = cos(Angle);
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76 | const double S = sin(Angle);
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77 | Matrix UU(3,3);
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78 | UU[0][0] = +C; UU[0][1] = +S; UU[0][2] = 0.0;
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79 | UU[1][0] = -S; UU[1][1] = +C; UU[1][2] = 0.0;
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80 | UU[2][0] = 0.0; UU[2][1] = 0.0; UU[2][2] = 1.0;
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81 | return UU;
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82 | }
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83 |
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84 | // Greenwich Mean Sidereal Time
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85 | ///////////////////////////////////////////////////////////////////////////
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86 | double t_astro::GMST(double Mjd_UT1) {
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87 |
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88 | const double Secs = 86400.0;
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89 |
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90 | double Mjd_0 = floor(Mjd_UT1);
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91 | double UT1 = Secs*(Mjd_UT1-Mjd_0);
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92 | double T_0 = (Mjd_0 -MJD_J2000)/36525.0;
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93 | double T = (Mjd_UT1-MJD_J2000)/36525.0;
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94 |
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95 | double gmst = 24110.54841 + 8640184.812866*T_0 + 1.002737909350795*UT1
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96 | + (0.093104-6.2e-6*T)*T*T;
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97 |
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98 | return 2.0*M_PI*Frac(gmst/Secs);
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99 | }
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100 |
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101 | // Nutation Matrix
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102 | ///////////////////////////////////////////////////////////////////////////
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103 | Matrix t_astro::NutMatrix(double Mjd_TT) {
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104 |
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105 | const double T = (Mjd_TT-MJD_J2000)/36525.0;
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106 |
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107 | double ls = 2.0*M_PI*Frac(0.993133+ 99.997306*T);
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108 | double D = 2.0*M_PI*Frac(0.827362+1236.853087*T);
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109 | double F = 2.0*M_PI*Frac(0.259089+1342.227826*T);
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110 | double N = 2.0*M_PI*Frac(0.347346- 5.372447*T);
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111 |
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112 | double dpsi = ( -17.200*sin(N) - 1.319*sin(2*(F-D+N)) - 0.227*sin(2*(F+N))
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113 | + 0.206*sin(2*N) + 0.143*sin(ls) ) / RHO_SEC;
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114 | double deps = ( + 9.203*cos(N) + 0.574*cos(2*(F-D+N)) + 0.098*cos(2*(F+N))
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115 | - 0.090*cos(2*N) ) / RHO_SEC;
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116 |
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117 | double eps = 0.4090928-2.2696E-4*T;
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118 |
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119 | return rotX(-eps-deps)*rotZ(-dpsi)*rotX(+eps);
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120 | }
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121 |
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122 | // Precession Matrix
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123 | ///////////////////////////////////////////////////////////////////////////
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124 | Matrix t_astro::PrecMatrix(double Mjd_1, double Mjd_2) {
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125 |
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126 | const double T = (Mjd_1-MJD_J2000)/36525.0;
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127 | const double dT = (Mjd_2-Mjd_1)/36525.0;
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128 |
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129 | double zeta = ( (2306.2181+(1.39656-0.000139*T)*T)+
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130 | ((0.30188-0.000344*T)+0.017998*dT)*dT )*dT/RHO_SEC;
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131 | double z = zeta + ( (0.79280+0.000411*T)+0.000205*dT)*dT*dT/RHO_SEC;
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132 | double theta = ( (2004.3109-(0.85330+0.000217*T)*T)-
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133 | ((0.42665+0.000217*T)+0.041833*dT)*dT )*dT/RHO_SEC;
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134 |
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135 | return rotZ(-z) * rotY(theta) * rotZ(-zeta);
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136 | }
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137 |
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138 | // Sun's position
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139 | ///////////////////////////////////////////////////////////////////////////
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140 | ColumnVector t_astro::Sun(double Mjd_TT) {
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141 |
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142 | const double eps = 23.43929111/RHO_DEG;
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143 | const double T = (Mjd_TT-MJD_J2000)/36525.0;
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144 |
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145 | double M = 2.0*M_PI * Frac ( 0.9931267 + 99.9973583*T);
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146 | double L = 2.0*M_PI * Frac ( 0.7859444 + M/2.0/M_PI +
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147 | (6892.0*sin(M)+72.0*sin(2.0*M)) / 1296.0e3);
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148 | double r = 149.619e9 - 2.499e9*cos(M) - 0.021e9*cos(2*M);
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149 |
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150 | ColumnVector r_Sun(3);
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151 | r_Sun << r*cos(L) << r*sin(L) << 0.0; r_Sun = rotX(-eps) * r_Sun;
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152 |
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153 | return rotZ(GMST(Mjd_TT))
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154 | * NutMatrix(Mjd_TT)
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155 | * PrecMatrix(MJD_J2000, Mjd_TT)
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156 | * r_Sun;
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157 | }
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158 |
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159 | // Moon's position
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160 | ///////////////////////////////////////////////////////////////////////////
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161 | ColumnVector t_astro::Moon(double Mjd_TT) {
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162 |
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163 | const double eps = 23.43929111/RHO_DEG;
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164 | const double T = (Mjd_TT-MJD_J2000)/36525.0;
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165 |
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166 | double L_0 = Frac ( 0.606433 + 1336.851344*T );
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167 | double l = 2.0*M_PI*Frac ( 0.374897 + 1325.552410*T );
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168 | double lp = 2.0*M_PI*Frac ( 0.993133 + 99.997361*T );
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169 | double D = 2.0*M_PI*Frac ( 0.827361 + 1236.853086*T );
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170 | double F = 2.0*M_PI*Frac ( 0.259086 + 1342.227825*T );
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171 |
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172 | double dL = +22640*sin(l) - 4586*sin(l-2*D) + 2370*sin(2*D) + 769*sin(2*l)
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173 | -668*sin(lp) - 412*sin(2*F) - 212*sin(2*l-2*D)- 206*sin(l+lp-2*D)
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174 | +192*sin(l+2*D) - 165*sin(lp-2*D) - 125*sin(D) - 110*sin(l+lp)
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175 | +148*sin(l-lp) - 55*sin(2*F-2*D);
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176 |
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177 | double L = 2.0*M_PI * Frac( L_0 + dL/1296.0e3 );
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178 |
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179 | double S = F + (dL+412*sin(2*F)+541*sin(lp)) / RHO_SEC;
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180 | double h = F-2*D;
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181 | double N = -526*sin(h) + 44*sin(l+h) - 31*sin(-l+h) - 23*sin(lp+h)
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182 | +11*sin(-lp+h) - 25*sin(-2*l+F) + 21*sin(-l+F);
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183 |
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184 | double B = ( 18520.0*sin(S) + N ) / RHO_SEC;
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185 |
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186 | double cosB = cos(B);
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187 |
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188 | double R = 385000e3 - 20905e3*cos(l) - 3699e3*cos(2*D-l) - 2956e3*cos(2*D)
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189 | -570e3*cos(2*l) + 246e3*cos(2*l-2*D) - 205e3*cos(lp-2*D)
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190 | -171e3*cos(l+2*D) - 152e3*cos(l+lp-2*D);
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191 |
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192 | ColumnVector r_Moon(3);
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193 | r_Moon << R*cos(L)*cosB << R*sin(L)*cosB << R*sin(B);
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194 | r_Moon = rotX(-eps) * r_Moon;
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195 |
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196 | return rotZ(GMST(Mjd_TT))
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197 | * NutMatrix(Mjd_TT)
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198 | * PrecMatrix(MJD_J2000, Mjd_TT)
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199 | * r_Moon;
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200 | }
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201 |
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202 | // Tidal Correction
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203 | ////////////////////////////////////////////////////////////////////////////
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204 | ColumnVector t_tides::displacement(const bncTime& time, const ColumnVector& xyz) {
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205 |
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206 | if (time.undef()) {
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207 | ColumnVector dX(3); dX = 0.0;
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208 | return dX;
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209 | }
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210 |
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211 | double Mjd = time.mjd() + time.daysec() / 86400.0;
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212 |
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213 | if (Mjd != _lastMjd) {
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214 | _lastMjd = Mjd;
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215 | _xSun = t_astro::Sun(Mjd);
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216 | _rSun = sqrt(DotProduct(_xSun,_xSun));
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217 | _xSun /= _rSun;
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218 | _xMoon = t_astro::Moon(Mjd);
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219 | _rMoon = sqrt(DotProduct(_xMoon,_xMoon));
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220 | _xMoon /= _rMoon;
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221 | }
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222 |
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223 | double rRec = sqrt(DotProduct(xyz, xyz));
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224 | ColumnVector xyzUnit = xyz / rRec;
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225 |
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226 | // Love's Numbers
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227 | // --------------
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228 | const double H2 = 0.6078;
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229 | const double L2 = 0.0847;
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230 |
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231 | // Tidal Displacement
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232 | // ------------------
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233 | double scSun = DotProduct(xyzUnit, _xSun);
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234 | double scMoon = DotProduct(xyzUnit, _xMoon);
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235 |
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236 | double p2Sun = 3.0 * (H2/2.0-L2) * scSun * scSun - H2/2.0;
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237 | double p2Moon = 3.0 * (H2/2.0-L2) * scMoon * scMoon - H2/2.0;
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238 |
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239 | double x2Sun = 3.0 * L2 * scSun;
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240 | double x2Moon = 3.0 * L2 * scMoon;
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241 |
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242 | const double gmWGS = 398.6005e12;
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243 | const double gms = 1.3271250e20;
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244 | const double gmm = 4.9027890e12;
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245 |
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246 | double facSun = gms / gmWGS *
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247 | (rRec * rRec * rRec * rRec) / (_rSun * _rSun * _rSun);
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248 |
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249 | double facMoon = gmm / gmWGS *
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250 | (rRec * rRec * rRec * rRec) / (_rMoon * _rMoon * _rMoon);
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251 |
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252 | ColumnVector dX = facSun * (x2Sun * _xSun + p2Sun * xyzUnit) +
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253 | facMoon * (x2Moon * _xMoon + p2Moon * xyzUnit);
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254 |
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255 | return dX;
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256 | }
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257 |
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258 | // Constructor
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259 | ///////////////////////////////////////////////////////////////////////////
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260 | t_loading::t_loading(const QString& fileName) {
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261 |
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262 | newBlqData = 0;
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263 | readFile(fileName);
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264 | printAll();
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265 | }
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266 |
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267 | t_loading::~t_loading() {
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268 |
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269 | if (newBlqData) {
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270 | delete newBlqData;
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271 | }
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272 |
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273 | QMapIterator<QString, t_blqData*> it(blqMap);
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274 | while (it.hasNext()) {
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275 | it.next();
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276 | delete it.value();
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277 | }
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278 | }
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279 |
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280 | t_irc t_loading::readFile(const QString& fileName) {
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281 | QFile inFile(fileName);
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282 | inFile.open(QIODevice::ReadOnly | QIODevice::Text);
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283 | QTextStream in(&inFile);
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284 | int row = 0;
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285 | QString site = QString();
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286 |
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287 | while ( !in.atEnd() ) {
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288 |
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289 | QString line = in.readLine();
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290 |
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291 | // skip empty lines and comments
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292 | if (line.indexOf("$$") != -1 || line.size() == 0) {
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293 | continue;
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294 | }
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295 |
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296 | line = line.trimmed();
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297 | QTextStream inLine(line.toAscii(), QIODevice::ReadOnly);
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298 |
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299 | switch (row) {
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300 | case 0:
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301 | site = line;
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302 | site = site.toUpper();
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303 | if (!newBlqData) {
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304 | newBlqData = new t_blqData;
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305 | newBlqData->amplitudes.ReSize(3,11);
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306 | newBlqData->phases.ReSize(3,11);
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307 | }
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308 | break;
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309 | case 1: case 2: case 3:
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310 | for (int ii = 0; ii < 11; ii++) {
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311 | inLine >> newBlqData->amplitudes[row-1][ii];
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312 | }
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313 | break;
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314 | case 4: case 5: case 6:
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315 | for (int ii = 0; ii < 11; ii++) {
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316 | inLine >> newBlqData->phases[row-4][ii];
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317 | }
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318 | break;
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319 | case 7:
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320 | if (newBlqData && !site.isEmpty()) {
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321 | blqMap[site] = newBlqData;
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322 | site = QString();
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323 | row = -1;
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324 | newBlqData = 0;
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325 | }
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326 | break;
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327 | }
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328 | row++;
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329 | }
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330 | inFile.close();
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331 | return success;
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332 | }
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333 |
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334 | // Print
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335 | ////////////////////////////////////////////////////////////////////////////
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336 | void t_loading::printAll() const {
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337 |
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338 | QMapIterator<QString, t_blqData*> it(blqMap);
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339 | while (it.hasNext()) {
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340 | it.next();
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341 | t_blqData* blq = it.value();
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342 | QString site = it.key();
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343 | cout << site.toStdString().c_str() << "\n";
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344 | for (int rr = 0; rr < 3; rr++) {
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345 | for (int cc = 0; cc < 11; cc++) {
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346 | cout << blq->amplitudes[rr][cc] << " ";
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347 | }
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348 | cout << endl;
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349 | }
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350 | for (int rr = 0; rr < 3; rr++) {
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351 | for (int cc = 0; cc < 11; cc++) {
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352 | cout << blq->phases[rr][cc] << " ";
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353 | }
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354 | cout << endl;
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355 | }
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356 | }
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357 | }
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358 |
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359 | // Constructor
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360 | ///////////////////////////////////////////////////////////////////////////
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361 | t_windUp::t_windUp() {
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362 | for (unsigned ii = 0; ii <= t_prn::MAXPRN; ii++) {
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363 | sumWind[ii] = 0.0;
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364 | lastEtime[ii] = 0.0;
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365 | }
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366 | }
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367 |
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368 | // Phase Wind-Up Correction
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369 | ///////////////////////////////////////////////////////////////////////////
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370 | double t_windUp::value(const bncTime& etime, const ColumnVector& rRec,
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371 | t_prn prn, const ColumnVector& rSat) {
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372 |
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373 | if (etime.mjddec() != lastEtime[prn.toInt()]) {
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374 |
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375 | // Unit Vector GPS Satellite --> Receiver
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376 | // --------------------------------------
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377 | ColumnVector rho = rRec - rSat;
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378 | rho /= rho.norm_Frobenius();
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379 |
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380 | // GPS Satellite unit Vectors sz, sy, sx
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381 | // -------------------------------------
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382 | ColumnVector sz = -rSat / rSat.norm_Frobenius();
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383 |
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384 | ColumnVector xSun = t_astro::Sun(etime.mjddec());
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385 | xSun /= xSun.norm_Frobenius();
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386 |
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387 | ColumnVector sy = crossproduct(sz, xSun);
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388 | ColumnVector sx = crossproduct(sy, sz);
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389 |
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390 | // Effective Dipole of the GPS Satellite Antenna
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391 | // ---------------------------------------------
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392 | ColumnVector dipSat = sx - rho * DotProduct(rho,sx)
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393 | - crossproduct(rho, sy);
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394 |
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395 | // Receiver unit Vectors rx, ry
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396 | // ----------------------------
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397 | ColumnVector rx(3);
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398 | ColumnVector ry(3);
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399 |
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400 | double recEll[3]; xyz2ell(rRec.data(), recEll) ;
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401 | double neu[3];
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402 |
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403 | neu[0] = 1.0;
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404 | neu[1] = 0.0;
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405 | neu[2] = 0.0;
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406 | neu2xyz(recEll, neu, rx.data());
|
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407 |
|
---|
408 | neu[0] = 0.0;
|
---|
409 | neu[1] = -1.0;
|
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410 | neu[2] = 0.0;
|
---|
411 | neu2xyz(recEll, neu, ry.data());
|
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412 |
|
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413 | // Effective Dipole of the Receiver Antenna
|
---|
414 | // ----------------------------------------
|
---|
415 | ColumnVector dipRec = rx - rho * DotProduct(rho,rx)
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416 | + crossproduct(rho, ry);
|
---|
417 |
|
---|
418 | // Resulting Effect
|
---|
419 | // ----------------
|
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420 | double alpha = DotProduct(dipSat,dipRec) /
|
---|
421 | (dipSat.norm_Frobenius() * dipRec.norm_Frobenius());
|
---|
422 |
|
---|
423 | if (alpha > 1.0) alpha = 1.0;
|
---|
424 | if (alpha < -1.0) alpha = -1.0;
|
---|
425 |
|
---|
426 | double dphi = acos(alpha) / 2.0 / M_PI; // in cycles
|
---|
427 |
|
---|
428 | if ( DotProduct(rho, crossproduct(dipSat, dipRec)) < 0.0 ) {
|
---|
429 | dphi = -dphi;
|
---|
430 | }
|
---|
431 |
|
---|
432 | if (lastEtime[prn.toInt()] == 0.0) {
|
---|
433 | sumWind[prn.toInt()] = dphi;
|
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434 | }
|
---|
435 | else {
|
---|
436 | sumWind[prn.toInt()] = nint(sumWind[prn.toInt()] - dphi) + dphi;
|
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437 | }
|
---|
438 |
|
---|
439 | lastEtime[prn.toInt()] = etime.mjddec();
|
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440 | }
|
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441 |
|
---|
442 | return sumWind[prn.toInt()];
|
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443 | }
|
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444 |
|
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445 | // Tropospheric Model (Saastamoinen)
|
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446 | ////////////////////////////////////////////////////////////////////////////
|
---|
447 | double t_tropo::delay_saast(const ColumnVector& xyz, double Ele) {
|
---|
448 |
|
---|
449 | Tracer tracer("bncModel::delay_saast");
|
---|
450 |
|
---|
451 | if (xyz[0] == 0.0 && xyz[1] == 0.0 && xyz[2] == 0.0) {
|
---|
452 | return 0.0;
|
---|
453 | }
|
---|
454 |
|
---|
455 | double ell[3];
|
---|
456 | xyz2ell(xyz.data(), ell);
|
---|
457 | double height = ell[2];
|
---|
458 |
|
---|
459 | double pp = 1013.25 * pow(1.0 - 2.26e-5 * height, 5.225);
|
---|
460 | double TT = 18.0 - height * 0.0065 + 273.15;
|
---|
461 | double hh = 50.0 * exp(-6.396e-4 * height);
|
---|
462 | double ee = hh / 100.0 * exp(-37.2465 + 0.213166*TT - 0.000256908*TT*TT);
|
---|
463 |
|
---|
464 | double h_km = height / 1000.0;
|
---|
465 |
|
---|
466 | if (h_km < 0.0) h_km = 0.0;
|
---|
467 | if (h_km > 5.0) h_km = 5.0;
|
---|
468 | int ii = int(h_km + 1); if (ii > 5) ii = 5;
|
---|
469 | double href = ii - 1;
|
---|
470 |
|
---|
471 | double bCor[6];
|
---|
472 | bCor[0] = 1.156;
|
---|
473 | bCor[1] = 1.006;
|
---|
474 | bCor[2] = 0.874;
|
---|
475 | bCor[3] = 0.757;
|
---|
476 | bCor[4] = 0.654;
|
---|
477 | bCor[5] = 0.563;
|
---|
478 |
|
---|
479 | double BB = bCor[ii-1] + (bCor[ii]-bCor[ii-1]) * (h_km - href);
|
---|
480 |
|
---|
481 | double zen = M_PI/2.0 - Ele;
|
---|
482 |
|
---|
483 | return (0.002277/cos(zen)) * (pp + ((1255.0/TT)+0.05)*ee - BB*(tan(zen)*tan(zen)));
|
---|
484 | }
|
---|
485 |
|
---|
486 | // Constructor
|
---|
487 | ///////////////////////////////////////////////////////////////////////////
|
---|
488 | t_iono::t_iono() {
|
---|
489 | _psiPP = _phiPP = _lambdaPP = _lonS = 0.0;
|
---|
490 | }
|
---|
491 |
|
---|
492 | t_iono::~t_iono() {}
|
---|
493 |
|
---|
494 | double t_iono::stec(const t_vTec* vTec, double signalPropagationTime,
|
---|
495 | const ColumnVector& rSat, const bncTime& epochTime,
|
---|
496 | const ColumnVector& xyzSta) {
|
---|
497 |
|
---|
498 | // Latitude, longitude, height are defined with respect to a spherical earth model
|
---|
499 | // -------------------------------------------------------------------------------
|
---|
500 | ColumnVector geocSta(3);
|
---|
501 | if (xyz2geoc(xyzSta.data(), geocSta.data()) != success) {
|
---|
502 | return 0.0;
|
---|
503 | }
|
---|
504 |
|
---|
505 | // satellite position rotated to the epoch of signal reception
|
---|
506 | // -----------------------------------------------------------
|
---|
507 | ColumnVector xyzSat(3);
|
---|
508 | double omegaZ = t_CST::omega * signalPropagationTime;
|
---|
509 | xyzSat[0] = rSat[0] * cos(omegaZ) + rSat[1] * sin(omegaZ);
|
---|
510 | xyzSat[1] = rSat[1] * cos(omegaZ) - rSat[0] * sin(omegaZ);
|
---|
511 | xyzSat[2] = rSat[2];
|
---|
512 |
|
---|
513 | // elevation and azimuth with respect to a spherical earth model
|
---|
514 | // -------------------------------------------------------------
|
---|
515 | ColumnVector rhoV = xyzSat - xyzSta;
|
---|
516 | double rho = rhoV.norm_Frobenius();
|
---|
517 | ColumnVector neu(3);
|
---|
518 | xyz2neu(geocSta.data(), rhoV.data(), neu.data());
|
---|
519 | double sphEle = acos( sqrt(neu[0]*neu[0] + neu[1]*neu[1]) / rho );
|
---|
520 | if (neu[2] < 0) {
|
---|
521 | sphEle *= -1.0;
|
---|
522 | }
|
---|
523 | double sphAzi = atan2(neu[1], neu[0]);
|
---|
524 |
|
---|
525 | double epoch = fmod(epochTime.gpssec(), 86400.0);
|
---|
526 |
|
---|
527 | double stec = 0.0;
|
---|
528 | for (unsigned ii = 0; ii < vTec->_layers.size(); ii++) {
|
---|
529 | piercePoint(vTec->_layers[ii]._height, epoch, geocSta.data(), sphEle, sphAzi);
|
---|
530 | double vtec = vtecSingleLayerContribution(vTec->_layers[ii]);
|
---|
531 | stec += vtec * sin(sphEle + _psiPP);
|
---|
532 | }
|
---|
533 | return stec;
|
---|
534 | }
|
---|
535 |
|
---|
536 | double t_iono::vtecSingleLayerContribution(const t_vTecLayer& vTecLayer) {
|
---|
537 |
|
---|
538 | double vtec = 0.0;
|
---|
539 | int N = vTecLayer._C.Nrows()-1;
|
---|
540 | int M = vTecLayer._C.Ncols()-1;
|
---|
541 | double fac;
|
---|
542 |
|
---|
543 | for (int n = 0; n <= N; n++) {
|
---|
544 | for (int m = 0; m <= min(n, M); m++) {
|
---|
545 | double pnm = associatedLegendreFunction(n, m, sin(_phiPP));
|
---|
546 | double a = double(factorial(n - m));
|
---|
547 | double b = double(factorial(n + m));
|
---|
548 | if (m == 0) {
|
---|
549 | fac = sqrt(2.0 * n + 1);
|
---|
550 | }
|
---|
551 | else {
|
---|
552 | fac = sqrt(2.0 * (2.0 * n + 1) * a / b);
|
---|
553 | }
|
---|
554 | pnm *= fac;
|
---|
555 | double Cnm_mlambda = vTecLayer._C[n][m] * cos(m * _lonS);
|
---|
556 | double Snm_mlambda = vTecLayer._S[n][m] * sin(m * _lonS);
|
---|
557 | vtec += (Snm_mlambda + Cnm_mlambda) * pnm;
|
---|
558 | }
|
---|
559 | }
|
---|
560 |
|
---|
561 | if (vtec < 0.0) {
|
---|
562 | return 0.0;
|
---|
563 | }
|
---|
564 |
|
---|
565 | return vtec;
|
---|
566 | }
|
---|
567 |
|
---|
568 | void t_iono::piercePoint(double layerHeight, double epoch, const double* geocSta,
|
---|
569 | double sphEle, double sphAzi) {
|
---|
570 |
|
---|
571 | double q = (t_CST::rgeoc + geocSta[2]) / (t_CST::rgeoc + layerHeight);
|
---|
572 |
|
---|
573 | _psiPP = M_PI/2 - sphEle - asin(q * cos(sphEle));
|
---|
574 |
|
---|
575 | _phiPP = asin(sin(geocSta[0]) * cos(_psiPP) + cos(geocSta[0]) * sin(_psiPP) * cos(sphAzi));
|
---|
576 |
|
---|
577 | if (( (geocSta[0]*180.0/M_PI > 0) && ( tan(_psiPP) * cos(sphAzi) > tan(M_PI/2 - geocSta[0])) ) ||
|
---|
578 | ( (geocSta[0]*180.0/M_PI < 0) && (-(tan(_psiPP) * cos(sphAzi)) > tan(M_PI/2 + geocSta[0])) )) {
|
---|
579 | _lambdaPP = geocSta[1] + M_PI - asin((sin(_psiPP) * sin(sphAzi) / cos(_phiPP)));
|
---|
580 | } else {
|
---|
581 | _lambdaPP = geocSta[1] + asin((sin(_psiPP) * sin(sphAzi) / cos(_phiPP)));
|
---|
582 | }
|
---|
583 |
|
---|
584 | _lonS = fmod((_lambdaPP + (epoch - 50400) * M_PI / 43200), 2*M_PI);
|
---|
585 |
|
---|
586 | return;
|
---|
587 | }
|
---|
588 |
|
---|