1 | /////////////////////////////////////////////////////////////////////////
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2 | // Starfield Generator
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3 | //
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4 | // (c) 2000 D. Petry
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5 | //
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6 | /////////////////////////////////////////////////////////////////////////
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7 |
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8 |
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9 | #include "starfield.h"
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10 |
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11 | #define PROGRAMID "$Id: starfield.cxx,v 1.3 2000-09-21 10:31:36 harald Exp $"
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12 |
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13 | /////////////////////////////////////////////////////////////////////////
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14 |
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15 | main(int argc, char **argv)
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16 | {
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17 |
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18 | parameters pars;
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19 | star stars[iMAXSTARS];
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20 | photon *photons;
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21 |
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22 | ifstream in;
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23 | FILE *catfile;
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24 | char parfilename[160];
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25 | char catfilename[160];
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26 |
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27 |
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28 | int i, j, k, numstars, subnumstars, starnumber, totalnumphot, photinside;
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29 | int totalphotinside, idum;
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30 | int istart_ra_h, iend_ra_h;
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31 | int nph[4]; // numbers of photons in the four wavebands
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32 | float lmin_nm[4] = {ULMIN_nm, BLMIN_nm, VLMIN_nm, RLMIN_nm}; // wave band definitions
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33 | float lmax_nm[4] = {ULMAX_nm, BLMAX_nm, VLMAX_nm, RLMAX_nm};
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34 | float theta_rad, costheta, phi_rad, randtime, lambda_nm, xdum_m, ydum_m;
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35 | float angdist;
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36 |
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37 | //welcome
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38 |
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39 | cout << "This is STARFIELD. (c) 2000 D. Petry\n";
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40 | cout << PROGRAMID << "\n";
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41 |
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42 | // check command line arguments
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43 |
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44 | if(argc == 1){
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45 | sprintf(parfilename, "starfield.par");
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46 | }
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47 | else{ // a filename was given
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48 | sprintf(parfilename, "%s", argv[1]);
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49 | }
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50 |
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51 | // read parameter file
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52 |
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53 | in.open(parfilename, ios::in); // open the parameter file
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54 |
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55 | if(!in){
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56 | cout << "Failed to open " << parfilename << "\n"
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57 | << "Value of stream \"in\" was " << in << "\n";
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58 | cout << "\nThere shoud be a parameter file "<< parfilename
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59 | <<" in the working directory with the following format:\n-----\n";
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60 | pars.usage(&cout);
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61 | cout << "-----\nExiting.\n";
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62 | exit(1);
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63 | }
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64 |
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65 | cout << "Opened " << parfilename << " for reading ...\n";
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66 |
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67 | if( !(pars.readparameters(&in)) ){ // read not OK?
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68 | if(!in.eof()){ // was the error not due to EOF?
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69 | cout << "Error: rdstate = " << in.rdstate() << "\n";
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70 | }
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71 | else{
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72 | cout << "Error: premature EOF in parameter file.\n";
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73 | }
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74 | exit(1);
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75 | }
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76 |
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77 | in.close();
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78 |
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79 | // Allocate memory for photons
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80 |
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81 | photons=new photon[iMAXPHOT];
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82 |
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83 |
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84 | // prepare loop over star catalog files
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85 |
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86 | cout << "SKY2000 - Master Star Catalog - Star Catalog Database, Version 2\n";
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87 | cout << "Sande C.B., Warren W.H.Jr., Tracewell D.A., Home A.T., Miller A.C.\n";
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88 | cout << "<Goddard Space Flight Center, Flight Dynamics Division (1998)>\n";
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89 |
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90 | angdist = fmod( pars.catalog_fov_deg / cos( pars.ct_dec_rad ), 360.);
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91 |
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92 | if(angdist > 180.){ // too near to the pole, have to loop over all files
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93 |
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94 | istart_ra_h = 0;
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95 | iend_ra_h = 23;
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96 |
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97 | }
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98 | else{ // can loop over selected files only
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99 |
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100 | istart_ra_h = (int) (pars.ct_ra_h - angdist / 360. * 24.) - 1;
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101 | iend_ra_h = (int) (pars.ct_ra_h + angdist / 360. * 24. ) + 1;
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102 |
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103 | }
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104 |
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105 | //read catalog
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106 |
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107 | i = 0;
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108 | for (j = istart_ra_h; j <= iend_ra_h; j++){
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109 |
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110 | subnumstars = 0;
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111 |
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112 | if ( j < 0){
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113 | idum = j + 24;
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114 | }
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115 | else if ( j > 23 ){
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116 | idum = j - 24;
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117 | }
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118 | else {
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119 | idum = j;
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120 | }
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121 |
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122 | sprintf(catfilename, "%s/sky%02d.dat", pars.datapath, idum);
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123 |
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124 | if((catfile = fopen(catfilename, "r")) == NULL){ // open the star catalog
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125 | cout << "Failed to open " << catfilename << "\n";
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126 | exit(1);
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127 | }
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128 | cout << "Opened file " << catfilename << " for reading ...\n";
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129 |
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130 | while( stars[i].readstar(catfile, pars.verbose) ){ // read next star OK
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131 |
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132 | angdist = acos( cos( pars.ct_dec_rad ) * cos( stars[i].dec_rad ) *
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133 | cos( stars[i].ra_rad - pars.ct_ra_rad ) +
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134 | sin( pars.ct_dec_rad ) * sin( stars[i].dec_rad ) );
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135 |
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136 | if( angdist < pars.catalog_fov_deg / 180. * PI ){ // star in Field Of View?
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137 |
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138 | stars[i].calcmissingmags(pars.verbose);
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139 | if (pars.verbose) stars[i].printstar();
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140 |
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141 | if( stars[i].umag > -100. ){
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142 | i++; // accept star
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143 | subnumstars++;
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144 | }
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145 | else{
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146 | cout << "Star rejected.\n";
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147 | }
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148 |
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149 | if( i > iMAXSTARS ){
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150 | i--;
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151 | cout << "Error: Star memory full. Accepted " << i << " stars.\n";
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152 | break;
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153 | }
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154 | }
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155 | }
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156 | if( feof(catfile) ){ // was EOF reached?
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157 | cout << "EOF reached; accepted "<< subnumstars << " stars from this segment.\n";
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158 | }
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159 | if( ferror(catfile) ){ // did an error occur?
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160 | cout << "Error while reading catalog file.\n";
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161 | exit(1);
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162 | }
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163 | fclose(catfile);
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164 | if(i == iMAXSTARS){
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165 | break;
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166 | }
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167 | }
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168 |
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169 | cout << "Accepted "<< i << " stars in total.\n";
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170 | numstars = i;
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171 |
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172 | // loop over all photons from all stars, filling their fields
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173 |
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174 | totalnumphot=0;
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175 |
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176 | totalphotinside=0;
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177 |
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178 | for(i=0; i<numstars;i++){
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179 |
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180 | starnumber=stars[i].icatnum;
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181 |
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182 | // calculate director cosines (see Montenbruck & Pfleger, 1989, p. 196)
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183 |
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184 | costheta = cos( pars.ct_dec_rad ) * cos( stars[i].dec_rad ) *
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185 | cos( stars[i].ra_rad - pars.ct_ra_rad ) +
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186 | sin( pars.ct_dec_rad ) * sin( stars[i].dec_rad );
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187 |
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188 | if(costheta == 0.){
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189 | cout << "Star number " << i << " (catalog number " << stars[i].icatnum <<
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190 | ") seems to be at 90 degrees distance from optical axis.\n ... will ignore it.";
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191 | continue;
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192 | }
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193 |
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194 | stars[i].u = -1. * cos( stars[i].dec_rad ) * sin( stars[i].ra_rad - pars.ct_ra_rad ) / costheta;
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195 |
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196 | stars[i].v = -1. * ( sin( pars.ct_dec_rad ) * cos( stars[i].dec_rad ) *
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197 | cos( stars[i].ra_rad - pars.ct_ra_rad ) -
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198 | cos( pars.ct_dec_rad ) * sin( stars[i].dec_rad )
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199 | ) / costheta;
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200 |
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201 | // calculate the "zenith angle" theta and "azimuth" phi of the star assuming
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202 | // the telecope points at the zenith
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203 | // take into account the ambiguity of acos()
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204 |
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205 | theta_rad = acos(costheta);
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206 |
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207 | if( stars[i].v >= 0. ){
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208 | phi_rad = acos(stars[i].u);
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209 | }
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210 | else{
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211 | phi_rad = 2.*PI - acos(stars[i].u);
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212 | }
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213 |
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214 | // calculate number of photons
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215 |
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216 | // mag_nphot() translates the star magnitude into number of photons,
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217 | // using the expression log(flux)=-0.4*m-22.42 for each waveband
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218 | // the resulting numbers ar stored in the array nph
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219 |
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220 | stars[i].mag_nphot(nph, pars.integtime_s, pars.mirr_radius_m, pars.verbose);
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221 |
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222 | // loop over all photons
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223 |
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224 | photinside=0;
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225 |
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226 | for(k=0; k < 4; k++){ // loop over wavebands
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227 |
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228 | for(j=0; j<nph[k]; j++){ // loop over photons of this waveband
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229 |
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230 | // Check if we have overflowed the alllowed ph number
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231 |
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232 | if(totalphotinside >= iMAXPHOT){
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233 | cout << "Warning: photon memory full. Can only store " << iMAXPHOT << " photons.\n";
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234 | break;
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235 | //exit(1);
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236 | }
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237 |
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238 | // for every photon, a pair of uniform random x,y coordinates ( x*x+y*y<300 ) is generated
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239 | // and a uniform random arrival time inside a time window given by the integration time.
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240 |
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241 | xdum_m=rand_coord(pars.mirr_radius_m);
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242 | ydum_m=rand_coord(pars.mirr_radius_m);
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243 |
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244 | if((xdum_m*xdum_m+ydum_m*ydum_m)<pars.mirr_radius_m*pars.mirr_radius_m){
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245 |
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246 | randtime = rand_time(pars.integtime_s);
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247 | lambda_nm = rand_lambda(lmin_nm[k], lmax_nm[k]);
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248 |
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249 | //fill the photon fields by using the member functions defined in photon.hxx
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250 |
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251 | photons[totalphotinside].starnum = starnumber;
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252 | photons[totalphotinside].arrtime_sec = randtime;
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253 | photons[totalphotinside].x_m = xdum_m;
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254 | photons[totalphotinside].y_m = ydum_m;
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255 | photons[totalphotinside].u = stars[i].u;
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256 | photons[totalphotinside].v = stars[i].v;
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257 | photons[totalphotinside].lambda_nm = lambda_nm;
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258 |
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259 | if(pars.verbose > 2)
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260 | cout << "PH " << starnumber << " " << randtime << " " << xdum_m << " "
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261 | << ydum_m << " " << stars[i].u << " " << stars[i].v << " " << lambda_nm
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262 | << "\n";
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263 |
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264 | photinside++;
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265 |
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266 | totalphotinside++;
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267 |
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268 | totalnumphot++;
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269 |
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270 | }
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271 | else{
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272 |
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273 | totalnumphot++;
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274 | continue;
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275 |
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276 | } // end if
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277 |
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278 | } // end photon loop
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279 | } // end waveband loop
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280 |
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281 | stars[i].numphot = photinside;
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282 | //if (i>81) break;
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283 | if (pars.verbose) cout<<"Star number= "<<i<< " (catalog number " <<
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284 | starnumber << ") Number of photons accepted = "<< photinside<<endl;
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285 |
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286 | } // end star loop
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287 |
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288 | cout << "Total number of photons accepted = " << totalphotinside << "\n";
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289 |
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290 | convertcorsika(
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291 | ((int)pars.ct_ra_h*10)*1000 + (int)(abs(pars.ct_dec_deg)*10), // the file id
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292 | totalphotinside, photons, pars.integtime_s, pars.verbose, pars.output_file);
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293 |
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294 | return 0;
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295 |
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296 | } // end main
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