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