コード例 #1
0
ファイル: bc-star-conjuncts.c プロジェクト: mkstarr/bcapps
void findmins (SpiceDouble beg, SpiceDouble end) {

  SpiceInt i, count;

  // SPICEDOUBLE_CELLs are static, so must reinit them each time, sigh
  SPICEDOUBLE_CELL(result, 200);
  SPICEDOUBLE_CELL(cnfine,2);
  scard_c(0,&result);
  scard_c(0,&cnfine);

  // create interval
  wninsd_c(beg,end,&cnfine);

  // get results
  gfuds_c(gfq,gfdecrx,"LOCMIN",0.,0.,86400.,MAXWIN,&cnfine,&result);

  count = wncard_c(&result); 

  for (i=0; i<count; i++) {
    wnfetd_c(&result,i,&beg,&end);
    // becuase beg and end are equal, overwriting end with actual value
    gfq(beg,&end);
    printf("M %f %f %f\n",et2jd(beg),r2d(end),r2d(sunminangle(beg,planetcount,planets)));
  }
}
コード例 #2
0
int main (int argc, char **argv) {

  SPICEDOUBLE_CELL (result, 2*MAXWIN);
  SPICEDOUBLE_CELL (cnfine, 2);
  // various formats
  SpiceChar begstr[TIMLEN], classic[100], terse[100];
  SpiceDouble beg,end,*array;
  SpiceInt count,i,j,house;

  furnsh_c("/home/barrycarter/BCGIT/ASTRO/standard.tm");

  // 1 second tolerance (serious overkill, but 1e-6 is default, worse!)
  gfstol_c(1.);
  
  // 1 year window
  wninsd_c(year2et(atof(argv[1])), year2et(atof(argv[2])), &cnfine);

  // TODO: figure out how to compute sizeof(iplanets) properly, this is hack
  for (j=0; j<sizeof(iplanets)/4; j++) {

    gplanet = iplanets[j];

    gfuds_c (gfq, gfdecrx, "=", 0., 0., 86400., MAXWIN, &cnfine, &result);
    count = wncard_c(&result);
    
    for (i=0; i<count; i++) {

      // find the time of event (beg == end in this case)
      wnfetd_c (&result, i, &beg, &end);

      // find ecliptic longitude (and if its increasing/decreasing)
      array = geom_info(gplanet, beg, FRAME, 399);

      // pretty print the time
      timout_c (beg, TIMFMT, TIMLEN, begstr);

      house = rint(array[11]*dpr_c()/30);
      if (array[17] < 0) {house--;}
      house = (house+12)%12;

      // the classic form
      sprintf(classic, "%s %s ENTERS %s %s",  begstr,  
	      planet2str(gplanet, ""), houses[house], 
	      array[17]<0?"RETROGRADE":"PROGRADE");

      sprintf(terse, "%lld %s%s%s", (long long) floor(beg+0.5), 
	      planet2str(gplanet, "TERSE"), house2str(house, "TERSE"),
	      array[17]<0?"-":"+");

      printf("%s %s\n", classic, terse);
    }
  }
  return(0);
}
コード例 #3
0
int main( int argc, char **argv ) {

  SpiceInt i,count,j;
  SPICEDOUBLE_CELL(result, 2*MAXWIN);
  SPICEDOUBLE_CELL(cnfine,2);
  char stime[255];
  SpiceDouble beg, end, ang;

  // fill the static planets array
  for (i=1; i<argc; i++) {planets[i] = atoi(argv[i]);}
  planetcount = argc-1;

  // 1 second tolerance (serious overkill, but 1e-6 is default, worse!)
  gfstol_c(1.);

  furnsh_c("/home/barrycarter/BCGIT/ASTRO/standard.tm");

  // DE431 limits
  wninsd_c (-479695089600.+86400*468, 479386728000., &cnfine);

  // 1970 to 2038 (all "Unix time") for testing
  //  wninsd_c(unix2et(0),unix2et(2147483647),&cnfine);

  gfuds_c(gfq,gfdecrx,"LOCMIN",0.,0.,86400.,MAXWIN,&cnfine,&result);
  count = wncard_c(&result); 

  for (i=0; i<count; i++) {
    // we don't use 'end' but need to pass it
    wnfetd_c(&result,i,&beg,&end);
    // find the angle at this time
    gfq(beg,&ang);
    // format time nicely
    timout_c(beg, "ERA YYYY##-MM-DD HR:MN:SC ::MCAL",255,stime);

    // print et and separation as degree
    printf("%f %f",beg,ang*dpr_c());
    // print out the planets involved (redundant, but useful)
    for (j=1; j<argc; j++) {printf(" %s",argv[j]);}
    printf(" %s\n",stime);



  }
  return 0;
}
コード例 #4
0
ファイル: bc-star-conjuncts.c プロジェクト: mkstarr/bcapps
int main (int argc, char **argv) {

  SpiceInt i, nres;
  SPICEDOUBLE_CELL(cnfine,2);
  SPICEDOUBLE_CELL(result,2*MAXWIN);
  SpiceDouble beg,end;

  furnsh_c("/home/barrycarter/BCGIT/ASTRO/standard.tm");

  // this will represent the stars position
  planets[0] = -1;

  // convert ra and dec to starpos
  radrec_c(1,atof(argv[1]),atof(argv[2]),starpos);

  // planets array and count
  for (i=1; i<argc-2; i++) {planets[i] = atoi(argv[i+2]);}
  planetcount = argc-2;

  printf("CONJUNCTIONS FOR %f degrees, planets: %s %s %d %d %d %d %d %d\n",r2d(MAXSEP),argv[1],argv[2],(int)planets[1],(int)planets[2],(int)planets[3],(int)planets[4],(int)planets[5],(int)planets[6]);

  // TODO: this is for testing only
  // wninsd_c(unix2et(0),unix2et(2147483647),&cnfine);
  wninsd_c (-479695089600.+86400*468, 479386728000., &cnfine);

  // 1 second tolerance (serious overkill, but 1e-6 is default, worse!)
  gfstol_c(1.);

  // find under MAXSEP degrees...
  // TODO: The 90 days below is just for testing, not accurate!!!!
  gfuds_c(gfq,gfdecrx,"<",MAXSEP,0.,86400.*90,MAXWIN,&cnfine,&result);

  nres = wncard_c(&result);

  for (i=0; i<nres; i++) {
    wnfetd_c(&result,i,&beg,&end);
    // R = range, M = min
    printf("R %f %f\n",et2jd(beg),et2jd(end));
    findmins(beg,end);
  }

  //  printf("There are %d results\n",wncard_c(&result));

  return 0;
}
コード例 #5
0
ファイル: bc-periapses.c プロジェクト: barrycarter/bcapps
int main (int argc, char **argv) {

  SPICEDOUBLE_CELL(cnfine,2);
  SPICEDOUBLE_CELL(result,2*MAXWIN);
  furnsh_c("/home/user/BCGIT/ASTRO/standard.tm");
  wninsd_c((SYEAR-2000.)*31556952.,(EYEAR-2000.)*31556952.,&cnfine);

  // all of DE431
  // wninsd_c (-479695089600.+86400*468, 479386728000., &cnfine);

  // 1 second tolerance (serious overkill, but 1e-6 is default, worse!)
  gfstol_c(1.);

  // NOTE: putting MAXSEP below is harmless if cond is LOCMIN or something
  gfuds_c(GFQ,gfdecrx,COND,MAXSEP,0.,86400.,MAXWIN,&cnfine,&result);
  show_results(LABEL,result,GFQ);

  return(0);
}