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elem2tle.cpp
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/* elem2tle.cpp: converts elements to TLE form & puts them
in the "standard" two-line format
Copyright (C) 2010, Project Pluto
This program is free software; you can redistribute it and/or
modify it under the terms of the GNU General Public License
as published by the Free Software Foundation; either version 2
of the License, or (at your option) any later version.
This program is distributed in the hope that it will be useful,
but WITHOUT ANY WARRANTY; without even the implied warranty of
MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
GNU General Public License for more details.
You should have received a copy of the GNU General Public License
along with this program; if not, write to the Free Software
Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA
02110-1301, USA. */
#include <stdio.h>
#include <string.h>
#include <stdlib.h>
#include <math.h>
#include "watdefs.h"
#include "afuncs.h"
#include "comets.h"
#include "norad.h"
#include "date.h"
const double earth_mass_over_sun_mass = 2.98994e-6;
#define GAUSS_K .01720209895
#define SOLAR_GM (GAUSS_K * GAUSS_K)
#define PI 3.141592653589793238462643383279502884197169399375105
#define J2000 2451545.0
int elements_to_tle( tle_t *tle, const ELEMENTS *elem);
int vector_to_tle( tle_t *tle, const double *state_vect, const double epoch);
int write_tle_from_vector( char *buff, const double *state_vect,
const double epoch, const char *norad_desig, const char *intl_desig);
void convert_elements( const double epoch_from, const double epoch_to,
double *incl, double *asc_node, double *arg_per); /* conv_ele.cpp */
#define centralize_angle(x) (fmod( (x) + PI * 10., PI + PI))
#define centralize_angle_and_cvt_to_degrees( x) \
(centralize_angle( x) * (180. / PI))
int elements_to_tle( tle_t *tle, const ELEMENTS *elem)
{
int rval = -1;
if( elem->ecc < .9999)
{
const double t0 =
elem->major_axis * sqrt( elem->major_axis / earth_mass_over_sun_mass);
double incl = elem->incl;
double asc_node = elem->asc_node;
double arg_per = elem->arg_per;
double mean_anomaly = elem->mean_anomaly;
tle->epoch = elem->epoch;
/* The elements are in J2000, but TLEs are given */
/* in epoch of date: */
convert_elements( 2000., 2000. + (elem->epoch - J2000) / 365.25,
&incl, &asc_node, &arg_per); /* conv_ele.cpp */
tle->xincl = centralize_angle( incl);
tle->xnodeo = centralize_angle( asc_node);
tle->omegao = centralize_angle( arg_per);
tle->xmo = centralize_angle( mean_anomaly);
tle->xno = (PI * 2.) / (t0 * 365.25 * minutes_per_day);
/* xno is now in radians per minute */
tle->eo = elem->ecc;
/* Address these three values later: */
tle->xndt2o = tle->xndd6o = tle->bstar = 0.;
rval = 0;
}
return( rval);
}
int vector_to_tle( tle_t *tle, const double *state_vect, const double epoch)
{
ELEMENTS elem;
int rval = -1;
elem.gm = SOLAR_GM * earth_mass_over_sun_mass;
calc_classical_elements( &elem, state_vect, epoch, 1);
if( elem.ecc < .9999)
{
elem.epoch = epoch;
elements_to_tle( tle, &elem);
rval = 0;
}
return( rval);
}
int write_tle_from_vector( char *buff, const double *state_vect,
const double epoch, const char *norad_desig, const char *intl_desig)
{
tle_t tle;
int rval = 0;
double revs_per_day;
memset( &tle, 0, sizeof( tle_t));
rval = vector_to_tle( &tle, state_vect, epoch);
revs_per_day = tle.xno * minutes_per_day / (2. * PI);
if( revs_per_day > 50.) /* meaningless suborbital TLE */
rval = -1;
if( !rval)
{
if( norad_desig)
tle.norad_number = atoi( norad_desig);
else
tle.norad_number = 0;
if( intl_desig)
strcpy( tle.intl_desig, intl_desig);
else
tle.intl_desig[0] = '\0';
tle.classification = 'U';
tle.ephemeris_type = '0';
write_elements_in_tle_format( buff, &tle);
}
else
*buff = '\0';
return( rval);
}