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SGP4.cpp
3204 lines (2997 loc) · 116 KB
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SGP4.cpp
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/* ----------------------------------------------------------------
*
* sgp4unit.cpp
*
* this file contains the sgp4 procedures for analytical propagation
* of a satellite. the code was originally released in the 1980 and 1986
* spacetrack papers. a detailed discussion of the theory and history
* may be found in the 2006 aiaa paper by vallado, crawford, hujsak,
* and kelso.
*
* companion code for
* fundamentals of astrodynamics and applications
* 2013
* by david vallado
*
* (w) 719-573-2600, email dvallado@agi.com, davallado@gmail.com
*
* current :
* 9 aug 14 alek lidtke
* removed hard-coded include paths
* changed a number of SGP4name to SGP4Funcs namespace idenitifier
* started using sscanf_s in lines 2277, 2290, 2305, 2320, and 2334
* started using scanf_s in lines 2391, 2401, 2412, 2423, 2445, 2455
* started using strcpy_s in lines 2879, 2889, 2911
* changes :
* 7 aug 14 david vallado
* update to msvs2013 c++
* 30 aug 10 david vallado
* delete unused variables in initl
* replace pow integer 2, 3 with multiplies for speed
* 3 nov 08 david vallado
* put returns in for error codes
* 29 sep 08 david vallado
* fix atime for faster operation in dspace
* add operationmode for afspc (a) or improved (i)
* performance mode
* 16 jun 08 david vallado
* update small eccentricity check
* 16 nov 07 david vallado
* misc fixes for better compliance
* 20 apr 07 david vallado
* misc fixes for constants
* 11 aug 06 david vallado
* chg lyddane choice back to strn3, constants, misc doc
* 15 dec 05 david vallado
* misc fixes
* 26 jul 05 david vallado
* fixes for paper
* note that each fix is preceded by a
* comment with "sgp4fix" and an explanation of
* what was changed
* 10 aug 04 david vallado
* 2nd printing baseline working
* 14 may 01 david vallado
* 2nd edition baseline
* 80 norad
* original baseline
* ---------------------------------------------------------------- */
#include "stdafx.h"
#include "SGP4.h"
//errors are from the order of routines...
//must be defined in order of use...
const char help = 'n';
FILE *dbgfile;
#define pi 3.14159265358979323846
/* ----------- local functions - only ever used internally by sgp4 ---------- */
static void dpper
(
double e3, double ee2, double peo, double pgho, double pho,
double pinco, double plo, double se2, double se3, double sgh2,
double sgh3, double sgh4, double sh2, double sh3, double si2,
double si3, double sl2, double sl3, double sl4, double t,
double xgh2, double xgh3, double xgh4, double xh2, double xh3,
double xi2, double xi3, double xl2, double xl3, double xl4,
double zmol, double zmos, double inclo,
char init,
double& ep, double& inclp, double& nodep, double& argpp, double& mp,
char opsmode
);
static void dscom
(
double epoch, double ep, double argpp, double tc, double inclp,
double nodep, double np,
double& snodm, double& cnodm, double& sinim, double& cosim, double& sinomm,
double& cosomm,double& day, double& e3, double& ee2, double& em,
double& emsq, double& gam, double& peo, double& pgho, double& pho,
double& pinco, double& plo, double& rtemsq, double& se2, double& se3,
double& sgh2, double& sgh3, double& sgh4, double& sh2, double& sh3,
double& si2, double& si3, double& sl2, double& sl3, double& sl4,
double& s1, double& s2, double& s3, double& s4, double& s5,
double& s6, double& s7, double& ss1, double& ss2, double& ss3,
double& ss4, double& ss5, double& ss6, double& ss7, double& sz1,
double& sz2, double& sz3, double& sz11, double& sz12, double& sz13,
double& sz21, double& sz22, double& sz23, double& sz31, double& sz32,
double& sz33, double& xgh2, double& xgh3, double& xgh4, double& xh2,
double& xh3, double& xi2, double& xi3, double& xl2, double& xl3,
double& xl4, double& nm, double& z1, double& z2, double& z3,
double& z11, double& z12, double& z13, double& z21, double& z22,
double& z23, double& z31, double& z32, double& z33, double& zmol,
double& zmos
);
static void dsinit
(
//sgp4fix no longer needed pass in xke
//gravconsttype whichconst,
double xke,
double cosim, double emsq, double argpo, double s1, double s2,
double s3, double s4, double s5, double sinim, double ss1,
double ss2, double ss3, double ss4, double ss5, double sz1,
double sz3, double sz11, double sz13, double sz21, double sz23,
double sz31, double sz33, double t, double tc, double gsto,
double mo, double mdot, double no, double nodeo, double nodedot,
double xpidot, double z1, double z3, double z11, double z13,
double z21, double z23, double z31, double z33, double ecco,
double eccsq, double& em, double& argpm, double& inclm, double& mm,
double& nm, double& nodem,
int& irez,
double& atime, double& d2201, double& d2211, double& d3210, double& d3222,
double& d4410, double& d4422, double& d5220, double& d5232, double& d5421,
double& d5433, double& dedt, double& didt, double& dmdt, double& dndt,
double& dnodt, double& domdt, double& del1, double& del2, double& del3,
double& xfact, double& xlamo, double& xli, double& xni
);
static void dspace
(
int irez,
double d2201, double d2211, double d3210, double d3222, double d4410,
double d4422, double d5220, double d5232, double d5421, double d5433,
double dedt, double del1, double del2, double del3, double didt,
double dmdt, double dnodt, double domdt, double argpo, double argpdot,
double t, double tc, double gsto, double xfact, double xlamo,
double no,
double& atime, double& em, double& argpm, double& inclm, double& xli,
double& mm, double& xni, double& nodem, double& dndt, double& nm
);
static void initl
(
// not needeed. included in satrec if needed later
// int satn,
// sgp4fix assin xke and j2
// gravconsttype whichconst,
double xke, double j2,
double ecco, double epoch, double inclo, double& no,
char& method,
double& ainv, double& ao, double& con41, double& con42, double& cosio,
double& cosio2,double& eccsq, double& omeosq, double& posq,
double& rp, double& rteosq,double& sinio , double& gsto, char opsmode
);
namespace SGP4Funcs{
/* -----------------------------------------------------------------------------
*
* procedure dpper
*
* this procedure provides deep space long period periodic contributions
* to the mean elements. by design, these periodics are zero at epoch.
* this used to be dscom which included initialization, but it's really a
* recurring function.
*
* author : david vallado 719-573-2600 28 jun 2005
*
* inputs :
* e3 -
* ee2 -
* peo -
* pgho -
* pho -
* pinco -
* plo -
* se2 , se3 , sgh2, sgh3, sgh4, sh2, sh3, si2, si3, sl2, sl3, sl4 -
* t -
* xh2, xh3, xi2, xi3, xl2, xl3, xl4 -
* zmol -
* zmos -
* ep - eccentricity 0.0 - 1.0
* inclo - inclination - needed for lyddane modification
* nodep - right ascension of ascending node
* argpp - argument of perigee
* mp - mean anomaly
*
* outputs :
* ep - eccentricity 0.0 - 1.0
* inclp - inclination
* nodep - right ascension of ascending node
* argpp - argument of perigee
* mp - mean anomaly
*
* locals :
* alfdp -
* betdp -
* cosip , sinip , cosop , sinop ,
* dalf -
* dbet -
* dls -
* f2, f3 -
* pe -
* pgh -
* ph -
* pinc -
* pl -
* sel , ses , sghl , sghs , shl , shs , sil , sinzf , sis ,
* sll , sls
* xls -
* xnoh -
* zf -
* zm -
*
* coupling :
* none.
*
* references :
* hoots, roehrich, norad spacetrack report #3 1980
* hoots, norad spacetrack report #6 1986
* hoots, schumacher and glover 2004
* vallado, crawford, hujsak, kelso 2006
----------------------------------------------------------------------------*/
static void dpper
(
double e3, double ee2, double peo, double pgho, double pho,
double pinco, double plo, double se2, double se3, double sgh2,
double sgh3, double sgh4, double sh2, double sh3, double si2,
double si3, double sl2, double sl3, double sl4, double t,
double xgh2, double xgh3, double xgh4, double xh2, double xh3,
double xi2, double xi3, double xl2, double xl3, double xl4,
double zmol, double zmos, double inclo,
char init,
double& ep, double& inclp, double& nodep, double& argpp, double& mp,
char opsmode
)
{
/* --------------------- local variables ------------------------ */
const double twopi = 2.0 * pi;
double alfdp, betdp, cosip, cosop, dalf, dbet, dls,
f2, f3, pe, pgh, ph, pinc, pl ,
sel, ses, sghl, sghs, shll, shs, sil,
sinip, sinop, sinzf, sis, sll, sls, xls,
xnoh, zf, zm, zel, zes, znl, zns;
/* ---------------------- constants ----------------------------- */
zns = 1.19459e-5;
zes = 0.01675;
znl = 1.5835218e-4;
zel = 0.05490;
/* --------------- calculate time varying periodics ----------- */
zm = zmos + zns * t;
// be sure that the initial call has time set to zero
if (init == 'y')
zm = zmos;
zf = zm + 2.0 * zes * sin(zm);
sinzf = sin(zf);
f2 = 0.5 * sinzf * sinzf - 0.25;
f3 = -0.5 * sinzf * cos(zf);
ses = se2* f2 + se3 * f3;
sis = si2 * f2 + si3 * f3;
sls = sl2 * f2 + sl3 * f3 + sl4 * sinzf;
sghs = sgh2 * f2 + sgh3 * f3 + sgh4 * sinzf;
shs = sh2 * f2 + sh3 * f3;
zm = zmol + znl * t;
if (init == 'y')
zm = zmol;
zf = zm + 2.0 * zel * sin(zm);
sinzf = sin(zf);
f2 = 0.5 * sinzf * sinzf - 0.25;
f3 = -0.5 * sinzf * cos(zf);
sel = ee2 * f2 + e3 * f3;
sil = xi2 * f2 + xi3 * f3;
sll = xl2 * f2 + xl3 * f3 + xl4 * sinzf;
sghl = xgh2 * f2 + xgh3 * f3 + xgh4 * sinzf;
shll = xh2 * f2 + xh3 * f3;
pe = ses + sel;
pinc = sis + sil;
pl = sls + sll;
pgh = sghs + sghl;
ph = shs + shll;
if (init == 'n')
{
pe = pe - peo;
pinc = pinc - pinco;
pl = pl - plo;
pgh = pgh - pgho;
ph = ph - pho;
inclp = inclp + pinc;
ep = ep + pe;
sinip = sin(inclp);
cosip = cos(inclp);
/* ----------------- apply periodics directly ------------ */
// sgp4fix for lyddane choice
// strn3 used original inclination - this is technically feasible
// gsfc used perturbed inclination - also technically feasible
// probably best to readjust the 0.2 limit value and limit discontinuity
// 0.2 rad = 11.45916 deg
// use next line for original strn3 approach and original inclination
// if (inclo >= 0.2)
// use next line for gsfc version and perturbed inclination
if (inclp >= 0.2)
{
ph = ph / sinip;
pgh = pgh - cosip * ph;
argpp = argpp + pgh;
nodep = nodep + ph;
mp = mp + pl;
}
else
{
/* ---- apply periodics with lyddane modification ---- */
sinop = sin(nodep);
cosop = cos(nodep);
alfdp = sinip * sinop;
betdp = sinip * cosop;
dalf = ph * cosop + pinc * cosip * sinop;
dbet = -ph * sinop + pinc * cosip * cosop;
alfdp = alfdp + dalf;
betdp = betdp + dbet;
nodep = fmod(nodep, twopi);
// sgp4fix for afspc written intrinsic functions
// nodep used without a trigonometric function ahead
if ((nodep < 0.0) && (opsmode == 'a'))
nodep = nodep + twopi;
xls = mp + argpp + cosip * nodep;
dls = pl + pgh - pinc * nodep * sinip;
xls = xls + dls;
xnoh = nodep;
nodep = atan2(alfdp, betdp);
// sgp4fix for afspc written intrinsic functions
// nodep used without a trigonometric function ahead
if ((nodep < 0.0) && (opsmode == 'a'))
nodep = nodep + twopi;
if (fabs(xnoh - nodep) > pi)
if (nodep < xnoh)
nodep = nodep + twopi;
else
nodep = nodep - twopi;
mp = mp + pl;
argpp = xls - mp - cosip * nodep;
}
} // if init == 'n'
//#include "debug1.cpp"
} // end dpper
/*-----------------------------------------------------------------------------
*
* procedure dscom
*
* this procedure provides deep space common items used by both the secular
* and periodics subroutines. input is provided as shown. this routine
* used to be called dpper, but the functions inside weren't well organized.
*
* author : david vallado 719-573-2600 28 jun 2005
*
* inputs :
* epoch -
* ep - eccentricity
* argpp - argument of perigee
* tc -
* inclp - inclination
* nodep - right ascension of ascending node
* np - mean motion
*
* outputs :
* sinim , cosim , sinomm , cosomm , snodm , cnodm
* day -
* e3 -
* ee2 -
* em - eccentricity
* emsq - eccentricity squared
* gam -
* peo -
* pgho -
* pho -
* pinco -
* plo -
* rtemsq -
* se2, se3 -
* sgh2, sgh3, sgh4 -
* sh2, sh3, si2, si3, sl2, sl3, sl4 -
* s1, s2, s3, s4, s5, s6, s7 -
* ss1, ss2, ss3, ss4, ss5, ss6, ss7, sz1, sz2, sz3 -
* sz11, sz12, sz13, sz21, sz22, sz23, sz31, sz32, sz33 -
* xgh2, xgh3, xgh4, xh2, xh3, xi2, xi3, xl2, xl3, xl4 -
* nm - mean motion
* z1, z2, z3, z11, z12, z13, z21, z22, z23, z31, z32, z33 -
* zmol -
* zmos -
*
* locals :
* a1, a2, a3, a4, a5, a6, a7, a8, a9, a10 -
* betasq -
* cc -
* ctem, stem -
* x1, x2, x3, x4, x5, x6, x7, x8 -
* xnodce -
* xnoi -
* zcosg , zsing , zcosgl , zsingl , zcosh , zsinh , zcoshl , zsinhl ,
* zcosi , zsini , zcosil , zsinil ,
* zx -
* zy -
*
* coupling :
* none.
*
* references :
* hoots, roehrich, norad spacetrack report #3 1980
* hoots, norad spacetrack report #6 1986
* hoots, schumacher and glover 2004
* vallado, crawford, hujsak, kelso 2006
----------------------------------------------------------------------------*/
static void dscom
(
double epoch, double ep, double argpp, double tc, double inclp,
double nodep, double np,
double& snodm, double& cnodm, double& sinim, double& cosim, double& sinomm,
double& cosomm,double& day, double& e3, double& ee2, double& em,
double& emsq, double& gam, double& peo, double& pgho, double& pho,
double& pinco, double& plo, double& rtemsq, double& se2, double& se3,
double& sgh2, double& sgh3, double& sgh4, double& sh2, double& sh3,
double& si2, double& si3, double& sl2, double& sl3, double& sl4,
double& s1, double& s2, double& s3, double& s4, double& s5,
double& s6, double& s7, double& ss1, double& ss2, double& ss3,
double& ss4, double& ss5, double& ss6, double& ss7, double& sz1,
double& sz2, double& sz3, double& sz11, double& sz12, double& sz13,
double& sz21, double& sz22, double& sz23, double& sz31, double& sz32,
double& sz33, double& xgh2, double& xgh3, double& xgh4, double& xh2,
double& xh3, double& xi2, double& xi3, double& xl2, double& xl3,
double& xl4, double& nm, double& z1, double& z2, double& z3,
double& z11, double& z12, double& z13, double& z21, double& z22,
double& z23, double& z31, double& z32, double& z33, double& zmol,
double& zmos
)
{
/* -------------------------- constants ------------------------- */
const double zes = 0.01675;
const double zel = 0.05490;
const double c1ss = 2.9864797e-6;
const double c1l = 4.7968065e-7;
const double zsinis = 0.39785416;
const double zcosis = 0.91744867;
const double zcosgs = 0.1945905;
const double zsings = -0.98088458;
const double twopi = 2.0 * pi;
/* --------------------- local variables ------------------------ */
int lsflg;
double a1 , a2 , a3 , a4 , a5 , a6 , a7 ,
a8 , a9 , a10 , betasq, cc , ctem , stem ,
x1 , x2 , x3 , x4 , x5 , x6 , x7 ,
x8 , xnodce, xnoi , zcosg , zcosgl, zcosh , zcoshl,
zcosi , zcosil, zsing , zsingl, zsinh , zsinhl, zsini ,
zsinil, zx , zy;
nm = np;
em = ep;
snodm = sin(nodep);
cnodm = cos(nodep);
sinomm = sin(argpp);
cosomm = cos(argpp);
sinim = sin(inclp);
cosim = cos(inclp);
emsq = em * em;
betasq = 1.0 - emsq;
rtemsq = sqrt(betasq);
/* ----------------- initialize lunar solar terms --------------- */
peo = 0.0;
pinco = 0.0;
plo = 0.0;
pgho = 0.0;
pho = 0.0;
day = epoch + 18261.5 + tc / 1440.0;
xnodce = fmod(4.5236020 - 9.2422029e-4 * day, twopi);
stem = sin(xnodce);
ctem = cos(xnodce);
zcosil = 0.91375164 - 0.03568096 * ctem;
zsinil = sqrt(1.0 - zcosil * zcosil);
zsinhl = 0.089683511 * stem / zsinil;
zcoshl = sqrt(1.0 - zsinhl * zsinhl);
gam = 5.8351514 + 0.0019443680 * day;
zx = 0.39785416 * stem / zsinil;
zy = zcoshl * ctem + 0.91744867 * zsinhl * stem;
zx = atan2(zx, zy);
zx = gam + zx - xnodce;
zcosgl = cos(zx);
zsingl = sin(zx);
/* ------------------------- do solar terms --------------------- */
zcosg = zcosgs;
zsing = zsings;
zcosi = zcosis;
zsini = zsinis;
zcosh = cnodm;
zsinh = snodm;
cc = c1ss;
xnoi = 1.0 / nm;
for (lsflg = 1; lsflg <= 2; lsflg++)
{
a1 = zcosg * zcosh + zsing * zcosi * zsinh;
a3 = -zsing * zcosh + zcosg * zcosi * zsinh;
a7 = -zcosg * zsinh + zsing * zcosi * zcosh;
a8 = zsing * zsini;
a9 = zsing * zsinh + zcosg * zcosi * zcosh;
a10 = zcosg * zsini;
a2 = cosim * a7 + sinim * a8;
a4 = cosim * a9 + sinim * a10;
a5 = -sinim * a7 + cosim * a8;
a6 = -sinim * a9 + cosim * a10;
x1 = a1 * cosomm + a2 * sinomm;
x2 = a3 * cosomm + a4 * sinomm;
x3 = -a1 * sinomm + a2 * cosomm;
x4 = -a3 * sinomm + a4 * cosomm;
x5 = a5 * sinomm;
x6 = a6 * sinomm;
x7 = a5 * cosomm;
x8 = a6 * cosomm;
z31 = 12.0 * x1 * x1 - 3.0 * x3 * x3;
z32 = 24.0 * x1 * x2 - 6.0 * x3 * x4;
z33 = 12.0 * x2 * x2 - 3.0 * x4 * x4;
z1 = 3.0 * (a1 * a1 + a2 * a2) + z31 * emsq;
z2 = 6.0 * (a1 * a3 + a2 * a4) + z32 * emsq;
z3 = 3.0 * (a3 * a3 + a4 * a4) + z33 * emsq;
z11 = -6.0 * a1 * a5 + emsq * (-24.0 * x1 * x7-6.0 * x3 * x5);
z12 = -6.0 * (a1 * a6 + a3 * a5) + emsq *
(-24.0 * (x2 * x7 + x1 * x8) - 6.0 * (x3 * x6 + x4 * x5));
z13 = -6.0 * a3 * a6 + emsq * (-24.0 * x2 * x8 - 6.0 * x4 * x6);
z21 = 6.0 * a2 * a5 + emsq * (24.0 * x1 * x5 - 6.0 * x3 * x7);
z22 = 6.0 * (a4 * a5 + a2 * a6) + emsq *
(24.0 * (x2 * x5 + x1 * x6) - 6.0 * (x4 * x7 + x3 * x8));
z23 = 6.0 * a4 * a6 + emsq * (24.0 * x2 * x6 - 6.0 * x4 * x8);
z1 = z1 + z1 + betasq * z31;
z2 = z2 + z2 + betasq * z32;
z3 = z3 + z3 + betasq * z33;
s3 = cc * xnoi;
s2 = -0.5 * s3 / rtemsq;
s4 = s3 * rtemsq;
s1 = -15.0 * em * s4;
s5 = x1 * x3 + x2 * x4;
s6 = x2 * x3 + x1 * x4;
s7 = x2 * x4 - x1 * x3;
/* ----------------------- do lunar terms ------------------- */
if (lsflg == 1)
{
ss1 = s1;
ss2 = s2;
ss3 = s3;
ss4 = s4;
ss5 = s5;
ss6 = s6;
ss7 = s7;
sz1 = z1;
sz2 = z2;
sz3 = z3;
sz11 = z11;
sz12 = z12;
sz13 = z13;
sz21 = z21;
sz22 = z22;
sz23 = z23;
sz31 = z31;
sz32 = z32;
sz33 = z33;
zcosg = zcosgl;
zsing = zsingl;
zcosi = zcosil;
zsini = zsinil;
zcosh = zcoshl * cnodm + zsinhl * snodm;
zsinh = snodm * zcoshl - cnodm * zsinhl;
cc = c1l;
}
}
zmol = fmod(4.7199672 + 0.22997150 * day - gam, twopi);
zmos = fmod(6.2565837 + 0.017201977 * day, twopi);
/* ------------------------ do solar terms ---------------------- */
se2 = 2.0 * ss1 * ss6;
se3 = 2.0 * ss1 * ss7;
si2 = 2.0 * ss2 * sz12;
si3 = 2.0 * ss2 * (sz13 - sz11);
sl2 = -2.0 * ss3 * sz2;
sl3 = -2.0 * ss3 * (sz3 - sz1);
sl4 = -2.0 * ss3 * (-21.0 - 9.0 * emsq) * zes;
sgh2 = 2.0 * ss4 * sz32;
sgh3 = 2.0 * ss4 * (sz33 - sz31);
sgh4 = -18.0 * ss4 * zes;
sh2 = -2.0 * ss2 * sz22;
sh3 = -2.0 * ss2 * (sz23 - sz21);
/* ------------------------ do lunar terms ---------------------- */
ee2 = 2.0 * s1 * s6;
e3 = 2.0 * s1 * s7;
xi2 = 2.0 * s2 * z12;
xi3 = 2.0 * s2 * (z13 - z11);
xl2 = -2.0 * s3 * z2;
xl3 = -2.0 * s3 * (z3 - z1);
xl4 = -2.0 * s3 * (-21.0 - 9.0 * emsq) * zel;
xgh2 = 2.0 * s4 * z32;
xgh3 = 2.0 * s4 * (z33 - z31);
xgh4 = -18.0 * s4 * zel;
xh2 = -2.0 * s2 * z22;
xh3 = -2.0 * s2 * (z23 - z21);
//#include "debug2.cpp"
} // end dscom
/*-----------------------------------------------------------------------------
*
* procedure dsinit
*
* this procedure provides deep space contributions to mean motion dot due
* to geopotential resonance with half day and one day orbits.
*
* author : david vallado 719-573-2600 28 jun 2005
*
* inputs :
* xke - reciprocal of tumin
* cosim, sinim-
* emsq - eccentricity squared
* argpo - argument of perigee
* s1, s2, s3, s4, s5 -
* ss1, ss2, ss3, ss4, ss5 -
* sz1, sz3, sz11, sz13, sz21, sz23, sz31, sz33 -
* t - time
* tc -
* gsto - greenwich sidereal time rad
* mo - mean anomaly
* mdot - mean anomaly dot (rate)
* no - mean motion
* nodeo - right ascension of ascending node
* nodedot - right ascension of ascending node dot (rate)
* xpidot -
* z1, z3, z11, z13, z21, z23, z31, z33 -
* eccm - eccentricity
* argpm - argument of perigee
* inclm - inclination
* mm - mean anomaly
* xn - mean motion
* nodem - right ascension of ascending node
*
* outputs :
* em - eccentricity
* argpm - argument of perigee
* inclm - inclination
* mm - mean anomaly
* nm - mean motion
* nodem - right ascension of ascending node
* irez - flag for resonance 0-none, 1-one day, 2-half day
* atime -
* d2201, d2211, d3210, d3222, d4410, d4422, d5220, d5232, d5421, d5433 -
* dedt -
* didt -
* dmdt -
* dndt -
* dnodt -
* domdt -
* del1, del2, del3 -
* ses , sghl , sghs , sgs , shl , shs , sis , sls
* theta -
* xfact -
* xlamo -
* xli -
* xni
*
* locals :
* ainv2 -
* aonv -
* cosisq -
* eoc -
* f220, f221, f311, f321, f322, f330, f441, f442, f522, f523, f542, f543 -
* g200, g201, g211, g300, g310, g322, g410, g422, g520, g521, g532, g533 -
* sini2 -
* temp -
* temp1 -
* theta -
* xno2 -
*
* coupling :
* getgravconst- no longer used
*
* references :
* hoots, roehrich, norad spacetrack report #3 1980
* hoots, norad spacetrack report #6 1986
* hoots, schumacher and glover 2004
* vallado, crawford, hujsak, kelso 2006
----------------------------------------------------------------------------*/
static void dsinit
(
// sgp4fix just send in xke as a constant and eliminate getgravconst call
// gravconsttype whichconst,
double xke,
double cosim, double emsq, double argpo, double s1, double s2,
double s3, double s4, double s5, double sinim, double ss1,
double ss2, double ss3, double ss4, double ss5, double sz1,
double sz3, double sz11, double sz13, double sz21, double sz23,
double sz31, double sz33, double t, double tc, double gsto,
double mo, double mdot, double no, double nodeo, double nodedot,
double xpidot, double z1, double z3, double z11, double z13,
double z21, double z23, double z31, double z33, double ecco,
double eccsq, double& em, double& argpm, double& inclm, double& mm,
double& nm, double& nodem,
int& irez,
double& atime, double& d2201, double& d2211, double& d3210, double& d3222,
double& d4410, double& d4422, double& d5220, double& d5232, double& d5421,
double& d5433, double& dedt, double& didt, double& dmdt, double& dndt,
double& dnodt, double& domdt, double& del1, double& del2, double& del3,
double& xfact, double& xlamo, double& xli, double& xni
)
{
/* --------------------- local variables ------------------------ */
const double twopi = 2.0 * pi;
double ainv2 , aonv=0.0, cosisq, eoc, f220 , f221 , f311 ,
f321 , f322 , f330 , f441 , f442 , f522 , f523 ,
f542 , f543 , g200 , g201 , g211 , g300 , g310 ,
g322 , g410 , g422 , g520 , g521 , g532 , g533 ,
ses , sgs , sghl , sghs , shs , shll , sis ,
sini2 , sls , temp , temp1 , theta , xno2 , q22 ,
q31 , q33 , root22, root44, root54, rptim , root32,
root52, x2o3 , znl , emo , zns , emsqo;
q22 = 1.7891679e-6;
q31 = 2.1460748e-6;
q33 = 2.2123015e-7;
root22 = 1.7891679e-6;
root44 = 7.3636953e-9;
root54 = 2.1765803e-9;
rptim = 4.37526908801129966e-3; // this equates to 7.29211514668855e-5 rad/sec
root32 = 3.7393792e-7;
root52 = 1.1428639e-7;
x2o3 = 2.0 / 3.0;
znl = 1.5835218e-4;
zns = 1.19459e-5;
// sgp4fix identify constants and allow alternate values
// just xke is used here so pass it in rather than have multiple calls
// getgravconst( whichconst, tumin, mu, radiusearthkm, xke, j2, j3, j4, j3oj2 );
/* -------------------- deep space initialization ------------ */
irez = 0;
if ((nm < 0.0052359877) && (nm > 0.0034906585))
irez = 1;
if ((nm >= 8.26e-3) && (nm <= 9.24e-3) && (em >= 0.5))
irez = 2;
/* ------------------------ do solar terms ------------------- */
ses = ss1 * zns * ss5;
sis = ss2 * zns * (sz11 + sz13);
sls = -zns * ss3 * (sz1 + sz3 - 14.0 - 6.0 * emsq);
sghs = ss4 * zns * (sz31 + sz33 - 6.0);
shs = -zns * ss2 * (sz21 + sz23);
// sgp4fix for 180 deg incl
if ((inclm < 5.2359877e-2) || (inclm > pi - 5.2359877e-2))
shs = 0.0;
if (sinim != 0.0)
shs = shs / sinim;
sgs = sghs - cosim * shs;
/* ------------------------- do lunar terms ------------------ */
dedt = ses + s1 * znl * s5;
didt = sis + s2 * znl * (z11 + z13);
dmdt = sls - znl * s3 * (z1 + z3 - 14.0 - 6.0 * emsq);
sghl = s4 * znl * (z31 + z33 - 6.0);
shll = -znl * s2 * (z21 + z23);
// sgp4fix for 180 deg incl
if ((inclm < 5.2359877e-2) || (inclm > pi - 5.2359877e-2))
shll = 0.0;
domdt = sgs + sghl;
dnodt = shs;
if (sinim != 0.0)
{
domdt = domdt - cosim / sinim * shll;
dnodt = dnodt + shll / sinim;
}
/* ----------- calculate deep space resonance effects -------- */
dndt = 0.0;
theta = fmod(gsto + tc * rptim, twopi);
em = em + dedt * t;
inclm = inclm + didt * t;
argpm = argpm + domdt * t;
nodem = nodem + dnodt * t;
mm = mm + dmdt * t;
// sgp4fix for negative inclinations
// the following if statement should be commented out
//if (inclm < 0.0)
// {
// inclm = -inclm;
// argpm = argpm - pi;
// nodem = nodem + pi;
// }
/* -------------- initialize the resonance terms ------------- */
if (irez != 0)
{
aonv = pow(nm / xke, x2o3);
/* ---------- geopotential resonance for 12 hour orbits ------ */
if (irez == 2)
{
cosisq = cosim * cosim;
emo = em;
em = ecco;
emsqo = emsq;
emsq = eccsq;
eoc = em * emsq;
g201 = -0.306 - (em - 0.64) * 0.440;
if (em <= 0.65)
{
g211 = 3.616 - 13.2470 * em + 16.2900 * emsq;
g310 = -19.302 + 117.3900 * em - 228.4190 * emsq + 156.5910 * eoc;
g322 = -18.9068 + 109.7927 * em - 214.6334 * emsq + 146.5816 * eoc;
g410 = -41.122 + 242.6940 * em - 471.0940 * emsq + 313.9530 * eoc;
g422 = -146.407 + 841.8800 * em - 1629.014 * emsq + 1083.4350 * eoc;
g520 = -532.114 + 3017.977 * em - 5740.032 * emsq + 3708.2760 * eoc;
}
else
{
g211 = -72.099 + 331.819 * em - 508.738 * emsq + 266.724 * eoc;
g310 = -346.844 + 1582.851 * em - 2415.925 * emsq + 1246.113 * eoc;
g322 = -342.585 + 1554.908 * em - 2366.899 * emsq + 1215.972 * eoc;
g410 = -1052.797 + 4758.686 * em - 7193.992 * emsq + 3651.957 * eoc;
g422 = -3581.690 + 16178.110 * em - 24462.770 * emsq + 12422.520 * eoc;
if (em > 0.715)
g520 =-5149.66 + 29936.92 * em - 54087.36 * emsq + 31324.56 * eoc;
else
g520 = 1464.74 - 4664.75 * em + 3763.64 * emsq;
}
if (em < 0.7)
{
g533 = -919.22770 + 4988.6100 * em - 9064.7700 * emsq + 5542.21 * eoc;
g521 = -822.71072 + 4568.6173 * em - 8491.4146 * emsq + 5337.524 * eoc;
g532 = -853.66600 + 4690.2500 * em - 8624.7700 * emsq + 5341.4 * eoc;
}
else
{
g533 =-37995.780 + 161616.52 * em - 229838.20 * emsq + 109377.94 * eoc;
g521 =-51752.104 + 218913.95 * em - 309468.16 * emsq + 146349.42 * eoc;
g532 =-40023.880 + 170470.89 * em - 242699.48 * emsq + 115605.82 * eoc;
}
sini2= sinim * sinim;
f220 = 0.75 * (1.0 + 2.0 * cosim+cosisq);
f221 = 1.5 * sini2;
f321 = 1.875 * sinim * (1.0 - 2.0 * cosim - 3.0 * cosisq);
f322 = -1.875 * sinim * (1.0 + 2.0 * cosim - 3.0 * cosisq);
f441 = 35.0 * sini2 * f220;
f442 = 39.3750 * sini2 * sini2;
f522 = 9.84375 * sinim * (sini2 * (1.0 - 2.0 * cosim- 5.0 * cosisq) +
0.33333333 * (-2.0 + 4.0 * cosim + 6.0 * cosisq) );
f523 = sinim * (4.92187512 * sini2 * (-2.0 - 4.0 * cosim +
10.0 * cosisq) + 6.56250012 * (1.0+2.0 * cosim - 3.0 * cosisq));
f542 = 29.53125 * sinim * (2.0 - 8.0 * cosim+cosisq *
(-12.0 + 8.0 * cosim + 10.0 * cosisq));
f543 = 29.53125 * sinim * (-2.0 - 8.0 * cosim+cosisq *
(12.0 + 8.0 * cosim - 10.0 * cosisq));
xno2 = nm * nm;
ainv2 = aonv * aonv;
temp1 = 3.0 * xno2 * ainv2;
temp = temp1 * root22;
d2201 = temp * f220 * g201;
d2211 = temp * f221 * g211;
temp1 = temp1 * aonv;
temp = temp1 * root32;
d3210 = temp * f321 * g310;
d3222 = temp * f322 * g322;
temp1 = temp1 * aonv;
temp = 2.0 * temp1 * root44;
d4410 = temp * f441 * g410;
d4422 = temp * f442 * g422;
temp1 = temp1 * aonv;
temp = temp1 * root52;
d5220 = temp * f522 * g520;
d5232 = temp * f523 * g532;
temp = 2.0 * temp1 * root54;
d5421 = temp * f542 * g521;
d5433 = temp * f543 * g533;
xlamo = fmod(mo + nodeo + nodeo-theta - theta, twopi);
xfact = mdot + dmdt + 2.0 * (nodedot + dnodt - rptim) - no;
em = emo;
emsq = emsqo;
}
/* ---------------- synchronous resonance terms -------------- */
if (irez == 1)
{
g200 = 1.0 + emsq * (-2.5 + 0.8125 * emsq);
g310 = 1.0 + 2.0 * emsq;
g300 = 1.0 + emsq * (-6.0 + 6.60937 * emsq);
f220 = 0.75 * (1.0 + cosim) * (1.0 + cosim);
f311 = 0.9375 * sinim * sinim * (1.0 + 3.0 * cosim) - 0.75 * (1.0 + cosim);
f330 = 1.0 + cosim;
f330 = 1.875 * f330 * f330 * f330;
del1 = 3.0 * nm * nm * aonv * aonv;
del2 = 2.0 * del1 * f220 * g200 * q22;
del3 = 3.0 * del1 * f330 * g300 * q33 * aonv;
del1 = del1 * f311 * g310 * q31 * aonv;
xlamo = fmod(mo + nodeo + argpo - theta, twopi);
xfact = mdot + xpidot - rptim + dmdt + domdt + dnodt - no;
}
/* ------------ for sgp4, initialize the integrator ---------- */
xli = xlamo;
xni = no;
atime = 0.0;
nm = no + dndt;
}
//#include "debug3.cpp"
} // end dsinit
/*-----------------------------------------------------------------------------
*
* procedure dspace
*
* this procedure provides deep space contributions to mean elements for
* perturbing third body. these effects have been averaged over one
* revolution of the sun and moon. for earth resonance effects, the
* effects have been averaged over no revolutions of the satellite.
* (mean motion)
*
* author : david vallado 719-573-2600 28 jun 2005
*
* inputs :
* d2201, d2211, d3210, d3222, d4410, d4422, d5220, d5232, d5421, d5433 -
* dedt -
* del1, del2, del3 -
* didt -
* dmdt -
* dnodt -
* domdt -
* irez - flag for resonance 0-none, 1-one day, 2-half day
* argpo - argument of perigee
* argpdot - argument of perigee dot (rate)
* t - time
* tc -
* gsto - gst
* xfact -
* xlamo -
* no - mean motion
* atime -
* em - eccentricity
* ft -
* argpm - argument of perigee
* inclm - inclination
* xli -
* mm - mean anomaly
* xni - mean motion
* nodem - right ascension of ascending node
*
* outputs :
* atime -
* em - eccentricity
* argpm - argument of perigee
* inclm - inclination
* xli -
* mm - mean anomaly
* xni -
* nodem - right ascension of ascending node
* dndt -
* nm - mean motion
*
* locals :
* delt -
* ft -
* theta -
* x2li -
* x2omi -
* xl -
* xldot -
* xnddt -
* xndt -
* xomi -
*
* coupling :
* none -
*
* references :
* hoots, roehrich, norad spacetrack report #3 1980
* hoots, norad spacetrack report #6 1986
* hoots, schumacher and glover 2004
* vallado, crawford, hujsak, kelso 2006