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AlignEq.ino
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AlignEq.ino
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// -----------------------------------------------------------------------------------
// GEOMETRIC ALIGN FOR EQ MOUNTS
//
// by Howard Dutton
//
// Copyright (C) 2012 to 2020 Howard Dutton
//
// -----------------------------------------------------------------------------------
// ADVANCED GEOMETRIC ALIGN FOR EQUATORIAL MOUNTS (GOTO ASSIST)
#if MOUNT_TYPE != ALTAZM
// Initialize
void TGeoAlign::init() {
avgDec=0.0;
avgHA =0.0;
ax1Cor=0; // align internal index for Axis1
ax2Cor=0; // align internal index for Axis2
altCor=0; // for geometric coordinate correction/align, - is below the pole, + above
azmCor=0; // - is right of the pole, + is left
doCor =0; // declination/optics orthogonal correction
pdCor =0; // declination/polar orthogonal correction
dfCor =0; // fork or declination axis flex
tfCor =0; // tube flex
geo_ready=false;
}
// remember the alignment between sessions
void TGeoAlign::readCoe() {
ax1Cor=nv.readFloat(EE_ax1Cor);
if (ax1Cor < -360 || ax1Cor > 360) { ax1Cor=0.0; DLF("ERR, readCoe(): bad NV ax1Cor"); }
ax2Cor=nv.readFloat(EE_ax2Cor);
if (ax2Cor < -360 || ax2Cor > 360) { ax2Cor=0.0; DLF("ERR, readCoe(): bad NV ax2Cor"); }
dfCor=nv.readFloat(EE_dfCor); // dfCor is ffCor for fork mounts
if (dfCor < -10 || dfCor > 10) { dfCor=0.0; DLF("ERR, readCoe(): bad NV dfCor"); }
tfCor=nv.readFloat(EE_tfCor);
if (tfCor < -10 || tfCor > 10) { tfCor=0.0; DLF("ERR, readCoe(): bad NV tfCor"); }
doCor=nv.readFloat(EE_doCor);
if (doCor < -10 || doCor > 10) { doCor=0.0; DLF("ERR, readCoe(): bad NV doCor"); }
pdCor=nv.readFloat(EE_pdCor);
if (pdCor < -10 || pdCor > 10) { pdCor=0.0; DLF("ERR, readCoe(): bad NV pdCor"); }
altCor=nv.readFloat(EE_altCor);
if (altCor < -10 || altCor > 10) { altCor=0.0; DLF("ERR, readCoe(): bad NV altCor"); }
azmCor=nv.readFloat(EE_azmCor);
if (azmCor < -10 || azmCor > 10) { azmCor=0.0; DLF("ERR, readCoe(): bad NV azmCor"); }
}
void TGeoAlign::writeCoe() {
nv.writeFloat(EE_ax1Cor,ax1Cor);
nv.writeFloat(EE_ax2Cor,ax2Cor);
nv.writeFloat(EE_dfCor,dfCor); // dfCor is ffCor for fork mounts
nv.writeFloat(EE_tfCor,tfCor);
nv.writeFloat(EE_doCor,doCor);
nv.writeFloat(EE_pdCor,pdCor);
nv.writeFloat(EE_altCor,altCor);
nv.writeFloat(EE_azmCor,azmCor);
}
// Status
bool TGeoAlign::isReady() {
return geo_ready;
}
// I=1 for 1st star, I=2 for 2nd star, I=3 for 3rd star
// N=total number of stars for this align (1 to 9)
// RA, Dec (all in degrees)
CommandErrors TGeoAlign::addStar(int I, int N, double RA, double Dec) {
// First star, just sync
if (I == 1) {
CommandErrors e=syncEqu(RA,Dec);
if (e != CE_NONE) return e;
}
mount[I-1].ha=getInstrAxis1()/Rad;
mount[I-1].dec=getInstrAxis2()/Rad;
actual[I-1].ha=haRange(LST()*15.0-RA)/Rad;
actual[I-1].dec=Dec/Rad;
if (getInstrPierSide() == PierSideWest) { actual[I-1].side=-1; mount[I-1].side=-1; } else
if (getInstrPierSide() == PierSideEast) { actual[I-1].side=1; mount[I-1].side=1; } else { actual[I-1].side=0; mount[I-1].side=0; }
// two or more stars and finished
if ((I >= 2) && (I == N)) model(N);
return CE_NONE;
}
// kick off modeling
void TGeoAlign::model(int n) {
static bool busy=false;
static int numStars=0;
if (busy) return; // busy
if (n > 0) { numStars=n; return; } // command
if (numStars > 0) { busy=true; autoModel(numStars); busy=false; numStars=0; } // waiting to solve
}
// returns the correction to be added to the requested RA,Dec to yield the actual RA,Dec that we will arrive at
void TGeoAlign::correct(double ha, double dec, double pierSide, double sf, double _deo, double _pd, double _pz, double _pe, double _df, double _ff, double _tf, double *h1, double *d1) {
double DO1,DOh;
double PD,PDh;
double PZ,PA;
double DF,DFd,TF,FF,FFd,TFh,TFd;
double cosDec=cos(dec);
double tanDec=tan(dec);
double sinHa=sin(ha);
double cosHa=cos(ha);
// ------------------------------------------------------------
// A. Misalignment due to tube/optics not being perp. to Dec axis
// negative numbers are further (S) from the NCP, swing to the
// equator and the effect on declination is 0. At the SCP it
// becomes a (N) offset. Unchanged with meridian flips.
DO1 =_deo*sf;
// works on HA. meridian flips effect this in HA
DOh = DO1*(1.0/cosDec)*pierSide;
// ------------------------------------------------------------
// B. Misalignment, Declination axis relative to Polar axis
// expressed as a correction to where the Polar axis is pointing
// negative numbers are further (S) from the NCP, swing to the
// equator and the effect on declination is 0.
// At the SCP it is, again, a (S) offset
PD =_pd*sf;
// works on HA.
PDh = -PD*tanDec*pierSide;
// ------------------------------------------------------------
// Misalignment, relative to NCP
// negative numbers are east of the pole
// C. polar left-right misalignment
PZ =_pz*sf;
// D. negative numbers are below the pole
// polar below-above misalignment
PA =_pe*sf;
// ------------------------------------------------------------
// Axis flex
DF =_df*sf;
DFd =-DF*(cosLat*cosHa+sinLat*tanDec);
// ------------------------------------------------------------
// Fork flex
FF =_ff*sf;
FFd =FF*cosHa;
// ------------------------------------------------------------
// Optical axis sag
TF =_tf*sf;
TFh =TF*(cosLat*sinHa*(1.0/cosDec));
TFd =TF*(cosLat*cosHa-sinLat*cosDec);
// ------------------------------------------------------------
*h1 =(-PZ*cosHa*tanDec + PA*sinHa*tanDec + DOh + PDh + TFh);
*d1 =(+PZ*sinHa + PA*cosHa + DFd + FFd + TFd);
}
void TGeoAlign::do_search(double sf, int p1, int p2, int p3, int p4, int p5, int p6, int p7, int p8, int p9)
{
long l,
_deo_m,_deo_p,
_pd_m,_pd_p,
_pz_m,_pz_p,
_pe_m,_pe_p,
_df_m,_df_p,
_tf_m,_tf_p,
_ff_m,_ff_p,
_oh_m,_oh_p,
_od_m,_od_p,
_deo,_pd,_pz,_pe, _df,_tf,_ff, _ode,_ohe;
double sf1=sf/(3600.0*Rad);
// search
// set Parameter Space
_deo_m=-p1+round(best_deo/sf); _deo_p=p1+round(best_deo/sf);
_pd_m =-p2+round(best_pd/sf); _pd_p=p2+round(best_pd/sf);
_pz_m =-p3+round(best_pz/sf); _pz_p=p3+round(best_pz/sf);
_pe_m =-p4+round(best_pe/sf); _pe_p=p4+round(best_pe/sf);
_tf_m =-p5+round(best_tf/sf); _tf_p=p5+round(best_tf/sf);
_ff_m =-p6+round(best_ff/sf); _ff_p=p6+round(best_ff/sf);
_df_m =-p7+round(best_df/sf); _df_p=p7+round(best_df/sf);
_od_m =-p8+round(best_ode/sf); _od_p=p8+round(best_ode/sf);
_oh_m =-p9+round(best_ohe/sf); _oh_p=p9+round(best_ohe/sf);
double md,mh;
for (_deo=_deo_m; _deo <= _deo_p; _deo++)
for (_pd=_pd_m; _pd <= _pd_p; _pd++)
for (_pz=_pz_m; _pz <= _pz_p; _pz++)
for (_pe=_pe_m; _pe <= _pe_p; _pe++)
for (_df=_df_m; _df <= _df_p; _df++)
for (_ff=_ff_m; _ff <= _ff_p; _ff++)
for (_tf=_tf_m; _tf <= _tf_p; _tf++)
for (_ohe=_oh_m; _ohe <= _oh_p; _ohe++)
for (_ode=_od_m; _ode <= _od_p; _ode++) {
ode=((double)_ode)*sf1;
odw=-ode;
ohe=((double)_ohe)*sf1;
ohw=ohe;
// check the combinations for all samples
for (l=0; l < num; l++) {
mh=mount[l].ha;
md=mount[l].dec;
if (mount[l].side == -1) // west of the mount
{
mh=mh+ohw;
md=md+odw;
} else
if (mount[l].side == 1) // east of the mount, default (fork mounts)
{
mh=mh+ohe;
md=md+ode;
}
correct(mh,md,mount[l].side,sf1,_deo,_pd,_pz,_pe,_df,_ff,_tf,&h1,&d1);
delta[l].ha=actual[l].ha-(mh-h1);
if (delta[l].ha > PI) delta[l].ha=delta[l].ha-PI*2.0; else
if (delta[l].ha < -PI) delta[l].ha=delta[l].ha+PI*2.0;
delta[l].dec=actual[l].dec-(md-d1);
delta[l].side=mount[l].side;
}
// calculate the standard deviations
sum1=0.0; for (l=0; l < num; l++) sum1=sum1+sq(delta[l].ha*cos(actual[l].dec)); sh=sqrt(sum1/(num-1));
sum1=0.0; for (l=0; l < num; l++) sum1=sum1+sq(delta[l].dec); sd=sqrt(sum1/(num-1));
max_dist=sqrt(sq(sh)+sq(sd));
// remember the best fit
if (max_dist < best_dist) {
best_dist =max_dist;
best_deo =((double)_deo)*sf;
best_pd =((double)_pd)*sf;
best_pz =((double)_pz)*sf;
best_pe =((double)_pe)*sf;
best_tf =((double)_tf)*sf;
best_df =((double)_df)*sf;
best_ff =((double)_ff)*sf;
if (p8 != 0) best_odw=odw*Rad*3600.0; else best_odw=best_pe/2.0;
if (p8 != 0) best_ode=ode*Rad*3600.0; else best_ode=-best_pe/2.0;
if (p9 != 0) best_ohw=ohw*Rad*3600.0;
if (p9 != 0) best_ohe=ohe*Rad*3600.0;
}
// keep the main loop running
loop2();
}
}
void TGeoAlign::autoModel(int n) {
num=n; // how many stars?
lat=latitude/Rad;
cosLat=cos(lat);
sinLat=sin(lat);
best_dist =3600.0*180.0;
best_deo =0.0;
best_pd =0.0;
best_pz =0.0;
best_pe =0.0;
best_tf =0.0;
best_ff =0.0;
best_df =0.0;
best_ode =0.0;
best_ohe =0.0;
// figure out the average HA offset as a starting point
ohe=0;
for (l=0; l < num; l++) {
h1=actual[l].ha-mount[l].ha;
if (h1 > PI) h1=h1-PI*2.0;
if (h1 < -PI) h1=h1+PI*2.0;
ohe=ohe+h1;
}
ohe=ohe/num; best_ohe=round(ohe*Rad*3600.0); best_ohw=best_ohe;
#if MOUNT_TYPE == FORK
Ff=1; Df=0;
#else
Ff=0; Df=1;
#endif
// only search for cone error if > 2 stars
int Do=0; if (num > 2) Do=1;
// search, this can handle about 9 degrees of polar misalignment, and 4 degrees of cone error
// DoPdPzPeTfFf Df OdOh
do_search(16384,0 ,0,1,1,0, 0, 0,1,1);
do_search( 8192,Do,0,1,1,0, 0, 0,1,1);
do_search( 4096,Do,0,1,1,0, 0, 0,1,1);
do_search( 2048,Do,0,1,1,0, 0, 0,1,1);
do_search( 1024,Do,0,1,1,0, 0, 0,1,1);
do_search( 512,Do,0,1,1,0, 0, 0,1,1);
#ifdef HAL_SLOW_PROCESSOR
// DoPdPzPeTfFf Df OdOh
do_search( 256,Do,0,1,1,0, 0, 0,1,1);
do_search( 128,Do,0,1,1,0, 0, 0,1,1);
#else
if (num > 4) {
// DoPdPzPeTfFf Df OdOh
do_search( 256,Do,1,1,1,0,Ff,Df,1,1);
do_search( 128,Do,1,1,1,1,Ff,Df,1,1);
do_search( 64,Do,1,1,1,1,Ff,Df,1,1);
#ifdef HAL_FAST_PROCESSOR
do_search( 32,Do,1,1,1,1,Ff,Df,1,1);
do_search( 16,Do,1,1,1,1,Ff,Df,1,1);
#endif
} else {
do_search( 256,Do,0,1,1,0, 0, 0,1,1);
do_search( 128,Do,0,1,1,0, 0, 0,1,1);
do_search( 64,Do,0,1,1,0, 0, 0,1,1);
do_search( 32,Do,0,1,1,0, 0, 0,1,1);
#ifdef HAL_FAST_PROCESSOR
do_search( 16,Do,0,1,1,0, 0, 0,1,1);
#endif
}
#endif
// geometric corrections
doCor=best_deo/3600.0;
pdCor=best_pd/3600.0;
azmCor=best_pz/3600.0;
altCor=best_pe/3600.0;
tfCor=best_tf/3600.0;
#if MOUNT_TYPE == FORK || MOUNT_TYPE == ALTAZM
dfCor=best_ff/3600.0;
#else
dfCor=best_df/3600.0;
#endif
ax1Cor=best_ohw/3600.0;
ax2Cor=best_odw/3600.0;
geo_ready=true;
}
// takes the topocentric refracted coordinates and applies corrections to arrive at instrument equatorial coordinates
void TGeoAlign::equToInstr(double HA, double Dec, double *HA1, double *Dec1, int PierSide) {
double p=1.0; if (PierSide == PierSideWest) p=-1.0;
if (Dec > 90.0) Dec=90.0;
if (Dec < -90.0) Dec=-90.0;
// breaks-down near the pole (limited to > 1' from pole)
if (fabs(Dec) < 89.9833) {
// initial rough guess at instrument HA,Dec
double h=HA/Rad;
double d=Dec/Rad;
for (int pass=0; pass < 3; pass++) {
double sinDec=sin(d);
double cosDec=cos(d);
double sinHA =sin(h);
double cosHA =cos(h);
// ------------------------------------------------------------
// misalignment due to tube/optics not being perp. to Dec axis
// negative numbers are further (S) from the NCP, swing to the
// equator and the effect on declination is 0. At the SCP it
// becomes a (N) offset. Unchanged with meridian flips.
// expressed as a correction to the Polar axis misalignment
double DOh=doCor*(1.0/cosDec)*p;
// ------------------------------------------------------------
// misalignment due to Dec axis being perp. to RA axis
double PDh=-pdCor*(sinDec/cosDec)*p;
#if MOUNT_TYPE == FORK
// Fork flex
double DFd=dfCor*cosHA;
#else
// Axis flex
double DFd=-dfCor*(cosLat*cosHA+sinLat*(sinDec/cosDec));
#endif
// Tube flex
double TFh=tfCor*(cosLat*sinHA*(1.0/cosDec));
double TFd=tfCor*(cosLat*cosHA-sinLat*cosDec);
// polar misalignment
double h1=-azmCor*cosHA*(sinDec/cosDec) + altCor*sinHA*(sinDec/cosDec);
double d1=+azmCor*sinHA + altCor*cosHA;
*HA1 =HA +(h1+PDh+DOh+TFh);
*Dec1=Dec+(d1+DFd+TFd);
// improved guess at instrument HA,Dec
h=*HA1/Rad;
d=*Dec1/Rad;
}
} else {
// just ignore the the correction if right on the pole
*HA1 =HA;
*Dec1=Dec;
}
// finally, apply the index offsets
*HA1=*HA1-ax1Cor;
*Dec1=*Dec1-ax2Cor*-p;
}
// takes the instrument equatorial coordinates and applies corrections to arrive at topocentric refracted coordinates
void TGeoAlign::instrToEqu(double HA, double Dec, double *HA1, double *Dec1, int PierSide) {
double p=1.0; if (PierSide == PierSideWest) p=-1.0;
HA =HA +ax1Cor;
Dec=Dec+ax2Cor*-p;
if (Dec > 90.0) Dec=90.0;
if (Dec < -90.0) Dec=-90.0;
// breaks-down near the pole (limited to > 1' from pole)
if (fabs(Dec) < 89.98333333) {
double h=HA/Rad;
double d=Dec/Rad;
double sinDec=sin(d);
double cosDec=cos(d);
double sinHA =sin(h);
double cosHA =cos(h);
// ------------------------------------------------------------
// misalignment due to tube/optics not being perp. to Dec axis
// negative numbers are further (S) from the NCP, swing to the
// equator and the effect on declination is 0. At the SCP it
// becomes a (N) offset. Unchanged with meridian flips.
// expressed as a correction to the Polar axis misalignment
double DOh=doCor*(1.0/cosDec)*p;
// as the above offset becomes zero near the equator, the affect
// works on HA instead. meridian flips affect this in HA
double PDh=-pdCor*(sinDec/cosDec)*p;
#if MOUNT_TYPE == FORK
// Fork flex
double DFd=dfCor*cosHA;
#else
// Axis flex
double DFd=-dfCor*(cosLat*cosHA+sinLat*(sinDec/cosDec));
#endif
// Tube flex
double TFh=tfCor*(cosLat*sinHA*(1.0/cosDec));
double TFd=tfCor*(cosLat*cosHA-sinLat*cosDec);
// ------------------------------------------------------------
// polar misalignment
double h1=-azmCor*cosHA*(sinDec/cosDec) + altCor*sinHA*(sinDec/cosDec);
double d1=+azmCor*sinHA + altCor*cosHA;
*HA1 =HA -(h1+PDh+DOh+TFh);
*Dec1=Dec-(d1+DFd+TFd);
} else {
// just ignore the the correction if right on the pole
*HA1=HA;
*Dec1=Dec;
}
while (*HA1 > 180.0) *HA1-=360.0;
while (*HA1 < -180.0) *HA1+=360.0;
if (*Dec1 > 90.0) *Dec1=90.0;
if (*Dec1 < -90.0) *Dec1=-90.0;
}
#endif