/*--------------------------------------------------------------------
 *
 *	Copyright (c) 1991-2024 by the GMT Team (https://www.generic-mapping-tools.org/team.html)
 *	See LICENSE.TXT file for copying and redistribution conditions.
 *
 *	This program is free software; you can redistribute it and/or modify
 *	it under the terms of the GNU Lesser General Public License as published by
 *	the Free Software Foundation; version 3 or 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 Lesser General Public License for more details.
 *
 *	Contact info: www.generic-mapping-tools.org
 *--------------------------------------------------------------------*/
/*
 * Brief synopsis: Compute the three components of earthtides as time-series or grids.
 * Optionally compute also Sun and Moon position in lon,lat
 *
 * Author:	Dennis Milbert (solid.f http://geodesyworld.github.io/SOFTS/solid.htm)
 *		Joaquim Luis (Translated to C and integrated in GMT)
 * Date:	12-JUN-2018
 * Version:	6 API
 */

#include "gmt_dev.h"
#include "longopt/earthtide_inc.h"

#define THIS_MODULE_CLASSIC_NAME	"earthtide"
#define THIS_MODULE_MODERN_NAME	"earthtide"
#define THIS_MODULE_LIB		"geodesy"
#define THIS_MODULE_PURPOSE	"Compute grids or time-series of solid Earth tides"
#define THIS_MODULE_KEYS	">D},GG),>DL,>DS"
#define THIS_MODULE_NEEDS	"R"
#define THIS_MODULE_OPTIONS	"-:RVbor" GMT_ADD_x_OPT

#define EARTH_RAD 6378137.0		// GRS80
#define ECC2 0.00669438002290341574957

enum earthtide_mode {
	X_COMP = 0,
	Y_COMP,
	Z_COMP,
	N_COMPS
};

struct EARTHTIDE_CTRL {
	struct EARTHTIDE_C {	/* -Cx/y */
		bool active;
		bool selected[N_COMPS];
		int n_selected;
	} C;
	struct EARTHTIDE_I {	/* -I (for checking only) */
		bool active;
	} I;
	struct EARTHTIDE_L {	/* -Cx/y */
		bool active;
		double x, y;
	} L;
	struct EARTHTIDE_S {	/* -S[<datum>] */
		bool active;
		struct GMT_DATUM datum;	/* Contains a, f, xyz[3] */
	} S;
	struct EARTHTIDE_G {	/* -G<file> */
		bool active;
		bool do_north, do_east, do_up;
		int  n;			/* Number of output grids specified via -G */
		char *file[N_COMPS];	/* Only first is used for commandline but API may need many */
	} G;
	struct EARTHTIDE_T {	/* -T[] */
		bool active;
		bool one_time;
		double time, start, stop;
		struct GMT_ARRAY T;
	} T;
};

static void *New_Ctrl (struct GMT_CTRL *GMT) {	/* Allocate and initialize a new control structure */
	struct EARTHTIDE_CTRL *C;

	C = gmt_M_memory (GMT, NULL, 1, struct EARTHTIDE_CTRL);

	/* Initialize values whose defaults are not 0/false/NULL */
	return (C);
}

static void Free_Ctrl (struct GMT_CTRL *GMT, struct EARTHTIDE_CTRL *C) {	/* Deallocate control structure */
	if (!C) return;
	for (unsigned int k = 0; k < N_COMPS; k++)
		if (C->G.file[k]) gmt_M_str_free (C->G.file[k]);
	gmt_free_array (GMT, & (C->T.T));
	gmt_M_free (GMT, C);
}

struct {
	int mjd0;
} mjdoff_;

#define mjdoff_1 mjdoff_

GMT_LOCAL double earthtide_d_mod (const double x, const double y) {
	double quotient;
	if ( (quotient = x / y) >= 0)
		quotient = floor (quotient);
	else
		quotient = -floor (-quotient);
	return (x - y * quotient );
}

/* ----------------------------------------------------------------------- */
GMT_LOCAL double earthtide_getutcmtai (double tsec, bool *leapflag) {

	int mjd0t;
	double ttsec, tai_utc = 0;

	/*  get utc - tai (s) */
	/*  "Julian Date Converter" */
	/*  http://aa.usno.navy.mil/data/docs/JulianDate.php */
	/*  or https://www.aavso.org/jd-calculator */
	/*  parameter (MJDUPPER=60306)    !*** upper limit, leap second table, 28 December 2023 */
	/* upper limit, leap second table, */
	/* lower limit, leap second table, */
	/* leap second table limit flag */
	/* leap second table limit flag */
	/* clone for tests (and do any rollover) */
	ttsec = tsec;
	mjd0t = mjdoff_1.mjd0;

	while (ttsec >= 86400.) {
		ttsec += -86400.;
		mjd0t++;
	}

	while (ttsec < 0) {
		ttsec += 86400.;
		mjd0t--;
	}

	/*  test upper table limit (upper limit set by bulletin C memos) */
	if (mjd0t > 60306) {
		*leapflag = true;		/* true means flag *IS* raised */
		return -37;				/* return the upper table value */
	}
	else if (mjd0t < 41317) {	/*  test lower table limit */
		*leapflag = true;		/* true means flag *IS* raised */
		return -10;				/* return the lower table value */
	}

	/*  http://maia.usno.navy.mil/ser7/tai-utc.dat */
	/* 1972 JAN  1 =JD 2441317.5  TAI-UTC=  10.0s */
	/* 1972 JUL  1 =JD 2441499.5  TAI-UTC=  11.0s */
	/* 1973 JAN  1 =JD 2441683.5  TAI-UTC=  12.0s */
	/* 1974 JAN  1 =JD 2442048.5  TAI-UTC=  13.0s */
	/* 1975 JAN  1 =JD 2442413.5  TAI-UTC=  14.0s */
	/* 1976 JAN  1 =JD 2442778.5  TAI-UTC=  15.0s */
	/* 1977 JAN  1 =JD 2443144.5  TAI-UTC=  16.0s */
	/* 1978 JAN  1 =JD 2443509.5  TAI-UTC=  17.0s */
	/* 1979 JAN  1 =JD 2443874.5  TAI-UTC=  18.0s */
	/* 1980 JAN  1 =JD 2444239.5  TAI-UTC=  19.0s */
	/* 1981 JUL  1 =JD 2444786.5  TAI-UTC=  20.0s */
	/* 1982 JUL  1 =JD 2445151.5  TAI-UTC=  21.0s */
	/* 1983 JUL  1 =JD 2445516.5  TAI-UTC=  22.0s */
	/* 1985 JUL  1 =JD 2446247.5  TAI-UTC=  23.0s */
	/* 1988 JAN  1 =JD 2447161.5  TAI-UTC=  24.0s */
	/* 1990 JAN  1 =JD 2447892.5  TAI-UTC=  25.0s */
	/* 1991 JAN  1 =JD 2448257.5  TAI-UTC=  26.0s */
	/* 1992 JUL  1 =JD 2448804.5  TAI-UTC=  27.0s */
	/* 1993 JUL  1 =JD 2449169.5  TAI-UTC=  28.0s */
	/* 1994 JUL  1 =JD 2449534.5  TAI-UTC=  29.0s */
	/* 1996 JAN  1 =JD 2450083.5  TAI-UTC=  30.0s */
	/* 1997 JUL  1 =JD 2450630.5  TAI-UTC=  31.0s */
	/* 1999 JAN  1 =JD 2451179.5  TAI-UTC=  32.0s */
	/* 2006 JAN  1 =JD 2453736.5  TAI-UTC=  33.0s */
	/* 2009 JAN  1 =JD 2454832.5  TAI-UTC=  34.0s */
	/* 2012 JUL  1 =JD 2456109.5  TAI-UTC=  35.0s */
	/* 2015 JUL  1 =JD 2457204.5  TAI-UTC=  36.0s */
	/* 2017 JAN  1 =JD 2457754.5  TAI-UTC=  37.0s */
	/*  other leap second references at: */
	/*  http://hpiers.obspm.fr/eoppc/bul/bulc/Leap_Second_History.dat */
	/*  http://hpiers.obspm.fr/eoppc/bul/bulc/bulletinc.dat */
	/* test against newest leaps first */
	if (mjd0t >= 57754)			/* 2017 JAN 1 = 57754 */
		tai_utc = 37.;
	else if (mjd0t >= 57204)    /* 2015 JUL 1 = 57204 */
		tai_utc = 36.;
	else if (mjd0t >= 56109)    /* 2012 JUL 1 = 56109 */
		tai_utc = 35.;
	else if (mjd0t >= 54832)    /* 2009 JAN 1 = 54832 */
		tai_utc = 34.;
	else if (mjd0t >= 53736)    /* 2006 JAN 1 = 53736 */
		tai_utc = 33.;
	else if (mjd0t >= 51179)    /* 1999 JAN 1 = 51179 */
		tai_utc = 32.;
	else if (mjd0t >= 50630)    /* 1997 JUL 1 = 50630 */
		tai_utc = 31.;
	else if (mjd0t >= 50083)    /* 1996 JAN 1 = 50083 */
		tai_utc = 30.;
	else if (mjd0t >= 49534)    /* 1994 JUL 1 = 49534 */
		tai_utc = 29.;
	else if (mjd0t >= 49169)    /* 1993 JUL 1 = 49169 */
		tai_utc = 28.;
	else if (mjd0t >= 48804)    /* 1992 JUL 1 = 48804 */
		tai_utc = 27.;
	else if (mjd0t >= 48257)    /* 1991 JAN 1 = 48257 */
		tai_utc = 26.;
	else if (mjd0t >= 47892)    /* 1990 JAN 1 = 47892 */
		tai_utc = 25.;
	else if (mjd0t >= 47161)    /* 1988 JAN 1 = 47161 */
		tai_utc = 24.;
	else if (mjd0t >= 46247)    /* 1985 JUL 1 = 46247 */
		tai_utc = 23.;
	else if (mjd0t >= 45516)    /* 1983 JUL 1 = 45516 */
		tai_utc = 22.;
	else if (mjd0t >= 45151)    /* 1982 JUL 1 = 45151 */
		tai_utc = 21.;
	else if (mjd0t >= 44786)    /* 1981 JUL 1 = 44786 */
		tai_utc = 20.;
	else if (mjd0t >= 44239)    /* 1980 JAN 1 = 44239 */
		tai_utc = 19.;
	else if (mjd0t >= 43874)    /* 1979 JAN 1 = 43874 */
		tai_utc = 18.;
	else if (mjd0t >= 43509)    /* 1978 JAN 1 = 43509 */
		tai_utc = 17.;
	else if (mjd0t >= 43144)    /* 1977 JAN 1 = 43144 */
		tai_utc = 16.;
	else if (mjd0t >= 42778)    /* 1976 JAN 1 = 42778 */
		tai_utc = 15.;
	else if (mjd0t >= 42413)    /* 1975 JAN 1 = 42413 */
		tai_utc = 14.;
	else if (mjd0t >= 42048)    /* 1974 JAN 1 = 42048 */
		tai_utc = 13.;
	else if (mjd0t >= 41683)    /* 1973 JAN 1 = 41683 */
		tai_utc = 12.;
	else if (mjd0t >= 41499)    /* 1972 JUL 1 = 41499 */
		tai_utc = 11.;
	else if (mjd0t >= 41317)    /* 1972 JAN 1 = 41317 */
		tai_utc = 10.;
	/* return utc - tai (in seconds) */
	return -tai_utc;
}

/* *********************************************************************** */
/* ** new supplemental time functions ************************************ */
/* *********************************************************************** */
/* ----------------------------------------------------------------------- */
GMT_LOCAL double earthtide_tai2tt (double ttai) {
	/*  convert tai (sec) to terrestrial time (sec) */
	/*  http://tycho.usno.navy.mil/systime.html */
	return ttai + 32.184;
}

/* ----------------------------------------------------------------------- */
#if 0
GMT_LOCAL double earthtide_gps2tai (double tgps) {
	/*  convert gps time (sec) to tai (sec) */
	/*  http://leapsecond.com/java/gpsclock.htm */
	/*  http://tycho.usno.navy.mil/leapsec.html */
	return tgps + 19;
}
/* ----------------------------------------------------------------------- */
GMT_LOCAL double earthtide_gps2ttt (double tgps) {
	double ttai;

	/* convert gps time (sec) to terrestrial time (sec) */
	ttai = earthtide_gps2tai (tgps);
	return earthtide_tai2tt (ttai);
}
#endif
/* ----------------------------------------------------------------------- */
GMT_LOCAL double earthtide_utc2tai (double tutc, bool *leapflag) {
	/* convert utc (sec) to tai (sec) */
	return tutc - earthtide_getutcmtai (tutc, leapflag);
}

/* ----------------------------------------------------------------------- */
GMT_LOCAL double earthtide_utc2ttt (double tutc, bool *leapflag) {
	double ttai;

	/* convert utc (sec) to terrestrial time (sec) */
	ttai = earthtide_utc2tai (tutc, leapflag);
	return earthtide_tai2tt (ttai);
}

/* ----------------------------------------------------------------------- */
GMT_LOCAL void earthtide_sprod (double *x, double *y, double *scal, double *r1, double *r2) {
	/*  computation of the scalar-product of two vectors and their norms */
	/*  input:   x (i),i=1,2,3  -- components of vector x */
	/*           y (i),i=1,2,3  -- components of vector y */
	/*  output:  scal          -- scalar product of x and y */
	/*           r1,r2         -- lengths of the two vectors x and y */

	*r1 = sqrt (x[0] * x[0] + x[1] * x[1] + x[2] * x[2]);
	*r2 = sqrt (y[0] * y[0] + y[1] * y[1] + y[2] * y[2]);
	*scal =    x[0] * y[0] + x[1] * y[1] + x[2] * y[2];
}

/* ----------------------------------------------------------------------- */
GMT_LOCAL double earthtide_enorm8 (double *a) {
	/* compute euclidean norm of a vector (of length 3) */
	return sqrt (a[0] * a[0] + a[1] * a[1] + a[2] * a[2]);
}

/* ----------------------------------------------------------------------- */
GMT_LOCAL void earthtide_st1idiu (double *xsta, double *xsun, double *xmon, double fac2sun, double fac2mon, double *xcorsta) {
	/* this subroutine gives the out-of-phase corrections induced by */
	/* mantle inelasticity in the diurnal band */
	/*  input: xsta,xsun,xmon,fac2sun,fac2mon */
	/* output: xcorsta */
	double dhi = -0.0025;
	double dli = -7e-4;
	double de, dn, dr, rsta, rmon, rsun, cosla, demon, sinla, dnmon, desun, drmon, dnsun, drsun;
	double cosphi, sinphi, cos2phi, inv_rsun2, inv_rmon2;

	rsta = earthtide_enorm8 (&xsta[0]);
	sinphi = xsta[2] / rsta;
	cosphi = sqrt (xsta[0] * xsta[0] + xsta[1] * xsta[1]) / rsta;
	cos2phi = cosphi * cosphi - sinphi * sinphi;
	sinla = xsta[1] / cosphi / rsta;
	cosla = xsta[0] / cosphi / rsta;
	rmon = earthtide_enorm8 (&xmon[0]);
	rsun = earthtide_enorm8 (&xsun[0]);
	inv_rsun2 = 1 / (rsun * rsun);
	inv_rmon2 = 1 / (rmon * rmon);
	drsun = dhi * -3 * sinphi  * cosphi  * fac2sun * xsun[2]  * (xsun[0] * sinla - xsun[1] * cosla) * inv_rsun2;
	drmon = dhi * -3 * sinphi  * cosphi  * fac2mon * xmon[2]  * (xmon[0] * sinla - xmon[1] * cosla) * inv_rmon2;
	dnsun = dli * -3 * cos2phi * fac2sun * xsun[2] * (xsun[0] * sinla - xsun[1] * cosla) * inv_rsun2;
	dnmon = dli * -3 * cos2phi * fac2mon * xmon[2] * (xmon[0] * sinla - xmon[1] * cosla) * inv_rmon2;
	desun = dli * -3 * sinphi  * fac2sun * xsun[2] * (xsun[0] * cosla + xsun[1] * sinla) * inv_rsun2;
	demon = dli * -3 * sinphi  * fac2mon * xmon[2] * (xmon[0] * cosla + xmon[1] * sinla) * inv_rmon2;
	dr = drsun + drmon;
	dn = dnsun + dnmon;
	de = desun + demon;
	xcorsta[0] = dr * cosla * cosphi - de * sinla - dn * sinphi * cosla;
	xcorsta[1] = dr * sinla * cosphi + de * cosla - dn * sinphi * sinla;
	xcorsta[2] = dr * sinphi + dn * cosphi;
}

/* ----------------------------------------------------------------------- */
GMT_LOCAL void earthtide_st1isem (double *xsta, double *xsun, double *xmon, double fac2sun, double fac2mon, double *xcorsta) {
	/* this subroutine gives the out-of-phase corrections induced by */
	/* mantle inelasticity in the diurnal band */
	/*  input: xsta,xsun,xmon,fac2sun,fac2mon */
	/* output: xcorsta */

	const double dhi = -0.0022;
	const double dli = -7e-4;
	double costwola, sintwola, de, dn, dr, rsta, rmon, rsun, cosla, demon, sinla, dnmon, desun, drmon, dnsun, drsun;
	double cosphi, sinphi, cosphi2, inv_rsun2, inv_rmon2, dif_xsun2, dif_xmon2, t;

	rsta = earthtide_enorm8 (&xsta[0]);
	sinphi = xsta[2] / rsta;
	cosphi = sqrt (xsta[0] * xsta[0] + xsta[1] * xsta[1]) / rsta;
	cosphi2 = cosphi * cosphi;
	sinla = xsta[1] / cosphi / rsta;
	cosla = xsta[0] / cosphi / rsta;
	costwola = cosla * cosla - sinla * sinla;
	sintwola = cosla * 2 * sinla;
	rmon = earthtide_enorm8 (&xmon[0]);
	rsun = earthtide_enorm8 (&xsun[0]);
	inv_rsun2 = 1 / (rsun * rsun);
	inv_rmon2 = 1 / (rmon * rmon);
	dif_xsun2 = xsun[0] * xsun[0] - xsun[1] * xsun[1];
	dif_xmon2 = xmon[0] * xmon[0] - xmon[1] * xmon[1];
	t = dhi * -0.75 * cosphi2;
	drsun = t * fac2sun * (dif_xsun2 * sintwola - xsun[0] * 2 * xsun[1] * costwola) * inv_rsun2;
	drmon = t * fac2mon * (dif_xmon2 * sintwola - xmon[0] * 2 * xmon[1] * costwola) * inv_rmon2;
	t = dli * 1.5 * sinphi;
	dnsun = t * cosphi * fac2sun * (dif_xsun2 * sintwola - xsun[0] * 2 * xsun[1] * costwola) * inv_rsun2;
	dnmon = t * cosphi * fac2mon * (dif_xmon2 * sintwola - xmon[0] * 2 * xmon[1] * costwola) * inv_rmon2;
	t = dli * -1.5 * cosphi;
	desun = t * fac2sun * (dif_xsun2 * costwola + xsun[0] * 2 * xsun[1] * sintwola) * inv_rsun2;
	demon = t * fac2mon * (dif_xmon2 * costwola + xmon[0] * 2 * xmon[1] * sintwola) * inv_rmon2;
	dr = drsun + drmon;
	dn = dnsun + dnmon;
	de = desun + demon;
	xcorsta[0] = dr * cosla * cosphi - de * sinla - dn * sinphi * cosla;
	xcorsta[1] = dr * sinla * cosphi + de * cosla - dn * sinphi * sinla;
	xcorsta[2] = dr * sinphi + dn * cosphi;
}

/* ----------------------------------------------------------------------- */
GMT_LOCAL void earthtide_st1l1 (double *xsta, double *xsun, double *xmon, double fac2sun, double fac2mon, double *xcorsta) {
	/* this subroutine gives the corrections induced by the latitude dependence */
	/* given by l^ (1) in mahtews et al (1991) */
	/*  input: xsta,xsun,xmon,fac3sun,fac3mon */
	/* output: xcorsta */

	double l1d = .0012;
	double l1sd = .0024;
	double costwola, sintwola, l1, de, dn, rsta, rmon, rsun, cosla, demon, sinla, dnmon, desun, dnsun;
	double cosphi, sinphi, cosphi2, sinphi2, inv_rsun2, inv_rmon2, dif_xsun2, dif_xmon2, t;

	rsta = earthtide_enorm8 (&xsta[0]);
	sinphi = xsta[2] / rsta;
	cosphi = sqrt (xsta[0] * xsta[0] + xsta[1] * xsta[1]) / rsta;
	sinla = xsta[1] / cosphi / rsta;
	cosla = xsta[0] / cosphi / rsta;
	rmon = earthtide_enorm8 (&xmon[0]);
	rsun = earthtide_enorm8 (&xsun[0]);
	/* ** for the diurnal band */
	l1 = l1d;
	sinphi2 = sinphi * sinphi;
	cosphi2 = cosphi * cosphi;
	inv_rsun2 = 1 / (rsun * rsun);
	inv_rmon2 = 1 / (rmon * rmon);
	dnsun = -l1 * sinphi2 * fac2sun * xsun[2] * (xsun[0] * cosla + xsun[1] * sinla) * inv_rsun2;
	dnmon = -l1 * sinphi2 * fac2mon * xmon[2] * (xmon[0] * cosla + xmon[1] * sinla) * inv_rmon2;
	t = l1 * sinphi * (cosphi2 - sinphi2);
	desun = t * fac2sun * xsun[2] * (xsun[0] * sinla - xsun[1] * cosla) * inv_rsun2;
	demon = t * fac2mon * xmon[2] * (xmon[0] * sinla - xmon[1] * cosla) * inv_rmon2;
	de = (desun + demon) * 3.;
	dn = (dnsun + dnmon) * 3.;
	xcorsta[0] = -de * sinla - dn * sinphi * cosla;
	xcorsta[1] =  de * cosla - dn * sinphi * sinla;
	xcorsta[2] =  dn * cosphi;
	/* ** for the semi-diurnal band */
	l1 = l1sd;
	costwola = cosla * cosla - sinla * sinla;
	sintwola = cosla * 2 * sinla;
	dif_xsun2 = xsun[0] * xsun[0] - xsun[1] * xsun[1];
	dif_xmon2 = xmon[0] * xmon[0] - xmon[1] * xmon[1];
	t = -l1 / 2 * sinphi  * cosphi;
	dnsun = t * fac2sun * (dif_xsun2 * costwola + xsun[0] * 2 * xsun[1] * sintwola) * inv_rsun2;
	dnmon = t * fac2mon * (dif_xmon2 * costwola + xmon[0] * 2 * xmon[1] * sintwola) * inv_rmon2;
	t = -l1 / 2 * sinphi2 * cosphi;
	desun = t * fac2sun * (dif_xsun2 * sintwola - xsun[0] * 2 * xsun[1] * costwola) * inv_rsun2;
	demon = t * fac2mon * (dif_xmon2 * sintwola - xmon[0] * 2 * xmon[1] * costwola) * inv_rmon2;
	de = (desun + demon) * 3;
	dn = (dnsun + dnmon) * 3;
	xcorsta[0] = xcorsta[0] - de * sinla - dn * sinphi * cosla;
	xcorsta[1] = xcorsta[1] + de * cosla - dn * sinphi * sinla;
	xcorsta[2] += dn * cosphi;
}

/* ----------------------------------------------------------------------- */
GMT_LOCAL void earthtide_step2diu (double *xsta, double fhr, double t, double *xcorsta) {
	/* last change:  vd   17 may 00   1:20 pm */
	/* these are the subroutines for the step2 of the tidal corrections. */
	/* they are called to account for the frequency dependence */
	/* of the love numbers. */

	static double datdi[279]	/* was [9][31] */ = { -3.,0.,2.,0.,0.,
		-.01,-.01,0.,0.,-3.,2.,0.,0.,0.,-.01,-.01,0.,0.,-2.,0.,1.,-1.,0.,
		-.02,-.01,0.,0.,-2.,0.,1.,0.,0.,-.08,0.,.01,.01,-2.,2.,-1.,0.,0.,
		-.02,-.01,0.,0.,-1.,0.,0.,-1.,0.,-.1,0.,0.,0.,-1.,0.,0.,0.,0.,
		-.51,0.,-.02,.03,-1.,2.,0.,0.,0.,.01,0.,0.,0.,0.,-2.,1.,0.,0.,.01,
		0.,0.,0.,0.,0.,-1.,0.,0.,.02,.01,0.,0.,0.,0.,1.,0.,0.,.06,0.,0.,
		0.,0.,0.,1.,1.,0.,.01,0.,0.,0.,0.,2.,-1.,0.,0.,.01,0.,0.,0.,1.,
		-3.,0.,0.,1.,-.06,0.,0.,0.,1.,-2.,0.,1.,0.,.01,0.,0.,0.,1.,-2.,0.,
		0.,0.,-1.23,-.07,.06,.01,1.,-1.,0.,0.,-1.,.02,0.,0.,0.,1.,-1.,0.,
		0.,1.,.04,0.,0.,0.,1.,0.,0.,-1.,0.,-.22,.01,.01,0.,1.,0.,0.,0.,0.,
		12.,-.78,-.67,-.03,1.,0.,0.,1.,0.,1.73,-.12,-.1,0.,1.,0.,0.,2.,0.,
		-.04,0.,0.,0.,1.,1.,0.,0.,-1.,-.5,-.01,.03,0.,1.,1.,0.,0.,1.,.01,
		0.,0.,0.,1.,1.,0.,1.,-1.,-.01,0.,0.,0.,1.,2.,-2.,0.,0.,-.01,0.,0.,
		0.,1.,2.,0.,0.,0.,-.11,.01,.01,0.,2.,-2.,1.,0.,0.,-.01,0.,0.,0.,
		2.,0.,-1.,0.,0.,-.02,.02,0.,.01,3.,0.,0.,0.,0.,0.,.01,0.,.01,3.,
		0.,0.,1.,0.,0.,.01,0.,0. };

	int i, j;
	double h, t2, t3, cosphi2, sinphi2, sin_tf, cos_tf;
	double p, s, de, dn, dr, pr, ps, zla, tau, zns, rsta, cosla, sinla, thetaf, cosphi, sinphi;

	/* ** note, following table is derived from dehanttideinelMJD.f (2000oct30 16:10) */
	/* ** has minor differences from that of dehanttideinel.f (2000apr17 14:10) */
	/* ** D.M. edited to strictly follow published table 7.5a (2006aug08 13:46) */
	/* ** cf. table 7.5a of IERS conventions 2003 (TN.32, pg.82) */
	/* ** columns are s,h,p,N',ps, dR (ip),dR (op),dT (ip),dT (op) */
	/* ** units of mm */
	/* ****----------------------------------------------------------------------- */
	/* ***** -2., 0., 1., 0., 0.,-0.08,-0.05, 0.01,-0.02,      !*** original entry */
	/* ****----------------------------------------------------------------------- */
	/* ****----------------------------------------------------------------------- */
	/* ***** -1., 0., 0.,-1., 0.,-0.10,-0.05, 0.0 ,-0.02,      !*** original entry */
	/* ****----------------------------------------------------------------------- */
	/* ***** -1., 0., 0., 0., 0.,-0.51,-0.26,-0.02,-0.12,      !*** original entry */
	/* ****----------------------------------------------------------------------- */
	/* ****----------------------------------------------------------------------- */
	/* *****  0., 0., 1., 0., 0., 0.06, 0.02, 0.0 , 0.01,      !*** original entry */
	/* ****----------------------------------------------------------------------- */
	/* ****----------------------------------------------------------------------- */
	/* *****  1.,-2., 0., 0., 0.,-1.23,-0.05, 0.06,-0.06,      !*** original entry */
	/* ****----------------------------------------------------------------------- */
	/* ****----------------------------------------------------------------------- */
	/* *****  1., 0., 0., 0., 0.,12.02,-0.45,-0.66, 0.17,      !*** original entry */
	/* ****----------------------------------------------------------------------- */
	/* *****  1., 0., 0., 1., 0., 1.73,-0.07,-0.10, 0.02,      !*** original entry */
	/* ****----------------------------------------------------------------------- */
	/* ****----------------------------------------------------------------------- */
	/* *****  1., 1., 0., 0.,-1.,-0.50, 0.0 , 0.03, 0.0,       !*** original entry */
	/* ****----------------------------------------------------------------------- */
	/* ****----------------------------------------------------------------------- */
	/* *****  0., 1., 0., 1.,-1.,-0.01, 0.0 , 0.0 , 0.0,       !*** original entry */
	/* ****----------------------------------------------------------------------- */
	/* ****----------------------------------------------------------------------- */
	/* *****  1., 2., 0., 0., 0.,-0.12, 0.01, 0.01, 0.0,       !*** original entry */
	/* ****----------------------------------------------------------------------- */
	/* *** table 7.5a */
	/* *** v.dehant 2 */
	t2 = t * t;
	t3 = t * t2;
	s = 218.31664563 + 481267.88194 * t - .0014663889 * t2 + 1.85139e-6 * t3;
	tau = fhr * 15. + 280.4606184 + t * 36000.7700536 + t * 3.8793e-4 * t - t3 * 2.58e-8 - s;
	pr = t * 1.396971278f + t * 3.08889e-4f * t + t3 * 2.1e-8f + t2 * 7e-9f;
	s += pr;
	h = t * 36000.7697489 + 280.46645 + t * 3.0322222e-4 * t + t3 * 2e-8f - t2 * 6.54e-9f;
	p = t * 4069.01363525 + 83.35324312 - t * .01032172222 * t - t3 * 1.24991e-5 + t2 * 5.263e-8;
	zns = t * 1934.13626197 + 234.95544499 - t * .00207561111 * t - t3 * 2.13944e-6 + t2 * 1.65e-8;
	ps = t * 1.71945766667 + 282.93734098 + t * 4.5688889e-4 * t - t3 * 1.778e-8 - t2 * 3.34e-9;
	/* ** reduce angles to between 0 and 360 */
	s = earthtide_d_mod (s, 360.);
	tau = earthtide_d_mod (tau, 360.);
	h = earthtide_d_mod (h, 360.);
	p = earthtide_d_mod (p, 360.);
	zns = earthtide_d_mod (zns, 360.);
	ps = earthtide_d_mod (ps, 360.);
	rsta = sqrt (xsta[0] * xsta[0] + xsta[1] * xsta[1] + xsta[2] * xsta[2]);
	sinphi = xsta[2] / rsta;
	cosphi = sqrt (xsta[0] * xsta[0] + xsta[1] * xsta[1]) / rsta;
	sinphi2 = sinphi * sinphi;
	cosphi2 = cosphi * cosphi;
	cosla = xsta[0] / cosphi / rsta;
	sinla = xsta[1] / cosphi / rsta;
	zla = atan2 (xsta[1], xsta[0]);
	for (i = 0; i < 3; i++) xcorsta[i] = 0;

	for (j = 1; j <= 31; j++) {
		thetaf = (tau + datdi[j * 9 - 9] * s + datdi[j * 9 - 8] * h + datdi[j * 9 - 7] * p + datdi[j * 9 - 6] * zns + datdi[j * 9 - 5] * ps) * D2R + zla;
		sin_tf = sin (thetaf);		cos_tf = cos (thetaf);
		dr     = datdi[j * 9 - 4] * 2 * sinphi * cosphi * sin_tf + datdi[j * 9 - 3] * 2 * sinphi * cosphi * cos_tf;
		dn     = datdi[j * 9 - 2] * (cosphi2 - sinphi2) * sin_tf + datdi[j * 9 - 1] * (cosphi2 - sinphi2) * cos_tf;
		/* following correction by V.Dehant to match eq.16b, p.81, 2003 Conventions */
		/* de=datdi (8,j)*sinphi*cos (thetaf+zla)+ */
		de = datdi[j * 9 - 2] * sinphi * cos_tf - datdi[j * 9 - 1] * sinphi * sin_tf;
		xcorsta[0] += (dr * cosla * cosphi - de * sinla - dn * sinphi * cosla);
		xcorsta[1] += (dr * sinla * cosphi + de * cosla - dn * sinphi * sinla);
		xcorsta[2] += (dr * sinphi + dn * cosphi);
	}

	for (i = 0; i < 3; ++i) xcorsta[i] /= 1e3;
}

/* ----------------------------------------------------------------------- */
GMT_LOCAL void earthtide_step2lon (double *xsta, double t, double *xcorsta) {
	/* cf. table 7.5b of IERS conventions 2003 (TN.32, pg.82) */
	/* columns are s,h,p,N',ps, dR (ip),dT (ip),dR (op),dT (op) */
	/* IERS cols.= s,h,p,N',ps, dR (ip),dR (op),dT (ip),dT (op) */
	/* units of mm */

	static double datdi[45]	/* was [9][5] */ = { 0.,0.,0.,1.,0.,.47,.23,
		.16,.07,0.,2.,0.,0.,0.,-.2,-.12,-.11,-.05,1.,0.,-1.,0.,0.,-.11,
		-.08,-.09,-.04,2.,0.,0.,0.,0.,-.13,-.11,-.15,-.07,2.,0.,0.,1.,0.,
		-.05,-.05,-.06,-.03 };

	int i, j;
	double h, t2, t3, t4;
	double p, s, de, dn, dr, pr, ps, zns, rsta, cosla, sinla, thetaf, cosphi, sinphi;

	t2 = t * t;		t3 = t * t2;		t4 = t2 * t2;
	s = 218.31664563 + 481267.88194 * t - .0014663889 * t2 + 1.85139e-6 * t3;
	pr = t * 1.396971278f + t2 * 3.08889e-4f + t3 * 2.1e-8f + t4 * 7e-9f;
	s += pr;
	h   = t * 36000.7697489 + 280.46645    + t2 * 3.0322222e-4 + t3 * 2e-8f      - t4 * 6.54e-9f;
	p   = t * 4069.01363525 + 83.35324312  - t2 * .01032172222 - t3 * 1.24991e-5 + t4 * 5.263e-8;
	zns = t * 1934.13626197 + 234.95544499 - t2 * .00207561111 - t3 * 2.13944e-6 + t4 * 1.65e-8;
	ps = t * 1.71945766667 + 282.93734098  + t2 * 4.5688889e-4 - t3 * 1.778e-8   - t4 * 3.34e-9;
	rsta = sqrt (xsta[0] * xsta[0] + xsta[1] * xsta[1] + xsta[2] * xsta[2]);
	sinphi = xsta[2] / rsta;
	cosphi = sqrt (xsta[0] * xsta[0] + xsta[1] * xsta[1]) / rsta;
	cosla = xsta[0] / cosphi / rsta;
	sinla = xsta[1] / cosphi / rsta;
	/* ** reduce angles to between 0 and 360 */
	s = earthtide_d_mod (s, 360.);
	/* **** tau=dmod (tau,360.d0)       !*** tau not used here--09jul28 */
	h = earthtide_d_mod (h, 360.);
	p = earthtide_d_mod (p, 360.);
	zns = earthtide_d_mod (zns, 360.);
	ps = earthtide_d_mod (ps, 360.);
	for (i = 0; i < 3; i++) xcorsta[i] /= 1e3;

	/* **             1 2 3 4   5   6      7      8      9 */
	/* ** columns are s,h,p,N',ps, dR (ip),dT (ip),dR (op),dT (op) */
	for (j = 1; j <= 5; j++) {
		thetaf = (datdi[j * 9 - 9] * s + datdi[j * 9 - 8] * h + datdi[j * 9 - 7] * p + datdi[j * 9 - 6] * zns + datdi[j * 9 - 5] * ps) * D2R;
		dr = datdi[j * 9 - 4] * (sinphi * sinphi * 3 - 1) / 2. * cos (thetaf) + datdi[j * 9 - 2] * (sinphi * sinphi * 3 - 1) / 2. * sin (thetaf);
		dn = datdi[j * 9 - 3] * (cosphi * sinphi * 2) * cos (thetaf) + datdi[j * 9 - 1] * (cosphi * sinphi * 2) * sin (thetaf);
		de = 0.;
		xcorsta[0] += dr * cosla * cosphi - de * sinla - dn * sinphi * cosla;
		xcorsta[1] += dr * sinla * cosphi + de * cosla - dn * sinphi * sinla;
		xcorsta[2] += dr * sinphi + dn * cosphi;
	}
	for (i = 0; i < 3; i++) xcorsta[i] /= 1e3;
}

/* ------------------------------------------------------------------------------- */
GMT_LOCAL void earthtide_detide (double *xsta, int mjd, double fmjd, double *xsun, double *xmon, double *dxtide, bool *leapflag) {
	/* Computation of tidal corrections of station displacements caused
	 * by lunar and solar gravitational attraction.  UTC version.
	 * step 1 (here general degree 2 and 3 corrections +
	 *         call earthtide_st1idiu + call earthtide_st1isem + call earthtide_st1l1)
	 *   + step 2 (call earthtide_step2diu + call earthtide_step2lon + call step2idiu)
	 * It has been decided that the step 3 un-correction for permanent tide
	 * would *not* be applied in order to avoid jump in the reference frame
	 * (this step 3 must added in order to get the mean tide station position
	 * and to be conformed with the iag resolution.)
	 * inputs:
	 *   xsta (i),i=1,2,3   -- geocentric position of the station (ITRF/ECEF)
	 *   xsun (i),i=1,2,3   -- geoc. position of the sun (ECEF)
	 *   xmon (i),i=1,2,3   -- geoc. position of the moon (ECEF)
	 *   mjd,fmjd          -- modified julian day (and fraction) (in GPS time)
	 * ***old calling sequence*****************************************************
	 *   dmjd               -- time in mean julian date (including day fraction)
	 *   fhr=hr+zmin/60.+sec/3600.   -- hr in the day
	 * outputs:
	 *   dxtide (i),i=1,2,3           -- displacement vector (ITRF)
	 *   flag              -- leap second table limit flag, false:flag not raised
	 * Author iers 1996 :  V. Dehant, S. Mathews and J. Gipson
	 *    (test between two subroutines)
	 * Author iers 2000 :  V. Dehant, C. Bruyninx and S. Mathews
	 *    (test in the bernese program by C. Bruyninx)
	 * Created:  96/03/23 (see above)
	 * Modified from dehanttideinelMJD.f by Dennis Milbert 2006sep10
	 * Bug fix regarding fhr (changed calling sequence, too)
	 * Modified to reflect table 7.5a and b IERS Conventions 2003
	 * Modified to use TT time system to call step 2 functions
	 * Sign correction by V.Dehant to match eq.16b, p.81, Conventions
	 * applied by Dennis Milbert 2007may05
	 * UTC version by Dennis Milbert 2018june01
	 */

	int i;
	double h20 = .6078;
	double l20 = .0847;
	double h3 = .292;
	double l3 = .015;
	double re_over_rsun, re_over_rmon, re;
	double mass_ratio_moon, mass_ratio_sun, t, t2, h2, l2, fhr, scm, scs;
	double rsta, rmon, rsun, p2mon, p3mon, x2mon, x3mon, p2sun, p3sun, x2sun, x3sun, scmon;
	double scsun, cosphi, dmjdtt, fmjdtt, tsectt, fac2mon, fac3mon, fac2sun, fac3sun;
	double tsecutc, xcorsta[3], inv_rsta;

	/* nominal second degree and third degree love numbers and shida numbers */

	/* internal support for new calling sequence */
	/* first, convert UTC time into TT time (and, bring leapflag into variable) */
	tsecutc = fmjd * 86400.;			/* UTC time (sec of day) */
	tsectt = earthtide_utc2ttt (tsecutc, leapflag);			/* TT  time (sec of day) */
	fmjdtt = tsectt / 86400.;			/* TT  time (fract. day) */
	dmjdtt = mjd + fmjdtt;
	/*  commented line was live code in dehanttideinelMJD.f */
	/*  changed on the suggestion of Dr. Don Kim, UNB -- 09mar21 */
	/*  Julian date for 2000 January 1 00:00:00.0 UT is  JD 2451544.5 */
	/*  MJD         for 2000 January 1 00:00:00.0 UT is MJD   51544.0 */
	/*  t= (dmjdtt-51545.d0)/36525.d0                !*** days to centuries, TT */
	/*  float MJD in TT */
	t = (dmjdtt - 51544.) / 36525.;			/* days to centuries, TT */
	fhr = (dmjdtt - (int) dmjdtt) * 24.;	/* hours in the day, TT */
	/* ** scalar product of station vector with sun/moon vector */
	earthtide_sprod (&xsta[0], &xsun[0], &scs, &rsta, &rsun);
	earthtide_sprod (&xsta[0], &xmon[0], &scm, &rsta, &rmon);
	scsun = scs / rsta / rsun;
	scmon = scm / rsta / rmon;
	/* ** computation of new h2 and l2 */
	cosphi = sqrt (xsta[0] * xsta[0] + xsta[1] * xsta[1]) / rsta;
	t2 = (1. - cosphi * 1.5 * cosphi);
	h2 = h20 - t2 * 6e-4;
	l2 = l20 + t2 * 2e-4;
	/* ** p2-term */
	t2 = (h2 / 2. - l2) * 3;
	p2sun = t2 * scsun * scsun - h2 / 2.;
	p2mon = t2 * scmon * scmon - h2 / 2.;
	/* ** p3-term */
	t2 = (h3 - l3 * 3.) * 2.5;
	p3sun = t2 * (scsun * scsun * scsun) + (l3 - h3) * 1.5 * scsun;
	p3mon = t2 * (scmon * scmon * scmon) + (l3 - h3) * 1.5 * scmon;
	/* ** term in direction of sun/moon vector */
	x2sun = l2 * 3. * scsun;
	x2mon = l2 * 3. * scmon;
	x3sun = l3 * 1.5 * (scsun * 5 * scsun - 1);
	x3mon = l3 * 1.5 * (scmon * 5 * scmon - 1);
	/* ** factors for sun/moon */
	mass_ratio_sun = 332945.943062;
	mass_ratio_moon = 0.012300034;
	re = 6378136.55;
	re_over_rsun = re / rsun;
	fac2sun = mass_ratio_sun * re * re_over_rsun * re_over_rsun * re_over_rsun;
	re_over_rmon = re / rmon;
	fac2mon = mass_ratio_moon * re * re_over_rmon * re_over_rmon * re_over_rmon;
	fac3sun = fac2sun * re_over_rsun;
	fac3mon = fac2mon * re_over_rmon;
	/* ** total displacement */
	inv_rsta = 1 / rsta;
	for (i = 0; i < 3; i++) {
		t2 = xsta[i] * inv_rsta;
		dxtide[i] = fac2sun * (x2sun * xsun[i] / rsun + p2sun * t2) +
					fac2mon * (x2mon * xmon[i] / rmon + p2mon * t2) +
					fac3sun * (x3sun * xsun[i] / rsun + p3sun * t2) +
					fac3mon * (x3mon * xmon[i] / rmon + p3mon * t2);
	}
	xcorsta[0] = xcorsta[1] = xcorsta[2] = 0;
	/* ** corrections for the out-of-phase part of love numbers */
	/* **     (part h_2^ (0)i and l_2^ (0)i ) */
	/* ** first, for the diurnal band */
	earthtide_st1idiu (&xsta[0], &xsun[0], &xmon[0], fac2sun, fac2mon, xcorsta);
	dxtide[0] += xcorsta[0];
	dxtide[1] += xcorsta[1];
	dxtide[2] += xcorsta[2];
	/* ** second, for the semi-diurnal band */
	earthtide_st1isem (&xsta[0], &xsun[0], &xmon[0], fac2sun, fac2mon, xcorsta);
	dxtide[0] += xcorsta[0];
	dxtide[1] += xcorsta[1];
	dxtide[2] += xcorsta[2];
	/* ** corrections for the latitude dependence of love numbers (part l^ (1) ) */
	earthtide_st1l1 (&xsta[0], &xsun[0], &xmon[0], fac2sun, fac2mon, xcorsta);
	dxtide[0] += xcorsta[0];
	dxtide[1] += xcorsta[1];
	dxtide[2] += xcorsta[2];
	/* ** consider corrections for step 2 */
	/* ** corrections for the diurnal band: */
	/* **  first, we need to know the date converted in julian centuries */
	/* **  this is now handled at top of code   (also convert to TT time system) */
	/* **** t= (dmjd-51545.)/36525. */
	/* **** fhr=dmjd-int (dmjd)             !*** this is/was a buggy line (day vs. hr) */
	/* **  second, the diurnal band corrections, */
	/* **   (in-phase and out-of-phase frequency dependence): */
	earthtide_step2diu (&xsta[0], fhr, t, xcorsta);
	dxtide[0] += xcorsta[0];
	dxtide[1] += xcorsta[1];
	dxtide[2] += xcorsta[2];
	/* **  corrections for the long-period band, */
	/* **   (in-phase and out-of-phase frequency dependence): */
	earthtide_step2lon (&xsta[0], t, xcorsta);
	dxtide[0] += xcorsta[0];
	dxtide[1] += xcorsta[1];
	dxtide[2] += xcorsta[2];
	/* ** consider corrections for step 3 */
	/* -----------------------------------------------------------------------
	 * The code below is commented to prevent restoring deformation
	 * due to permanent tide.  All the code above removes
	 * total tidal deformation with conventional Love numbers.
	 * The code above realizes a conventional tide free crust (i.e. ITRF).
	 * This does NOT conform to Resolution 16 of the 18th General Assembly
	 * of the IAG (1983).  This resolution has not been implemented by
	 * the space geodesy community in general (c.f. IERS Conventions 2003).
	 * -----------------------------------------------------------------------
	 * ** uncorrect for the permanent tide  (only if you want mean tide system)
	 * **   pi=3.141592654
	 * **   sinphi=xsta (3)/rsta
	 * **   cosphi=dsqrt (xsta (1)**2+xsta (2)**2)/rsta
	 * **   cosla=xsta (1)/cosphi/rsta
	 * **   sinla=xsta (2)/cosphi/rsta
	 * **   dr=-dsqrt (5./4./pi)*h2*0.31460* (3./2.*sinphi**2-0.5)
	 * **   dn=-dsqrt (5./4./pi)*l2*0.31460*3.*cosphi*sinphi
	 * **   dxtide (1)=dxtide (1)-dr*cosla*cosphi+dn*cosla*sinphi
	 * **   dxtide (2)=dxtide (2)-dr*sinla*cosphi+dn*sinla*sinphi
	 * **   dxtide (3)=dxtide (3)-dr*sinphi      -dn*cosphi
	 */
}

/* ******************************************************************************* */
GMT_LOCAL void earthtide_getghar (int mjd, double fmjd, double *ghar) {
	/* convert mjd/fmjd in UTC time to Greenwich hour angle (in radians)
	 * "satellite orbits: models, methods, applications" montenbruck & gill (2000)
	 * section 2.3.1, pg. 33
	 * need UTC to get sidereal time  ("astronomy on the personal computer", 4th ed)
	 *                               (pg.43, montenbruck & pfleger, springer, 2005)
	 */
	int i;
	double ghad, fmjdutc, tsecutc;

	tsecutc = fmjd * 86400.;			/* UTC time (sec of day) */
	fmjdutc = tsecutc / 86400.;			/* UTC time (fract. day) */
	/*  d = MJD - 51544.5d0                               !*** footnote
	 *  greenwich hour angle for J2000  (12:00:00 on 1 Jan 2000)
	 *  ghad = 100.46061837504d0 + 360.9856473662862d0*d  !*** eq. 2.85 (+digits)
	 */
	ghad = (mjd - 51544 + (fmjdutc - 0.5)) * 360.9856473662862 + 280.46061837504;	/* days since J2000 */

	/* normalize to 0-360 and convert to radians */
	i = (int) (ghad / 360.);
	*ghar = (ghad - i * 360.) * D2R;

	while (*ghar > TWO_PI)
		*ghar -= TWO_PI;

	while (*ghar < 0.)
		*ghar += TWO_PI;
}

/* ----------------------------------------------------------------------- */
GMT_LOCAL void earthtide_rge (double lat, double lon, double *u, double *v, double *w, double x, double y, double z) {
	/* given a rectangular cartesian system (x,y,z) */
	/* compute a geodetic h cartesian sys   (u,v,w) */
	static double cb, cl, sb, sl;

	sincos (lat, &sb, &cb);
	sincos (lon, &sl, &cl);
	*u = -sb * cl * x - sb * sl * y + cb * z;
	*v = -sl * x + cl * y;
	*w = cb * cl * x + cb * sl * y + sb * z;
}

/* ----------------------------------------------------------------------- */
GMT_LOCAL void earthtide_rot1 (double theta, double x, double y, double z, double *u, double *v, double *w) {
	/* ** rotate coordinate axes about 1 axis by angle of theta radians */
	/* ** x,y,z transformed into u,v,w */
	static double c, s;

	sincos (theta, &s, &c);
	*u = x;
	*v = c * y + s * z;
	*w = c * z - s * y;
}

/* ----------------------------------------------------------------------- */
GMT_LOCAL void earthtide_rot3 (double theta, double x, double y, double z, double *u, double *v, double *w) {
	/* rotate coordinate axes about 3 axis by angle of theta radians */
	/* x,y,z transformed into u,v,w */
	static double c, s;

	sincos (theta, &s, &c);
	*u = c * x + s * y;
	*v = c * y - s * x;
	*w = z;
}

/* ------------------------------------------------------------------------------- */
GMT_LOCAL void earthtide_moonxyz (int mjd, double fmjd, double *rm, bool *leapflag) {
	/* get low-precision, geocentric coordinates for moon (ECEF)
	 * UTC Version
	 * input:  mjd/fmjd, is Modified Julian Date (and fractional) in UTC time
	 * output: rm, is geocentric lunar position vector [m] in ECEF
	 *		   lflag  -- leap second table limit flag,  false:flag not raised
	 * 1."satellite orbits: models, methods, applications" montenbruck & gill (2000)
	 * section 3.3.2, pg. 72-73
	 * 2."astronomy on the personal computer, 4th ed." montenbruck & pfleger (2005)
	 * section 3.2, pg. 38-39  routine MiniMoon
	 */
	double d2, d__, f, q, t, t1, t2, t3, el, el0;
	double rm1, rm2, rm3, elp, rse, ghar, oblir, tjdtt;
	double cselat, selatd,  selond, fmjdtt, tsectt, tsecutc;

	/* ** use TT for lunar ephemerides */
	tsecutc = fmjd * 86400;	        		/* UTC time (sec of day) */
	tsectt  = earthtide_utc2ttt (tsecutc, leapflag);	/* TT  time (sec ofday)  */
	fmjdtt  = tsectt / 86400.;				/* TT  time (fract. day) */

	/* julian centuries since 1.5 january 2000 (J2000) */
	/*   (note: also low precision use of mjd --> tjd) */
	tjdtt = mjd + fmjdtt + 2400000.5;		/* Julian Date, TT */
	t = (tjdtt - 2451545.) / 36525.;		/*  julian centuries, TT */

	/* el0 -- mean longitude of Moon (deg) */
	/* el  -- mean anomaly of Moon (deg) */
	/* elp -- mean anomaly of Sun  (deg) */
	/* f   -- mean angular distance of Moon from ascending node (deg) */
	/* d   -- difference between mean longitudes of Sun and Moon (deg) */
	/* equations 3.47, p.72 */
	el0 = t * 481267.88088 + 218.31617 - t * 1.3972f;
	el  = t * 477198.86753 + 134.96292;
	elp = t * 35999.04944  + 357.52543;
	f   = t * 483202.01873 + 93.27283;
	d__ = t * 445267.11135 + 297.85027;
	d2  = 2 * d__;
	/* ** longitude w.r.t. equinox and ecliptic of year 2000 */
	selond = el0 + sin (el * D2R) * 22640.0/3600. + sin ( (el + el) * D2R) * 769./3600. -
			 sin ( (el - d2) * D2R) * 4586.0/3600. + sin (d2 * D2R) * 2370.0/3600. -
			 sin (elp * D2R) * 668.0/3600. - sin ( (f + f) * D2R) * 412.0/3600. -
			 sin ( (el + el - d2) * D2R) * 212.0/3600. - sin ( (el + elp - d2) * D2R) * 206.0/3600. +
			 sin ( (el + d2) * D2R) * 192.0/3600. - sin ( (elp - d2) * D2R) * 165.0/3600. +
			 sin ( (el - elp) * D2R) * 148.0/3600. - sin (d__ * D2R) * 125.0/3600. -
			 sin ( (el + elp) * D2R) * 110.0/3600. - sin ( (f + f - d2) * D2R) * 55.0/3600.;
	/* latitude w.r.t. equinox and ecliptic of year 2000 */
	/*  eq 3.48, p.72 */
	q = sin ( (f + f) * D2R) * 412.0/3600. + sin (elp * D2R) * 541.0/3600.;
	/*  temporary ter */
	selatd = sin ( (f + selond - el0 + q) * D2R) * 18520.0/3600. -
			 sin ( (f - d2) * D2R) * 526.0/3600. + sin ( (el + f - d2) * D2R) * 44.0/3600. -
			 sin ( (-el + f - d2) * D2R) * 31.0/3600. - sin ( (-el - el + f) * D2R) * 25.0/3600. -
			 sin ( (elp + f - d2) * D2R) * 23.0/3600. + sin ( (-el + f) * D2R) * 21.0/3600. +
			 sin ( (-elp + f - d2) * D2R) * 11.0/3600.;
	/* distance from Earth center to Moon (m) */
	/*  eq 3.49, p.72 */
	rse = 3.85e8 - cos (el * D2R) * 2.0905e7 - cos ( (d2 - el) * D2R) * 3.699e6 - cos (d2 * D2R) * 2.956e6
		- cos ( (el + el) * D2R) * 5.7e5 + cos ( (el + el - d2) * D2R) * 2.46e5 - cos ( (elp - d2) * D2R) *
		2.05e5 - cos ( (el + d2) * D2R) * 1.71e5 - cos ( (el + elp - d2) * D2R) * 1.52e5;
	/* convert spherical ecliptic coordinates to equatorial cartesian */
	/* precession of equinox wrt. J2000   (p.71) */
	/*  eq 3.50, p.72 */
	selond += t * 1.3972;
	/* position vector of moon (mean equinox & ecliptic of J2000) (EME2000, ICRF) */
	/*                         (plus long. advance due to precession -- eq. above) */
	selatd *= D2R;
	selond *= D2R;
	oblir = 23.43929111 * D2R;			/* obliquity of the J2000 eclipti */
	cselat = cos (selatd);
	t1 = rse * cos (selond) * cselat;		/* meters          !*** eq. 3.51, */
	t2 = rse * sin (selond) * cselat;		/* meters          !*** eq. 3.51, */
	t3 = rse * sin (selatd);					/* meters          !*** eq. 3.51, */
	earthtide_rot1 (-oblir, t1, t2, t3, &rm1, &rm2, &rm3);
	/* convert position vector of moon to ECEF  (ignore polar motion/LOD) */
	/*  eq. 3.51, */
	earthtide_getghar (mjd, fmjd, &ghar);						/* sec 2.3.1, */
	earthtide_rot3 (ghar, rm1, rm2, rm3, &rm[0], &rm[1], &rm[2]); /* eq. 2.89, */
}

/* ******************************************************************************* */
GMT_LOCAL void earthtide_sunxyz (int mjd, double fmjd, double *rs, bool *leapflag) {
	/* get low-precision, geocentric coordinates for sun (ECEF)
	 * input, mjd/fmjd, is Modified Julian Date (and fractional) in UTC time
	 * output, rs, is geocentric solar position vector [m] in ECEF
	 *      	  lflag  -- leap second table limit flag,  false:flag not raised
	 * 1."satellite orbits: models, methods, applications" montenbruck & gill (2000)
	 * section 3.3.2, pg. 70-71
	 * 2."astronomy on the personal computer, 4th ed." montenbruck & pfleger (2005)
	 * section 3.2, pg. 39  routine MiniSun
	 */
	double r__, t, em, em2, rs1, rs2, rs3, obe;
	double ghar, opod, slon, emdeg, slond, tjdtt, sslon;
	double fmjdtt, tsectt, tsecutc;

	/* ** mean elements for year 2000, sun ecliptic orbit wrt. Earth */
	obe = 23.43929111 * D2R;			/* obliquity of the J2000 ecliptic */
	opod = 282.94;
	/*  use TT for solar ephemerides */
	/*  RAAN + arg.peri.  (deg.) */
	tsecutc = fmjd * 86400.;			/* UTC time (sec of */
	tsectt = earthtide_utc2ttt (tsecutc, leapflag);/* TT  time (sec of */
	fmjdtt = tsectt / 86400.;
	/* julian centuries since 1.5 january 2000 (J2000) */
	/*   (note: also low precision use of mjd --> tjd) */
	/*  TT  time (fract. */
	tjdtt = mjd + fmjdtt + 2400000.5;	/* Julian Date, TT */
	t = (tjdtt - 2451545.) / 36525.;	/* julian centuries, */
	emdeg = t * 35999.049 + 357.5256;	/* degrees */
	em = emdeg * D2R;
	em2 = em + em;
	/* ** series expansions in mean anomaly, em   (eq. 3.43, p.71) */
	/* *** radians */
	r__ = (149.619 - cos (em) * 2.499 - cos (em2) * 0.021) * 1e9; /* *** m. */
	slond = opod + emdeg + (sin (em) * 6892 + sin (em2) * 72) / 3600.;	/* precession of equinox wrt. J2000   (p.71) */
	slond += t * 1.3972;
	/* position vector of sun (mean equinox & ecliptic of J2000) (EME2000, ICRF) */
	/*                        (plus long. advance due to precession -- eq. above) */
	slon = slond * D2R;
	sslon = sin (slon);
	rs1 = r__ * cos (slon);				/* meters  !*** eq. 3.46, */
	rs2 = r__ * sslon * cos (obe);		/* meters  !*** eq. 3.46, */
	rs3 = r__ * sslon * sin (obe);
	/* ** convert position vector of sun to ECEF  (ignore polar motion/LOD) */
	/* meters             !*** eq. 3.46, */
	earthtide_getghar (mjd, fmjd, &ghar);			/* sec 2.3.1, */
	earthtide_rot3 (ghar, rs1, rs2, rs3, &rs[0], &rs[1], &rs[2]);		/* eq. 2.89, */
}

/* ----------------------------------------------------------------------- */
GMT_LOCAL void earthtide_geoxyz (double lat, double lon, double eht, double *x, double *y, double *z) {
	/* convert geodetic lat, long, ellip ht. to x,y,z */
	double w, w2, en, cla, sla, t;

	sincos (lat, &sla, &cla);
	w2 = 1. - ECC2 * sla * sla;
	w = sqrt (w2);
	en = EARTH_RAD / w;
	t = (en + eht) * cla;
	*x = t * cos (lon);
	*y = t * sin (lon);
	*z = (en * (1. - ECC2) + eht) * sla;
}


/* *********************************************************************** */
/* ** time conversion **************************************************** */
/* *********************************************************************** */
GMT_LOCAL void earthtide_setjd0 (int iyr, int imo, int idy) {
	/* set the integer part of a modified julian date as epoch, mjd0
	   the modified julian day is derived from civil time as in earthtide_civmjd ()
	   allows single number expression of time in seconds w.r.t. mjd0 */
	static int m, y, it1, it2, mjd;

	if (imo <= 2) {
		y = iyr - 1;
		m = imo + 12;
	} else {
		y = iyr;
		m = imo;
	}
	it1 = (int) (y * 365.25);
	it2 = (int) ( (m + 1) * 30.6001);
	mjd = it1 + it2 + idy - 679019;
	/* ** now set the epoch for future time computations */
	mjdoff_1.mjd0 = mjd;
}

/* *********************************************************************** */
GMT_LOCAL void earthtide_civmjd (int iyr, int imo, int idy, int ihr, int imn, double sec, int *mjd, double *fmjd) {
	/* convert civil date to modified julian date */
	/* imo in range 1-12, idy in range 1-31 */
	/* only valid in range mar-1900 through feb-2100     (leap year protocols) */
	/* ref: hofmann-wellenhof, 2nd ed., pg 34-35 */
	/* operation confirmed against table 3.3 values on pg.34 */
	int m, y, it1, it2;

	if (imo <= 2) {
		y = iyr - 1;
		m = imo + 12;
	}
	else {
		y = iyr;
		m = imo;
	}
	it1 = (int) (y * 365.25);
	it2 = (int) ( (m + 1) * 30.6001);
	*mjd = it1 + it2 + idy - 679019;
	*fmjd = (ihr * 3600 + imn * 60 + sec) / 86400.;
}

GMT_LOCAL void earthtide_mjdciv (int mjd, double fmjd, int *iyr, int *imo, int *idy, int *ihr, int *imn, double *sec) {
	/* convert modified julian date to civil date */
	/* imo in range 1-12, idy in range 1-31 */
	/* only valid in range mar-1900 through feb-2100 */
	/* ref: hofmann-wellenhof, 2nd ed., pg 34-35 */
	/* operation confirmed for leap years (incl. year 2000) */
	static int ia, ib, ic, id, ie, it1, it2, it3;
	static double rjd, tmp;

	rjd = mjd + fmjd + 2400000.5;
	ia = (int) (rjd + .5);
	ib = ia + 1537;
	ic = (int) ( (ib - 122.1) / 365.25);
	id = (int) (ic * 365.25);
	ie = (int) ( (ib - id) / 30.6001);
	/* the fractional part of a julian day is fractional mjd + 0.5
	   therefore, fractional part of julian day + 0.5 is fractional mjd */
	it1  = (int) (ie * 30.6001);
	*idy = (int) (ib - id - it1 +fmjd);
	it2  = (int) (ie / 14.);
	*imo = ie - 1 - it2 * 12;
	it3  = (int) ( (*imo + 7) / 10.);
	*iyr = ic - 4715 - it3;
	tmp  = fmjd * 24.;
	*ihr = (int)tmp;
	tmp  = (tmp - *ihr) * 60.;
	*imn = (int)tmp;
	*sec = (tmp - *imn) * 60.;
}

/* ------------------------------------------------------------------------------------------------------- */
GMT_LOCAL void earthtide_sun_moon_track (struct GMT_CTRL *GMT, struct GMT_GCAL *Cal, struct GMT_ARRAY T) {
	/* Get the Sun & Moon position at times starting time */
	bool leapflag = false;
	uint64_t k;
	int mjd, year, month, day, hour, min;
	double fmjd, rsun[3], tdel2 = 0, rmoon[3], out[7], convd[3];
	struct GMT_RECORD *Out = NULL;

	Out = gmt_new_record (GMT, out, NULL);	/* Since we only need to worry about numerics in this module */

	gmt_set_column_type (GMT, GMT_OUT, 1, GMT_IS_LON);
	gmt_set_column_type (GMT, GMT_OUT, 2, GMT_IS_LAT);
	gmt_set_column_type (GMT, GMT_OUT, 4, GMT_IS_LON);
	gmt_set_column_type (GMT, GMT_OUT, 5, GMT_IS_LAT);

	if (T.count){
		tdel2 = (T.max-T.min) / ( (T.inc - 1) * 24 * 3600);
	}
	else {
		if (T.unit == 'm')
			tdel2 = 1.0 / (24 * 60);	/* 1 minute steps */
		else if (T.unit == 's')
			tdel2 = 1.0 / (24 * 3600);	/* 1 seconds steps (????) */
		else if (T.unit == 'h')
			tdel2 = 1.0 / 24;		/* 1 hour steps */
		else if (T.unit == 'd')
			tdel2 = 1.0;		/* 1 day steps */

		tdel2 *= T.inc;
	}

	if (T.n > 1 && tdel2 < (0.5 / 86400)) {
		tdel2 = 0.5 / 86400;
		GMT_Report (GMT->parent, GMT_MSG_ERROR, "Time interval too low, must be at least 0.5 s. Reset to 0.5\n");
	}

	year = (int)Cal->year;	month = (int)Cal->month;	day = (int)Cal->day_m;	/* Screw the unsigned ints */
	hour = (int)Cal->hour;	min = (int)Cal->min;
	earthtide_civmjd (year, month, day, hour, min, Cal->sec, &mjd, &fmjd);
	earthtide_mjdciv (mjd, fmjd, &year, &month, &day, &hour, &min, &Cal->sec);	/* normalize civil time */
	earthtide_setjd0 (year, month, day);
	for (k = 0; k < T.n; k++) {
		earthtide_sunxyz (mjd, fmjd, rsun, &leapflag);      /* mjd/fmjd in UTC */
		earthtide_moonxyz (mjd, fmjd, rmoon, &leapflag);
		earthtide_mjdciv (mjd, fmjd + 1.1574074074074074e-8, &year, &month, &day, &hour, &min, &Cal->sec);
		//out[0] = hour * 3600 + min * 60;
		out[0] = T.array[k];
		gmt_ECEF_inverse (GMT, rsun, convd);
		out[1] = convd[0];	out[2] = convd[1];	out[3] = convd[2];
		gmt_ECEF_inverse (GMT, rmoon, convd);
		out[4] = convd[0];	out[5] = convd[1];	out[6] = convd[2];
		fmjd += tdel2;
		fmjd = (int) (round (fmjd * 86400)) / 86400.0;		/* force 1 sec. granularity */
		GMT_Put_Record (GMT->parent, GMT_WRITE_DATA, Out);	/* Write this to output */
	}
	gmt_M_free (GMT, Out);
}

/* ----------------------------------------------------------------------- */
GMT_LOCAL void earthtide_solid_grd (struct GMT_CTRL *GMT, struct EARTHTIDE_CTRL *Ctrl, struct GMT_GCAL *Cal, struct GMT_GRID **Grid) {
	bool leapflag;
	int k, mjd, year, month, day, hour, min;
	uint32_t row, col, n_columns = 0, n_rows = 0;
	size_t ij_n = 0, ij_e = 0, ij_u = 0, n_inc = 0, e_inc = 0, u_inc = 0;
	gmt_grdfloat *grd_n, *grd_e, *grd_u;
	double fmjd, xsta[3], rsun[3], etide[3], rmoon[3];
	double lat, ut, vt, wt, *lons;
	double west = 0, south = 0, x_inc = 0, y_inc = 0;

	/* Select which indices to increment based on user selection */
	/* Use the trick of not incrementing the indices of unwanted arrays to avoid IF branches inside the loops */
	if (Ctrl->G.do_east) {
		grd_e = Grid[X_COMP]->data;
		e_inc = 1;
	}
	else
		grd_e = (gmt_grdfloat *)malloc (1 * sizeof (gmt_grdfloat));

	if (Ctrl->G.do_north) {
		grd_n = Grid[Y_COMP]->data;
		n_inc = 1;
	}
	else
		grd_n = (gmt_grdfloat *)malloc (1 * sizeof (gmt_grdfloat));

	if (Ctrl->G.do_up) {
		grd_u = Grid[Z_COMP]->data;
		u_inc = 1;
	}
	else
		grd_u = (gmt_grdfloat *)malloc (1 * sizeof (gmt_grdfloat));

	/* Get header params. Since all three have the same dims we stop when we find the first grid required */
	for (k = 0; k < N_COMPS; k++) {
		if (Ctrl->C.selected[k]) {
			n_columns = Grid[k]->header->n_columns;		n_rows = Grid[k]->header->n_rows;
			west = Grid[k]->header->wesn[XLO];		south = Grid[k]->header->wesn[YLO];
			x_inc = Grid[k]->header->inc[GMT_X];		y_inc = Grid[k]->header->inc[GMT_Y];
			break;
		}
	}
	year = (int)Cal->year;	month = (int)Cal->month;	day = (int)Cal->day_m;	/* Screw the unsigned ints */
	hour = (int)Cal->hour;	min = (int)Cal->min;
	leapflag = false;                       /* false means flag not raised */
	earthtide_civmjd (year, month, day, hour, min, Cal->sec, &mjd, &fmjd);
	earthtide_mjdciv (mjd, fmjd, &year, &month, &day, &hour, &min, &Cal->sec);	/* normalize civil time */
	earthtide_setjd0 (year, month, day);
	earthtide_sunxyz (mjd, fmjd, rsun, &leapflag);
	earthtide_moonxyz (mjd, fmjd, rmoon, &leapflag);

	/* Generate a vector of longitudes in radians and put them in the [0 360] interval */
	lons = (double *)malloc (n_columns * sizeof (double));
	for (col = 0; col < n_columns; col++) {
		lons[col] = west + col * x_inc;
		if (lons[col] < 0) lons[col] += 360;
		lons[col] *= D2R;
	}

	for (row = n_rows; row > 0; row--) {
		lat = (south + (row - 1) * y_inc) * D2R;
		for (col = 0; col < n_columns; col++) {
			earthtide_geoxyz (lat, lons[col], 0, &xsta[0], &xsta[1], &xsta[2]);
			earthtide_detide (xsta, mjd, fmjd, rsun, rmoon, etide, &leapflag);
			/* determine local geodetic horizon components (topocentric) */
			earthtide_rge (lat, lons[col], &ut, &vt, &wt, etide[0], etide[1], etide[2]);		/* tide vect */
			grd_n[ij_n] = (gmt_grdfloat)vt;
			grd_e[ij_e] = (gmt_grdfloat)ut;
			grd_u[ij_u] = (gmt_grdfloat)wt;
			ij_n += n_inc;
			ij_e += e_inc;
			ij_u += u_inc;
		}
	}
	if (leapflag)
		GMT_Report (GMT->parent, GMT_MSG_WARNING, "time crossed leap seconds table boundaries. Boundary edge used instead.");

	/* Free these that were never used anyway */
	if (!Ctrl->G.do_north) free (grd_n);
	if (!Ctrl->G.do_east) free (grd_e);
	if (!Ctrl->G.do_up) free (grd_u);
	free (lons);
}

/* ------------------------------------------------------------------------------------------------------- */
GMT_LOCAL void earthtide_solid_ts (struct GMT_CTRL *GMT, struct GMT_GCAL *Cal, double lon, double lat, struct GMT_ARRAY T) {
	/* iyr	year    [1901-2099] */
	/* imo	month number [1-12] */
	/* idy	day          [1-31] */
	/* lat	Lat. (pos N.) [- 90, +90] */
	/* lon	Lon. (pos E.) [-360,+360] */
	bool leapflag = false;
	uint64_t k;
	int mjd, year, month, day, hour, min;
	double d__2, ut, vt, wt;
	double fmjd, xsta[3], rsun[3], tdel2 = 0, etide[3], rmoon[3], out[4];
	struct GMT_RECORD *Out = NULL;

	/* position of observing point (positive East) */
	if (lon < 0)    lon += 360;
	if (lon >= 360) lon += -360;

	lat *= D2R;
	lon *= D2R;
	earthtide_geoxyz (lat, lon, 0, &xsta[0], &xsta[1], &xsta[2]);

	Out = gmt_new_record (GMT, out, NULL);	/* Since we only need to worry about numerics in this module */

	if (T.count){
		tdel2 = (T.max-T.min) / ( (T.inc - 1) * 24 * 3600);
	}
	else {
		if (T.unit == 'm')
		tdel2 = 1.0 / (24 * 60);	/* 1 minute steps */
		else if (T.unit == 's')
			tdel2 = 1.0 / (24 * 3600);	/* 1 second steps (????) */
		else if (T.unit == 'h')
			tdel2 = 1.0 / 24;			/* 1 hour steps */
		else if (T.unit == 'd')
			tdel2 = 1.0;		/* 1 day steps */

		tdel2 *= T.inc;
	}

	if (T.n > 1 && tdel2 < (0.5 / 86400)) {
		tdel2 = 0.5 / 86400;
		GMT_Report (GMT->parent, GMT_MSG_ERROR, "Time interval too low, must be at least 0.5 s. Reset to 0.5\n");
	}

	/* here comes the sun  (and the moon)  (go, tide!) */
	year = (int)Cal->year;	month = (int)Cal->month;	day = (int)Cal->day_m;	/* Screw the unsigned ints */
	hour = (int)Cal->hour;	min = (int)Cal->min;
	earthtide_civmjd (year, month, day, hour, min, Cal->sec, &mjd, &fmjd);
	earthtide_mjdciv (mjd, fmjd, &year, &month, &day, &hour, &min, &Cal->sec);	/* normalize civil time */
	earthtide_setjd0 (year, month, day);
	for (k = 0; k < T.n; k++) {
		leapflag = false;                       /* false means flag not raised */
		earthtide_sunxyz (mjd, fmjd, rsun, &leapflag);      /* mjd/fmjd in UTC */
		earthtide_moonxyz (mjd, fmjd, rmoon, &leapflag);
		earthtide_detide (xsta, mjd, fmjd, rsun, rmoon, etide, &leapflag);
		/* determine local geodetic horizon components (topocentric) */
		earthtide_rge (lat, lon, &ut, &vt, &wt, etide[0], etide[1], etide[2]);		/* tide vect */
		d__2 = Cal->sec - 0.001;
		earthtide_mjdciv (mjd, fmjd + 1.1574074074074074e-8, &year, &month, &day, &hour, &min, &d__2);
		//out[0] = hour * 3600 + min * 60 + Cal->sec;
		out[0] = T.array[k];
		out[1] = ut;
		out[2] = vt;
		out[3] = wt;
		fmjd += tdel2;
		fmjd = (int) (round (fmjd * 86400)) / 86400.0;	/* force 1 sec. granularity */
		GMT_Put_Record (GMT->parent, GMT_WRITE_DATA, Out);	/* Write this to output */
	}

	gmt_M_free (GMT, Out);

	if (leapflag)
		GMT_Report (GMT->parent, GMT_MSG_WARNING, "time crossed leap seconds table boundaries. Boundary edge used instead.");
}

/* ------------------------------------------------------------------------------------------------------- */
static int usage (struct GMTAPI_CTRL *API, int level) {
	const char *name = gmt_show_name_and_purpose (API, THIS_MODULE_LIB, THIS_MODULE_CLASSIC_NAME, THIS_MODULE_PURPOSE);
	if (level == GMT_MODULE_PURPOSE) return (GMT_NOERROR);
	GMT_Usage (API, 0, "usage: %s [-G<outgrid>] [-C<comp>] [%s] [-L<lon>/<lat>] [%s] [-S] [-T[<min>/<max>/]<inc>[+i|n]] "
		"[%s] [%s] [%s] [%s]%s[%s]\n", name, GMT_I_OPT, GMT_Rgeo_OPT, GMT_V_OPT, GMT_bo_OPT, GMT_o_OPT,
		GMT_r_OPT, GMT_x_OPT, GMT_PAR_OPT);

	if (level == GMT_SYNOPSIS) return (GMT_MODULE_SYNOPSIS);

	GMT_Message (API, GMT_TIME_NONE, "  REQUIRED ARGUMENTS:\n");
	GMT_Usage (API, 2, "(Note: One of -G, -L, or -S is required.)");
	gmt_outgrid_syntax (API, 'G', "Specify file name for output grid file (s). "
		"If more than one component is set via -C then <outgrid> must contain %%s to format component code.");
	GMT_Usage (API, 1, "\n-L<lon>/<lat>");
	GMT_Usage (API, -2, "Geographical coordinate where to compute the time-series.");
	GMT_Usage (API, 1, "\n-S Output position of Sun and Moon in geographical coordinates plus "
		"distance in meters. Output is a Mx7 matrix, where M is the number of "
		"times (set by -T) and columns are time, sun_lon, sun_lat, sun_dist "
		"moon_lon, moon_lat, moon_dist.");
	GMT_Message (API, GMT_TIME_NONE, "\n  OPTIONAL ARGUMENTS:\n");
	GMT_Usage (API, 1, "\n-C<comp>");
	if (API->external)
		GMT_Usage (API, -2, "List of comma-separated components to be written as grids. Choose from");
	else
		GMT_Usage (API, -2, "List of comma-separated components to be written as grids (requires -G). Choose from");
	GMT_Usage (API, 3, "x|e: Get x|east component.");
	GMT_Usage (API, 3, "y|n: Get y|north component.");
	GMT_Usage (API, 3, "z|v: Get z|vertical component [Default].");
	GMT_Option (API, "I");
	GMT_Option (API, "R");
	GMT_Usage (API, 1, "\n-T[<min>/<max>/]<inc>[+i|n]");
	GMT_Usage (API, -2, "Make evenly spaced output time steps from <min> to <max> by <inc>. Optional modifiers:");
	GMT_Usage (API, 3, "+n Indicate <inc> is the number of t-values to produce over the range instead of increment.");
	GMT_Usage (API, 3, "+i Indicate <inc> is the reciprocal of desired <inc> (e.g., 3 for 0.3333.....).");
	GMT_Usage (API, -2, "Append a valid time unit (%s) to the increment. "
		"Notes: If no -T is provided get current time in UTC from the computer clock. "
		"If no -G or -S are provided then -T is interpreted to mean compute a time-series "
		"at the location specified by -L, making -L mandatory. "
		"When -G and -T only first time T series is considered.", GMT_TIME_UNITS_DISPLAY);
	GMT_Option (API, "V,b,o,r,x,.");

	return (GMT_MODULE_USAGE);
}

static int parse (struct GMT_CTRL *GMT, struct EARTHTIDE_CTRL *Ctrl, struct GMT_OPTION *options) {
	/* This parses the options provided to earthtide and sets parameters in CTRL.
	 * Any GMT common options will override values set previously by other commands.
	 * It also replaces any file names specified as input or output with the data ID
	 * returned when registering these sources/destinations with the API.
	 */

	unsigned int n_errors = 0, pos = 0;
	char txt_a[GMT_LEN64] = {""}, txt_b[GMT_LEN64] = {""}, p[GMT_LEN16] = {""};
	struct GMT_OPTION *opt = NULL;
	struct GMTAPI_CTRL *API = GMT->parent;

	for (opt = options; opt; opt = opt->next) {
		switch (opt->option) {

			case '<':	/* Skip input files */
				if (GMT_Get_FilePath (API, GMT_IS_DATASET, GMT_IN, GMT_FILE_REMOTE, &(opt->arg))) n_errors++;
				break;

			/* Processes program-specific parameters */

			case 'C':	/* Requires -G and selects which components should be written as grids */
				n_errors += gmt_M_repeated_module_option (API, Ctrl->C.active);
				while ( (gmt_strtok (opt->arg, ",", &pos, p)) && Ctrl->C.n_selected < N_COMPS) {
					switch (p[0]) {
						case 'x': case 'e':		Ctrl->C.selected[X_COMP] = Ctrl->G.do_east = true;	break;
						case 'y': case 'n':		Ctrl->C.selected[Y_COMP] = Ctrl->G.do_north = true;	break;
						case 'z': case 'v':		Ctrl->C.selected[Z_COMP] = Ctrl->G.do_up = true;		break;
						default:
							GMT_Report (API, GMT_MSG_ERROR, "Unrecognized field argument %s in -C.!\n", p);
							n_errors++;
							break;
					}
					Ctrl->C.n_selected++;
				}
				if (Ctrl->C.n_selected == 0) {
					GMT_Report (API, GMT_MSG_ERROR, "-C requires comma-separated component arguments.\n");
					n_errors++;
				}
				break;
			case 'G':	/* Output filename */
				n_errors += gmt_M_repeated_module_option (API, Ctrl->G.active);
				if (!GMT->parent->external && Ctrl->G.n) {	/* Command line interface */
					GMT_Report (API, GMT_MSG_ERROR, "-G can only be set once!\n");
					n_errors++;
				}
				else {
					Ctrl->G.file[Ctrl->G.n] = strdup (opt->arg);
					if (GMT_Get_FilePath (API, GMT_IS_GRID, GMT_OUT, GMT_FILE_LOCAL, &(Ctrl->G.file[Ctrl->G.n]))) n_errors++;
				}

				if (!GMT->parent->external) {		/* Copy the name into the 3 slots to simplify the grid writing algo */
					Ctrl->G.file[Y_COMP] = strdup (opt->arg);
					Ctrl->G.file[Z_COMP] = strdup (opt->arg);
				}
				break;
			case 'I':	/* Grid spacings */
				n_errors += gmt_M_repeated_module_option (API, Ctrl->I.active);
				n_errors += gmt_parse_inc_option (GMT, 'I', opt->arg);
				break;
			case 'L':	/* Location for time-series */
				n_errors += gmt_M_repeated_module_option (API, Ctrl->L.active);
				if (sscanf (opt->arg, "%[^/]/%s", txt_a, txt_b) != 2) {
					GMT_Report (API, GMT_MSG_ERROR, "Option -C: Expected -C<lon>/<lat>\n");
					n_errors++;
				}
				else {
					n_errors += gmt_verify_expectations (GMT, GMT_IS_LON, gmt_scanf_arg (GMT, txt_a, GMT_IS_LON,
					                                     false, &Ctrl->L.x), txt_a);
					n_errors += gmt_verify_expectations (GMT, GMT_IS_LAT, gmt_scanf_arg (GMT, txt_b, GMT_IS_LAT,
					                                     false, &Ctrl->L.y), txt_b);
					if (n_errors) GMT_Report (API, GMT_MSG_ERROR,
					                          "Option -C: Undecipherable argument %s\n", opt->arg);
				}
				break;
			case 'S':
				n_errors += gmt_M_repeated_module_option (API, Ctrl->S.active);
				if (gmt_set_datum (GMT, opt->arg, &Ctrl->S.datum) == -1) n_errors++;
				break;
			case 'T':	/* Select time range for time-series tide estimates */
				n_errors += gmt_M_repeated_module_option (API, Ctrl->T.active);
				if (!opt->arg) {
					GMT_Report (API, GMT_MSG_ERROR, "Option -T: must provide a valid date\n", opt->arg);
					n_errors++;
					break;
				}
				n_errors += gmt_parse_array (GMT, 'T', opt->arg, & (Ctrl->T.T), GMT_ARRAY_TIME | GMT_ARRAY_SCALAR | GMT_ARRAY_UNIQUE, 0);

				break;
			default:	/* Report bad options */
				n_errors += gmt_default_option_error (GMT, opt);
				break;
		}
	}

	if (Ctrl->G.active) {
		if (Ctrl->C.active && Ctrl->C.n_selected > 1 && !GMT->parent->external && !strstr (Ctrl->G.file[X_COMP], "%s")) {
			GMT_Report (API, GMT_MSG_ERROR, "-G file format must contain a %%s for field type substitution.\n");
			n_errors++;
		}
		if (!Ctrl->C.active) {	/* Default to vertical component */
			Ctrl->C.selected[Z_COMP] = Ctrl->G.do_up = true;
			Ctrl->C.n_selected = 1;
		}
	}

	if (Ctrl->G.active) {	/* implicitly set -Rd */
		if (!GMT->common.R.active[RSET]) {	/* implicitly set -Rd */
			GMT->common.R.active[RSET] = true;
			GMT->common.R.wesn[XLO] = -180.0;	GMT->common.R.wesn[XHI] = 180.0;
			GMT->common.R.wesn[YLO] = -90.0;	GMT->common.R.wesn[YHI] = +90.0;
			gmt_set_geographic (GMT, GMT_IN);
			if (!GMT->common.R.inc[0])
				n_errors += gmt_parse_inc_option (GMT, 'I', "0.5");
		}
		else if (!GMT->common.R.inc[0]) {
			GMT_Report (API, GMT_MSG_ERROR, "When setting -R must set -I too!\n");
			n_errors++;
		}
	}

	n_errors += gmt_M_check_condition (GMT, Ctrl->G.active && (GMT->common.R.inc[GMT_X] <= 0 || GMT->common.R.inc[GMT_Y] <= 0),
	                                   "Option -I: Absent or no positive increment (s)\n");
	n_errors += gmt_M_check_condition (GMT, !Ctrl->L.active && !Ctrl->G.active && !Ctrl->S.active,
	                                   "Must specify -S, -G or -L options\n");
	if (!GMT->parent->external)
		n_errors += gmt_M_check_condition (GMT, Ctrl->T.active && !Ctrl->L.active && !Ctrl->S.active && !Ctrl->G.active,
		                                   "Option -T: requires one of -G, -L, or -S.\n");

	return (n_errors ? GMT_PARSE_ERROR : GMT_NOERROR);
}

#define bailout(code) {gmt_M_free_options (mode); return (code);}
#define Return(code) {Free_Ctrl (GMT, Ctrl); gmt_end_module (GMT, GMT_cpy); bailout (code);}

EXTERN_MSC int GMT_earthtide (void *V_API, int mode, void *args) {
	int error = 0;
	struct EARTHTIDE_CTRL *Ctrl = NULL;
	struct GMT_CTRL *GMT = NULL, *GMT_cpy = NULL;
	struct GMT_OPTION *options = NULL;
	struct GMT_GCAL cal_start;
	struct GMTAPI_CTRL *API = gmt_get_api_ptr (V_API);	/* Cast from void to GMTAPI_CTRL pointer */

	/*----------------------- Standard module initialization and parsing ----------------------*/

	if (API == NULL) return (GMT_NOT_A_SESSION);
	if (mode == GMT_MODULE_PURPOSE) return (usage (API, GMT_MODULE_PURPOSE));	/* Return the purpose of program */
	options = GMT_Create_Options (API, mode, args);	if (API->error) return (API->error);	/* Set or get option list */

	if ( (error = gmt_report_usage (API, options, 0, usage)) != GMT_NOERROR) bailout (error);	/* Give usage if requested */

	/* Parse the command-line arguments */

	if ( (GMT = gmt_init_module (API, THIS_MODULE_LIB, THIS_MODULE_CLASSIC_NAME, THIS_MODULE_KEYS, THIS_MODULE_NEEDS, module_kw, &options, &GMT_cpy)) == NULL) bailout (API->error); /* Save current state */
	if (GMT_Parse_Common (API, THIS_MODULE_OPTIONS, options)) Return (API->error);
	Ctrl = New_Ctrl (GMT);	/* Allocate and initialize a new control structure */
	if ( (error = parse (GMT, Ctrl, options)) != 0) Return (error);

	/*---------------------------- This is the earthtide main code ----------------------------*/

	if (!Ctrl->T.active) {	/* Select the current day as the time to evaluate */
		time_t rawtime;
		struct tm *timeinfo;
		gmt_gcal_from_rd (GMT, GMT->current.time.today_rata_die, &cal_start);
		time (&rawtime);
		timeinfo = gmtime (&rawtime);			/* Get the time in UTC */
		cal_start.hour = timeinfo->tm_hour;
		cal_start.min  = timeinfo->tm_min;
		cal_start.sec  = timeinfo->tm_sec;
		Ctrl->T.T.min = Ctrl->T.T.max = gmt_rdc2dt (GMT, GMT->current.time.today_rata_die, (cal_start.hour * 60 + cal_start.min) * 60 + cal_start.sec);
	}
	else
		gmt_gcal_from_dt (GMT, Ctrl->T.T.min, &cal_start);

	gmt_M_tic (GMT);

	if (Ctrl->G.active) {	/* Return/write 1-3 grids */
		int k, kk;
		char file[PATH_MAX] = {""}, *code[N_COMPS] = {"e", "n", "v"}, *comp_info[3] = {"x|east solid Earth tide component", "y|north solid Earth tide component", "z|vertical solid Earth tide component"};
		struct GMT_GRID *Grid[N_COMPS] = {NULL, NULL, NULL};

		gmt_set_geographic (GMT, GMT_OUT);
		for (k = 0; k < N_COMPS; k++) {
			if (!Ctrl->C.selected[k]) continue;
			/* Create the empty grid and allocate space */
			if ( (Grid[k] = GMT_Create_Data (API, GMT_IS_GRID, GMT_IS_SURFACE, GMT_CONTAINER_AND_DATA, NULL, NULL, NULL,
			                             GMT->common.R.registration, 0, NULL)) == NULL)
				Return (API->error);

			strcpy (Grid[k]->header->z_units, "solid-earth-tide [meter]");
			if (GMT_Set_Comment (API, GMT_IS_GRID, GMT_COMMENT_IS_OPTION | GMT_COMMENT_IS_COMMAND, options, Grid[k]))
				Return (API->error);
			if (GMT_Set_Comment (API, GMT_IS_GRID, GMT_COMMENT_IS_REMARK, comp_info[k], Grid[k]))
				Return (API->error);
		}

		earthtide_solid_grd (GMT, Ctrl, &cal_start, Grid);	/* Evaluate the chosen component (s) on the grids */

		/* Now write the one to three grids */
		for (k = kk = 0; k < N_COMPS; k++) {
			if (!Ctrl->C.selected[k]) continue;
			if (!API->external) kk = k;	/* On command line we pick item k from an array of 3 items */
			if (strstr (Ctrl->G.file[kk], "%s"))
				sprintf (file, Ctrl->G.file[kk], code[k]);
			else
				strncpy (file, Ctrl->G.file[kk], PATH_MAX-1);

			if (GMT_Write_Data (API, GMT_IS_GRID, GMT_IS_FILE, GMT_IS_SURFACE, GMT_CONTAINER_AND_DATA, NULL, file, Grid[k]) != GMT_NOERROR) {
				Return (API->error);
			}
			kk++;	/* For the external interface we take them in the order given as there is not an array of 3 */
		}
	}
	else {	/* Write data table with 4 or 7 columns to stdout */
		int n_out = 4;	/* If -L */
		if (Ctrl->S.active) {
			gmt_ECEF_init (GMT, &Ctrl->S.datum);
			n_out = 7;
		}
		if (gmt_create_array (GMT, 'T', & (Ctrl->T.T), NULL, NULL)) /* Get the array built or read */
			Return (GMT_RUNTIME_ERROR);

		if (!Ctrl->T.T.count && (strchr ("dhms", Ctrl->T.T.unit) == NULL)){
			GMT_Report (GMT->parent, GMT_MSG_ERROR, "Must specify valid interval unit (d|h|m|s)\n");
			return GMT_PARSE_ERROR;
		}

		if (Ctrl->T.one_time)
			Ctrl->T.T.n = 1;

		/* Specify output expected columns */
		if ( (error = GMT_Set_Columns (API, GMT_OUT, n_out, GMT_COL_FIX_NO_TEXT)) != GMT_NOERROR)
			Return (error);

		/* Specify that output are points in a dataset */
		if (GMT_Init_IO (API, GMT_IS_DATASET, GMT_IS_POINT, GMT_OUT, GMT_ADD_DEFAULT, 0, options) != GMT_NOERROR) 	/* Registers default output destination, unless already set */
			Return (API->error);

		if (GMT_Begin_IO (API, GMT_IS_DATASET, GMT_OUT, GMT_HEADER_ON) != GMT_NOERROR) 	/* Enables data output and sets access mode */
			Return (API->error);

		if (GMT_Set_Geometry (API, GMT_OUT, GMT_IS_POINT) != GMT_NOERROR) 	/* Sets output geometry */
			Return (API->error);

		gmt_set_column_type (GMT, GMT_OUT, 0, GMT_IS_ABSTIME);	/* Common for both tables; other column types set in the two functions */

		if (Ctrl->S.active)
			earthtide_sun_moon_track (GMT, &cal_start, Ctrl->T.T);
		else
			earthtide_solid_ts (GMT, &cal_start, Ctrl->L.x, Ctrl->L.y, Ctrl->T.T);

		if (GMT_End_IO (API, GMT_OUT, 0) != GMT_NOERROR) 	/* Disables further data output */
			Return (API->error);
	}

	gmt_M_toc (GMT,"");		/* Print total run time, but only if -Vt was set */

	Return (GMT_NOERROR);
}
