Uses of Class
de.kah2.zodiac.nova4jmt.api.LnEquPosn

Packages that use LnEquPosn

Package	Description
de.kah2.zodiac.nova4jmt
de.kah2.zodiac.nova4jmt.solarsystem
de.kah2.zodiac.nova4jmt.util

Uses of LnEquPosn in de.kah2.zodiac.nova4jmt

Methods in de.kah2.zodiac.nova4jmt with parameters of type LnEquPosn

Modifier and Type	Method and Description
static int	RiseSet.check_coords(LnLnlatPosn observer, double H1, BigDecimal horizon, LnEquPosn object)
static int	RiseSet.check_coords(LnLnlatPosn observer, double H1, double horizon, LnEquPosn object)
static void	Utility.ln_equ_to_hequ(LnEquPosn pos, LnhEquPosn hpos) void ln_equ_to_hequ(LnEquPosn pos, LnhEquPosn hpos) \brief human double equatorial position to human readable equatorial position \ingroup conversion
static double	AngularSeparation.ln_get_angular_separation(LnEquPosn posn1, LnEquPosn posn2) Chap 17 page 115
static void	ApparentPosition.ln_get_apparent_posn(LnEquPosn mean_position, LnEquPosn proper_motion, double JD, LnEquPosn position) void ln_get_apparent_posn(struct ln_equ_posn *mean_position, struct ln_equ_posn *proper_motion, double JD, struct ln_equ_posn *position) \param mean_position Mean position of object \param proper_motion Proper motion of object \param JD Julian Day \param position Pointer to store new object position Calculate the apparent equatorial position of a star from its mean equatorial position.
static void	Transform.ln_get_ecl_from_equ(LnEquPosn object, double JD, LnLnlatPosn position) Equ 12.1, 12.2 Pg 88
static void	EllipticMotion.ln_get_ell_body_equ_coords(double JD, LnEllOrbit orbit, LnEquPosn posn) void ln_get_ell_body_equ_coords(double JD, LnEllOrbit orbit, LnEquPosn posn) \param JD Julian Day.
static void	Aberration.ln_get_equ_aber(LnEquPosn mean_position, double JD, LnEquPosn position) Equ 22.1, 22.1, 22.3, 22.4
static void	Transform.ln_get_equ_from_ecl(LnLnlatPosn object, double JD, LnEquPosn position) Equ 12.3, 12.4 pg 89
static void	Transform.ln_get_equ_from_gal(LnGalPosn gal, LnEquPosn equ) Pg 94
static void	Transform.ln_get_equ_from_hrz(LnHrzPosn object, LnLnlatPosn observer, double JD, LnEquPosn position) void ln_get_equ_from_hrz( ln_hrz_posn *object, LnLnlatPosnobserver, double JD, LnEquPosn position) \param object Object coordinates.
static void	ProperMotion.ln_get_equ_pm_epoch(LnEquPosn mean_position, LnEquPosn proper_motion, double JD, double epoch_JD, LnEquPosn position) Example 20.b, pg 126
static void	ProperMotion.ln_get_equ_pm(LnEquPosn mean_position, LnEquPosn proper_motion, double JD, LnEquPosn position) Example 20.b pg 126
static void	Precession.ln_get_equ_prec(LnEquPosn mean_position, double JD, LnEquPosn position) void ln_get_equ_prec(struct ln_equ_posn *mean_position, double JD, struct ln_equ_posn *position) \param mean_position Mean object position \param JD Julian day \param position Pointer to store new object position.
static void	Precession.ln_get_equ_prec2(LnEquPosn mean_position, double fromJD, double toJD, LnEquPosn position) void ln_get_equ_prec2(struct ln_equ_posn *mean_position, double fromJD, double toJD, struct ln_equ_posn *position); \param mean_position Mean object position \param fromJD Julian day (start) \param toJD Julian day (end) \param position Pointer to store new object position.
static void	Transform.ln_get_equ2000_from_gal(LnGalPosn gal, LnEquPosn equ) void ln_get_equ2000_from_gal( LnGalPosn gal, LnEquPosn equ) \param gal Galactic coordinates.
static void	Transform.ln_get_gal_from_equ(LnEquPosn equ, LnGalPosn gal) Pg 94
static void	Transform.ln_get_gal_from_equ2000(LnEquPosn equ, LnGalPosn gal) void ln_get_gal_from_equ2000( LnEquPosn equ, LnGalPosn gal) \param equ J2000 equatorial coordinates.
static double	HeliocentricTime.ln_get_heliocentric_time_diff(double JD, LnEquPosn object) double ln_get_heliocentric_time_diff(double JD, struct ln_equ_posn *object) \param JD Julian day \param object Pointer to object (RA, DEC) for which heliocentric correction will be caculated \return Heliocentric correction in fraction of day Calculate heliocentric corection for object at given coordinates and on given date.
static void	Transform.ln_get_hrz_from_equ_sidereal_time(LnEquPosn object, LnLnlatPosn observer, double sidereal, LnHrzPosn position)
static void	Transform.ln_get_hrz_from_equ(LnEquPosn object, LnLnlatPosn observer, double JD, LnHrzPosn position) Equ 12.1,12.2 pg 88 TODO: Transform horizontal coordinates to galactic coordinates.
static void	HyperbolicMotion.ln_get_hyp_body_equ_coords(double JD, LnHypOrbit orbit, LnEquPosn posn) void ln_get_hyp_body_equ_coords(double JD, LnHypOrbit orbit, LnEquPosn posn) \param JD Julian Day.
static int	RiseSet.ln_get_object_next_rst_horizon(double JD, LnLnlatPosn observer, LnEquPosn object, BigDecimal horizon, LnRstTime rst) int ln_get_object_next_rst_horizon(double JD, LnLnlatPosn observer, LnEquPosn object, double horizon, LnRstTime rst); \param JD Julian day \param observer Observers position \param object Object position \param horizon Horizon height \param rst Pointer to store Rise, Set and Transit time in JD \return 0 for success, 1 for circumpolar (above the horizon), -1 for circumpolar (bellow the horizon) Calculate the time of next rise, set and transit (crosses the local meridian at upper culmination) time of the object for the given Julian day and horizon.
static int	RiseSet.ln_get_object_next_rst(double JD, LnLnlatPosn observer, LnEquPosn object, LnRstTime rst) int ln_get_object_next_rst(double JD, LnLnlatPosn observer, LnEquPosn object, LnRstTime rst); \param JD Julian day \param observer Observers position \param object Object position \param rst Pointer to store Rise, Set and Transit time in JD \return 0 for success, 1 for circumpolar (above the horizon), -1 for circumpolar (bellow the horizon) Calculate the time of next rise, set and transit (crosses the local meridian at upper culmination) time of the object for the given Julian day and horizon.
static int	RiseSet.ln_get_object_rst_horizon_offset(double JD, LnLnlatPosn observer, LnEquPosn object, BigDecimal horizon, LnRstTime rst, double ut_offset)
static int	RiseSet.ln_get_object_rst_horizon(double JD, LnLnlatPosn observer, LnEquPosn object, BigDecimal horizon, LnRstTime rst) int ln_get_object_rst_horizon(double JD, LnLnlatPosn observer, LnEquPosn object, long double horizon, LnRstTime rst); \param JD Julian day \param observer Observers position \param object Object position \param horizon Horizon height \param rst Pointer to store Rise, Set and Transit time in JD \return 0 for success, 1 for circumpolar (above the horizon), -1 for circumpolar (bellow the horizon) Calculate the time the rise, set and transit (crosses the local meridian at upper culmination) time of the object for the given Julian day and horizon.
static int	RiseSet.ln_get_object_rst(double JD, LnLnlatPosn observer, LnEquPosn object, LnRstTime rst) int ln_get_object_rst(double JD, LnLnlatPosn observer, LnEquPosn object, LnRstTime rst); \param JD Julian day \param observer Observers position \param object Object position \param rst Pointer to store Rise, Set and Transit time in JD \return 0 for success, 1 for circumpolar (above the horizon), -1 for circumpolar (bellow the horizon) Calculate the time the rise, set and transit (crosses the local meridian at upper culmination) time of the object for the given Julian day.
static void	ParabolicMotion.ln_get_par_body_equ_coords(double JD, LnParOrbit orbit, LnEquPosn posn) void ln_get_par_body_equ_coords(double JD, LnParOrbit orbit, LnEquPosn posn) \param JD Julian Day.
static void	Parallax.ln_get_parallax_ha(LnEquPosn object, double au_distance, LnLnlatPosn observer, double height, double H, LnEquPosn parallax) Equ 39.1, 39.2, 39.3 Pg 263 and 264
static void	Parallax.ln_get_parallax(LnEquPosn object, double au_distance, LnLnlatPosn observer, double height, double JD, LnEquPosn parallax) Equ 39.1, 39.2, 39.3 Pg 263 and 264
static double	AngularSeparation.ln_get_rel_posn_angle(LnEquPosn posn1, LnEquPosn posn2) Chapt 17, page 116
static void	Utility.ln_hequ_to_equ(LnhEquPosn hpos, LnEquPosn pos) void ln_hequ_to_equ(LnhEquPosn hpos, LnEquPosn pos) \brief human readable equatorial position to double equatorial position \ingroup conversion

Uses of LnEquPosn in de.kah2.zodiac.nova4jmt.solarsystem

Methods in de.kah2.zodiac.nova4jmt.solarsystem with parameters of type LnEquPosn

Modifier and Type	Method and Description
static void	Jupiter.ln_get_jupiter_equ_coords(double JD, LnEquPosn position) void ln_get_jupiter_equ_coords(double JD, LnEquPosn position); \param JD julian Day \param position Pointer to store position Calculates Jupiter's equatorial position for given julian day.
static void	Lunar.ln_get_lunar_equ_coords_prec(double JD, LnEquPosn position, double precision) void ln_get_lunar_equ_coords_prec(double JD, LnEquPosn position, double precision); \param JD Julian Day \param position Pointer to a LnLnlatPosn to store result.
static void	Lunar.ln_get_lunar_equ_coords(double JD, LnEquPosn position) void ln_get_lunar_equ_coords(double JD, LnEquPosn position); \param JD Julian Day \param position Pointer to a LnLnlatPosn to store result.
static void	Mars.ln_get_mars_equ_coords(double JD, LnEquPosn position) void ln_get_mars_equ_coords(double JD, LnEquPosn position); \param JD julian Day \param position Pointer to store position Calculates Mars equatorial position for given julian day.
static void	Mercury.ln_get_mercury_equ_coords(double JD, LnEquPosn position) void ln_get_mercury_equ_coords(double JD, LnEquPosn position); \param JD julian Day \param position Pointer to store position Calculates Mercury's equatorial position for given julian day.
static void	Neptune.ln_get_neptune_equ_coords(double JD, LnEquPosn position) void ln_get_neptune_equ_coords(double JD, LnEquPosn position); \param JD julian Day \param position Pointer to store position Calculates Neptune's equatorial position for given julian day.
static void	Pluto.ln_get_pluto_equ_coords(double JD, LnEquPosn position) void ln_get_pluto_equ_coords(double JD, LnEquPosn position); \param JD julian Day \param position Pointer to store position Calculates Pluto's equatorial position for the given julian day.
static void	Saturn.ln_get_saturn_equ_coords(double JD, LnEquPosn position) void ln_get_saturn_equ_coords(double JD, LnEquPosn position); \param JD julian Day \param position Pointer to store position Calculates Saturn's equatorial position for given julian day.
static void	Solar.ln_get_solar_equ_coords(double JD, LnEquPosn position) void ln_get_solar_equ_coords(double JD, LnEquPosn position) \param JD Julian day \param position Pointer to store calculated solar position.
static void	Uranus.ln_get_uranus_equ_coords(double JD, LnEquPosn position) void ln_get_uranus_equ_coords(double JD, LnEquPosn position); \param JD julian Day \param position pointer to store position Calculates uranus's equatorial position for given julian day.
static void	Venus.ln_get_venus_equ_coords(double JD, LnEquPosn position) void ln_get_venus_equ_coords(double JD, LnEquPosn *position); \param JD Julian Day \param position Pointer to store position Calculates Venus's equatorial position for given julian day.

Uses of LnEquPosn in de.kah2.zodiac.nova4jmt.util

Methods in de.kah2.zodiac.nova4jmt.util with parameters of type LnEquPosn

Modifier and Type	Method and Description
void	IGetEquBodyCoords.get_equ_body_coords(double JD, LnEquPosn position)
void	IGetMotionBodyCoords.get_motion_body_coords(double JD, T orbit, LnEquPosn posn)