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SuperNOVAS v1.5
The NOVAS C library, made better
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This module provides a set of functions that define an astronomical observer location, or ones that relate to observer location. More...
Functions | |
int | aberration (const double *pos, const double *vobs, double lighttime, double *out) |
Corrects position vector for aberration of light. | |
int | bary2obs (const double *pos, const double *pos_obs, double *out, double *restrict lighttime) |
Moves the origin of coordinates from the barycenter of the solar system to the observer (or the geocenter); i.e., this function accounts for parallax (annual+geocentric or just annual). | |
short | light_time (double jd_tdb, const object *restrict body, const double *pos_obs, double tlight0, enum novas_accuracy accuracy, double *pos_src_obs, double *restrict tlight) |
Computes the geocentric position of a solar system body, as antedated for light-time. | |
int | light_time2 (double jd_tdb, const object *restrict body, const double *restrict pos_obs, double tlight0, enum novas_accuracy accuracy, double *p_src_obs, double *restrict v_ssb, double *restrict tlight) |
Computes the geocentric position and velocity of a solar system body, as antedated for light-time. | |
int | make_airborne_observer (const on_surface *location, const double *vel, observer *obs) |
Populates an 'observer' data structure for an observer moving relative to the surface of Earth, such as an airborne observer. | |
int | make_gps_observer (double latitude, double longitude, double height, observer *obs) |
Initializes an observer data structure for a ground-based observer with the specified GPS / WGS84 location, and sets mean (annual) weather parameters based on that location. | |
int | make_gps_site (double latitude, double longitude, double height, on_surface *site) |
Initializes an observing site with the specified GPS / WGS84 location, and sets mean (annual) weather parameters based on that location. | |
int | make_in_space (const double *sc_pos, const double *sc_vel, in_space *loc) |
Populates an 'in_space' data structure, for an observer situated on a near-Earth spacecraft, with the provided position and velocity components. | |
int | make_itrf_observer (double latitude, double longitude, double height, observer *obs) |
Initializes an observer data structure for a ground-based observer with the specified International Terrestrial Reference Frame (ITRF) / GRS80 location, and sets mean (annual) weather parameters based on that location. | |
int | make_itrf_site (double latitude, double longitude, double height, on_surface *site) |
Initializes an observing site with the specified International Terrestrial Reference Frame (ITRF) / GRS80 location, and sets mean (annual) weather parameters based on that location. | |
short | make_observer (enum novas_observer_place where, const on_surface *loc_surface, const in_space *loc_space, observer *obs) |
int | make_observer_at_geocenter (observer *restrict obs) |
Populates an 'observer' data structure for a hypothetical observer located at Earth's geocenter. | |
int | make_observer_at_site (const on_surface *restrict site, observer *restrict obs) |
Initializes an observer data structure for a ground-based observer at the specified observing site, and sets mean (annual) weather parameters based on that location. | |
int | make_observer_in_space (const double *sc_pos, const double *sc_vel, observer *obs) |
Populates an 'observer' data structure, for an observer situated on a near-Earth spacecraft, with the specified geocentric position and velocity vectors. | |
int | make_observer_on_surface (double latitude, double longitude, double height, double temperature, double pressure, observer *restrict obs) |
int | make_on_surface (double latitude, double longitude, double height, double temperature, double pressure, on_surface *restrict loc) |
int | make_solar_system_observer (const double *sc_pos, const double *sc_vel, observer *obs) |
Populates an 'observer' data structure, for an observer situated on a near-Earth spacecraft, with the specified geocentric position and velocity vectors. | |
int | make_xyz_site (const double *restrict xyz, on_surface *restrict site) |
Initializes an observing site with the specified Cartesian geocentric xyz location, and sets mean (annual) weather parameters based on that location. | |
int | novas_set_default_weather (on_surface *site) |
Sets default weather parameters based on an approximate global model to the mean annualized temperatures, based on Feulner et al. | |
int | obs_planets (double jd_tdb, enum novas_accuracy accuracy, const double *restrict pos_obs, int pl_mask, novas_planet_bundle *restrict planets) |
Calculates the positions and velocities for the Solar-system bodies, e.g. | |
int | obs_posvel (double jd_tdb, double ut1_to_tt, enum novas_accuracy accuracy, const observer *restrict obs, const double *restrict geo_pos, const double *restrict geo_vel, double *restrict pos, double *restrict vel) |
Calculates the ICRS position and velocity of the observer relative to the Solar System Barycenter (SSB). | |
This module provides a set of functions that define an astronomical observer location, or ones that relate to observer location.
The following type of observer locations are supported:
make_gps_observer()
make_itrs_observer()
make_xyz_site()
and make_site_observer()
b. airborne observers, via a location (e.g. make_gps_site()
, make_itrf_site()
or make_xyz_site()
), and a ground velocity using make_airborne_observer()
.make_observer_in_space()
specifying momentary position and velocity w.r.t. the geocenter.make_observer_at_geocecenter()
.make_solar_system_observer()
, specifying a momentary barycentric (that is w.r.t. the SSB) position and velocity vector.Once an observer is defined, it maybe used to set up an observing frame for a specific time of observation. Observing frames allow efficient and precise position calculations from an observer's point-of-view.
int aberration | ( | const double * | pos, |
const double * | vobs, | ||
double | lighttime, | ||
double * | out ) |
Corrects position vector for aberration of light.
Algorithm includes relativistic terms.
NOTES:
place()
to account for aberration when calculating the position of the source. REFERENCES:
pos | [AU] Position vector of source relative to observer | |
vobs | [AU/day] Velocity vector of observer, relative to the solar system barycenter. | |
lighttime | [day] Light time from object to Earth (if known). Or set to 0, and this function will compute it as needed. | |
[out] | out | [AU] Position vector, referred to origin at center of mass of the Earth, corrected for aberration. It can be the same vector as one of the inputs. |
References novas_vlen().
int bary2obs | ( | const double * | pos, |
const double * | pos_obs, | ||
double * | out, | ||
double *restrict | lighttime ) |
Moves the origin of coordinates from the barycenter of the solar system to the observer (or the geocenter); i.e., this function accounts for parallax (annual+geocentric or just annual).
REFERENCES:
pos | [AU] Position vector, referred to origin at solar system barycenter. | |
pos_obs | [AU] Position vector of observer (or the geocenter), with respect to origin at solar system barycenter. | |
[out] | out | [AU] Position vector, referred to origin at center of mass of the Earth. It may be NULL if not required, or be the same vector as either of the inputs. |
[out] | lighttime | [day] Light time from object to Earth. It may be NULL if not required. |
References novas_vlen().
short light_time | ( | double | jd_tdb, |
const object *restrict | body, | ||
const double * | pos_obs, | ||
double | tlight0, | ||
enum novas_accuracy | accuracy, | ||
double * | pos_src_obs, | ||
double *restrict | tlight ) |
Computes the geocentric position of a solar system body, as antedated for light-time.
jd_tdb | [day] Barycentric Dynamical Time (TDB) based Julian date | |
body | Pointer to structure containing the designation for the solar system body | |
pos_obs | [AU] Position 3-vector of observer (or the geocenter), with respect to origin at solar system barycenter, referred to ICRS axes. | |
tlight0 | [day] First approximation to light-time (can be set to 0.0 if not readily available – it will then be computed as needed). | |
accuracy | NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1) | |
[out] | pos_src_obs | [AU] Position 3-vector of body, with respect to origin at observer (or the geocenter), referred to ICRS axes. It can be the same vector as either of the inputs. |
[out] | tlight | [day] Calculated light time |
References light_time2().
int light_time2 | ( | double | jd_tdb, |
const object *restrict | body, | ||
const double *restrict | pos_obs, | ||
double | tlight0, | ||
enum novas_accuracy | accuracy, | ||
double * | p_src_obs, | ||
double *restrict | v_ssb, | ||
double *restrict | tlight ) |
Computes the geocentric position and velocity of a solar system body, as antedated for light-time.
It is effectively the same as the original NOVAS C light_time(), except that this returns the antedated source velocity vector also.
NOTES:
novas_geom_posvel()
or place()
to calculate observed positions, radial velocity, and distance for the time when the observed light originated from the source. jd_tdb | [day] Barycentric Dynamical Time (TDB) based Julian date | |
body | Pointer to structure containing the designation for the solar system body | |
pos_obs | [AU] Position 3-vector of observer (or the geocenter), with respect to origin at solar system barycenter, referred to ICRS axes. | |
tlight0 | [day] First approximation to light-time (can be set to 0.0 if not readily avasilable – so it will be calculated as needed). | |
accuracy | NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1) | |
[out] | p_src_obs | [AU] Position 3-vector of body, relative to observer, referred to ICRS axes, components in AU. |
[out] | v_ssb | [AU/day] Velocity 3-vector of body, with respect to the Solar-system barycenter, referred to ICRS axes. |
[out] | tlight | [day] Calculated light time, or NAN when returning with an error code. |
References bary2obs(), ephemeris(), NOVAS_BARYCENTER, NOVAS_FULL_ACCURACY, and novas_inv_max_iter.
int make_airborne_observer | ( | const on_surface * | location, |
const double * | vel, | ||
observer * | obs ) |
Populates an 'observer' data structure for an observer moving relative to the surface of Earth, such as an airborne observer.
Airborne observers have an earth fixed momentary location, defined by longitude, latitude, and altitude, the same was as for a stationary observer on Earth, but are moving relative to the surface, such as in an aircraft or balloon observatory.
location | Current geodetic location, e.g. as populated with make_gps_site() or similar. | |
vel | [km/s] Surface velocity. | |
[out] | obs | Pointer to data structure to populate. |
References IN_SPACE_INIT, make_observer(), NOVAS_AIRBORNE_OBSERVER, and in_space::sc_vel.
int make_gps_observer | ( | double | latitude, |
double | longitude, | ||
double | height, | ||
observer * | obs ) |
Initializes an observer data structure for a ground-based observer with the specified GPS / WGS84 location, and sets mean (annual) weather parameters based on that location.
For the highest (μas / mm level) precision, you probably should use an ITRF location instead of a GPS based location.
latitude | [deg] Geodetic (GPS / WGS84) latitude north positive. | |
longitude | [deg] Geodetic (GPS / WGS84) longitude east positive. | |
height | [m] Geodetic (GPS / WGS84) altitude above sea level of the observer. | |
[out] | obs | Pointer to the data structure to populate. |
References make_gps_site(), and make_observer_at_site().
int make_gps_site | ( | double | latitude, |
double | longitude, | ||
double | height, | ||
on_surface * | site ) |
Initializes an observing site with the specified GPS / WGS84 location, and sets mean (annual) weather parameters based on that location.
For the highest (μas / mm level) precision, you probably should use an ITRF location instead of a GPS based location.
latitude | [deg] Geodetic (GPS / WGS84) latitude; north positive. | |
longitude | [deg] Geodetic (GPS / WGS84) longitude; east positive. | |
height | [m] Geodetic (GPS / WGS84) altitude above sea level of the observer. | |
[out] | site | Pointer to the data structure to populate. |
References make_itrf_site(), novas_cartesian_to_geodetic(), novas_geodetic_to_cartesian(), NOVAS_GRS80_ELLIPSOID, and NOVAS_WGS84_ELLIPSOID.
int make_in_space | ( | const double * | sc_pos, |
const double * | sc_vel, | ||
in_space * | loc ) |
Populates an 'in_space' data structure, for an observer situated on a near-Earth spacecraft, with the provided position and velocity components.
Both input vectors are assumed with respect to true equator and equinox of date.
sc_pos | [km] Geocentric (x, y, z) position vector. NULL defaults to the origin | |
sc_vel | [km/s] Geocentric (x, y, z) velocity vector. NULL defaults to zero speed. | |
[out] | loc | Pointer to earth-orbit location data structure to populate. |
References in_space::sc_pos, and in_space::sc_vel.
int make_itrf_observer | ( | double | latitude, |
double | longitude, | ||
double | height, | ||
observer * | obs ) |
Initializes an observer data structure for a ground-based observer with the specified International Terrestrial Reference Frame (ITRF) / GRS80 location, and sets mean (annual) weather parameters based on that location.
For the highest precision (μas level) applications you should make sure that the location provided here and the Earth-orientation parameters (EOP) used (in setting novas_timescale
and in novas_make_frame()
) are provided in the same ITRF realization. You can use novas_itrf_transform_eop()
to change the ITRF realization for the EOP values, if necessary.
latitude | [deg] Geodetic (ITRF / GRS80) latitude; north positive. | |
longitude | [deg] Geodetic (ITRF / GRS80) longitude; east positive. | |
height | [m] Geodetic (ITRF / GRS80) altitude above sea level of the observer. | |
[out] | obs | Pointer to the data structure to populate. |
References make_itrf_site(), and make_observer_at_site().
int make_itrf_site | ( | double | latitude, |
double | longitude, | ||
double | height, | ||
on_surface * | site ) |
Initializes an observing site with the specified International Terrestrial Reference Frame (ITRF) / GRS80 location, and sets mean (annual) weather parameters based on that location.
For the highest precision (μas level) applications you should make sure that the location provided here and the Earth-orientation parameters (EOP) used (in setting novas_timescale
and in novas_make_frame()
) are provided in the same ITRF realization. You can use novas_itrf_transform_eop()
to change the ITRF realization for the EOP values, if necessary.
latitude | [deg] Geodetic (ITRF / GRS80) latitude; north positive. | |
longitude | [deg] Geodetic (ITRF / GRS80) longitude; east positive. | |
height | [m] Geodetic (ITRF / GRS80) altitude above sea level of the observer. | |
[out] | site | Pointer to the data structure to populate. |
References on_surface::height, on_surface::latitude, on_surface::longitude, and novas_set_default_weather().
short make_observer | ( | enum novas_observer_place | where, |
const on_surface * | loc_surface, | ||
const in_space * | loc_space, | ||
observer * | obs ) |
make_itrf_observer()
, make_gps_observer()
, make_observer_at_site()
, make_airborne_observer()
make_solar_system_observer(), or
make_observer_at_geocenter()`. This function will be available for the foreseeable future also.Populates an 'observer' data structure given the parameters. The output data structure may be used an the the inputs to NOVAS-C functions, such as make_frame()
or place()
.
where | The location type of the observer | |
loc_surface | Pointer to data structure that defines a location on Earth's surface. Used only if 'where' is NOVAS_OBSERVER_ON_EARTH, otherwise can be NULL. | |
loc_space | Pointer to data structure that defines a near-Earth location in space. Used only if 'where' is NOVAS_OBSERVER_IN_EARTH_ORBIT, otherwise can be NULL. | |
[out] | obs | Pointer to observer data structure to populate. |
References observer::near_earth, NOVAS_AIRBORNE_OBSERVER, NOVAS_OBSERVER_AT_GEOCENTER, NOVAS_OBSERVER_IN_EARTH_ORBIT, NOVAS_OBSERVER_ON_EARTH, NOVAS_SOLAR_SYSTEM_OBSERVER, observer::on_surf, in_space::sc_vel, and observer::where.
int make_observer_at_geocenter | ( | observer *restrict | obs | ) |
Populates an 'observer' data structure for a hypothetical observer located at Earth's geocenter.
The output data structure may be used an the the inputs to NOVAS-C functions, such as make_frame()
or place()
.
[out] | obs | Pointer to data structure to populate. |
References make_observer(), and NOVAS_OBSERVER_AT_GEOCENTER.
int make_observer_at_site | ( | const on_surface *restrict | site, |
observer *restrict | obs ) |
Initializes an observer data structure for a ground-based observer at the specified observing site, and sets mean (annual) weather parameters based on that location.
site | Pointer to observing site data structure. | |
[out] | obs | Pointer to the data structure to populate. |
References NOVAS_OBSERVER_ON_EARTH.
int make_observer_in_space | ( | const double * | sc_pos, |
const double * | sc_vel, | ||
observer * | obs ) |
Populates an 'observer' data structure, for an observer situated on a near-Earth spacecraft, with the specified geocentric position and velocity vectors.
Both input vectors are with respect to true equator and equinox of date. The output data structure may be used an the the inputs to NOVAS-C functions, such as make_frame()
or place()
.
sc_pos | [km] Geocentric (x, y, z) position vector. | |
sc_vel | [km/s] Geocentric (x, y, z) velocity vector. | |
[out] | obs | Pointer to the data structure to populate |
References make_in_space(), make_observer(), and NOVAS_OBSERVER_IN_EARTH_ORBIT.
int make_observer_on_surface | ( | double | latitude, |
double | longitude, | ||
double | height, | ||
double | temperature, | ||
double | pressure, | ||
observer *restrict | obs ) |
make_itrf_observer()
, make_gps_observer()
, or make_observer_at_site()
instead (all of which set default mean annual weather parameters for approximate refraction correction), and optionally set actual weather data afterwards, based on the measurements available. This function will be available for the foreseeable future also.Initializes an observer data structure with the specified ITRF / GRS80 location, and he specified local pressure and temperature. This old NOVAS C function does not set humidity. Thus, if humidity is needed for refraction correction, then you should set it explicitly after this call.
NOTES:
novas_itrf_transform()
, possibly after novas_geodetic_to_cartesian()
with NOVAS_GRS80_ELLIPSOID
as necessary for polar ITRF coordinates. novas_cartesian_to_geodetic()
with NOVAS_GRS80_ELLIPSOID
as the reference ellipsoid parameter. latitude | [deg] Geodetic (ITRF / GRS80) latitude; north positive. | |
longitude | [deg] Geodetic (ITRF / GRS80) longitude; east positive. | |
height | [m] Geodetic (ITRF / GRS80) altitude above sea level of the observer. | |
temperature | [C] Temperature (degrees Celsius). | |
pressure | [mbar] Atmospheric pressure. | |
[out] | obs | Pointer to the data structure to populate. |
References make_observer(), make_on_surface(), and NOVAS_OBSERVER_ON_EARTH.
int make_on_surface | ( | double | latitude, |
double | longitude, | ||
double | height, | ||
double | temperature, | ||
double | pressure, | ||
on_surface *restrict | loc ) |
make_itrf_site()
or make_gps_site()
instead (both of which set default mean annual weather parameters for approximate refraction correction), and optionally set actual weather data afterwards, based on the measurements available. This function will be available for the foreseeable future also.Populates an 'on_surface' data structure, for an observer on the surface of the Earth, with the given parameters.
Note, that because this is an original NOVAS C routine, it does not have an argument to set a humidity value (e.g. for radio refraction). As such, the humidity is set to a a default mean annual value for the location. To set an actual humidity, set the output structure's field after calling this funcion.
NOTES
humidity
) that was not yet part of the on_surface
structure in v1.0. As such, linking SuperNOVAS v1.1 or later with application code compiled for SuperNOVAS v1.0 can result in memory corruption or segmentation fault when this function is called. To be safe, make sure your application has been (re)compiled against SuperNOVAS v1.1 or later. novas_itrf_transform()
, possibly after novas_geodetic_to_cartesian()
with NOVAS_GRS80_ELLIPSOID
as necessary for polar ITRF coordinates. novas_cartesian_to_geodetic()
with NOVAS_GRS80_ELLIPSOID
as the reference ellipsoid parameter. make_gps_site()
instead, and then set weather parameters afterwards as necessary. latitude | [deg] Geodetic (ITRF / GRS80) latitude; north positive. | |
longitude | [deg] Geodetic (ITRF / GRS80) longitude; east positive. | |
height | [m] Geodetic (ITRF / GSR80) altitude above sea level of the observer. | |
temperature | [C] Temperature (degrees Celsius) [-120:70]. | |
pressure | [mbar] Atmospheric pressure [0:1200]. | |
[out] | loc | Pointer to Earth location data structure to populate. |
References make_itrf_site().
int make_solar_system_observer | ( | const double * | sc_pos, |
const double * | sc_vel, | ||
observer * | obs ) |
Populates an 'observer' data structure, for an observer situated on a near-Earth spacecraft, with the specified geocentric position and velocity vectors.
Solar-system observers are similar to observers in Earth-orbit but their momentary position and velocity is defined relative to the Solar System Barycenter, instead of the geocenter.
sc_pos | [AU] Solar-system barycentric (x, y, z) position vector in ICRS. | |
sc_vel | [AU/day] Solar-system barycentric (x, y, z) velocity vector in ICRS. | |
[out] | obs | Pointer to the data structure to populate |
References make_in_space(), make_observer(), and NOVAS_SOLAR_SYSTEM_OBSERVER.
int make_xyz_site | ( | const double *restrict | xyz, |
on_surface *restrict | site ) |
Initializes an observing site with the specified Cartesian geocentric xyz location, and sets mean (annual) weather parameters based on that location.
For the highest precision (μas level) applications you should make sure that the site coordinates and the Earth-orientation parameters (EOP) used (in setting novas_timescale
and in novas_make_frame()
) are provided in the same ITRF realization. You can use novas_itrf_transform()
or novas_itrf_transform_eop()
to change the ITRF realization for the site coordinates and/or the EOP values, if necessary.
xyz | [m] Cartesian geocentric position. | |
[out] | site | Pointer to the data structure to populate. |
References make_itrf_site(), novas_cartesian_to_geodetic(), and NOVAS_GRS80_ELLIPSOID.
int novas_set_default_weather | ( | on_surface * | site | ) |
Sets default weather parameters based on an approximate global model to the mean annualized temperatures, based on Feulner et al.
(2013), and scaling relations with altitude (up to 12 km).
Humidity is set to 70% at sea level (which is a typical value globally), and adjusted to decrease with altitude linearly at a rate of 7.5% per km up to 8000 meters. Above that a quadratic model is assumed, peaking at 45% at 14 km – based on the measured distribution by Mendez-Astudillo et al. (2021). Finally above 20.8 km, zero humidity is assumed.
These parameters are all very approximate, but in the absence of measured data, they represent a best guess default model of sorts.
REFERENCES:
[in,out] | site | Site containing geodetic loation as input, and poulated with typical mean weather parameters for the output. |
References on_surface::height, on_surface::humidity, on_surface::latitude, on_surface::pressure, and on_surface::temperature.
int obs_planets | ( | double | jd_tdb, |
enum novas_accuracy | accuracy, | ||
const double *restrict | pos_obs, | ||
int | pl_mask, | ||
novas_planet_bundle *restrict | planets ) |
Calculates the positions and velocities for the Solar-system bodies, e.g.
for use for gravitational deflection calculations. The planet positions are calculated relative to the observer location, while velocities are w.r.t. the SSB. Both positions and velocities are antedated for light travel time, so they accurately reflect the apparent position (and barycentric motion) of the bodies from the observer's perspective.
jd_tdb | [day] Barycentric Dynamical Time (TDB) based Julian date | |
accuracy | NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1). In full accuracy mode, it will calculate the deflection due to the Sun, Jupiter, Saturn and Earth. In reduced accuracy mode, only the deflection due to the Sun is calculated. | |
pos_obs | [AU] Position 3-vector of observer (or the geocenter), with respect to origin at solar system barycenter, referred to ICRS axes. | |
pl_mask | Bitwise (1 << planet-number) mask indicating which planets to request data for. See enum novas_planet for the enumeration of planet numbers. | |
[out] | planets | Pointer to apparent planet data to populate. The planets with non-zero mask bits will have have positions and velocities calculated. See enum novas_planet for the enumeration of planet numbers. |
References light_time2(), make_planet(), novas_debug(), NOVAS_DEBUG_EXTRA, NOVAS_DEBUG_OFF, novas_get_debug_mode(), NOVAS_PLANETS, and NOVAS_SUN.
int obs_posvel | ( | double | jd_tdb, |
double | ut1_to_tt, | ||
enum novas_accuracy | accuracy, | ||
const observer *restrict | obs, | ||
const double *restrict | geo_pos, | ||
const double *restrict | geo_vel, | ||
double *restrict | pos, | ||
double *restrict | vel ) |
Calculates the ICRS position and velocity of the observer relative to the Solar System Barycenter (SSB).
jd_tdb | [day] Barycentric Dynamical Time (TDB) based Julian date. | |
ut1_to_tt | [s] TT - UT1 time difference. Used only when 'location->where' is NOVAS_OBSERVER_ON_EARTH (1) or NOVAS_OBSERVER_IN_EARTH_ORBIT (2). | |
accuracy | NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1) | |
obs | The observer location, relative to which the output positions and velocities are to be calculated | |
geo_pos | [AU] ICRS position vector of the geocenter w.r.t. the Solar System Barycenter (SSB). If either geo_pos or geo_vel is NULL, it will be calculated when needed. | |
geo_vel | [AU/day] ICRS velocity vector of the geocenter w.r.t. the Solar System Barycenter (SSB). If either geo_pos or geo_vel is NULL, it will be calculated when needed. | |
[out] | pos | [AU] Position 3-vector of the observer w.r.t. the Solar System Barycenter (SSB). It may be NULL if not required. |
[out] | vel | [AU/day] Velocity 3-vector of the observer w.r.t. the Solar System Barycenter (SSB). It must be distinct from the pos output vector, and may be NULL if not required. |
References ephemeris(), geo_posvel(), NOVAS_AIRBORNE_OBSERVER, NOVAS_BARYCENTER, NOVAS_EARTH_INIT, NOVAS_OBSERVER_IN_EARTH_ORBIT, NOVAS_OBSERVER_ON_EARTH, NOVAS_OBSERVER_PLACES, NOVAS_SOLAR_SYSTEM_OBSERVER, and tt2tdb().