From c0b6c80e567c79f156a97d0560056a14e9caab77 Mon Sep 17 00:00:00 2001 From: github-actions Date: Sat, 9 Nov 2024 12:17:31 +0000 Subject: [PATCH] [automated site update] --- .../dir_68267d1309a1af8e8297ef4c3efbcdba.html | 4 + .../dir_68267d1309a1af8e8297ef4c3efbcdba.js | 2 + .../dir_d44c64559bbebec7f509842c48db8b23.html | 2 + .../dir_d44c64559bbebec7f509842c48db8b23.js | 1 + apidoc/html/files.html | 37 +- apidoc/html/globals.html | 16 +- apidoc/html/globals_a.html | 140 +++++ apidoc/html/globals_defs.html | 11 + apidoc/html/globals_dup.js | 3 +- apidoc/html/globals_enum.html | 1 + apidoc/html/globals_eval.html | 2 + apidoc/html/globals_func_g.html | 2 + apidoc/html/globals_func_n.html | 14 +- apidoc/html/globals_g.html | 6 +- apidoc/html/globals_n.html | 37 +- apidoc/html/globals_p.html | 4 +- apidoc/html/index.html | 68 ++- apidoc/html/md_CHANGELOG.html | 3 + apidoc/html/md_LEGACY.html | 30 +- apidoc/html/menudata.js | 4 +- apidoc/html/naif_8c.html | 250 +++++++++ apidoc/html/naif_8c.js | 7 + apidoc/html/naif_8h.html | 156 ++++++ apidoc/html/naif_8h.js | 8 + apidoc/html/navtreedata.js | 19 +- apidoc/html/navtreeindex0.js | 230 ++++---- apidoc/html/navtreeindex1.js | 500 +++++++++--------- apidoc/html/navtreeindex2.js | 368 ++++++------- apidoc/html/navtreeindex3.js | 110 ++-- apidoc/html/novas_8c.html | 72 ++- apidoc/html/novas_8c.js | 2 + apidoc/html/novas_8h.html | 8 +- apidoc/html/search/all_10.js | 38 +- apidoc/html/search/all_11.js | 199 +------ apidoc/html/search/all_12.js | 217 +++++++- apidoc/html/search/all_13.js | 67 +-- apidoc/html/search/all_14.js | 69 ++- apidoc/html/search/all_15.js | 87 +-- apidoc/html/search/all_16.js | 98 ++-- apidoc/html/search/all_17.js | 42 +- apidoc/html/search/all_18.js | 16 +- apidoc/html/search/all_19.js | 17 +- apidoc/html/search/all_1a.js | 8 +- apidoc/html/search/all_1b.js | 2 +- apidoc/html/search/all_1c.js | 4 + apidoc/html/search/all_4.js | 37 +- apidoc/html/search/all_5.js | 44 +- apidoc/html/search/all_6.js | 46 +- apidoc/html/search/all_7.js | 59 ++- apidoc/html/search/all_8.js | 57 +- apidoc/html/search/all_9.js | 54 +- apidoc/html/search/all_a.js | 39 +- apidoc/html/search/all_b.js | 26 +- apidoc/html/search/all_c.js | 25 +- apidoc/html/search/all_d.js | 32 +- apidoc/html/search/all_e.js | 11 +- apidoc/html/search/all_f.js | 15 +- apidoc/html/search/defines_0.js | 3 +- apidoc/html/search/defines_1.js | 3 +- apidoc/html/search/defines_2.js | 2 +- apidoc/html/search/defines_3.js | 7 +- apidoc/html/search/defines_4.js | 7 +- apidoc/html/search/defines_5.js | 2 +- apidoc/html/search/defines_6.js | 2 +- apidoc/html/search/defines_7.js | 2 +- apidoc/html/search/defines_8.js | 33 +- apidoc/html/search/defines_9.js | 39 +- apidoc/html/search/defines_a.js | 9 +- apidoc/html/search/defines_b.js | 9 +- apidoc/html/search/defines_c.js | 2 +- apidoc/html/search/defines_d.js | 4 + apidoc/html/search/enums_0.js | 25 +- apidoc/html/search/enumvalues_4.js | 78 +-- apidoc/html/search/files_2.js | 14 +- apidoc/html/search/files_4.js | 11 +- apidoc/html/search/functions_6.js | 18 +- apidoc/html/search/functions_c.js | 80 +-- apidoc/html/search/searchdata.js | 4 +- apidoc/html/solarsystem_8h.html | 225 +++++++- apidoc/html/solarsystem_8h.js | 10 + apidoc/html/solsys-calceph_8c.html | 247 +++++++++ apidoc/html/solsys-calceph_8c.js | 6 + apidoc/html/solsys1_8c.html | 4 +- apidoc/html/super_8c.html | 8 +- apidoc/html/toc.xml | 46 +- apidoc/man/man3/md_CHANGELOG.3 | 6 + apidoc/man/man3/naif.c.3 | 153 ++++++ apidoc/man/man3/naif.h.3 | 50 ++ apidoc/man/man3/novas.c.3 | 74 +++ apidoc/man/man3/novas.h.3 | 6 +- apidoc/man/man3/solarsystem.h.3 | 227 +++++++- apidoc/man/man3/solsys-calceph.c.3 | 135 +++++ apidoc/man/man3/solsys1.c.3 | 4 +- apidoc/man/man3/super.c.3 | 6 +- apidoc/supernovas.tag | 177 +++++++ doc/CHANGELOG.md | 18 + doc/README.md | 84 ++- 97 files changed, 3736 insertions(+), 1530 deletions(-) create mode 100644 apidoc/html/globals_a.html create mode 100644 apidoc/html/naif_8c.html create mode 100644 apidoc/html/naif_8c.js create mode 100644 apidoc/html/naif_8h.html create mode 100644 apidoc/html/naif_8h.js create mode 100644 apidoc/html/search/all_1c.js create mode 100644 apidoc/html/search/defines_d.js create mode 100644 apidoc/html/solsys-calceph_8c.html create mode 100644 apidoc/html/solsys-calceph_8c.js create mode 100644 apidoc/man/man3/naif.c.3 create mode 100644 apidoc/man/man3/naif.h.3 create mode 100644 apidoc/man/man3/solsys-calceph.c.3 diff --git a/apidoc/html/dir_68267d1309a1af8e8297ef4c3efbcdba.html b/apidoc/html/dir_68267d1309a1af8e8297ef4c3efbcdba.html index 145b8680..926b88e7 100644 --- a/apidoc/html/dir_68267d1309a1af8e8297ef4c3efbcdba.html +++ b/apidoc/html/dir_68267d1309a1af8e8297ef4c3efbcdba.html @@ -121,6 +121,8 @@    frames.c   + naif.c +   novas.c    novascon.c @@ -129,6 +131,8 @@    refract.c   + solsys-calceph.c +   solsys-ephem.c    solsys1.c diff --git a/apidoc/html/dir_68267d1309a1af8e8297ef4c3efbcdba.js b/apidoc/html/dir_68267d1309a1af8e8297ef4c3efbcdba.js index 5e327f08..40b15c7c 100644 --- a/apidoc/html/dir_68267d1309a1af8e8297ef4c3efbcdba.js +++ b/apidoc/html/dir_68267d1309a1af8e8297ef4c3efbcdba.js @@ -2,10 +2,12 @@ var dir_68267d1309a1af8e8297ef4c3efbcdba = [ [ "eph_manager.c", "eph__manager_8c.html", "eph__manager_8c" ], [ "frames.c", "frames_8c.html", "frames_8c" ], + [ "naif.c", "naif_8c.html", "naif_8c" ], [ "novas.c", "novas_8c.html", "novas_8c" ], [ "novascon.c", "novascon_8c.html", "novascon_8c" ], [ "nutation.c", "nutation_8c.html", "nutation_8c" ], [ "refract.c", "refract_8c.html", "refract_8c" ], + [ "solsys-calceph.c", "solsys-calceph_8c.html", "solsys-calceph_8c" ], [ "solsys-ephem.c", "solsys-ephem_8c.html", "solsys-ephem_8c" ], [ "solsys1.c", "solsys1_8c.html", "solsys1_8c" ], [ "solsys2.c", "solsys2_8c.html", "solsys2_8c" ], diff --git a/apidoc/html/dir_d44c64559bbebec7f509842c48db8b23.html b/apidoc/html/dir_d44c64559bbebec7f509842c48db8b23.html index 1e55ecf3..0f8e8c6f 100644 --- a/apidoc/html/dir_d44c64559bbebec7f509842c48db8b23.html +++ b/apidoc/html/dir_d44c64559bbebec7f509842c48db8b23.html @@ -117,6 +117,8 @@ + + diff --git a/apidoc/html/dir_d44c64559bbebec7f509842c48db8b23.js b/apidoc/html/dir_d44c64559bbebec7f509842c48db8b23.js index 42b9ac85..4322cc27 100644 --- a/apidoc/html/dir_d44c64559bbebec7f509842c48db8b23.js +++ b/apidoc/html/dir_d44c64559bbebec7f509842c48db8b23.js @@ -1,5 +1,6 @@ var dir_d44c64559bbebec7f509842c48db8b23 = [ + [ "naif.h", "naif_8h.html", "naif_8h" ], [ "novas.h", "novas_8h.html", "novas_8h" ], [ "novascon.h", "novascon_8h.html", "novascon_8h" ], [ "nutation.h", "nutation_8h.html", "nutation_8h" ], diff --git a/apidoc/html/files.html b/apidoc/html/files.html index e3af8c8b..d3c63d8b 100644 --- a/apidoc/html/files.html +++ b/apidoc/html/files.html @@ -117,23 +117,26 @@
Here is a list of all documented files with brief descriptions:
[detail level 12]

Files

 naif.h
 
 novas.h
 
 novascon.h
- - - - - - - - - - - - - - - - - + + + + + + + + + + + + + + + + + + + +
 ▼ include
 novas.h
 novascon.h
 nutation.h
 solarsystem.h
 ▼ src
 eph_manager.c
 frames.c
 novas.c
 novascon.c
 nutation.c
 refract.c
 solsys-ephem.c
 solsys1.c
 solsys2.c
 solsys3.c
 super.c
 timescale.c
 naif.h
 novas.h
 novascon.h
 nutation.h
 solarsystem.h
 ▼ src
 eph_manager.c
 frames.c
 naif.c
 novas.c
 novascon.c
 nutation.c
 refract.c
 solsys-calceph.c
 solsys-ephem.c
 solsys1.c
 solsys2.c
 solsys3.c
 super.c
 timescale.c
diff --git a/apidoc/html/globals.html b/apidoc/html/globals.html index 7a6a2d87..4a34c6c7 100644 --- a/apidoc/html/globals.html +++ b/apidoc/html/globals.html @@ -113,20 +113,8 @@
Here is a list of all documented functions, variables, defines, enums, and typedefs with links to the documentation:
-

- a -

diff --git a/apidoc/html/globals_a.html b/apidoc/html/globals_a.html new file mode 100644 index 00000000..a1335f6b --- /dev/null +++ b/apidoc/html/globals_a.html @@ -0,0 +1,140 @@ + + + + + + + + + + + + + + + + + + + + +SuperNOVAS: Globals + + + + + + + + + + + + + + + +
+
+ + + + + + + +
+
SuperNOVAS v1.2 +
+
The NOVAS C library, made better
+
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+
+ +
+
+
+ +
+ +
+
+ + +
+
+
+
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+
Loading...
+
Searching...
+
No Matches
+
+
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+ +
+
Here is a list of all documented functions, variables, defines, enums, and typedefs with links to the documentation:
+ +

- a -

+
+
+ + + + diff --git a/apidoc/html/globals_defs.html b/apidoc/html/globals_defs.html index 60614c76..578cdb1e 100644 --- a/apidoc/html/globals_defs.html +++ b/apidoc/html/globals_defs.html @@ -113,6 +113,11 @@
Here is a list of all documented macros with links to the documentation:
+

- _ -

+ +

- a -

diff --git a/apidoc/html/index.html b/apidoc/html/index.html index 21b64de6..963db51c 100644 --- a/apidoc/html/index.html +++ b/apidoc/html/index.html @@ -160,7 +160,7 @@

@@ -198,9 +198,10 @@

The SuperNOVAS distribution contains a GNU Makefile, which is suitable for compiling the library (as well as local documentation, and tests, etc.) on POSIX systems such as Linux, BSD, MacOS X, or Cygwin or WSL. (At this point we do not provide a similar native build setup for Windows, but speak up if you would like to add it yourself!)

Before compiling the library take a look a config.mk and edit it as necessary for your needs, or else define the necessary variables in the shell prior to invoking make. For example:

@@ -273,7 +274,7 @@

// 16h26m20.1918s, -26d19m23.138s (B1950), proper motion -12.11, -23.30 mas/year,
// parallax 5.89 mas, radial velocity -3.4 km/s.
make_cat_entry("Antares", "FK4", 1, 16.43894213, -26.323094, -12.11, -23.30, 5.89, -3.4, &star);
-
make_cat_entry
short make_cat_entry(const char *star_name, const char *catalog, long cat_num, double ra, double dec, double pm_ra, double pm_dec, double parallax, double rad_vel, cat_entry *star)
Definition novas.c:6315
+
make_cat_entry
short make_cat_entry(const char *star_name, const char *catalog, long cat_num, double ra, double dec, double pm_ra, double pm_dec, double parallax, double rad_vel, cat_entry *star)
Definition novas.c:6355
cat_entry
Definition novas.h:601

We must convert these coordinates to the now standard ICRS system for calculations in SuperNOVAS, first by calculating equivalent J2000 coordinates, by applying the proper motion and the appropriate precession. Then, we apply a small adjustment to convert from J2000 to ICRS coordinates.

// First change the catalog coordinates (in place) to the J2000 (FK5) system...
@@ -281,7 +282,7 @@

// Then convert J2000 coordinates to ICRS (also in place). Here the dates don't matter...
transform_cat(CHANGE_J2000_TO_ICRS, 0.0, &star, 0.0, "ICRS", &star);
-
transform_cat
short transform_cat(enum novas_transform_type option, double jd_tt_in, const cat_entry *in, double jd_tt_out, const char *out_id, cat_entry *out)
Definition novas.c:5824
+
transform_cat
short transform_cat(enum novas_transform_type option, double jd_tt_in, const cat_entry *in, double jd_tt_out, const char *out_id, cat_entry *out)
Definition novas.c:5864
NOVAS_JD_J2000
#define NOVAS_JD_J2000
[day] Julian date at J2000
Definition novas.h:107
NOVAS_JD_B1950
#define NOVAS_JD_B1950
[day] Julian date at B1950
Definition novas.h:113
CHANGE_J2000_TO_ICRS
@ CHANGE_J2000_TO_ICRS
Definition novas.h:495
@@ -300,7 +301,7 @@

// Specify the location we are observing from
// 50.7374 deg N, 7.0982 deg E, 60m elevation
make_observer_on_surface(50.7374, 7.0982, 60.0, 0.0, 0.0, &obs);
-
make_observer_on_surface
int make_observer_on_surface(double latitude, double longitude, double height, double temperature, double pressure, observer *obs)
Definition novas.c:6562
+
make_observer_on_surface
int make_observer_on_surface(double latitude, double longitude, double height, double temperature, double pressure, observer *obs)
Definition novas.c:6602
observer
Definition novas.h:670

Similarly, you can also specify observers in Earth orbit, in Sun orbit, at the geocenter, or at the Solar-system barycenter.

@@ -379,9 +380,9 @@

// Set the function to use for calculating all other solar-system bodies
set_ephem_provider(my_ephemeris_provider_function);
-
set_planet_provider_hp
int set_planet_provider_hp(novas_planet_provider_hp func)
Definition novas.c:663
-
set_ephem_provider
int set_ephem_provider(novas_ephem_provider func)
Definition novas.c:5603
-
set_planet_provider
int set_planet_provider(novas_planet_provider func)
Definition novas.c:640
+
set_planet_provider_hp
int set_planet_provider_hp(novas_planet_provider_hp func)
Definition novas.c:682
+
set_ephem_provider
int set_ephem_provider(novas_ephem_provider func)
Definition novas.c:5641
+
set_planet_provider
int set_planet_provider(novas_planet_provider func)
Definition novas.c:641

Instead of make_cat_object() you define your source as an object with an name or ID number that is used by the ephemeris service you provided. For major planets you might want to use make_planet(), if they use a novas_planet_provider function to access ephemeris data with their NOVAS IDs, or else make_ephem_object() for more generic ephemeris handling via a user-provided novas_ephem_provider. E.g.:

object mars, ceres; // Hold data on solar-system bodies.
@@ -391,9 +392,9 @@

// Ceres will be handled by the generic ephemeris provider function, which let's say
// uses the NAIF ID of 2000001
make_ephem_object("Ceres", 2000001, &ceres);
-
make_planet
int make_planet(enum novas_planet num, object *planet)
Definition novas.c:6453
+
make_planet
int make_planet(enum novas_planet num, object *planet)
Definition novas.c:6493
NOVAS_MARS
@ NOVAS_MARS
Major planet number for the Mars in NOVAS.
Definition novas.h:265
-
make_ephem_object
int make_ephem_object(const char *name, long num, object *body)
Definition super.c:1018
+
make_ephem_object
int make_ephem_object(const char *name, long num, object *body)
Definition super.c:1022

Other than that, it's the same spiel as before, e.g.:

int status = novas_sky_pos(&mars, &obs_frame, NOVAS_TOD, &apparent);
if(status) {
@@ -515,6 +516,9 @@

  • New novas_make_redshifted_object() to simplify the creation of distant catalog sources that are characterized with a redshift measure rather than a radial velocity value.
  • New generic redshift-handling functions novas_v2z(), novas_z2v(),
  • New functions to calculate and apply additional gravitational redshift corrections for light that originates near massive gravitating bodies (other than major planets, or Sun or Moon), or for observers located near massive gravitating bodies (other than the Sun and Earth). The added functions are grav_redshift(), redhift_vrad(), unredshift_vrad(), novas_z_add(), and novas_z_inv().
    • +
  • CALCEPH integration: novas_use_calceph() and/or novas_use_calceph_planets() to specify and use ephemeris data via CALCEPH for Solar-system sources in general, and for major planets specifically; and novas_calceph_use_ids() to specify whether object.number in NOVAS_EPHEM_OBJECT type objects is a NAIF ID (default) or else a CALCEPH ID number of the Solar-system body.
    • +
  • NAIF/NOVAS ID conversions for major planets (and Sun, Moon, SSB): novas_to_naif_planet(), novas_to_dexxx_planet(), and naif_to_novas_planet().
    • +
  • Access to custom ephemeris provider functions: get_planet_provider() and get_planet_provider_hp().

    • @@ -545,8 +549,10 @@

    External Solar-system ephemeris data or services

    If you want to use SuperNOVAS to calculate positions for a range of Solar-system objects, and/or to do it with sufficient precision, you will have to integrate it with a suitable provider of ephemeris data, such as JPL Horizons or the Minor Planet Center. Given the NOVAS C heritage, and some added SuperNOVAS flexibility in this area, you have several options on doing that. These are listed from the most flexible (and preferred) to the least flexible (old ways).

    +

    NASA/JPL also provides generic ephemerides for the major planets, satellites thereof, the 300 largest asteroids, the Lagrange points, and some Earth orbiting stations.

    @@ -561,7 +567,7 @@

    }
    novas_origin
    novas_origin
    Definition novas.h:461

    which takes an object ID number (such as a NAIF) an object name, and a split TDB date (for precision) as it inputs, and returns the type of origin with corresponding ICRS position and velocity vectors in the supplied pointer locations. The function can use either the ID number or the name to identify the object or file (whatever is the most appropriate for the implementation). The positions and velocities may be returned either relative to the SSB or relative to the heliocenter, and accordingly, your function should set the value pointed at by origin to NOVAS_BARYCENTER or NOVAS_HELIOCENTER accordingly. Positions and velocities are rectangular ICRS x,y,z vectors in units of AU and AU/day respectively.

    -

    This way you can easily integrate current ephemeris data for JPL Horizons, e.g. using CALCEPH or the CSPICE toolkit, or for the Minor Planet Center (MPC), or whatever other ephemeris service you prefer.

    +

    This way you can easily integrate current ephemeris data for JPL Horizons, e.g. using the CSPICE toolkit, or for the Minor Planet Center (MPC), or whatever other ephemeris service you prefer.

    Once you have your adapter function, you can set it as your ephemeris service via set_ephem_provider():

    set_ephem_provider(my_ephem_reader);

    By default, your custom my_ephem_reader function will be used for 'minor planets' only (i.e. anything other than the major planets, the Sun, Moon, and the Solar System Barycenter). And, you can use the same function for the mentioned 'major planets' also via:

    @@ -570,11 +576,39 @@

    planet_ephem_provider
    short planet_ephem_provider(double jd_tdb, enum novas_planet body, enum novas_origin origin, double *position, double *velocity)
    Definition solsys-ephem.c:104
    planet_ephem_provider_hp
    short planet_ephem_provider_hp(const double jd_tdb[2], enum novas_planet body, enum novas_origin origin, double *position, double *velocity)
    Definition solsys-ephem.c:45

    provided you compiled SuperNOVAS with BUILTIN_SOLSYS_EPHEM = 1 (in config.mk), or else you link your code against solsys-ephem.c explicitly. Easy-peasy.

    -

    +

    +Built-in support for CALCEPH integration

    +

    The CALCEPH library provides an easy-to-use access to JPL and INPOP ephemeris files from C/C++. As of version 1.2, we provide built-in support for integrating the CALCEPH C library with SuperNOVAS for handling Solar-system objects.

    +

    Prior to building SuperNOVAS simply set CALCEPH_SUPPORT to 1 in config.mk or in your shell. Depending on the build target, it will build libsolsys-calceph.so[.1] (target shared) or libsolsys-calceph.a (target static) libraries, which provide the novas_use_calceph() and novas_use_calceph_planets() functions.

    +

    Of course, you will need access to the CALCEPH C development files (C headers and unversioned libraries) for the build to succeed. Here is an example on how you'd use CALCEPH with SuperNOVAS in your application code:

    +
    #include <calceph.h>
    +
    +
    // You can open a set of JPL/INPOP ephemeris files with CALCEPH...
    +
    t_calcephbin *eph = calceph_open_array(...);
    +
    +
    // Then use them as your generic SuperNOVAS ephemeris provider
    +
    int status = novas_use_calceph(eph);
    +
    if(status < 0) {
    +
    // Ooops something went wrong...
    +
    }
    +
    +
    // -----------------------------------------------------------------------
    +
    // Optionally you may use a separate ephemeris data for major planets
    +
    // (or if planet ephemeris was included in 'eph' above, you don't have to)
    +
    t_calcephbin *pleph = calceph_open(...);
    +
    int status = novas_use_calceph(pleph);
    +
    if(status < 0) {
    +
    // Ooops something went wrong...
    +
    }
    +
    novas_use_calceph
    int novas_use_calceph(t_calcephbin *eph)
    Definition solsys-calceph.c:355
    +

    You can obtain readily available standard ephemeris files from NASA/JPL, such as DE440, which covers the major planets, plus Sun, Moon, and Solar-System Barycenter (SSB) for times between 1550 AD and 2650 AD. Or, you can use the JPL HORIZONS system to generate cutom ephemeris data for pretty much all known solar systems bodies, down to the tiniest rocks. All of these should work with the solsys-calceph plugin.

    +

    And, when linking your application, don't forget to add -lsolsys-calceph to your link flags. That's all there is to it.

    +

    +

    Built-in support for (old) JPL major planet ephemerides

    If you only need support for major planets, you may be able to use one of the modules included in the SuperNOVAS distribution. The modules solsys1.c and solsys2.c provide built-in support to older JPL ephemerides (DE200 to DE421), either via the eph_manager interface of solsys1.c or via the FORTRAN pleph interface with solsys2.c.

    -

    +

    Planets via <tt>eph_manager</tt>

    To use the eph_manager interface for planet 1997 JPL planet ephemeris (DE200 through DE421), you must either build SuperNOVAS with BUILTIN_SOLSYS1 = 1 in config.mk, or else link your application with solsys1.c and eph_manager.c from SuperNOVAS explicitly. If you want eph_manager to be your default ephemeris provider (the old way) you might also want to set DEFAULT_SOLSYS = 1 in config.mk. Otherwise, your application should set eph_manager as your planetary ephemeris provider at runtime via:

    set_planet_provider(planet_eph_manager);
    @@ -592,7 +626,7 @@

    ephem_close
    short ephem_close(void)
    Definition eph_manager.c:224

    Note, that at any given time eph_manager can have only one ephemeris data file opened. You cannot use it to retrieve data from multiple ephemeris input files at the same time. (But you can with the CSPICE toolkit, which you can integrate as discussed further above!)

    That's all, except the warning that this method will not work with newer JPL ephemeris data, beyond DE421.

    -

    +

    Planets via JPL's <tt>pleph</tt> FORTRAN interface

    To interface eith the JPL PLEPH library (FORTRAN) for planet ephemerides, you must either build SuperNOVAS with BUILTIN_SOLSYS2 = 1 in config.mk, or else link your application with solsys2.c and your appropriately modified jplint.f (from the examples sub-directory) explicitly, together with the JPL PLEPH library. If you want this to be your default ephemeris provider (the old way) you might also want to set DEFAULT_SOLSYS = 2 in config.mk. Otherwise, your application should set your planetary ephemeris provider at runtime via:

    set_planet_provider(planet_jplint);
    @@ -601,14 +635,14 @@

    planet_jplint
    short planet_jplint(double jd_tdb, enum novas_planet body, enum novas_origin origin, double *position, double *velocity)
    Definition solsys2.c:86

    Integrating JPL ephemeris data this way can be arduous. You will need to compile and link FORTRAN with C (not the end of the world), but you may also have to modify jplint.f (providing the intermediate FORTRAN jplint_() / jplihp_() interfaces to pleph_()) to work with the version of pleph.f that you will be using. Unless you already have code that relies on this method, you are probably better off choosing one of the other ways for integrating planetary ephemeris data with SuperNOVAS.

    -

    +

    Explicit linking of custom ephemeris functions

    Finally, if none of the above is appealing, and you are fond of the old ways, you may compile SuperNOVAS with the DEFAULT_SOLSYS option disabled (commented, removed, or else set to 0), and then link your own implementation of solarsystem() and solarsystem_hp() calls with your application.

    For Solar-system objects other than the major planets, you may also provide your own readeph() implementation. (In this case you will want to set DEFAULT_READEPH in config.mk to specify your source code for that function before building the SuperNOVAS library, or else disable that option entirely (e.g. by commenting or removing it), and link your application explicitly with your readeph() implementation.

    The downside of this approach is that your SuperNOVAS library will not be usable without invariably providing a solarsystem() / solarsystem_hp() and/or readeph() implementations for every application that you will want to use SuperNOVAS with. This is why the runtime configuration of the ephemeris provider functions is the best and most generic way to add your preferred implementations while also providing some minimum default implementations for other users of the library, who may not need your ephemeris service, or have no need for planet data beyond the approximate positions for the Earth and Sun.

    -

    +

    Runtime debug support

    You can enable or disable debugging output to stderr with novas_debug(enum novas_debug_mode), where the argument is one of the defined constants from novas.h:

    @@ -624,7 +658,7 @@

    The main difference between NOVAS_DEBUG_ON and NOVAS_DEBUG_EXTRA is that the latter will treat minor issues as errors also, while the former may ignore them. For example, place() will return normally by default if it cannot calculate gravitational bending around massive planets in full accuracy mode. It is unlikely that this omission would significantly alter the result in most cases, except for some very specific ones when observing in a direction close to a major planet. Thus, with NOVAS_DEBUG_ON, place() go about as usual even if the Jupiter's position is not known. However, NOVAS_DEBUG_EXTRA will not give it a free pass, and will make place() return an error (and print the trace) if it cannot properly account for gravitational bending around the major planets as it is expected to.

    -

    +

    Release schedule

    A predictable release schedule and process can help manage expectations and reduce stress on adopters and developers alike.

    Releases of the library shall follow a quarterly release schedule. You may expect upcoming releases to be published around February 1, May 1, August 1, and/or November 1 each year, on an as-needed basis. That means that if there are outstanding bugs, or new pull requests (PRs), you may expect a release that addresses these in the upcoming quarter. The dates are placeholders only, with no guarantee that a new release will actually be available every quarter. If nothing of note comes up, a potential release date may pass without a release being published.

    diff --git a/apidoc/html/md_CHANGELOG.html b/apidoc/html/md_CHANGELOG.html index 65e27083..0caf3efe 100644 --- a/apidoc/html/md_CHANGELOG.html +++ b/apidoc/html/md_CHANGELOG.html @@ -125,6 +125,9 @@

  • #57: New novas_make_redshifted_object() to simplify the creation of distant catalog sources that are characterized with a redshift measure rather than a radial velocity value.
  • #57: New generic redshift-handling functions novas_v2z(), novas_z2v(),
  • #58: New functions to calculate and apply additional gravitational redshift corrections for light that originates near massive gravitating bodies (other than major planets, or Sun or Moon), or for observers located near massive gravitating bodies (other than the Sun and Earth). The added functions are grav_redshift(), redhift_vrad(), unredshift_vrad(), novas_z_add(), and novas_z_inv().
    • +
  • #83: CALCEPH integration: novas_use_calceph() and/or novas_use_calceph_planets() to specify and use ephemeris data via CALCEPH for Solar-system sources in general, and for major planets specifically; and novas_calceph_use_ids() to specify whether object.number in NOVAS_EPHEM_OBJECT type objects is a NAIF ID (default) or else a CALCEPH ID number of the Solar-system body. These functions are provided by the libsolsys-calceph.so[.1] and/or .a plugin libraries, which are built contingent on the CALCEPH_SUPPORT variable being set to 1 prior to the build. The build of the plugin module requires an accessible installation of the CALCEPH development files (C headers and unversioned static or shared libraries depending on the needs of the build).
    • +
  • NOVAS-NAIF conversions for major planets (and Sun, Moon, SSB): novas_to_naif_planet() (planet centers), novas_to_dexxx_planet() (mixed planet center/barycenter for DExxx ephemeris files), and the inverse naif_to_novas_planet().
    • +
  • Added get_planet_provider() and get_planet_provider_hp() functions for convenience to return the solarsystem() / solarsystem_hp() type custom planet ephemeris provider functions currently configured, so they may be used directly, outside of ephemeris() calls.

    • [1.1.1] - 2024-10-28

    diff --git a/apidoc/html/md_LEGACY.html b/apidoc/html/md_LEGACY.html index ad3eece5..ce2738ea 100644 --- a/apidoc/html/md_LEGACY.html +++ b/apidoc/html/md_LEGACY.html @@ -132,7 +132,7 @@

    // 16h26m20.1918s, -26d19m23.138s (B1950), proper motion -12.11, -23.30 mas/year,
    // parallax 5.89 mas, radial velocity -3.4 km/s.
    make_cat_entry("Antares", "FK4", 1, 16.43894213, -26.323094, -12.11, -23.30, 5.89, -3.4, &source);
    -
    make_cat_entry
    short make_cat_entry(const char *star_name, const char *catalog, long cat_num, double ra, double dec, double pm_ra, double pm_dec, double parallax, double rad_vel, cat_entry *star)
    Definition novas.c:6315
    +
    make_cat_entry
    short make_cat_entry(const char *star_name, const char *catalog, long cat_num, double ra, double dec, double pm_ra, double pm_dec, double parallax, double rad_vel, cat_entry *star)
    Definition novas.c:6355
    cat_entry
    Definition novas.h:601

    We must convert these coordinates to the now standard ICRS system for calculations in SuperNOVAS, first by calculating equivalent J2000 coordinates, by applying the proper motion and the appropriate precession. Then, we apply a small adjustment to convert from J2000 to ICRS coordinates.

    // First change the catalog coordinates (in place) to the J2000 (FK5) system...
    @@ -140,7 +140,7 @@

    // Then convert J2000 coordinates to ICRS (also in place). Here the dates don't matter...
    transform_cat(CHANGE_J2000_TO_ICRS, 0.0, &source, 0.0, "ICRS", &source);
    -
    transform_cat
    short transform_cat(enum novas_transform_type option, double jd_tt_in, const cat_entry *in, double jd_tt_out, const char *out_id, cat_entry *out)
    Definition novas.c:5824
    +
    transform_cat
    short transform_cat(enum novas_transform_type option, double jd_tt_in, const cat_entry *in, double jd_tt_out, const char *out_id, cat_entry *out)
    Definition novas.c:5864
    NOVAS_J2000
    @ NOVAS_J2000
    Definition novas.h:347
    CHANGE_J2000_TO_ICRS
    @ CHANGE_J2000_TO_ICRS
    Definition novas.h:495
    CHANGE_EPOCH
    @ CHANGE_EPOCH
    The combined equivalent of PROPER_MOTION and PRECESSION together.
    Definition novas.h:491
    @@ -153,7 +153,7 @@

    // Specify the location we are observing from
    // 50.7374 deg N, 7.0982 deg E, 60m elevation
    make_observer_on_surface(50.7374, 7.0982, 60.0, 0.0, 0.0, &obs);
    -
    make_observer_on_surface
    int make_observer_on_surface(double latitude, double longitude, double height, double temperature, double pressure, observer *obs)
    Definition novas.c:6562
    +
    make_observer_on_surface
    int make_observer_on_surface(double latitude, double longitude, double height, double temperature, double pressure, observer *obs)
    Definition novas.c:6602
    observer
    Definition novas.h:670

    Specify the time of observation

    @@ -171,7 +171,7 @@

    // We'll also need the TT - UT1 difference, which we can obtain from what we already
    // defined above
    double ut1_to_tt = get_ut1_to_tt(leap_seconds, dut1);
    -
    julian_date
    double julian_date(short year, short month, short day, double hour)
    Definition novas.c:6206
    +
    julian_date
    double julian_date(short year, short month, short day, double hour)
    Definition novas.c:6246
    get_ut1_to_tt
    double get_ut1_to_tt(int leap_seconds, double dut1)
    Definition super.c:60
    get_utc_to_tt
    double get_utc_to_tt(int leap_seconds)
    Definition super.c:32

    @@ -182,7 +182,7 @@

    double dy = ...;
    cel_pole(jd_tt, POLE_OFFSETS_X_Y, dx, dy);
    -
    cel_pole
    short cel_pole(double jd_tt, enum novas_pole_offset_type type, double dpole1, double dpole2)
    Definition novas.c:3022
    +
    cel_pole
    short cel_pole(double jd_tt, enum novas_pole_offset_type type, double dpole1, double dpole2)
    Definition novas.c:3058
    POLE_OFFSETS_X_Y
    @ POLE_OFFSETS_X_Y
    Offsets are dx, dy pairs (IAU 2006 precession-nutation model)
    Definition novas.h:446

    Calculate apparent positions on sky

    @@ -197,7 +197,7 @@

    // Oops, something went wrong...
    return -1;
    }
    -
    place_star
    int place_star(double jd_tt, const cat_entry *star, const observer *obs, double ut1_to_tt, enum novas_reference_system system, enum novas_accuracy accuracy, sky_pos *pos)
    Definition novas.c:702
    +
    place_star
    int place_star(double jd_tt, const cat_entry *star, const observer *obs, double ut1_to_tt, enum novas_reference_system system, enum novas_accuracy accuracy, sky_pos *pos)
    Definition novas.c:738
    NOVAS_FULL_ACCURACY
    @ NOVAS_FULL_ACCURACY
    Definition novas.h:391
    NOVAS_CIRS
    @ NOVAS_CIRS
    Definition novas.h:339
    sky_pos
    Definition novas.h:688
    @@ -210,7 +210,7 @@

    // Convert the rectangular equatorial unit vector to R.A. [h] and declination [deg]
    vector2radec(pos.r_hat, &ra, &dec);
    -
    vector2radec
    short vector2radec(const double *pos, double *ra, double *dec)
    Definition novas.c:4832
    +
    vector2radec
    short vector2radec(const double *pos, double *ra, double *dec)
    Definition novas.c:4868
    sky_pos::r_hat
    double r_hat[3]
    unit vector toward object (dimensionless)
    Definition novas.h:689

    Alternatively, you can simply call radec_star() instead of place_star() to get apparent R.A. and declination in a single step if you do not need the sky_pos data otherwise. If you followed the less-precise old methodology (Lieske et. al. 1977) thus far, calculating TOD coordinates, you are done here.

    If, however, you calculated the position in CIRS with the more precise IAU 2006 methodology (as we did in the example above), you have one more step to go still. The CIRS equator is the true equator of date, however its origin (CIO) is not the true equinox of date. Thus, we must correct for the difference of the origins to get the true apparent R.A.:

    @@ -233,7 +233,7 @@

    If you followed the old (Lieske et al. 1977) method instead to calculate sky_pos in the less precise TOD coordinate system, then you'd simply replace the cirs_to_itrs() call above with tod_to_itrs() accordingly.

    You can additionally apply an approximate optical refraction correction for the astrometric (unrefracted) zenith angle, if you want, e.g.:

    zd -= refract_astro(&obs.on_surf, NOVAS_STANDARD_ATMOSPHERE, zd);
    -
    refract_astro
    double refract_astro(const on_surface *location, enum novas_refraction_model option, double zd_astro)
    Definition novas.c:6086
    +
    refract_astro
    double refract_astro(const on_surface *location, enum novas_refraction_model option, double zd_astro)
    Definition novas.c:6126
    NOVAS_STANDARD_ATMOSPHERE
    @ NOVAS_STANDARD_ATMOSPHERE
    Definition novas.h:410
    observer::on_surf
    on_surface on_surf
    Definition novas.h:675

    @@ -249,12 +249,12 @@

    // Set the function to use for calculating all sorts of solar-system bodies
    set_ephem_provider(my_ephemeris_provider_function);
    -
    set_planet_provider_hp
    int set_planet_provider_hp(novas_planet_provider_hp func)
    Definition novas.c:663
    -
    set_ephem_provider
    int set_ephem_provider(novas_ephem_provider func)
    Definition novas.c:5603
    -
    set_planet_provider
    int set_planet_provider(novas_planet_provider func)
    Definition novas.c:640
    +
    set_planet_provider_hp
    int set_planet_provider_hp(novas_planet_provider_hp func)
    Definition novas.c:682
    +
    set_ephem_provider
    int set_ephem_provider(novas_ephem_provider func)
    Definition novas.c:5641
    +
    set_planet_provider
    int set_planet_provider(novas_planet_provider func)
    Definition novas.c:641

    You can use tt2tdb() to convert Terrestrial Time (TT) to Barycentric Dynamic Time (TDB) for your ephemeris provider functions (they only differ when you really need extreme precision – for most applications you can used TT and TDB interchangeably in the present era):

    double jd_tdb = jd_tt + tt2tdb(jd_tt) / 86400.0;
    -
    tt2tdb
    double tt2tdb(double jd_tt)
    Definition novas.c:5047
    +
    tt2tdb
    double tt2tdb(double jd_tt)
    Definition novas.c:5083

    Instead of make_cat_entry() you define your source as an object with an name or ID number that is used by the ephemeris service you provided. For major planets you might want to use make_planet(), if they use a novas_planet_provider function to access ephemeris data with their NOVAS IDs, or else make_ephem_object() for more generic ephemeris handling via a user-provided novas_ephem_provider. E.g.:

    object mars, ceres; // Hold data on solar-system bodies.
    @@ -264,16 +264,16 @@

    // Ceres will be handled by the generic ephemeris provider function, which let's say
    // uses the NAIF ID of 2000001
    make_ephem_object("Ceres", 2000001, &ceres);
    -
    make_planet
    int make_planet(enum novas_planet num, object *planet)
    Definition novas.c:6453
    +
    make_planet
    int make_planet(enum novas_planet num, object *planet)
    Definition novas.c:6493
    NOVAS_MARS
    @ NOVAS_MARS
    Major planet number for the Mars in NOVAS.
    Definition novas.h:265
    -
    make_ephem_object
    int make_ephem_object(const char *name, long num, object *body)
    Definition super.c:1018
    +
    make_ephem_object
    int make_ephem_object(const char *name, long num, object *body)
    Definition super.c:1022

    Other than that, it's the same spiel as before, except using the appropriate place() for generic celestial targets instead of place_star() for the sidereal sources (or else radec_planet() instead of radec_star()). E.g.:

    int status = place(jd_tt, &mars, &obs, ut1_to_tt, NOVAS_CIRS, NOVAS_FULL_ACCURACY, &pos);
    if(status) {
    // Oops, something went wrong...
    ...
    }
    -
    place
    short place(double jd_tt, const object *source, const observer *location, double ut1_to_tt, enum novas_reference_system coord_sys, enum novas_accuracy accuracy, sky_pos *output)
    Definition novas.c:1497
    +
    place
    short place(double jd_tt, const object *source, const observer *location, double ut1_to_tt, enum novas_reference_system coord_sys, enum novas_accuracy accuracy, sky_pos *output)
    Definition novas.c:1533
    diff --git a/apidoc/html/menudata.js b/apidoc/html/menudata.js index 99b5bc27..98c773c2 100644 --- a/apidoc/html/menudata.js +++ b/apidoc/html/menudata.js @@ -77,7 +77,8 @@ var menudata={children:[ {text:"File List",url:"files.html"}, {text:"Globals",url:"globals.html",children:[ {text:"All",url:"globals.html",children:[ -{text:"a",url:"globals.html#index_a"}, +{text:"_",url:"globals.html#index__5F"}, +{text:"a",url:"globals_a.html#index_a"}, {text:"b",url:"globals_b.html#index_b"}, {text:"c",url:"globals_c.html#index_c"}, {text:"d",url:"globals_d.html#index_d"}, @@ -150,6 +151,7 @@ var menudata={children:[ {text:"p",url:"globals_eval.html#index_p"}, {text:"w",url:"globals_eval.html#index_w"}]}, {text:"Macros",url:"globals_defs.html",children:[ +{text:"_",url:"globals_defs.html#index__5F"}, {text:"a",url:"globals_defs.html#index_a"}, {text:"b",url:"globals_defs.html#index_b"}, {text:"c",url:"globals_defs.html#index_c"}, diff --git a/apidoc/html/naif_8c.html b/apidoc/html/naif_8c.html new file mode 100644 index 00000000..c5887082 --- /dev/null +++ b/apidoc/html/naif_8c.html @@ -0,0 +1,250 @@ + + + + + + + + + + + + + + + + + + + + +SuperNOVAS: src/naif.c File Reference + + + + + + + + + + + + + + + +
    +
    +

    + + + + + + +
    +
    SuperNOVAS v1.2 +
    +
    The NOVAS C library, made better
    +
    + + + + + + + + + +
    + +
    +
    +
    + +
    + +
    +
    + + +
    +
    +
    +
    +
    +
    Loading...
    +
    Searching...
    +
    No Matches
    +
    +
    +
    +
    + +
    +
    +Macros | +Functions
    +
    naif.c File Reference
    +
    +
    + + + + + +

    +Macros

    +#define __NOVAS_INTERNAL_API__
     Use definitions meant for internal use by SuperNOVAS only.
     
    + + + + + + + +

    +Functions

    enum novas_planet naif_to_novas_planet (long id)
     
    long novas_to_dexxx_planet (enum novas_planet id)
     
    long novas_to_naif_planet (enum novas_planet id)
     
    +

    Detailed Description

    +
    Date
    Created on Nov 6, 2024
    +
    Author
    Attila Kovacs
    +

    Solar system ID mappings between NOVAS and NASA's Navigation and Ancillary Information Facility (NAIF), which is used by the JPL ephemeris systems. The two differ for the numbering convention for major planets, the Sun, Moon, Solar-System Barycenter (SSB) and the Earth-Moon Barycenter (EMB). NOVAS does not have predefined IDs beyond this set (and no defined ID for EMB), thus for all other objects we'll assume and use NOVAS IDs that match NAIF.

    +
    Since
    1.2
    +

    Function Documentation

    + +

    ◆ naif_to_novas_planet()

    + +
    +
    + + + + + + + + +
    enum novas_planet naif_to_novas_planet (long id)
    +
    +

    Converts a NAIF ID to a NOVAS major planet ID. It account for the different IDs used for Sun, Moon and SSB. Otherwise NAIF planet barycenters are mapped to the corresponding bodies, except EMB (3), which will return -1. NAIF body centers n99 (e.g. 399 for Earth), are mapped to the corresponding NOVAS planet number n. All other NAIF IDs will return -1, indicating no match to a NOVAS planet ID.

    +
    Parameters
    + + +
    idThe NAIF ID of the major planet of interest
    +
    +
    +
    Returns
    the NOVAS ID for the same object (which may or may not be different from the input), or -1 if the NAIF ID cannot be matched to a NOVAS major planet.
    +
    See also
    novas_to_naif_planet()
    +
    +novas_to_dexxx_planet()
    +
    Author
    Attila Kovacs
    +
    Since
    1.2
    + +

    References NAIF_EMB, NAIF_MOON, NAIF_SSB, NAIF_SUN, NOVAS_MERCURY, NOVAS_MOON, NOVAS_PLUTO, NOVAS_SSB, and NOVAS_SUN.

    + +
    +
    + +

    ◆ novas_to_dexxx_planet()

    + +
    +
    + + + + + + + + +
    long novas_to_dexxx_planet (enum novas_planet id)
    +
    +

    Converts a NOVAS Solar-system body ID to a NAIF Solar-system body ID for DExxx ephemeris files. The DExxx (e.g. DE440) ephemeris files use NAIF IDs, but for most planets contain barycentric data only rather than that of the planet center. For Earth-based observations, it only really makes a difference whether the 3 is used for the Earth-Moon Barycenter (EMB) or 399 for the geocenter.

    +
    Parameters
    + + +
    idThe NOVAS ID of the major planet of interest
    +
    +
    +
    Returns
    the NAIF ID for the same object (which may or may not be different from the input), as appropriate for use in the DExxx ephemeris files.
    +
    See also
    novas_to_naif_planet()
    +
    +naif_to_novas_planet()
    +
    Author
    Attila Kovacs
    +
    Since
    1.2
    + +

    References NAIF_EARTH, NAIF_MOON, NAIF_SSB, NAIF_SUN, NOVAS_EARTH, NOVAS_MERCURY, NOVAS_MOON, NOVAS_PLUTO, NOVAS_SSB, and NOVAS_SUN.

    + +
    +
    + +

    ◆ novas_to_naif_planet()

    + +
    +
    + + + + + + + + +
    long novas_to_naif_planet (enum novas_planet id)
    +
    +

    Converts a NOVAS Solar-system body ID to a NAIF Solar-system body ID. NOVAS and NAIF use slightly different IDs for major planets, the Moon, and the Solar-system Barycenter (SSB). In NOVAS, major planets are have IDs ranging from 1 through 9, but for NAIF 1–9 are the planetary barycenters and the planet centers have numbers in the hundreds ending with 99 (e.g. the center of Earth is NAIF 399; 3 is the NOVAS ID for Earth and the NAIF ID for the Earth-Moon Barycenter [EMB]). The Sun and Moon also have distinct IDs in NAIF vs NOVAS.

    +
    Parameters
    + + +
    idThe NOVAS ID of the major planet of interest
    +
    +
    +
    Returns
    the NAIF ID for the same object or planet center (which may or may not be different from the input)
    +
    See also
    naif_to_novas_planet()
    +
    Author
    Attila Kovacs
    +
    Since
    1.2
    + +

    References NAIF_MOON, NAIF_SSB, NAIF_SUN, NOVAS_MERCURY, NOVAS_MOON, NOVAS_PLUTO, NOVAS_SSB, and NOVAS_SUN.

    + +
    +
    +
    +
    + + + + diff --git a/apidoc/html/naif_8c.js b/apidoc/html/naif_8c.js new file mode 100644 index 00000000..138eabd4 --- /dev/null +++ b/apidoc/html/naif_8c.js @@ -0,0 +1,7 @@ +var naif_8c = +[ + [ "__NOVAS_INTERNAL_API__", "naif_8c.html#af46d8e51fc53d94b0d48c8201c3c84a6", null ], + [ "naif_to_novas_planet", "naif_8c.html#a1c4b3f67a3b82808dd16ae43dfaf0f86", null ], + [ "novas_to_dexxx_planet", "naif_8c.html#ac3eb54acf22dc155879163de89c6865e", null ], + [ "novas_to_naif_planet", "naif_8c.html#ab51ac9bdf7736e1c1582e0981046daf3", null ] +]; \ No newline at end of file diff --git a/apidoc/html/naif_8h.html b/apidoc/html/naif_8h.html new file mode 100644 index 00000000..66885216 --- /dev/null +++ b/apidoc/html/naif_8h.html @@ -0,0 +1,156 @@ + + + + + + + + + + + + + + + + + + + + +SuperNOVAS: include/naif.h File Reference + + + + + + + + + + + + + + + +
    +
    + + + + + + + +
    +
    SuperNOVAS v1.2 +
    +
    The NOVAS C library, made better
    +
    +
    + + + + + + + +
    +
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    +
    Loading...
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    Searching...
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    No Matches
    +
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    +
    + +
    +
    +Macros
    +
    naif.h File Reference
    +
    +
    + + + + + + + + + + + + + + + + + +

    +Macros

    +#define NAIF_EARTH   399
     NAIF ID for the geocenter.
     
    +#define NAIF_EMB   3
     NAIF ID for the Earth-Moon Barycenter (EMB)
     
    +#define NAIF_MOON   301
     NAIF ID for the Moon.
     
    +#define NAIF_SSB   0
     NAIF ID for the Solar-System Barycenter (SSB)
     
    +#define NAIF_SUN   10
     NAIF_ID for the Sun.
     
    +

    Detailed Description

    +
    Date
    Created on Nov 6, 2024
    +
    Author
    Attila Kovacs
    +
    +
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+novas_planet_provider_hp get_planet_provider_hp () +  short grav_def (double jd_tdb, enum novas_observer_place unused, enum novas_accuracy accuracy, const double *pos_src, const double *pos_obs, double *out)   int grav_planets (const double *pos_src, const double *pos_obs, const novas_planet_bundle *planets, double *out) @@ -2493,10 +2497,66 @@

    Returns
    the currently defined function for accessing ephemeris data for minor planets or satellites, ot NULL if no function was set via set_ephem_provider() previously.
    See also
    set_ephem_provider()
    +get_planet_provider()
    +
    +get_planet_provider_hp()
    +
    ephemeris()
    Since
    1.0
    Author
    Attila Kovacs
    + + + +

    ◆ get_planet_provider()

    + +
    +
    + + + + + + + +
    novas_planet_provider get_planet_provider ()
    +
    +

    Returns the custom (low-precision) ephemeris provider function for major planets (and Sun, Moon, SSB), if any.

    +
    Returns
    the custom (low-precision) planet ephemeris provider function.
    +
    Author
    Attila Kovacs
    +
    Since
    1.2
    +
    See also
    set_planet_provider()
    +
    +get_planet_provider_hp()
    +
    +get_ephem_provider()
    + +
    +
    + +

    ◆ get_planet_provider_hp()

    + +
    +
    + + + + + + + +
    novas_planet_provider_hp get_planet_provider_hp ()
    +
    +

    Returns the custom high-precision ephemeris provider function for major planets (and Sun, Moon, SSB), if any.

    +
    Returns
    the custom high-precision planet ephemeris provider function.
    +
    Author
    Attila Kovacs
    +
    Since
    1.2
    +
    See also
    set_planet_provider_hp()
    +
    +get_planet_provider()
    +
    +get_ephem_provider()
    +
    @@ -5456,6 +5516,10 @@

    Author
    Attila Kovacs
    See also
    get_ephem_provider()
    +set_planet_provider()
    +
    +set_planet_provider_hp()
    +
    ephemeris()
    @@ -5513,7 +5577,9 @@

    Author
    Attila Kovacs
    Since
    1.0
    -
    See also
    set_planet_provider_hp()
    +
    See also
    get_planet_provider()
    +
    +set_planet_provider_hp()
    solarsystem()
    @@ -5545,7 +5611,9 @@

    Author
    Attila Kovacs

    Since
    1.0
    -
    See also
    set_planet_provider()
    +
    See also
    get_planet_provider_hp()
    +
    +set_planet_provider()
    solarsystem_hp()
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    Parameters
    - - + +
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    numSolar-system body ID number (e.g. NAIF)
    nameName of object. By default converted to upper-case, unless novas_case_sensitive() was called with a non-zero argument. Max. SIZE_OF_OBJ_NAME long, including termination. If the ephemeris provider uses names, then the name should match those of the ephemeris provider – otherwise it is not important.
    numSolar-system body ID number (e.g. NAIF). The number should match the needs of the ephemeris provider used with NOVAS. (If the ephemeris provider is by name and not ID number, then the number here is not important).
    [out]bodyPointer to structure to populate.

    Returns
    0 if successful, or else -1 if the 'planet' pointer is NULL or the name is too long.
    -
    See also
    make_planet()
    +
    See also
    set_ephem_provider()
    +
    +make_planet()
    make_cat_entry()
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['novas_5fset_5funix_5ftime_27',['novas_set_unix_time',['../timescale_8c.html#abacd89aa380c85da2d3c19a7e2187df3',1,'novas_set_unix_time(time_t unix_time, long nanos, int leap, double dut1, novas_timespec *time): timescale.c'],['../novas_8h.html#abacd89aa380c85da2d3c19a7e2187df3',1,'novas_set_unix_time(time_t unix_time, long nanos, int leap, double dut1, novas_timespec *time): timescale.c']]], + ['novas_5fsky_5fpos_28',['novas_sky_pos',['../frames_8c.html#a4e894a83f3065bbb706212d1267dd2ab',1,'novas_sky_pos(const object *object, const novas_frame *frame, enum novas_reference_system sys, sky_pos *out): frames.c'],['../novas_8h.html#a3539b76356a7f8853fbb639aaa6bf02e',1,'novas_sky_pos(const object *object, const novas_frame *frame, enum novas_reference_system sys, sky_pos *output): frames.c']]], + ['novas_5fstandard_5frefraction_29',['novas_standard_refraction',['../refract_8c.html#ab04bff3b97c132e358e11c3a5b7a3081',1,'novas_standard_refraction(double jd_tt, const on_surface *loc, enum 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b/apidoc/html/search/searchdata.js index 8ceaf45d..1356dc89 100644 --- a/apidoc/html/search/searchdata.js +++ b/apidoc/html/search/searchdata.js @@ -1,6 +1,6 @@ var indexSectionsWithContent = { - 0: "0123abcdefghijklmnoprstuvwxy", + 0: "0123_abcdefghijklmnoprstuvwxy", 1: "cinors", 2: "efnrst", 3: "abcdefghijlmnoprstuvw", @@ -8,7 +8,7 @@ var indexSectionsWithContent = 5: "nr", 6: "n", 7: "ceijnpw", - 8: "abcdehimnrstx", + 8: "_abcdehimnrstx", 9: "acdlopstw" }; diff --git a/apidoc/html/solarsystem_8h.html b/apidoc/html/solarsystem_8h.html index 7472d537..fd8f4001 100644 --- a/apidoc/html/solarsystem_8h.html +++ b/apidoc/html/solarsystem_8h.html @@ -112,12 +112,21 @@
    +Macros | Typedefs | +Enumerations | Functions
    solarsystem.h File Reference
    + + + + +

    +Macros

    +#define NOVAS_ID_TYPES   (NOVAS_ID_CALCEPH + 1)
     Number of different Solar-system body ID types enumerated.
     
    @@ -127,6 +136,13 @@

    Typedefs

    typedef int(* novas_ephem_provider) (const char *name, long id, double jd_tdb_high, double jd_tdb_low, enum novas_origin *origin, double *pos, double *vel)
    typedef short(* novas_planet_provider_hp) (const double jd_tdb[2], enum novas_planet body, enum novas_origin origin, double *position, double *velocity)
     
    + + + +

    +Enumerations

    enum  novas_id_type { NOVAS_ID_NAIF = 0 +, NOVAS_ID_CALCEPH + }
     
    @@ -137,6 +153,16 @@ + + + + + + + + + + @@ -192,10 +218,11 @@

    Function to obtain ephemeris data for minor planets, which are not handled by the solarsystem() type calls. The library does not provide a default implementation, but users can provide their own, either as a default statically compiled readeph() implementation, or else a dynamically defined one via ephemeris_set_reader().

    +

    Note, that implementations would typically use either the name or the ID argument to identify the object for which ephemeris data is requested. As such you only need to specify the one that is going to be used.

    Parameters

    Functions

    short earth_sun_calc (double jd_tdb, enum novas_planet body, enum novas_origin origin, double *position, double *velocity)
     
    novas_ephem_provider get_ephem_provider ()
     
    novas_planet_provider get_planet_provider ()
     
    novas_planet_provider_hp get_planet_provider_hp ()
     
    enum novas_planet naif_to_novas_planet (long id)
     
    long novas_to_dexxx_planet (enum novas_planet id)
     
    long novas_to_naif_planet (enum novas_planet id)
     
    short planet_eph_manager (double jd_tdb, enum novas_planet body, enum novas_origin origin, double *position, double *velocity)
     
    short planet_eph_manager_hp (const double jd_tdb[2], enum novas_planet body, enum novas_origin origin, double *position, double *velocity)
    - - + + @@ -277,6 +304,31 @@

    ephemeris() + + +

    Enumeration Type Documentation

    + +

    ◆ novas_id_type

    + +
    +
    +

    idThe ID number of the solar-system body for which the position in desired.
    nameThe name of the solar-system body
    nameThe name of the solar-system body (in case the ephemeris provider is name based, otherwiase it may be NULL).
    idThe ID number of the solar-system body for which the position in desired. (Typically a NAIF ID, or else an appropriate ID for the implementation – corresponding minor planet objects should be created with the same type of ID.). If the ephemeris provider is name based the ID is not used an can be set to anything (-1 might be a good default).
    jd_tdb_high[day] The high-order part of Barycentric Dynamical Time (TDB) based Julian date for which to find the position and velocity. Typically this may be the integer part of the Julian date for high-precision calculations, or else the entire Julian date for reduced precision.
    jd_tdb_low[day] The low-order part of Barycentric Dynamical Time (TDB) based Julian date for which to find the position and velocity. Typically this may be the fractional part of the Julian date for high-precision calculations, or else 0.0 if the date is defined entirely by the high-order component for reduced precision.
    [out]originSet to NOVAS_BARYCENTER or NOVAS_HELIOCENTER to indicate relative to which the ephemeris positions/velocities are reported.
    + + + +
    enum novas_id_type
    +
    +

    Solar-system body IDs to use as object.number with NOVAS_EPHEM_OBJECT types. JPL ephemerides use NAIF IDs to identify objects in the Solar-system, which is thus the most widely adopted convention for numbering Solar-system bodies. But other numbering systems also exists, for example the CALCEPH library uses its own convention for the numbering of asteroids.

    +
    See also
    object
    +
    +NOVAS_EPHEM_OBJECT
    + + + +
    Enumerator
    NOVAS_ID_NAIF 

    If the ephemeris provider should use NAIF IDs.

    +
    NOVAS_ID_CALCEPH 

    If the ephemeris provider should use CALCEPH IDs.

    +
    +

    Function Documentation

    @@ -471,10 +523,163 @@

    Returns
    the currently defined function for accessing ephemeris data for minor planets or satellites, ot NULL if no function was set via set_ephem_provider() previously.

    See also
    set_ephem_provider()
    +get_planet_provider()
    +
    +get_planet_provider_hp()
    +
    ephemeris()
    Since
    1.0
    Author
    Attila Kovacs
    + + + +

    ◆ get_planet_provider()

    + +
    +
    + + + + + + + +
    novas_planet_provider get_planet_provider ()
    +
    +

    Returns the custom (low-precision) ephemeris provider function for major planets (and Sun, Moon, SSB), if any.

    +
    Returns
    the custom (low-precision) planet ephemeris provider function.
    +
    Author
    Attila Kovacs
    +
    Since
    1.2
    +
    See also
    set_planet_provider()
    +
    +get_planet_provider_hp()
    +
    +get_ephem_provider()
    + +
    +
    + +

    ◆ get_planet_provider_hp()

    + +
    +
    + + + + + + + +
    novas_planet_provider_hp get_planet_provider_hp ()
    +
    +

    Returns the custom high-precision ephemeris provider function for major planets (and Sun, Moon, SSB), if any.

    +
    Returns
    the custom high-precision planet ephemeris provider function.
    +
    Author
    Attila Kovacs
    +
    Since
    1.2
    +
    See also
    set_planet_provider_hp()
    +
    +get_planet_provider()
    +
    +get_ephem_provider()
    + +
    +
    + +

    ◆ naif_to_novas_planet()

    + +
    +
    + + + + + + + + +
    enum novas_planet naif_to_novas_planet (long id)
    +
    +

    Converts a NAIF ID to a NOVAS major planet ID. It account for the different IDs used for Sun, Moon and SSB. Otherwise NAIF planet barycenters are mapped to the corresponding bodies, except EMB (3), which will return -1. NAIF body centers n99 (e.g. 399 for Earth), are mapped to the corresponding NOVAS planet number n. All other NAIF IDs will return -1, indicating no match to a NOVAS planet ID.

    +
    Parameters
    + + +
    idThe NAIF ID of the major planet of interest
    +
    +
    +
    Returns
    the NOVAS ID for the same object (which may or may not be different from the input), or -1 if the NAIF ID cannot be matched to a NOVAS major planet.
    +
    See also
    novas_to_naif_planet()
    +
    +novas_to_dexxx_planet()
    +
    Author
    Attila Kovacs
    +
    Since
    1.2
    + +

    References NAIF_EMB, NAIF_MOON, NAIF_SSB, NAIF_SUN, NOVAS_MERCURY, NOVAS_MOON, NOVAS_PLUTO, NOVAS_SSB, and NOVAS_SUN.

    + +
    +
    + +

    ◆ novas_to_dexxx_planet()

    + +
    +
    + + + + + + + + +
    long novas_to_dexxx_planet (enum novas_planet id)
    +
    +

    Converts a NOVAS Solar-system body ID to a NAIF Solar-system body ID for DExxx ephemeris files. The DExxx (e.g. DE440) ephemeris files use NAIF IDs, but for most planets contain barycentric data only rather than that of the planet center. For Earth-based observations, it only really makes a difference whether the 3 is used for the Earth-Moon Barycenter (EMB) or 399 for the geocenter.

    +
    Parameters
    + + +
    idThe NOVAS ID of the major planet of interest
    +
    +
    +
    Returns
    the NAIF ID for the same object (which may or may not be different from the input), as appropriate for use in the DExxx ephemeris files.
    +
    See also
    novas_to_naif_planet()
    +
    +naif_to_novas_planet()
    +
    Author
    Attila Kovacs
    +
    Since
    1.2
    + +

    References NAIF_EARTH, NAIF_MOON, NAIF_SSB, NAIF_SUN, NOVAS_EARTH, NOVAS_MERCURY, NOVAS_MOON, NOVAS_PLUTO, NOVAS_SSB, and NOVAS_SUN.

    + +
    +
    + +

    ◆ novas_to_naif_planet()

    + +
    +
    + + + + + + + + +
    long novas_to_naif_planet (enum novas_planet id)
    +
    +

    Converts a NOVAS Solar-system body ID to a NAIF Solar-system body ID. NOVAS and NAIF use slightly different IDs for major planets, the Moon, and the Solar-system Barycenter (SSB). In NOVAS, major planets are have IDs ranging from 1 through 9, but for NAIF 1–9 are the planetary barycenters and the planet centers have numbers in the hundreds ending with 99 (e.g. the center of Earth is NAIF 399; 3 is the NOVAS ID for Earth and the NAIF ID for the Earth-Moon Barycenter [EMB]). The Sun and Moon also have distinct IDs in NAIF vs NOVAS.

    +
    Parameters
    + + +
    idThe NOVAS ID of the major planet of interest
    +
    +
    +
    Returns
    the NAIF ID for the same object or planet center (which may or may not be different from the input)
    +
    See also
    naif_to_novas_planet()
    +
    Author
    Attila Kovacs
    +
    Since
    1.2
    + +

    References NAIF_MOON, NAIF_SSB, NAIF_SUN, NOVAS_MERCURY, NOVAS_MOON, NOVAS_PLUTO, NOVAS_SSB, and NOVAS_SUN.

    +
    @@ -521,7 +726,7 @@

    Provides an interface between the JPL direct-access solar system ephemerides and NOVAS-C for regular (reduced) precision applications.

    -

    This function and planet_ephemeris() were designed to work with the 1997 version of the JPL ephemerides, as noted in the references.

    +

    This function and planet_eph_manager_hp() were designed to work with the 1997 version of the JPL ephemerides, as noted in the references.

    The user must create the binary ephemeris files using software from JPL, and open the file using function ephem_open(), prior to calling this function.

    REFERENCES:

    1. @@ -600,7 +805,7 @@

      Provides an interface between the JPL direct-access solar system ephemerides and NOVAS-C for highest precision applications.

      -

      This function and planet_ephemeris() were designed to work with the 1997 version of the JPL ephemerides, as noted in the references.

      +

      This function and planet_eph_manager() were designed to work with the 1997 version of the JPL ephemerides, as noted in the references.

      The user must create the binary ephemeris files using software from JPL, and open the file using function ephem_open(), prior to calling this function.

      REFERENCES:

      1. @@ -1008,6 +1213,10 @@

        Author
        Attila Kovacs

    See also
    get_ephem_provider()
    +set_planet_provider()
    +
    +set_planet_provider_hp()
    +
    ephemeris()
    @@ -1036,7 +1245,9 @@

    Author
    Attila Kovacs

    Since
    1.0
    -
    See also
    set_planet_provider_hp()
    +
    See also
    get_planet_provider()
    +
    +set_planet_provider_hp()
    solarsystem()
    @@ -1068,7 +1279,9 @@

    Author
    Attila Kovacs

    Since
    1.0
    -
    See also
    set_planet_provider()
    +
    See also
    get_planet_provider_hp()
    +
    +set_planet_provider()
    solarsystem_hp()
    diff --git a/apidoc/html/solarsystem_8h.js b/apidoc/html/solarsystem_8h.js index 5a4fc88f..006083fa 100644 --- a/apidoc/html/solarsystem_8h.js +++ b/apidoc/html/solarsystem_8h.js @@ -1,12 +1,22 @@ var solarsystem_8h = [ + [ "NOVAS_ID_TYPES", "solarsystem_8h.html#a9a736e59fc9bfdc92b7245aa37d529ee", null ], [ "novas_ephem_provider", "solarsystem_8h.html#ac2ae695519a5b600a105243f4e30c3ab", null ], [ "novas_planet_provider", "solarsystem_8h.html#ae7eb9e64aa00ee757946488fa99351ec", null ], [ "novas_planet_provider_hp", "solarsystem_8h.html#a85ed597fa94ecf72653e64f4afa7f833", null ], + [ "novas_id_type", "solarsystem_8h.html#ac42df1db80fbcb6f7a72de80d9f9c531", [ + [ "NOVAS_ID_NAIF", "solarsystem_8h.html#ac42df1db80fbcb6f7a72de80d9f9c531ab3e6efc1ad89e02f915df25265ec32db", null ], + [ "NOVAS_ID_CALCEPH", "solarsystem_8h.html#ac42df1db80fbcb6f7a72de80d9f9c531a074c723dfc1f03c82d52347c46ee0719", null ] + ] ], [ "earth_sun_calc", "solarsystem_8h.html#ab5d74f84f8e75e90dfc30ebde562d076", null ], [ "earth_sun_calc_hp", "solarsystem_8h.html#a3e6398e29968a48f9de090e82423750f", null ], [ "enable_earth_sun_hp", "solarsystem_8h.html#a279bca0519117cee9a3bd4382f38e7ad", null ], [ "get_ephem_provider", "solarsystem_8h.html#aa6fad38297a49ba78a6bd49cedf889b1", null ], + [ "get_planet_provider", "solarsystem_8h.html#a0f0a786b5614a788c02b37a462eae2d2", null ], + [ "get_planet_provider_hp", "solarsystem_8h.html#ae45badb450c1ca73920d982e12346c5b", null ], + [ "naif_to_novas_planet", "solarsystem_8h.html#a1c4b3f67a3b82808dd16ae43dfaf0f86", null ], + [ "novas_to_dexxx_planet", "solarsystem_8h.html#ac3eb54acf22dc155879163de89c6865e", null ], + [ "novas_to_naif_planet", "solarsystem_8h.html#ab51ac9bdf7736e1c1582e0981046daf3", null ], [ "planet_eph_manager", "solarsystem_8h.html#a71d2bfef45818d56e359205c57db0694", null ], [ "planet_eph_manager_hp", "solarsystem_8h.html#acacfbde919107d0514da5c7d8508917b", null ], [ "planet_ephem_provider", "solarsystem_8h.html#a61c60adf57c00d797fac94bb5841c271", null ], diff --git a/apidoc/html/solsys-calceph_8c.html b/apidoc/html/solsys-calceph_8c.html new file mode 100644 index 00000000..3085012b --- /dev/null +++ b/apidoc/html/solsys-calceph_8c.html @@ -0,0 +1,247 @@ + + + + + + + + + + + + + + + + + + + + +SuperNOVAS: src/solsys-calceph.c File Reference + + + + + + + + + + + + + + + +
    +
    + + + + + + + +
    +
    SuperNOVAS v1.2 +
    +
    The NOVAS C library, made better
    +
    +
    + + + + + + + +
    +
    + +
    +
    +
    + +
    + +
    +
    + + +
    +
    +
    +
    +
    +
    Loading...
    +
    Searching...
    +
    No Matches
    +
    +
    +
    +
    + +
    +
    +Functions
    +
    solsys-calceph.c File Reference
    +
    +
    + + + + + + + + +

    +Functions

    int novas_calceph_use_ids (enum novas_id_type idtype)
     
    int novas_use_calceph (t_calcephbin *eph)
     
    int novas_use_calceph_planets (t_calcephbin *eph)
     
    +

    Detailed Description

    +
    Author
    A. Kovacs
    +

    SuperNOVAS major planet ephemeris lookup implementation via the CALCEPH C library See https://calceph.imcce.fr/docs/4.0.0/html/c/

    +

    CALCEPH source code is at https://gitlab.obspm.fr/imcce_calceph/calceph

    +

    Function Documentation

    + +

    ◆ novas_calceph_use_ids()

    + +
    +
    + + + + + + + + +
    int novas_calceph_use_ids (enum novas_id_type idtype)
    +
    +

    Sets the type of Solar-system body IDs to use as object.number with NOVAS_EPHEM_OBJECT types. CALCEPH supports the use of both NAIF and its own numbering system to identify Solar-system bodies. So, this function gives you the choice on which numbering system you want to use in object data structures. The choice does not affect major planets (which always use the NOVAS numbering scheme), or catalog objects.

    +
    Parameters
    + + +
    idtypeNOVAS_ID_NAIF to use NAIF IDs (default) or else NOVAS_ID_CALCEPH to use the CALCEPH body numbering convention for object.
    +
    +
    +
    Returns
    0 if successful or else -1 (errno set to EINVAL) if the input value is invalid.
    +
    See also
    object
    +
    +NOVAS_EPHEM_OBJECT
    + +

    References NOVAS_ID_CALCEPH, and NOVAS_ID_NAIF.

    + +
    +
    + +

    ◆ novas_use_calceph()

    + +
    +
    + + + + + + + + +
    int novas_use_calceph (t_calcephbin * eph)
    +
    +

    Sets a ephemeris provider for Solar-system objects using the CALCEPH C library and the specified set of ephemeris files. If the supplied ephemeris files contain data for major planets also, they can be used by planet_calceph() / planet_calceph_hp() also, unless a separate CALCEPH ephemeris data is set via novas_use_calceph_planets().

    +

    The call also make CALCEPH the default ephemeris provider for all types of Solar-system objects. If you want to use another provider for major planets, you need to call set_planet_provider() / set_planet_provider_hp() afterwards to specify a different provider for major planets (and Sun, Moon, SSB).

    +
    Parameters
    + + +
    ephPointer to the CALCEPH ephemeris data that have been opened.
    +
    +
    +
    Returns
    0 if successful, or else -1 (errno will indicate the type of error).
    +
    See also
    novas_calceph_use_ids()
    +
    +novas_use_calceph_planets()
    +
    +set_ephem_provider()
    +
    Author
    Attila Kovacs
    +
    Since
    1.2
    + +

    References novas_use_calceph_planets(), and set_ephem_provider().

    + +
    +
    + +

    ◆ novas_use_calceph_planets()

    + +
    +
    + + + + + + + + +
    int novas_use_calceph_planets (t_calcephbin * eph)
    +
    +

    Sets a ephemeris provider for the major planets (and Sun, Moon, and SSB) using the CALCEPH C library and the specified ephemeris data.

    +

    The call also make CALCEPH the default ephemeris providers for major planets.

    +
    Parameters
    + + +
    ephPointer to the CALCEPH ephemeris data for the major planets (including Sun, Moon, and SSB) that have been opened.
    +
    +
    +
    Returns
    0 if successful, or else -1 (errno will indicate the type of error).
    +
    See also
    novas_use_calceph()
    +
    +set_planet_provider()
    +
    +set_planet_provider_hp()
    +
    Author
    Attila Kovacs
    +
    Since
    1.2
    + +

    References set_planet_provider(), and set_planet_provider_hp().

    + +
    +
    +
    +
    + + + + diff --git a/apidoc/html/solsys-calceph_8c.js b/apidoc/html/solsys-calceph_8c.js new file mode 100644 index 00000000..5810810a --- /dev/null +++ b/apidoc/html/solsys-calceph_8c.js @@ -0,0 +1,6 @@ +var solsys_calceph_8c = +[ + [ "novas_calceph_use_ids", "solsys-calceph_8c.html#a5531b937a5bb5491cb475d2536346ad8", null ], + [ "novas_use_calceph", "solsys-calceph_8c.html#a35fc86a939602ec910dbdfde180d7f31", null ], + [ "novas_use_calceph_planets", "solsys-calceph_8c.html#ab86ec03898e658c86c671a8b6399e331", null ] +]; \ No newline at end of file diff --git a/apidoc/html/solsys1_8c.html b/apidoc/html/solsys1_8c.html index 384fdc30..793249df 100644 --- a/apidoc/html/solsys1_8c.html +++ b/apidoc/html/solsys1_8c.html @@ -184,7 +184,7 @@

    Provides an interface between the JPL direct-access solar system ephemerides and NOVAS-C for regular (reduced) precision applications.

    -

    This function and planet_ephemeris() were designed to work with the 1997 version of the JPL ephemerides, as noted in the references.

    +

    This function and planet_eph_manager_hp() were designed to work with the 1997 version of the JPL ephemerides, as noted in the references.

    The user must create the binary ephemeris files using software from JPL, and open the file using function ephem_open(), prior to calling this function.

    REFERENCES:

    1. @@ -263,7 +263,7 @@

      Provides an interface between the JPL direct-access solar system ephemerides and NOVAS-C for highest precision applications.

      -

      This function and planet_ephemeris() were designed to work with the 1997 version of the JPL ephemerides, as noted in the references.

      +

      This function and planet_eph_manager() were designed to work with the 1997 version of the JPL ephemerides, as noted in the references.

      The user must create the binary ephemeris files using software from JPL, and open the file using function ephem_open(), prior to calling this function.

      REFERENCES:

      1. diff --git a/apidoc/html/super_8c.html b/apidoc/html/super_8c.html index 15bf7685..6231a5f5 100644 --- a/apidoc/html/super_8c.html +++ b/apidoc/html/super_8c.html @@ -1367,14 +1367,16 @@

        Parameters
        - - + +
        nameName of object. By default converted to upper-case, unless novas_case_sensitive() was called with a non-zero argument. Max. SIZE_OF_OBJ_NAME long, including termination.
        numSolar-system body ID number (e.g. NAIF)
        nameName of object. By default converted to upper-case, unless novas_case_sensitive() was called with a non-zero argument. Max. SIZE_OF_OBJ_NAME long, including termination. If the ephemeris provider uses names, then the name should match those of the ephemeris provider – otherwise it is not important.
        numSolar-system body ID number (e.g. NAIF). The number should match the needs of the ephemeris provider used with NOVAS. (If the ephemeris provider is by name and not ID number, then the number here is not important).
        [out]bodyPointer to structure to populate.

    Returns
    0 if successful, or else -1 if the 'planet' pointer is NULL or the name is too long.
    -
    See also
    make_planet()
    +
    See also
    set_ephem_provider()
    +
    +make_planet()
    make_cat_entry()
    diff --git a/apidoc/html/toc.xml b/apidoc/html/toc.xml index 5a60b295..3330f9d7 100644 --- a/apidoc/html/toc.xml +++ b/apidoc/html/toc.xml @@ -34,14 +34,15 @@ - - - + + + + - + - - + + @@ -196,6 +197,13 @@ + + + + + + + @@ -647,13 +655,23 @@ + + + + + + + + + + @@ -709,6 +727,12 @@ + + + + + + @@ -742,6 +766,8 @@ + + @@ -837,6 +863,11 @@ + + + + + @@ -917,7 +948,8 @@ - + + diff --git a/apidoc/man/man3/md_CHANGELOG.3 b/apidoc/man/man3/md_CHANGELOG.3 index 67f320bc..b4fe9a11 100644 --- a/apidoc/man/man3/md_CHANGELOG.3 +++ b/apidoc/man/man3/md_CHANGELOG.3 @@ -18,6 +18,12 @@ Changes expected for the next bug-fix release, expected around 1 December 2024\& #57: New generic redshift-handling functions \fC\fBnovas_v2z()\fP\fP, \fC\fBnovas_z2v()\fP\fP, .IP "\(bu" 2 #58: New functions to calculate and apply additional gravitational redshift corrections for light that originates near massive gravitating bodies (other than major planets, or Sun or Moon), or for observers located near massive gravitating bodies (other than the Sun and Earth)\&. The added functions are \fC\fBgrav_redshift()\fP\fP, \fCredhift_vrad()\fP, \fC\fBunredshift_vrad()\fP\fP, \fC\fBnovas_z_add()\fP\fP, and \fC\fBnovas_z_inv()\fP\fP\&. +.IP "\(bu" 2 +#83: CALCEPH integration: \fC\fBnovas_use_calceph()\fP\fP and/or \fC\fBnovas_use_calceph_planets()\fP\fP to specify and use ephemeris data via CALCEPH for Solar-system sources in general, and for major planets specifically; and \fC\fBnovas_calceph_use_ids()\fP\fP to specify whether \fC\fBobject\&.number\fP\fP in \fCNOVAS_EPHEM_OBJECT\fP type objects is a NAIF ID (default) or else a CALCEPH ID number of the Solar-system body\&. These functions are provided by the \fClibsolsys-calceph\&.so[\&.1]\fP and/or \fC\&.a\fP plugin libraries, which are built contingent on the \fCCALCEPH_SUPPORT\fP variable being set to 1 prior to the build\&. The build of the plugin module requires an accessible installation of the CALCEPH development files (C headers and unversioned static or shared libraries depending on the needs of the build)\&. +.IP "\(bu" 2 +NOVAS-NAIF conversions for major planets (and Sun, Moon, SSB): \fC\fBnovas_to_naif_planet()\fP\fP (planet centers), \fC\fBnovas_to_dexxx_planet()\fP\fP (mixed planet center/barycenter for DExxx ephemeris files), and the inverse \fC\fBnaif_to_novas_planet()\fP\fP\&. +.IP "\(bu" 2 +Added \fC\fBget_planet_provider()\fP\fP and \fC\fBget_planet_provider_hp()\fP\fP functions for convenience to return the \fC\fBsolarsystem()\fP\fP / \fC\fBsolarsystem_hp()\fP\fP type custom planet ephemeris provider functions currently configured, so they may be used directly, outside of \fC\fBephemeris()\fP\fP calls\&. .PP .SH "[1\&.1\&.1] - 2024-10-28" .PP diff --git a/apidoc/man/man3/naif.c.3 b/apidoc/man/man3/naif.c.3 new file mode 100644 index 00000000..77bda956 --- /dev/null +++ b/apidoc/man/man3/naif.c.3 @@ -0,0 +1,153 @@ +.TH "src/naif.c" 3 "Version v1.2" "SuperNOVAS" \" -*- nroff -*- +.ad l +.nh +.SH NAME +src/naif.c +.SH SYNOPSIS +.br +.PP +.SS "Macros" + +.in +1c +.ti -1c +.RI "#define \fB__NOVAS_INTERNAL_API__\fP" +.br +.RI "Use definitions meant for internal use by SuperNOVAS only\&. " +.in -1c +.SS "Functions" + +.in +1c +.ti -1c +.RI "enum \fBnovas_planet\fP \fBnaif_to_novas_planet\fP (long id)" +.br +.ti -1c +.RI "long \fBnovas_to_dexxx_planet\fP (enum \fBnovas_planet\fP id)" +.br +.ti -1c +.RI "long \fBnovas_to_naif_planet\fP (enum \fBnovas_planet\fP id)" +.br +.in -1c +.SH "Detailed Description" +.PP + +.PP +\fBDate\fP +.RS 4 +Created on Nov 6, 2024 +.RE +.PP +\fBAuthor\fP +.RS 4 +Attila Kovacs +.RE +.PP +Solar system ID mappings between NOVAS and NASA's Navigation and Ancillary Information Facility (NAIF), which is used by the JPL ephemeris systems\&. The two differ for the numbering convention for major planets, the Sun, Moon, Solar-System Barycenter (SSB) and the Earth-Moon Barycenter (EMB)\&. NOVAS does not have predefined IDs beyond this set (and no defined ID for EMB), thus for all other objects we'll assume and use NOVAS IDs that match NAIF\&. +.PP +\fBSince\fP +.RS 4 +1\&.2 +.RE +.PP + +.SH "Function Documentation" +.PP +.SS "enum \fBnovas_planet\fP naif_to_novas_planet (long id)" +Converts a NAIF ID to a NOVAS major planet ID\&. It account for the different IDs used for Sun, Moon and SSB\&. Otherwise NAIF planet barycenters are mapped to the corresponding bodies, except EMB (3), which will return -1\&. NAIF body centers \fIn\fP99 (e\&.g\&. 399 for Earth), are mapped to the corresponding NOVAS planet number \fIn\fP\&. All other NAIF IDs will return -1, indicating no match to a NOVAS planet ID\&. +.PP +\fBParameters\fP +.RS 4 +\fIid\fP The NAIF ID of the major planet of interest +.RE +.PP +\fBReturns\fP +.RS 4 +the NOVAS ID for the same object (which may or may not be different from the input), or -1 if the NAIF ID cannot be matched to a NOVAS major planet\&. +.RE +.PP +\fBSee also\fP +.RS 4 +\fBnovas_to_naif_planet()\fP +.PP +\fBnovas_to_dexxx_planet()\fP +.RE +.PP +\fBAuthor\fP +.RS 4 +Attila Kovacs +.RE +.PP +\fBSince\fP +.RS 4 +1\&.2 +.RE +.PP + +.PP +References \fBNAIF_EMB\fP, \fBNAIF_MOON\fP, \fBNAIF_SSB\fP, \fBNAIF_SUN\fP, \fBNOVAS_MERCURY\fP, \fBNOVAS_MOON\fP, \fBNOVAS_PLUTO\fP, \fBNOVAS_SSB\fP, and \fBNOVAS_SUN\fP\&. +.SS "long novas_to_dexxx_planet (enum \fBnovas_planet\fP id)" +Converts a NOVAS Solar-system body ID to a NAIF Solar-system body ID for DExxx ephemeris files\&. The DExxx (e\&.g\&. DE440) ephemeris files use NAIF IDs, but for most planets contain barycentric data only rather than that of the planet center\&. For Earth-based observations, it only really makes a difference whether the 3 is used for the Earth-Moon Barycenter (EMB) or 399 for the geocenter\&. +.PP +\fBParameters\fP +.RS 4 +\fIid\fP The NOVAS ID of the major planet of interest +.RE +.PP +\fBReturns\fP +.RS 4 +the NAIF ID for the same object (which may or may not be different from the input), as appropriate for use in the DExxx ephemeris files\&. +.RE +.PP +\fBSee also\fP +.RS 4 +\fBnovas_to_naif_planet()\fP +.PP +\fBnaif_to_novas_planet()\fP +.RE +.PP +\fBAuthor\fP +.RS 4 +Attila Kovacs +.RE +.PP +\fBSince\fP +.RS 4 +1\&.2 +.RE +.PP + +.PP +References \fBNAIF_EARTH\fP, \fBNAIF_MOON\fP, \fBNAIF_SSB\fP, \fBNAIF_SUN\fP, \fBNOVAS_EARTH\fP, \fBNOVAS_MERCURY\fP, \fBNOVAS_MOON\fP, \fBNOVAS_PLUTO\fP, \fBNOVAS_SSB\fP, and \fBNOVAS_SUN\fP\&. +.SS "long novas_to_naif_planet (enum \fBnovas_planet\fP id)" +Converts a NOVAS Solar-system body ID to a NAIF Solar-system body ID\&. NOVAS and NAIF use slightly different IDs for major planets, the Moon, and the Solar-system Barycenter (SSB)\&. In NOVAS, major planets are have IDs ranging from 1 through 9, but for NAIF 1--9 are the planetary barycenters and the planet centers have numbers in the hundreds ending with 99 (e\&.g\&. the center of Earth is NAIF 399; 3 is the NOVAS ID for Earth and the NAIF ID for the Earth-Moon Barycenter [EMB])\&. The Sun and Moon also have distinct IDs in NAIF vs NOVAS\&. +.PP +\fBParameters\fP +.RS 4 +\fIid\fP The NOVAS ID of the major planet of interest +.RE +.PP +\fBReturns\fP +.RS 4 +the NAIF ID for the same object or planet center (which may or may not be different from the input) +.RE +.PP +\fBSee also\fP +.RS 4 +\fBnaif_to_novas_planet()\fP +.RE +.PP +\fBAuthor\fP +.RS 4 +Attila Kovacs +.RE +.PP +\fBSince\fP +.RS 4 +1\&.2 +.RE +.PP + +.PP +References \fBNAIF_MOON\fP, \fBNAIF_SSB\fP, \fBNAIF_SUN\fP, \fBNOVAS_MERCURY\fP, \fBNOVAS_MOON\fP, \fBNOVAS_PLUTO\fP, \fBNOVAS_SSB\fP, and \fBNOVAS_SUN\fP\&. +.SH "Author" +.PP +Generated automatically by Doxygen for SuperNOVAS from the source code\&. diff --git a/apidoc/man/man3/naif.h.3 b/apidoc/man/man3/naif.h.3 new file mode 100644 index 00000000..4893ecfe --- /dev/null +++ b/apidoc/man/man3/naif.h.3 @@ -0,0 +1,50 @@ +.TH "include/naif.h" 3 "Version v1.2" "SuperNOVAS" \" -*- nroff -*- +.ad l +.nh +.SH NAME +include/naif.h +.SH SYNOPSIS +.br +.PP +.SS "Macros" + +.in +1c +.ti -1c +.RI "#define \fBNAIF_EARTH\fP 399" +.br +.RI "NAIF ID for the geocenter\&. " +.ti -1c +.RI "#define \fBNAIF_EMB\fP 3" +.br +.RI "NAIF ID for the Earth-Moon Barycenter (EMB) " +.ti -1c +.RI "#define \fBNAIF_MOON\fP 301" +.br +.RI "NAIF ID for the Moon\&. " +.ti -1c +.RI "#define \fBNAIF_SSB\fP 0" +.br +.RI "NAIF ID for the Solar-System Barycenter (SSB) " +.ti -1c +.RI "#define \fBNAIF_SUN\fP 10" +.br +.RI "NAIF_ID for the Sun\&. " +.in -1c +.SH "Detailed Description" +.PP + +.PP +\fBDate\fP +.RS 4 +Created on Nov 6, 2024 +.RE +.PP +\fBAuthor\fP +.RS 4 +Attila Kovacs +.RE +.PP + +.SH "Author" +.PP +Generated automatically by Doxygen for SuperNOVAS from the source code\&. diff --git a/apidoc/man/man3/novas.c.3 b/apidoc/man/man3/novas.c.3 index ab5baf15..68810b76 100644 --- a/apidoc/man/man3/novas.c.3 +++ b/apidoc/man/man3/novas.c.3 @@ -106,6 +106,12 @@ src/novas.c .RI "\fBnovas_ephem_provider\fP \fBget_ephem_provider\fP ()" .br .ti -1c +.RI "\fBnovas_planet_provider\fP \fBget_planet_provider\fP ()" +.br +.ti -1c +.RI "\fBnovas_planet_provider_hp\fP \fBget_planet_provider_hp\fP ()" +.br +.ti -1c .RI "short \fBgrav_def\fP (double jd_tdb, enum \fBnovas_observer_place\fP unused, enum \fBnovas_accuracy\fP accuracy, const double *pos_src, const double *pos_obs, double *out)" .br .ti -1c @@ -1649,6 +1655,10 @@ the currently defined function for accessing ephemeris data for minor planets or .RS 4 \fBset_ephem_provider()\fP .PP +\fBget_planet_provider()\fP +.PP +\fBget_planet_provider_hp()\fP +.PP \fBephemeris()\fP .RE .PP @@ -1663,6 +1673,62 @@ Attila Kovacs .RE .PP +.SS "\fBnovas_planet_provider\fP get_planet_provider ()" +Returns the custom (low-precision) ephemeris provider function for major planets (and Sun, Moon, SSB), if any\&. +.PP +\fBReturns\fP +.RS 4 +the custom (low-precision) planet ephemeris provider function\&. +.RE +.PP +\fBAuthor\fP +.RS 4 +Attila Kovacs +.RE +.PP +\fBSince\fP +.RS 4 +1\&.2 +.RE +.PP +\fBSee also\fP +.RS 4 +\fBset_planet_provider()\fP +.PP +\fBget_planet_provider_hp()\fP +.PP +\fBget_ephem_provider()\fP +.RE +.PP + +.SS "\fBnovas_planet_provider_hp\fP get_planet_provider_hp ()" +Returns the custom high-precision ephemeris provider function for major planets (and Sun, Moon, SSB), if any\&. +.PP +\fBReturns\fP +.RS 4 +the custom high-precision planet ephemeris provider function\&. +.RE +.PP +\fBAuthor\fP +.RS 4 +Attila Kovacs +.RE +.PP +\fBSince\fP +.RS 4 +1\&.2 +.RE +.PP +\fBSee also\fP +.RS 4 +\fBset_planet_provider_hp()\fP +.PP +\fBget_planet_provider()\fP +.PP +\fBget_ephem_provider()\fP +.RE +.PP + .SS "short grav_def (double jd_tdb, enum \fBnovas_observer_place\fP unused, enum \fBnovas_accuracy\fP accuracy, const double * pos_src, const double * pos_obs, double * out)" Computes the total gravitational deflection of light for the observed object due to the major gravitating bodies in the solar system\&. This function valid for an observed body within the solar system as well as for a star\&. .PP @@ -3551,6 +3617,10 @@ Attila Kovacs .RS 4 \fBget_ephem_provider()\fP .PP +\fBset_planet_provider()\fP +.PP +\fBset_planet_provider_hp()\fP +.PP \fBephemeris()\fP .RE .PP @@ -3604,6 +3674,8 @@ Attila Kovacs .PP \fBSee also\fP .RS 4 +\fBget_planet_provider()\fP +.PP \fBset_planet_provider_hp()\fP .PP \fBsolarsystem()\fP @@ -3632,6 +3704,8 @@ Attila Kovacs .PP \fBSee also\fP .RS 4 +\fBget_planet_provider_hp()\fP +.PP \fBset_planet_provider()\fP .PP \fBsolarsystem_hp()\fP diff --git a/apidoc/man/man3/novas.h.3 b/apidoc/man/man3/novas.h.3 index e7072644..b8739891 100644 --- a/apidoc/man/man3/novas.h.3 +++ b/apidoc/man/man3/novas.h.3 @@ -4116,9 +4116,9 @@ Sets a celestial object to be a Solar-system ephemeris body\&. Typically this wo .PP \fBParameters\fP .RS 4 -\fIname\fP Name of object\&. By default converted to upper-case, unless \fBnovas_case_sensitive()\fP was called with a non-zero argument\&. Max\&. SIZE_OF_OBJ_NAME long, including termination\&. +\fIname\fP Name of object\&. By default converted to upper-case, unless \fBnovas_case_sensitive()\fP was called with a non-zero argument\&. Max\&. SIZE_OF_OBJ_NAME long, including termination\&. If the ephemeris provider uses names, then the name should match those of the ephemeris provider -- otherwise it is not important\&. .br -\fInum\fP Solar-system body ID number (e\&.g\&. NAIF) +\fInum\fP Solar-system body ID number (e\&.g\&. NAIF)\&. The number should match the needs of the ephemeris provider used with NOVAS\&. (If the ephemeris provider is by name and not ID number, then the number here is not important)\&. .br \fIbody\fP Pointer to structure to populate\&. .RE @@ -4130,6 +4130,8 @@ Sets a celestial object to be a Solar-system ephemeris body\&. Typically this wo .PP \fBSee also\fP .RS 4 +\fBset_ephem_provider()\fP +.PP \fBmake_planet()\fP .PP \fBmake_cat_entry()\fP diff --git a/apidoc/man/man3/solarsystem.h.3 b/apidoc/man/man3/solarsystem.h.3 index 04e7b910..df857eb4 100644 --- a/apidoc/man/man3/solarsystem.h.3 +++ b/apidoc/man/man3/solarsystem.h.3 @@ -6,6 +6,14 @@ include/solarsystem.h .SH SYNOPSIS .br .PP +.SS "Macros" + +.in +1c +.ti -1c +.RI "#define \fBNOVAS_ID_TYPES\fP (\fBNOVAS_ID_CALCEPH\fP + 1)" +.br +.RI "Number of different Solar-system body ID types enumerated\&. " +.in -1c .SS "Typedefs" .in +1c @@ -19,6 +27,13 @@ include/solarsystem.h .RI "typedef short(* \fBnovas_planet_provider_hp\fP) (const double jd_tdb[2], enum \fBnovas_planet\fP body, enum \fBnovas_origin\fP origin, double *position, double *velocity)" .br .in -1c +.SS "Enumerations" + +.in +1c +.ti -1c +.RI "enum \fBnovas_id_type\fP { \fBNOVAS_ID_NAIF\fP = 0, \fBNOVAS_ID_CALCEPH\fP }" +.br +.in -1c .SS "Functions" .in +1c @@ -35,6 +50,21 @@ include/solarsystem.h .RI "\fBnovas_ephem_provider\fP \fBget_ephem_provider\fP ()" .br .ti -1c +.RI "\fBnovas_planet_provider\fP \fBget_planet_provider\fP ()" +.br +.ti -1c +.RI "\fBnovas_planet_provider_hp\fP \fBget_planet_provider_hp\fP ()" +.br +.ti -1c +.RI "enum \fBnovas_planet\fP \fBnaif_to_novas_planet\fP (long id)" +.br +.ti -1c +.RI "long \fBnovas_to_dexxx_planet\fP (enum \fBnovas_planet\fP id)" +.br +.ti -1c +.RI "long \fBnovas_to_naif_planet\fP (enum \fBnovas_planet\fP id)" +.br +.ti -1c .RI "short \fBplanet_eph_manager\fP (double jd_tdb, enum \fBnovas_planet\fP body, enum \fBnovas_origin\fP origin, double *position, double *velocity)" .br .ti -1c @@ -113,11 +143,13 @@ U\&. S\&. Naval Observatory .SS "typedef int(* novas_ephem_provider) (const char *name, long id, double jd_tdb_high, double jd_tdb_low, enum \fBnovas_origin\fP *origin, double *pos, double *vel)" Function to obtain ephemeris data for minor planets, which are not handled by the \fBsolarsystem()\fP type calls\&. The library does not provide a default implementation, but users can provide their own, either as a default statically compiled \fBreadeph()\fP implementation, or else a dynamically defined one via ephemeris_set_reader()\&. .PP +Note, that implementations would typically use either the name or the ID argument to identify the object for which ephemeris data is requested\&. As such you only need to specify the one that is going to be used\&. +.PP \fBParameters\fP .RS 4 -\fIid\fP The ID number of the solar-system body for which the position in desired\&. +\fIname\fP The name of the solar-system body (in case the ephemeris provider is name based, otherwiase it may be NULL)\&. .br -\fIname\fP The name of the solar-system body +\fIid\fP The ID number of the solar-system body for which the position in desired\&. (Typically a NAIF ID, or else an appropriate ID for the implementation -- corresponding minor planet objects should be created with the same type of ID\&.)\&. If the ephemeris provider is name based the ID is not used an can be set to anything (-1 might be a good default)\&. .br \fIjd_tdb_high\fP [day] The high-order part of Barycentric Dynamical Time (TDB) based Julian date for which to find the position and velocity\&. Typically this may be the integer part of the Julian date for high-precision calculations, or else the entire Julian date for reduced precision\&. .br @@ -221,6 +253,28 @@ novas_solarsystem_func .RE .PP +.SH "Enumeration Type Documentation" +.PP +.SS "enum \fBnovas_id_type\fP" +Solar-system body IDs to use as \fBobject\&.number\fP with NOVAS_EPHEM_OBJECT types\&. JPL ephemerides use \fCNAIF IDs\fP to identify objects in the Solar-system, which is thus the most widely adopted convention for numbering Solar-system bodies\&. But other numbering systems also exists, for example the CALCEPH library uses its own convention for the numbering of asteroids\&. +.PP +\fBSee also\fP +.RS 4 +\fBobject\fP +.PP +\fBNOVAS_EPHEM_OBJECT\fP +.RE +.PP + +.PP +\fBEnumerator\fP +.in +1c +.TP +\fB\fINOVAS_ID_NAIF \fP\fP +If the ephemeris provider should use NAIF IDs\&. +.TP +\fB\fINOVAS_ID_CALCEPH \fP\fP +If the ephemeris provider should use CALCEPH IDs\&. .SH "Function Documentation" .PP .SS "short earth_sun_calc (double jd_tdb, enum \fBnovas_planet\fP body, enum \fBnovas_origin\fP origin, double * position, double * velocity)" @@ -336,6 +390,10 @@ the currently defined function for accessing ephemeris data for minor planets or .RS 4 \fBset_ephem_provider()\fP .PP +\fBget_planet_provider()\fP +.PP +\fBget_planet_provider_hp()\fP +.PP \fBephemeris()\fP .RE .PP @@ -350,10 +408,163 @@ Attila Kovacs .RE .PP +.SS "\fBnovas_planet_provider\fP get_planet_provider ()" +Returns the custom (low-precision) ephemeris provider function for major planets (and Sun, Moon, SSB), if any\&. +.PP +\fBReturns\fP +.RS 4 +the custom (low-precision) planet ephemeris provider function\&. +.RE +.PP +\fBAuthor\fP +.RS 4 +Attila Kovacs +.RE +.PP +\fBSince\fP +.RS 4 +1\&.2 +.RE +.PP +\fBSee also\fP +.RS 4 +\fBset_planet_provider()\fP +.PP +\fBget_planet_provider_hp()\fP +.PP +\fBget_ephem_provider()\fP +.RE +.PP + +.SS "\fBnovas_planet_provider_hp\fP get_planet_provider_hp ()" +Returns the custom high-precision ephemeris provider function for major planets (and Sun, Moon, SSB), if any\&. +.PP +\fBReturns\fP +.RS 4 +the custom high-precision planet ephemeris provider function\&. +.RE +.PP +\fBAuthor\fP +.RS 4 +Attila Kovacs +.RE +.PP +\fBSince\fP +.RS 4 +1\&.2 +.RE +.PP +\fBSee also\fP +.RS 4 +\fBset_planet_provider_hp()\fP +.PP +\fBget_planet_provider()\fP +.PP +\fBget_ephem_provider()\fP +.RE +.PP + +.SS "enum \fBnovas_planet\fP naif_to_novas_planet (long id)" +Converts a NAIF ID to a NOVAS major planet ID\&. It account for the different IDs used for Sun, Moon and SSB\&. Otherwise NAIF planet barycenters are mapped to the corresponding bodies, except EMB (3), which will return -1\&. NAIF body centers \fIn\fP99 (e\&.g\&. 399 for Earth), are mapped to the corresponding NOVAS planet number \fIn\fP\&. All other NAIF IDs will return -1, indicating no match to a NOVAS planet ID\&. +.PP +\fBParameters\fP +.RS 4 +\fIid\fP The NAIF ID of the major planet of interest +.RE +.PP +\fBReturns\fP +.RS 4 +the NOVAS ID for the same object (which may or may not be different from the input), or -1 if the NAIF ID cannot be matched to a NOVAS major planet\&. +.RE +.PP +\fBSee also\fP +.RS 4 +\fBnovas_to_naif_planet()\fP +.PP +\fBnovas_to_dexxx_planet()\fP +.RE +.PP +\fBAuthor\fP +.RS 4 +Attila Kovacs +.RE +.PP +\fBSince\fP +.RS 4 +1\&.2 +.RE +.PP + +.PP +References \fBNAIF_EMB\fP, \fBNAIF_MOON\fP, \fBNAIF_SSB\fP, \fBNAIF_SUN\fP, \fBNOVAS_MERCURY\fP, \fBNOVAS_MOON\fP, \fBNOVAS_PLUTO\fP, \fBNOVAS_SSB\fP, and \fBNOVAS_SUN\fP\&. +.SS "long novas_to_dexxx_planet (enum \fBnovas_planet\fP id)" +Converts a NOVAS Solar-system body ID to a NAIF Solar-system body ID for DExxx ephemeris files\&. The DExxx (e\&.g\&. DE440) ephemeris files use NAIF IDs, but for most planets contain barycentric data only rather than that of the planet center\&. For Earth-based observations, it only really makes a difference whether the 3 is used for the Earth-Moon Barycenter (EMB) or 399 for the geocenter\&. +.PP +\fBParameters\fP +.RS 4 +\fIid\fP The NOVAS ID of the major planet of interest +.RE +.PP +\fBReturns\fP +.RS 4 +the NAIF ID for the same object (which may or may not be different from the input), as appropriate for use in the DExxx ephemeris files\&. +.RE +.PP +\fBSee also\fP +.RS 4 +\fBnovas_to_naif_planet()\fP +.PP +\fBnaif_to_novas_planet()\fP +.RE +.PP +\fBAuthor\fP +.RS 4 +Attila Kovacs +.RE +.PP +\fBSince\fP +.RS 4 +1\&.2 +.RE +.PP + +.PP +References \fBNAIF_EARTH\fP, \fBNAIF_MOON\fP, \fBNAIF_SSB\fP, \fBNAIF_SUN\fP, \fBNOVAS_EARTH\fP, \fBNOVAS_MERCURY\fP, \fBNOVAS_MOON\fP, \fBNOVAS_PLUTO\fP, \fBNOVAS_SSB\fP, and \fBNOVAS_SUN\fP\&. +.SS "long novas_to_naif_planet (enum \fBnovas_planet\fP id)" +Converts a NOVAS Solar-system body ID to a NAIF Solar-system body ID\&. NOVAS and NAIF use slightly different IDs for major planets, the Moon, and the Solar-system Barycenter (SSB)\&. In NOVAS, major planets are have IDs ranging from 1 through 9, but for NAIF 1--9 are the planetary barycenters and the planet centers have numbers in the hundreds ending with 99 (e\&.g\&. the center of Earth is NAIF 399; 3 is the NOVAS ID for Earth and the NAIF ID for the Earth-Moon Barycenter [EMB])\&. The Sun and Moon also have distinct IDs in NAIF vs NOVAS\&. +.PP +\fBParameters\fP +.RS 4 +\fIid\fP The NOVAS ID of the major planet of interest +.RE +.PP +\fBReturns\fP +.RS 4 +the NAIF ID for the same object or planet center (which may or may not be different from the input) +.RE +.PP +\fBSee also\fP +.RS 4 +\fBnaif_to_novas_planet()\fP +.RE +.PP +\fBAuthor\fP +.RS 4 +Attila Kovacs +.RE +.PP +\fBSince\fP +.RS 4 +1\&.2 +.RE +.PP + +.PP +References \fBNAIF_MOON\fP, \fBNAIF_SSB\fP, \fBNAIF_SUN\fP, \fBNOVAS_MERCURY\fP, \fBNOVAS_MOON\fP, \fBNOVAS_PLUTO\fP, \fBNOVAS_SSB\fP, and \fBNOVAS_SUN\fP\&. .SS "short planet_eph_manager (double jd_tdb, enum \fBnovas_planet\fP body, enum \fBnovas_origin\fP origin, double * position, double * velocity)" Provides an interface between the JPL direct-access solar system ephemerides and NOVAS-C for regular (reduced) precision applications\&. .PP -This function and \fBplanet_ephemeris()\fP were designed to work with the 1997 version of the JPL ephemerides, as noted in the references\&. +This function and \fBplanet_eph_manager_hp()\fP were designed to work with the 1997 version of the JPL ephemerides, as noted in the references\&. .PP The user must create the binary ephemeris files using software from JPL, and open the file using function \fBephem_open()\fP, prior to calling this function\&. .PP @@ -408,7 +619,7 @@ References \fBplanet_eph_manager_hp()\fP\&. .SS "short planet_eph_manager_hp (const double jd_tdb[2], enum \fBnovas_planet\fP body, enum \fBnovas_origin\fP origin, double * position, double * velocity)" Provides an interface between the JPL direct-access solar system ephemerides and NOVAS-C for highest precision applications\&. .PP -This function and \fBplanet_ephemeris()\fP were designed to work with the 1997 version of the JPL ephemerides, as noted in the references\&. +This function and \fBplanet_eph_manager()\fP were designed to work with the 1997 version of the JPL ephemerides, as noted in the references\&. .PP The user must create the binary ephemeris files using software from JPL, and open the file using function \fBephem_open()\fP, prior to calling this function\&. .PP @@ -724,6 +935,10 @@ Attila Kovacs .RS 4 \fBget_ephem_provider()\fP .PP +\fBset_planet_provider()\fP +.PP +\fBset_planet_provider_hp()\fP +.PP \fBephemeris()\fP .RE .PP @@ -748,6 +963,8 @@ Attila Kovacs .PP \fBSee also\fP .RS 4 +\fBget_planet_provider()\fP +.PP \fBset_planet_provider_hp()\fP .PP \fBsolarsystem()\fP @@ -776,6 +993,8 @@ Attila Kovacs .PP \fBSee also\fP .RS 4 +\fBget_planet_provider_hp()\fP +.PP \fBset_planet_provider()\fP .PP \fBsolarsystem_hp()\fP diff --git a/apidoc/man/man3/solsys-calceph.c.3 b/apidoc/man/man3/solsys-calceph.c.3 new file mode 100644 index 00000000..a13febf5 --- /dev/null +++ b/apidoc/man/man3/solsys-calceph.c.3 @@ -0,0 +1,135 @@ +.TH "src/solsys-calceph.c" 3 "Version v1.2" "SuperNOVAS" \" -*- nroff -*- +.ad l +.nh +.SH NAME +src/solsys-calceph.c +.SH SYNOPSIS +.br +.PP +.SS "Functions" + +.in +1c +.ti -1c +.RI "int \fBnovas_calceph_use_ids\fP (enum \fBnovas_id_type\fP idtype)" +.br +.ti -1c +.RI "int \fBnovas_use_calceph\fP (t_calcephbin *eph)" +.br +.ti -1c +.RI "int \fBnovas_use_calceph_planets\fP (t_calcephbin *eph)" +.br +.in -1c +.SH "Detailed Description" +.PP + +.PP +\fBAuthor\fP +.RS 4 +A\&. Kovacs +.RE +.PP +SuperNOVAS major planet ephemeris lookup implementation via the CALCEPH C library See https://calceph.imcce.fr/docs/4.0.0/html/c/ +.PP +CALCEPH source code is at https://gitlab.obspm.fr/imcce_calceph/calceph +.SH "Function Documentation" +.PP +.SS "int novas_calceph_use_ids (enum \fBnovas_id_type\fP idtype)" +Sets the type of Solar-system body IDs to use as \fBobject\&.number\fP with NOVAS_EPHEM_OBJECT types\&. CALCEPH supports the use of both NAIF and its own numbering system to identify Solar-system bodies\&. So, this function gives you the choice on which numbering system you want to use in object data structures\&. The choice does not affect major planets (which always use the NOVAS numbering scheme), or catalog objects\&. +.PP +\fBParameters\fP +.RS 4 +\fIidtype\fP NOVAS_ID_NAIF to use NAIF IDs (default) or else NOVAS_ID_CALCEPH to use the CALCEPH body numbering convention for object\&. +.RE +.PP +\fBReturns\fP +.RS 4 +0 if successful or else -1 (errno set to EINVAL) if the input value is invalid\&. +.RE +.PP +\fBSee also\fP +.RS 4 +\fBobject\fP +.PP +\fBNOVAS_EPHEM_OBJECT\fP +.RE +.PP + +.PP +References \fBNOVAS_ID_CALCEPH\fP, and \fBNOVAS_ID_NAIF\fP\&. +.SS "int novas_use_calceph (t_calcephbin * eph)" +Sets a ephemeris provider for Solar-system objects using the CALCEPH C library and the specified set of ephemeris files\&. If the supplied ephemeris files contain data for major planets also, they can be used by planet_calceph() / planet_calceph_hp() also, unless a separate CALCEPH ephemeris data is set via \fBnovas_use_calceph_planets()\fP\&. +.PP +The call also make CALCEPH the default ephemeris provider for all types of Solar-system objects\&. If you want to use another provider for major planets, you need to call \fBset_planet_provider()\fP / \fBset_planet_provider_hp()\fP afterwards to specify a different provider for major planets (and Sun, Moon, SSB)\&. +.PP +\fBParameters\fP +.RS 4 +\fIeph\fP Pointer to the CALCEPH ephemeris data that have been opened\&. +.RE +.PP +\fBReturns\fP +.RS 4 +0 if successful, or else -1 (errno will indicate the type of error)\&. +.RE +.PP +\fBSee also\fP +.RS 4 +\fBnovas_calceph_use_ids()\fP +.PP +\fBnovas_use_calceph_planets()\fP +.PP +\fBset_ephem_provider()\fP +.RE +.PP +\fBAuthor\fP +.RS 4 +Attila Kovacs +.RE +.PP +\fBSince\fP +.RS 4 +1\&.2 +.RE +.PP + +.PP +References \fBnovas_use_calceph_planets()\fP, and \fBset_ephem_provider()\fP\&. +.SS "int novas_use_calceph_planets (t_calcephbin * eph)" +Sets a ephemeris provider for the major planets (and Sun, Moon, and SSB) using the CALCEPH C library and the specified ephemeris data\&. +.PP +The call also make CALCEPH the default ephemeris providers for major planets\&. +.PP +\fBParameters\fP +.RS 4 +\fIeph\fP Pointer to the CALCEPH ephemeris data for the major planets (including Sun, Moon, and SSB) that have been opened\&. +.RE +.PP +\fBReturns\fP +.RS 4 +0 if successful, or else -1 (errno will indicate the type of error)\&. +.RE +.PP +\fBSee also\fP +.RS 4 +\fBnovas_use_calceph()\fP +.PP +\fBset_planet_provider()\fP +.PP +\fBset_planet_provider_hp()\fP +.RE +.PP +\fBAuthor\fP +.RS 4 +Attila Kovacs +.RE +.PP +\fBSince\fP +.RS 4 +1\&.2 +.RE +.PP + +.PP +References \fBset_planet_provider()\fP, and \fBset_planet_provider_hp()\fP\&. +.SH "Author" +.PP +Generated automatically by Doxygen for SuperNOVAS from the source code\&. diff --git a/apidoc/man/man3/solsys1.c.3 b/apidoc/man/man3/solsys1.c.3 index 5780f1f9..a94bf62c 100644 --- a/apidoc/man/man3/solsys1.c.3 +++ b/apidoc/man/man3/solsys1.c.3 @@ -56,7 +56,7 @@ U\&. S\&. Naval Observatory .SS "short planet_eph_manager (double jd_tdb, enum \fBnovas_planet\fP body, enum \fBnovas_origin\fP origin, double * position, double * velocity)" Provides an interface between the JPL direct-access solar system ephemerides and NOVAS-C for regular (reduced) precision applications\&. .PP -This function and \fBplanet_ephemeris()\fP were designed to work with the 1997 version of the JPL ephemerides, as noted in the references\&. +This function and \fBplanet_eph_manager_hp()\fP were designed to work with the 1997 version of the JPL ephemerides, as noted in the references\&. .PP The user must create the binary ephemeris files using software from JPL, and open the file using function \fBephem_open()\fP, prior to calling this function\&. .PP @@ -111,7 +111,7 @@ References \fBplanet_eph_manager_hp()\fP\&. .SS "short planet_eph_manager_hp (const double jd_tdb[2], enum \fBnovas_planet\fP body, enum \fBnovas_origin\fP origin, double * position, double * velocity)" Provides an interface between the JPL direct-access solar system ephemerides and NOVAS-C for highest precision applications\&. .PP -This function and \fBplanet_ephemeris()\fP were designed to work with the 1997 version of the JPL ephemerides, as noted in the references\&. +This function and \fBplanet_eph_manager()\fP were designed to work with the 1997 version of the JPL ephemerides, as noted in the references\&. .PP The user must create the binary ephemeris files using software from JPL, and open the file using function \fBephem_open()\fP, prior to calling this function\&. .PP diff --git a/apidoc/man/man3/super.c.3 b/apidoc/man/man3/super.c.3 index 18a775e2..50f5d5c3 100644 --- a/apidoc/man/man3/super.c.3 +++ b/apidoc/man/man3/super.c.3 @@ -948,9 +948,9 @@ Sets a celestial object to be a Solar-system ephemeris body\&. Typically this wo .PP \fBParameters\fP .RS 4 -\fIname\fP Name of object\&. By default converted to upper-case, unless \fBnovas_case_sensitive()\fP was called with a non-zero argument\&. Max\&. SIZE_OF_OBJ_NAME long, including termination\&. +\fIname\fP Name of object\&. By default converted to upper-case, unless \fBnovas_case_sensitive()\fP was called with a non-zero argument\&. Max\&. SIZE_OF_OBJ_NAME long, including termination\&. If the ephemeris provider uses names, then the name should match those of the ephemeris provider -- otherwise it is not important\&. .br -\fInum\fP Solar-system body ID number (e\&.g\&. NAIF) +\fInum\fP Solar-system body ID number (e\&.g\&. NAIF)\&. The number should match the needs of the ephemeris provider used with NOVAS\&. (If the ephemeris provider is by name and not ID number, then the number here is not important)\&. .br \fIbody\fP Pointer to structure to populate\&. .RE @@ -962,6 +962,8 @@ Sets a celestial object to be a Solar-system ephemeris body\&. Typically this wo .PP \fBSee also\fP .RS 4 +\fBset_ephem_provider()\fP +.PP \fBmake_planet()\fP .PP \fBmake_cat_entry()\fP diff --git a/apidoc/supernovas.tag b/apidoc/supernovas.tag index dbe3f05f..0d679bf0 100644 --- a/apidoc/supernovas.tag +++ b/apidoc/supernovas.tag @@ -1,5 +1,45 @@ + + naif.h + include/ + naif_8h.html + + #define + NAIF_EARTH + naif_8h.html + a58a3ee779a2235702283b32a762df2f6 + + + + #define + NAIF_EMB + naif_8h.html + a71a4a929a85a2b77c2adb2284894ca9d + + + + #define + NAIF_MOON + naif_8h.html + a172c6c114d2f18ae91003a1f293682bc + + + + #define + NAIF_SSB + naif_8h.html + a4a8e127d97f48f2ef918b61182436490 + + + + #define + NAIF_SUN + naif_8h.html + a4a4d693821f595d86497eb2befc746c1 + + + novas.h include/ @@ -2203,6 +2243,13 @@ include/ solarsystem_8h.html novas.h + + #define + NOVAS_ID_TYPES + solarsystem_8h.html + a9a736e59fc9bfdc92b7245aa37d529ee + + int(* novas_ephem_provider @@ -2224,6 +2271,25 @@ a85ed597fa94ecf72653e64f4afa7f833 )(const double jd_tdb[2], enum novas_planet body, enum novas_origin origin, double *position, double *velocity) + + + novas_id_type + solarsystem_8h.html + ac42df1db80fbcb6f7a72de80d9f9c531 + + + + NOVAS_ID_NAIF + solarsystem_8h.html + ac42df1db80fbcb6f7a72de80d9f9c531ab3e6efc1ad89e02f915df25265ec32db + + + + NOVAS_ID_CALCEPH + solarsystem_8h.html + ac42df1db80fbcb6f7a72de80d9f9c531a074c723dfc1f03c82d52347c46ee0719 + + short earth_sun_calc @@ -2252,6 +2318,41 @@ aa6fad38297a49ba78a6bd49cedf889b1 () + + novas_planet_provider + get_planet_provider + solarsystem_8h.html + a0f0a786b5614a788c02b37a462eae2d2 + () + + + novas_planet_provider_hp + get_planet_provider_hp + solarsystem_8h.html + ae45badb450c1ca73920d982e12346c5b + () + + + enum novas_planet + naif_to_novas_planet + solarsystem_8h.html + a1c4b3f67a3b82808dd16ae43dfaf0f86 + (long id) + + + long + novas_to_dexxx_planet + solarsystem_8h.html + ac3eb54acf22dc155879163de89c6865e + (enum novas_planet id) + + + long + novas_to_naif_planet + solarsystem_8h.html + ab51ac9bdf7736e1c1582e0981046daf3 + (enum novas_planet id) + short planet_eph_manager @@ -2601,6 +2702,41 @@ (const double *in, const novas_transform *transform, double *out) + + naif.c + src/ + naif_8c.html + novas.h + naif.h + + #define + __NOVAS_INTERNAL_API__ + naif_8c.html + af46d8e51fc53d94b0d48c8201c3c84a6 + + + + enum novas_planet + naif_to_novas_planet + naif_8c.html + a1c4b3f67a3b82808dd16ae43dfaf0f86 + (long id) + + + long + novas_to_dexxx_planet + naif_8c.html + ac3eb54acf22dc155879163de89c6865e + (enum novas_planet id) + + + long + novas_to_naif_planet + naif_8c.html + ab51ac9bdf7736e1c1582e0981046daf3 + (enum novas_planet id) + + novas.c src/ @@ -2829,6 +2965,20 @@ aa6fad38297a49ba78a6bd49cedf889b1 () + + novas_planet_provider + get_planet_provider + novas_8c.html + a0f0a786b5614a788c02b37a462eae2d2 + () + + + novas_planet_provider_hp + get_planet_provider_hp + novas_8c.html + ae45badb450c1ca73920d982e12346c5b + () + short grav_def @@ -3465,6 +3615,32 @@ (double jd_tt, const on_surface *loc, enum novas_refraction_type type, double el) + + solsys-calceph.c + src/ + solsys-calceph_8c.html + + int + novas_calceph_use_ids + solsys-calceph_8c.html + a5531b937a5bb5491cb475d2536346ad8 + (enum novas_id_type idtype) + + + int + novas_use_calceph + solsys-calceph_8c.html + a35fc86a939602ec910dbdfde180d7f31 + (t_calcephbin *eph) + + + int + novas_use_calceph_planets + solsys-calceph_8c.html + ab86ec03898e658c86c671a8b6399e331 + (t_calcephbin *eph) + + solsys-ephem.c src/ @@ -4569,6 +4745,7 @@ api-changes solarsystem universal-ephemerides + calceph-integration builtin-ephem-readers explicit-ephem-linking debug-support diff --git a/doc/CHANGELOG.md b/doc/CHANGELOG.md index 28195ce3..0110bc80 100644 --- a/doc/CHANGELOG.md +++ b/doc/CHANGELOG.md @@ -6,6 +6,7 @@ file. The format is based on [Keep a Changelog](https://keepachangelog.com/en/1.1.0/), and this project adheres to [Semantic Versioning](https://semver.org/spec/v2.0.0.html). + ## [Unreleased] Changes expected for the next bug-fix release, expected around 1 December 2024. @@ -22,7 +23,24 @@ Changes expected for the next bug-fix release, expected around 1 December 2024. gravitating bodies (other than the Sun and Earth). The added functions are `grav_redshift()`, `redhift_vrad()`, `unredshift_vrad()`, `novas_z_add()`, and `novas_z_inv()`. + - #83: CALCEPH integration: `novas_use_calceph()` and/or `novas_use_calceph_planets()` to specify and use ephemeris + data via CALCEPH for Solar-system sources in general, and for major planets specifically; and + `novas_calceph_use_ids()` to specify whether `object.number` in `NOVAS_EPHEM_OBJECT` type objects is a NAIF ID + (default) or else a CALCEPH ID number of the Solar-system body. These functions are provided by the + `libsolsys-calceph.so[.1]` and/or `.a` plugin libraries, which are built contingent on the `CALCEPH_SUPPORT` + variable being set to 1 prior to the build. The build of the plugin module requires an accessible installation of + the CALCEPH development files (C headers and unversioned static or shared libraries depending on the needs of the + build). + + - NOVAS-NAIF conversions for major planets (and Sun, Moon, SSB): `novas_to_naif_planet()` (planet centers), + `novas_to_dexxx_planet()` (mixed planet center/barycenter for DExxx ephemeris files), and the inverse + `naif_to_novas_planet()`. + - Added `get_planet_provider()` and `get_planet_provider_hp()` functions for convenience to return the `solarsystem()` + / `solarsystem_hp()` type custom planet ephemeris provider functions currently configured, so they may be used + directly, outside of `ephemeris()` calls. + + ## [1.1.1] - 2024-10-28 Bug fix release. Nothing too scary, mainly just a collection of smaller fixes and improvements. diff --git a/doc/README.md b/doc/README.md index 505b88a3..41dfc609 100644 --- a/doc/README.md +++ b/doc/README.md @@ -68,7 +68,7 @@ Outside contributions are very welcome. See - [NOVAS](https://aa.usno.navy.mil/software/novas_info) home page at the US Naval Observatory. - [CALCEPH C library](https://calceph.imcce.fr/docs/4.0.0/html/c/index.html) for integrating Solar-system ephemeris from JPL and/or in INPOP 2.0/3.0 format. - - [SPICE toolkit](https://naif.jpl.nasa.gov/naif/toolkit.html) for integrating Solar-system ephemeris + - [NAIF SPICE toolkit](https://naif.jpl.nasa.gov/naif/toolkit.html) for integrating Solar-system ephemeris via from JPL. - [IAU Minor Planet Center](https://www.minorplanetcenter.net/iau/mpc.html) provides another source of ephemeris data. @@ -165,9 +165,10 @@ Before compiling the library take a look a `config.mk` and edit it as necessary the necessary variables in the shell prior to invoking `make`. For example: - Choose which planet calculator function routines are built into the library (for example to provide - `earth_sun_calc()` set `BUILTIN_SOLSYS3 = 1` and/or for `planet_ephem_provider()` set `BUILTIN_SOLSYS_EPHEM = 1`. - You can then specify these functions as the default planet calculator for `ephemeris()` in your application - dynamically via `set_planet_provider()`. + `earth_sun_calc()` set `BUILTIN_SOLSYS3 = 1` and/or for `planet_ephem_provider()` set `BUILTIN_SOLSYS_EPHEM = 1`, + and or for `planet_calceph()` / `novas_calceph()` set `BUILTIN_SOLSYS_CALCEPH = 1`. You can then specify these + functions as the default planet calculator for `ephemeris()` in your application dynamically via + `set_planet_provider()`. - Choose which stock planetary calculator module (if any) should provide a default `solarsystem()` implementation for `ephemeris()` calls by setting `DEFAULT_SOLSYS` to 1 -- 3 for `solsys1.c` trough `solsys3.c`, respectively. If you @@ -179,6 +180,13 @@ the necessary variables in the shell prior to invoking `make`. For example: one tries to use the functions from `solsys1.c`). Note, that a `readeph()` implementation is not always necessary and you can provide a superior ephemeris reader implementation at runtime via the `set_ephem_provider()` call. + - You can enable integration with the [CALCEPH](https://www.imcce.fr/recherche/equipes/asd/calceph/) C library, by + setting `CALCEPH_SUPPORT = 1` in `config.mk` or in the shell prior to the build. When enabled it will build + `libsolsys-calceph.so[.1]` and/or `.a` supplemental libraries, depending on the build target. The build of the + modules requires an accessible installation of the CALCEPH development files (C headers and unversioned static or + shared libraries depending on the needs of the build). You might want to set `LD_LIBRARY_PATH`, and/or `CPPFLAGS` + to include an appropriate `-I` option, to help locate these prior to calling `make`. + - If you want to use the CIO locator binary file for `cio_location()`, you can specify the path to the CIO locator file (e.g. `/usr/local/share/supernovas/CIO_RA.TXT`) on your system e.g. by setting the `CIO_LOCATOR_FILE` shell variable prior to calling `make`. (The CIO locator file is not at all necessary for the functioning of the library, @@ -784,7 +792,15 @@ before that level of accuracy is reached. gravitating bodies (other than the Sun and Earth). The added functions are `grav_redshift()`, `redhift_vrad()`, `unredshift_vrad()`, `novas_z_add()`, and `novas_z_inv()`. - + - CALCEPH integration: `novas_use_calceph()` and/or `novas_use_calceph_planets()` to specify and use ephemeris data + via CALCEPH for Solar-system sources in general, and for major planets specifically; and `novas_calceph_use_ids()` + to specify whether `object.number` in `NOVAS_EPHEM_OBJECT` type objects is a NAIF ID (default) or else a CALCEPH ID + number of the Solar-system body. + + - NAIF/NOVAS ID conversions for major planets (and Sun, Moon, SSB): `novas_to_naif_planet()`, + `novas_to_dexxx_planet()`, and `naif_to_novas_planet()`. + + - Access to custom ephemeris provider functions: `get_planet_provider()` and `get_planet_provider_hp()`. @@ -867,15 +883,18 @@ before that level of accuracy is reached. ## External Solar-system ephemeris data or services - If you want to use SuperNOVAS to calculate positions for a range of Solar-system objects, and/or to do it with sufficient precision, you will have to integrate it with a suitable provider of ephemeris data, such as [JPL Horizons](https://ssd.jpl.nasa.gov/horizons/app.html#/) or the [Minor Planet Center](https://www.minorplanetcenter.net/iau/mpc.html). Given the NOVAS C heritage, and some added SuperNOVAS flexibility in this area, you have several options on doing that. These are listed from the most flexible -(and preferred) to the least flexible (old ways). +(and preferred) to the least flexible (old ways). + +NASA/JPL also provides [generic ephemerides](https://naif.jpl.nasa.gov/pub/naif/generic_kernels/spk/) for the major +planets, satellites thereof, the 300 largest asteroids, the Lagrange points, and some Earth orbiting stations. - [Universal ephemeris data / service integration](#universal-ephemerides) + - [Built-in support for CALCEPH integration](#calceph-integration) - [Built-in support for (old) JPL major planet ephemerides](#builtin-ephem-readers) - [Explicit linking of custom ephemeris functions](#explicit-ephem-linking) @@ -902,8 +921,7 @@ heliocenter, and accordingly, your function should set the value pointed at by o `NOVAS_HELIOCENTER` accordingly. Positions and velocities are rectangular ICRS _x,y,z_ vectors in units of AU and AU/day respectively. -This way you can easily integrate current ephemeris data for JPL Horizons, e.g. using -[CALCEPH](https://calceph.imcce.fr/docs/4.0.0/html/c/index.html) or the +This way you can easily integrate current ephemeris data for JPL Horizons, e.g. using the [CSPICE toolkit](https://naif.jpl.nasa.gov/naif/toolkit.html), or for the Minor Planet Center (MPC), or whatever other ephemeris service you prefer. @@ -926,6 +944,54 @@ provided you compiled SuperNOVAS with `BUILTIN_SOLSYS_EPHEM = 1` (in `config.mk` `solsys-ephem.c` explicitly. Easy-peasy. + +### Built-in support for CALCEPH integration + +The [CALCEPH](https://www.imcce.fr/recherche/equipes/asd/calceph/) library provides an easy-to-use access to JPL and +INPOP ephemeris files from C/C++. As of version 1.2, we provide built-in support for integrating the CALCEPH C library +with SuperNOVAS for handling Solar-system objects. + +Prior to building SuperNOVAS simply set `CALCEPH_SUPPORT` to 1 in `config.mk` or in your shell. Depending on the +build target, it will build `libsolsys-calceph.so[.1]` (target `shared`) or `libsolsys-calceph.a` (target `static`) +libraries, which provide the `novas_use_calceph()` and `novas_use_calceph_planets()` functions. + +Of course, you will need access to the CALCEPH C development files (C headers and unversioned libraries) for the build +to succeed. Here is an example on how you'd use CALCEPH with SuperNOVAS in your application code: + +```c + #include + + // You can open a set of JPL/INPOP ephemeris files with CALCEPH... + t_calcephbin *eph = calceph_open_array(...); + + // Then use them as your generic SuperNOVAS ephemeris provider + int status = novas_use_calceph(eph); + if(status < 0) { + // Ooops something went wrong... + } + + // ----------------------------------------------------------------------- + // Optionally you may use a separate ephemeris data for major planets + // (or if planet ephemeris was included in 'eph' above, you don't have to) + t_calcephbin *pleph = calceph_open(...); + int status = novas_use_calceph(pleph); + if(status < 0) { + // Ooops something went wrong... + } +``` + +You can obtain readily available standard ephemeris files from +[NASA/JPL](https://naif.jpl.nasa.gov/pub/naif/generic_kernels/spk/), such as +[DE440](https://naif.jpl.nasa.gov/pub/naif/generic_kernels/spk/planets/de440.bsp), which covers the major planets, plus +Sun, Moon, and Solar-System Barycenter (SSB) for times between 1550 AD and 2650 AD. Or, you can use the +[JPL HORIZONS](https://ssd.jpl.nasa.gov/horizons/app.html#/) system to generate cutom ephemeris data for pretty much +all known solar systems bodies, down to the tiniest rocks. All of these should work with the `solsys-calceph` plugin. + +And, when linking your application, don't forget to add `-lsolsys-calceph` to your link flags. That's all there is to +it. + + + ### Built-in support for (old) JPL major planet ephemerides