v1.2.0-rc2 #99
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-
Added
Redshifted motion handling #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.Redshifted motion handling #57: New generic redshift-handling functions
novas_v2z()
,novas_z2v()
,Redshift utilities #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()
, andnovas_z_inv()
.Add support for CALCEPH #83: CALCEPH integration:
novas_use_calceph()
and/ornovas_use_calceph_planets()
to specify and use ephemeris data via CALCEPH for Solar-system sources in general, and for major planets specifically; andnovas_calceph_use_ids()
to specify whetherobject.number
inNOVAS_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 thelibsolsys-calceph.so[.1]
and/or.a
plugin libraries, which are built contingent on theCALCEPH_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).Add support for NAIF CSPICE #86: NAIF CSPICE integration:
novas_use_cspice()
,novas_use_cspice_planets()
,novas_use_cspice_ephem()
to use the NAIF CSPICE library for all Solar-system sources, major planets only, or for other bodies only.NOVAS_EPHEM_OBJECTS
should use NAIF IDs with CSPICE (or else -1 for name-based lookup). Also providescspice_add_kernel()
andcspice_remove_kernel()
functions for convenience to manage the set of active kernels (Further CSPICE support, improved error handling #89). These functions are provided by thelibsolsys-cspice.so[.1]
and/or.a
plugin libraries, which are built contingent on theCSPICE_SUPPORT
variable being set to 1 prior to the build. The build of the plugin module requires an accessible installation of the CSPICE development files (C headers and unversioned static or shared libraries depending on the needs of the build).Add novas_planet_for_name() #87: Added
novas_planet_for_name()
function to return the NOVAS planet ID for a given (case insensitive) name.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 inversenaif_to_novas_planet()
.Added
get_planet_provider()
andget_planet_provider_hp()
functions for convenience to return thesolarsystem()
/solarsystem_hp()
type custom planet ephemeris provider functions currently configured, so they may be used directly, outside ofephemeris()
calls.Add make install target #93: Now supporting
make install
with prefix support (e.g.make prefix=/opt install
to install under/opt
). You can also set other standard directory variables, as prescribed in the GNU standard to further customize the install locations.Add orbital elements processing #95, Orbitals continued #98: Added support for using orbital elements.
object.type
can now be set toNOVAS_ORBITAL_OBJECT
, whose orbit can be defined by the set ofnovas_orbital_elements
, relative to anovas_orbital_system
. You can initialize anobject
with a set of orbital elements usingmake_orbital_object()
, and for planetary satellite orbits you might usenovas_set_orbsys_pole()
. For orbital objects,ephemeris()
will call on the newnovas_orbit_posvel()
to calculate positions. While orbital elements do not always yield precise positions, they can for shorter periods, provided that the orbital elements are up-to-date. For example, the Minor Planer Center (MPC) publishes accurate orbital elements for all known asteroids and comets regularly. For newly discovered objects, this may be the only and/or most accurate information available anywhere.EMB and Pluto Barycenter #97: Added
NOVAS_EMB
(Earth-Moon Barycenter) andNOVAS_PLUTO_BARYCENTER
toenum novas_planets
to distinguish from the planet center in calculations.Orbitals continued #98: Added
gcrs_to_tod()
/tod_to_gcrs()
andgcrs_to_mod()
/mod_to_gcrs()
vector conversion functions for convenience.SuperNOVAS headers now include each other as system-headers, not local headers. This is unlikely to affect anything really but it is more proper for an installation of the library, and works with our own
Makefile
too.Changed
Orbital elements based calculations #96: Changed
object
structure to includenovas_orbital_elements
forNOVAS_ORBITAL_OBJECT
types.EMB and Pluto Barycenter #97: Updated
NOVAS_PLANETS
,NOVAS_PLANET_NAMES_INIT
, andNOVAS_RMASS_INIT
macros to include the added planet constants.This discussion was created from the release v1.2.0-rc2.
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