Added some doxygen comments.
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@@ -1,6 +1,7 @@
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// ephemeris.hxx -- Top level class for calculating current positions of
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// astronomical objects
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//
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/** \file ephemeris.hxx
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* Top level class for calculating current positions of astronomical objects.
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*/
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// Top level interface written by Curtis Olson, started March 2000.
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//
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// All the core code underneath this is written by Durk Talsma. See
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@@ -48,6 +49,25 @@
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#include <simgear/ephemeris/stardata.hxx>
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/** Ephemeris class
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*
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* Introduction
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*
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* The SGEphemeris class computes and stores the positions of the Sun,
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* the Moon, the planets, and the brightest stars. These positions
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* can then be used to accurately render the dominant visible items in
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* the Earth's sky. Note, this class isn't intended for use in an
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* interplanetary/interstellar/intergalactic type application. It is
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* calculates everything relative to the Earth and is therefore best
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* suited for Earth centric applications.
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*
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* The positions of the various astronomical objects are time
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* dependent, so to maintain accuracy, you will need to periodically
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* call the update() method. The SGTime class conveniently provides
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* the two time related values you need to pass to the update()
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* method.
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*/
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class SGEphemeris {
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Star *our_sun;
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@@ -71,40 +91,82 @@ class SGEphemeris {
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public:
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// Constructor
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/**
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* Constructor.
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* This creates an instance of the SGEphemeris object. When
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* calling the constructor you need to provide a path pointing to
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* your star database file.
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* @param path path to your star database */
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SGEphemeris( const string &path );
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// Destructor
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/** Destructor */
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~SGEphemeris( void );
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// Update (recalculate) the positions of all objects for the
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// specified time
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/**
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* Update (recalculate) the positions of all objects for the
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* specified time. The update() method requires you to pass in
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* the current modified Julian date, the current local sidereal
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* time, and the current latitude. The update() method is designed
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* to be called by the host application before every frame.
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* @param mjd modified julian date
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* @param lst current local sidereal time
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* @param lat current latitude
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*/
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void update(double mjd, double lst, double lat);
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// sun
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/**
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* Returns a pointer to a Star class containing all the positional
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* information for Earth's Sun.
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*/
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inline Star *get_sun() const { return our_sun; }
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/** Returns the right ascension of the Sun. */
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inline double getSunRightAscension() const {
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return our_sun->getRightAscension();
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}
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/** Returns the declination of the Sun. */
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inline double getSunDeclination() const {
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return our_sun->getDeclination();
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}
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// moon
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/**
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* Returns a pointer to a Moon class containing all the positional
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* information for Earth's Moon.
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*/
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inline MoonPos *get_moon() const { return moon; }
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/** Returns the right ascension of the Moon. */
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inline double getMoonRightAscension() const {
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return moon->getRightAscension();
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}
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/** Returns the declination of the Moon. */
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inline double getMoonDeclination() const {
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return moon->getDeclination();
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}
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// planets
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/** Returns the numbers of defined planets. */
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inline int getNumPlanets() const { return nplanets; }
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/**
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* Returns a pointer to an array of planet data in sgdVec3
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* format. (See plib.sourceforge.net for information on plib and
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* the ``sg'' package.) An sgdVec3 is a 3 element double
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* array. The first element is the right ascension of the planet,
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* the second is the declination, and the third is the magnitude.
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*/
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inline sgdVec3 *getPlanets() { return planets; }
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// planets
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/** Returns the numbers of defined stars. */
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inline int getNumStars() const { return stars->getNumStars(); }
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/**
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* Returns a pointer to an array of star data in sgdVec3
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* format. An The first element of the sgdVec3 is the right
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* ascension of the planet, the second is the declination, and the
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* third is the magnitude.
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*/
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inline sgdVec3 *getStars() { return stars->getStars(); }
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};
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