/* This file is part of libkholidays. Copyright (c) 2004 Allen Winter This library is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 2 of the License, or (at your option) any later version. This library is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, write to the Free Software Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301 USA In addition, as a special exception, the copyright holders give permission to link the code of this program with any edition of the TQt library by Trolltech AS, Norway (or with modified versions of TQt that use the same license as TQt), and distribute linked combinations including the two. You must obey the GNU General Public License in all respects for all of the code used other than TQt. If you modify this file, you may extend this exception to your version of the file, but you are not obligated to do so. If you do not wish to do so, delete this exception statement from your version. */ #ifndef KHOLIDAYS_LUNARPHASE_H #define KHOLIDAYS_LUNARPHASE_H /** Represents and manages a Lunar Phase A Lunar Phase can be one of the following: + "new": the moon is not visible; or traditionally: first visible crescent of the Moon. For religious purposes, the new month begins when the first crescent moon can be seen. Thus, it is impossible to be certain in advance of when months will begin; in particular, the exact date on which Ramadan will begin is not known in advance. In Saudi Arabia, observers are sent up in airplanes if the weather is cloudy when the new moon is expected. + "first quarter": the right 50% of the moon is visible. + "full": the moon is fully visible. + "last quarter": the left 50% of the moon is visible. A very good description of the lunar phases can be read at the Wikipedia, http://en.wikipedia.org/wiki/Lunar_phase In the southern hemisphere the order of the phases is reversed. So, to be accurate we need to know the hemisphere. Note that crescent and gibbous phases are not currently supported. */ #include #include #include class LunarPhase { public: enum Phase { New, FirstQ, LastQ, Full, None }; enum Hemisphere { Northern, Southern }; LunarPhase( Hemisphere hemisphere = Northern ); ~LunarPhase(); /** Return the lunar phase for the specified Gregorian date. The enum 'None' is returned if one of the supported phases does not occur on the date. @param date compute the lunar phase for the specified Gregorian date. */ Phase phase( const TQDate &date ) const; /** Return the lunar phase as a text string for the specified date. A null string is returned if one of the supported phases does not occur on the date. @param date compute the lunar phase for the specified Gregorian date. */ TQString phaseStr( const TQDate &date ) const; /** Set the hemisphere. @param hemisphere Hemisphere */ void setHemisphere( Hemisphere hemisphere = Northern ); /** Return the hemisphere. */ Hemisphere hemisphere() const; /** Return hemisphere as a clear text string. */ TQString hemisphereStr() const; /** Return the string representation of hemisphere. */ static TQString hemisphereName( Hemisphere hemisphere ); /** Return the string representation of phase. @param phase the lunar phase. */ static TQString phaseName( Phase phase ); private: /** Return the phase of the moon as a percentage of full @param t is the time since the Epoch, measured in seconds. @return the percent fullness [0,100] of the moon. */ double percentFull( uint t ) const; /** Convert degrees to radians. @param degree degrees to convert. @return degrees in radians. */ double degreesToRadians( double degree ) const; /** Adjust value so that 0 <= degree <= 360. @param degree a pointer to the degree value. */ void adj360( double *degree ) const; Hemisphere mHemisphere; }; #endif