void HuntPhase(int startdate, int starttim, int phas, int *date, int *time)
{
int utcd, utct;
int y, m, d;
int h, min, s;
int d1, t1;
double k1, k2, jd, jdorig;
double nt1, nt2;
/* Convert from local to UTC */
LocalToUTC(startdate, starttim, &utcd, &utct);
/* Convert from Remind representation to year/mon/day */
FromJulian(utcd, &y, &m, &d);
/* Convert to a true Julian date -- sorry for the name clashes! */
jdorig = jtime(y, m, d, (utct / 60), (utct % 60), 0);
jd = jdorig - 45.0;
nt1 = meanphase(jd, 0.0, &k1);
while(1) {
jd += synmonth;
nt2 = meanphase(jd, 0.0, &k2);
if (nt1 <= jdorig && nt2 > jdorig) break;
nt1 = nt2;
k1 = k2;
}
jd = truephase(k1, phas/4.0);
if (jd < jdorig) jd = truephase(k2, phas/4.0);
/* Convert back to Remind format */
jyear(jd, &y, &m, &d);
jhms(jd, &h, &min, &s);
d1 = Julian(y, m, d);
t1 = h*60 + min;
UTCToLocal(d1, t1, date, time);
}
BOOL
isFullMoonDay( long _yy, long _mm, long _dd )
{
double jd, aom, cphase, cdist, cangdia, csund, csuang, lptime;
long yy, mm, dd, hh, mmm, ss; /* (直前の)朔の年月日時分秒 */
long uyy, umm, udd, uhh, ummm, uss; /* UTC変換後の現在日時 */
double phasar[5];
double t1;
int __y, __m, __d;
long tt;
struct tm *lm;
time_t t = 0;
/*
* timezone を求める (UTC とローカル時間の時差を求める)
*/
lm = localtime( &t );
#ifdef UNIX
# ifndef SYSV
/* BSD系のUNIXでは、以下の処理が必要
* (ANSI C 登場以前の UNIX では、BSD系でない場合でも、別途対応が必要
* であると思われる)
*/
if ( (lm->tm_isdst != 0) && (lm->tm_isdst != 1) ) {
lm->tm_isdst = 0;
lm->tm_gmtoff = 9 * 60 * 60;
lm->tm_zone = "JST";
}
_tzname[lm->tm_isdst] = lm->tm_zone;
_timezone = -(lm->tm_gmtoff);
# endif
#else /* !UNIX */
# ifdef WIN32
{
OSVERSIONINFO osverInfo;
BOOL ret;
osverInfo.dwOSVersionInfoSize = sizeof ( OSVERSIONINFO );
if ( ret = GetVersionEx( &osverInfo ) ) {
if ( (osverInfo.dwPlatformId == VER_PLATFORM_WIN32_WINDOWS) ||
(osverInfo.dwPlatformId == VER_PLATFORM_WIN32s ) ) {
/* Windows 3.x (Win32S環境), Windows95, Windows98 の場合は、
* 以下の処理が必要
*/
lm->tm_isdst = 0;
_tzname[lm->tm_isdst] = "JST";
_timezone = -(9 * 60 * 60);
}
}
}
# endif
#endif
/*
* ローカル時間で指定された年月日時分秒を UTC に変換する
*/
t1 = ((double)absoluteFromGregorian( _dd, _mm, _yy )) * 24.0 + _timezone;
tt = _timezone;
uyy = _yy;
umm = _mm;
udd = _dd;
uhh = 0;
ummm = 0;
uss = 0;
if ( tt < 0 ) {
gregorianFromAbsolute( absoluteFromGregorian( _dd, _mm, _yy ) - 1,
&__d, &__m, &__y );
uyy = __y;
umm = __m;
udd = __d;
}
else if ( tt > 24 * 60 * 60 ) {
gregorianFromAbsolute( absoluteFromGregorian( _dd, _mm, _yy ) + 1,
&__d, &__m, &__y );
uyy = __y;
umm = __m;
udd = __d;
}
uhh = (_timezone / (60 * 60)) % 24;
if ( uhh < 0 )
uhh += 24;
ummm = (_timezone / 60) % 60;
if ( ummm < 0 )
ummm += 60;
uss = _timezone % 60;
if ( uss < 0 )
uss += 60;
/*
* UTC をユリウス日に変換する
*/
jd = jtime( uyy, umm, udd, uhh, ummm, uss );
/*
* 当該ユリウス日の直前の朔の日時を求める
*/
yy = 0;
(void)phase( jd + 1, &cphase, &aom, &cdist, &cangdia, &csund, &csuang );
phasehunt( jd, phasar );
lptime = phasar[2];
jyear( lptime, &yy, &mm, &dd );
jhms( lptime, &hh, &mmm, &ss );
return ( ( (yy == _yy) && (mm == _mm) && (dd == _dd) ) ? TRUE : FALSE );
}
void
tamo_moon( long _yy, long _mm, long _dd, long _hh, long _mmm, long _ss,
int flag )
{
double jd, aom, cphase, cdist, cangdia, csund, csuang, lptime;
long yy, mm, dd, hh, mmm, ss; /* (直前の)朔の年月日時分秒 */
long uyy, umm, udd, uhh, ummm, uss; /* UTC変換後の現在日時 */
double phasar[5];
long lunation;
static double nptime = 0.0; /* Next new moon time */
double t1, t2;
int __y, __m, __d;
long tt;
struct tm *lm;
time_t t = 0;
/*
* timezone を求める (UTC とローカル時間の時差を求める)
*/
lm = localtime( &t );
#ifdef UNIX
# ifndef SYSV
/* BSD系のUNIXでは、以下の処理が必要
* (ANSI C 登場以前の UNIX では、BSD系でない場合でも、別途対応が必要
* であると思われる)
*/
if ( (lm->tm_isdst != 0) && (lm->tm_isdst != 1) ) {
lm->tm_isdst = 0;
lm->tm_gmtoff = 9 * 60 * 60;
lm->tm_zone = "JST";
}
_tzname[lm->tm_isdst] = lm->tm_zone;
_timezone = -(lm->tm_gmtoff);
# endif
#else /* !UNIX */
# ifdef WIN32
{
OSVERSIONINFO osverInfo;
BOOL ret;
osverInfo.dwOSVersionInfoSize = sizeof ( OSVERSIONINFO );
if ( ret = GetVersionEx( &osverInfo ) ) {
if ( (osverInfo.dwPlatformId == VER_PLATFORM_WIN32_WINDOWS) ||
(osverInfo.dwPlatformId == VER_PLATFORM_WIN32s ) ) {
/* Windows 3.x (Win32S環境), Windows95, Windows98 の場合は、
* 以下の処理が必要
*/
lm->tm_isdst = 0;
_tzname[lm->tm_isdst] = "JST";
_timezone = -(9 * 60 * 60);
}
}
}
# endif
#endif
/*
* ローカル時間で指定された年月日時分秒を UTC に変換する
*/
t1 = ((((double)absoluteFromGregorian( _dd, _mm, _yy ) * 24.0 +
(double)_hh) * 60.0) + (double)_mmm) * 60.0 +
(double)_ss + (double)_timezone;
tt = (_hh * 60 + _mmm) * 60 + _ss + _timezone;
uyy = _yy;
umm = _mm;
udd = _dd;
uhh = _hh;
ummm = _mmm;
uss = _ss;
if ( tt < 0 ) {
gregorianFromAbsolute( absoluteFromGregorian( _dd, _mm, _yy ) - 1,
&__d, &__m, &__y );
uyy = __y;
umm = __m;
udd = __d;
}
else if ( tt > 24 * 60 * 60 ) {
gregorianFromAbsolute( absoluteFromGregorian( _dd, _mm, _yy ) + 1,
&__d, &__m, &__y );
uyy = __y;
umm = __m;
udd = __d;
}
uhh = ((uhh * 60 * 60 + _timezone) / (60 * 60)) % 24;
if ( uhh < 0 )
uhh += 24;
ummm = ((ummm * 60 + _timezone) / 60) % 60;
if ( ummm < 0 )
ummm += 60;
uss = (uss + _timezone) % 60;
if ( uss < 0 )
uss += 60;
/*
* UTC をユリウス日に変換する
*/
jd = jtime( uyy, umm, udd, uhh, ummm, uss );
/*
* 当該ユリウス日の直前の朔の日時を求める
*/
yy = 0;
(void)phase( jd + 1, &cphase, &aom, &cdist, &cangdia, &csund, &csuang );
phasehunt( jd, phasar );
lptime = phasar[0];
lunation = (long)(floor(((lptime + 7.0) - lunatbase) / synmonth) + 1.0);
jyear( lptime, &yy, &mm, &dd );
jhms( lptime, &hh, &mmm, &ss );
/*
* 朔の日時(ユリウス日)を UTC に変換する
*/
t2 = ((((double)absoluteFromGregorian( dd, mm, yy ) * 24.0 +
(double)hh) * 60.0) + (double)mmm) * 60.0 + (double)ss;
/*
* 2つの UTC の差分を元に月齢を求める
*/
aom = qpom3( t1, t2 );
if ( aom < 0.0 )
aom += synmonth;
/*
* 結果を出力する
*/
if ( flag ) {
printf( "<TABLE BORDER=\"0\" SUMMARY=\"月齢\">\n<TR><TD>月齢" );
}
else {
if ( !strncmp( _tzname[lm->tm_isdst], "東京", 4 ) )
printf( "%d年%02d月%02d日 %02d時%02d分%02d秒(JST)現在の月齢",
_yy, _mm, _dd, _hh, _mmm, _ss );
else if ( _tzname[lm->tm_isdst][0] )
printf( "%d年%02d月%02d日 %02d時%02d分%02d秒(%s)現在の月齢",
_yy, _mm, _dd, _hh, _mmm, _ss, _tzname[lm->tm_isdst] );
else
printf( "%d年%02d月%02d日 %02d時%02d分%02d秒現在の月齢",
_yy, _mm, _dd, _hh, _mmm, _ss );
}
printf( "%s%.1f (%02d日%02d時%02d分)",
flag ? "</TD><TD>" : ":\n ",
aom /*+ 0.05*/,
(int) aom, ((int) (24 * (aom - floor(aom)))),
((int) (1440 * (aom - floor(aom)))) % 60 );
printf( " %s[輝度: %.1f%%]",
flag ? "<BR>" : " ",
(1.0 - cos((2.0 * PI * aom) / (LPERIOD / 86400.0))) / 2.0 * 100.0 );
if ( flag ) {
printf( "</TD>\n<TD ROWSPAN=5><IMG SRC=" );
printf(
#ifdef RIMNET
"\"/~tsupo/qpom/image/moon%2.2d.gif\"",
#else
"\"qpom/image/moon%2.2d.gif\"",
#endif
(int)(100.0 * (aom /*+ 0.05*/) / (LPERIOD / 86400.0)) );
printf( " WIDTH=\"110\" HEIGHT=\"110\"" );
printf( " ALIGN=\"LEFT\" BORDER=2 ALT=\"[%1d day old Moon]\">\n",
(long)(aom /*+ 0.05*/));
printf( "</TD></TR>\n<TR><TD>" );
}
else {
putchar( '\n' );
}
printf( "地球-月の距離%s%ldkm%s(地球赤道半径の%.1f倍)\n",
flag ? "</TD><TD>" : ": ",
(long) cdist,
flag ? "<BR>" : " ",
cdist / earthrad );
if ( flag )
printf( "</TD></TR>\n<TR><TD>" );
printf( "月の視差%s%.4f度\n",
flag ? "</TD><TD>" : ": ",
cangdia );
if ( flag )
printf( "</TD></TR>\n<TR><TD>" );
printf( "地球-太陽の距離%s%.0fkm%s(%.3f天文単位)\n",
flag ? "</TD><TD>" : ": ",
csund,
flag ? "<BR>" : " ",
csund / sunsmax );
if ( flag )
printf( "</TD></TR>\n<TR><TD>" );
printf( "太陽の視差%s%.4f度\n",
flag ? "</TD><TD>" : ": ",
csuang );
if ( flag )
printf( "</TD></TR>\n<TR><TD>" );
printf( "朔%s%ld年%02ld月%02ld日 %02ld時%02ld分 UTC ",
flag ? "</TD><TD COLSPAN=2>" : ": ",
yy, mm, dd, hh, mmm );
printf( "(Lunation %ld)\n", lunation );
if ( flag )
printf( "</TD></TR>\n<TR><TD>" );
lptime = phasar[1];
jyear( lptime, &yy, &mm, &dd );
jhms( lptime, &hh, &mmm, &ss );
printf( "上弦%s%ld年%02ld月%02ld日 %02ld時%02ld分 UTC\n",
flag ? "</TD><TD COLSPAN=2>" : ": ",
yy, mm, dd, hh, mmm );
if ( flag )
printf( "</TD></TR>\n<TR><TD>" );
lptime = phasar[2];
jyear( lptime, &yy, &mm, &dd );
jhms( lptime, &hh, &mmm, &ss );
printf( "望%s%ld年%02ld月%02ld日 %02ld時%02ld分 UTC\n",
flag ? "</TD><TD COLSPAN=2>" : ": ",
yy, mm, dd, hh, mmm );
if ( flag )
printf( "</TD></TR>\n<TR><TD>" );
lptime = phasar[3];
jyear( lptime, &yy, &mm, &dd );
jhms( lptime, &hh, &mmm, &ss );
printf( "下弦%s%ld年%02ld月%02ld日 %02ld時%02ld分 UTC\n",
flag ? "</TD><TD COLSPAN=2>" : ": ",
yy, mm, dd, hh, mmm );
if ( flag )
printf( "</TD></TR>\n<TR><TD>" );
nptime = phasar[4];
jyear( nptime, &yy, &mm, &dd );
jhms( nptime, &hh, &mmm, &ss );
printf( "次の朔%s%ld年%02ld月%02ld日 %02ld時%02ld分 UTC ",
flag ? "</TD><TD COLSPAN=2>" : ": ",
yy, mm, dd, hh, mmm );
printf( "(Lunation %ld)\n", lunation + 1 );
if ( flag )
printf( "</TD></TR>\n</TABLE>\n" );
#ifdef __TEST_20030507__
if ( !flag ) {
double target = 0.0;
lptime = phasar[0];
jyear( lptime, &yy, &mm, &dd );
jhms( lptime, &hh, &mmm, &ss );
printf( " 月齢 %f : %ld年%02ld月%02ld日 %02ld時%02ld分 UTC\n",
target, yy, mm, dd, hh, mmm );
target += 1.0;
do {
jyear( lptime, &yy, &mm, &dd );
jhms( lptime, &hh, &mmm, &ss );
/*
t1 = ((((double)absoluteFromGregorian( dd, mm, yy ) * 24.0 +
(double)hh) * 60.0) + (double)mmm) * 60.0 +
(double)ss;
// aom = qpom3( t1, t2 );
*/
jd = jtime( yy, mm, dd, hh, mmm, ss );
phase( jd + 1, &cphase, &aom, &cdist, &cangdia, &csund, &csuang );
/*
if ( aom < 0.0 )
aom += synmonth;
*/
// printf( "aom = %f\n", aom );
/*
jyear( lptime, &yy, &mm, &dd );
jhms( lptime, &hh, &mmm, &ss );
printf( " 月齢 %f : %ld年%02ld月%02ld日 %02ld時%02ld分 UTC\n",
aom, yy, mm, dd, hh, mmm );
*/
// if ( aom > 1.0 )
// break;
if ( floor(target * 100.0) == floor(aom * 100.00) ) {
printf( " 月齢 %f : %ld年%02ld月%02ld日 %02ld時%02ld分 UTC\n",
target - 1.0, yy, mm, dd, hh, mmm );
target += 1.0;
}
lptime += 1.0 / (24.0 * 3600.0);
/* lptime += 0.001; */
} while ( floor(aom * 100.00) != 0.0 );
lptime = phasar[4];
jyear( lptime, &yy, &mm, &dd );
jhms( lptime, &hh, &mmm, &ss );
printf( " 月齢 %f : %ld年%02ld月%02ld日 %02ld時%02ld分 UTC\n",
target, yy, mm, dd, hh, mmm );
}
#endif /* __TEST_20030507__ */
}