更换岁差、章动算法

This commit is contained in:
2025-09-18 13:16:04 +08:00
parent 9f688024e8
commit 543abcafa5
23 changed files with 1215 additions and 339 deletions
+59 -7
View File
@@ -21,7 +21,7 @@ func StarHeight(jde, ra, dec, lon, lat, timezone float64) float64 {
return ArcSin(sinHeight)
}
//StarAzimuth 星体的方位角
// StarAzimuth 星体的方位角
// 传入 jde时间、瞬时赤经、瞬时赤纬、经度、纬度、时区,jde时间应为时区时间
// 返回方位角,单位为度,正北为0,度数顺时针增加,取值范围[0-360)
func StarAzimuth(jde, ra, dec, lon, lat, timezone float64) float64 {
@@ -46,7 +46,7 @@ func StarAzimuth(jde, ra, dec, lon, lat, timezone float64) float64 {
return Azimuth
}
//StarHourAngle 星体的时角
// StarHourAngle 星体的时角
// 传入 jde时间、瞬时赤经、瞬时赤纬、经度、时区,jde时间应为时区时间
// 返回时角
func StarHourAngle(jde, ra, lon, timezone float64) float64 {
@@ -58,17 +58,69 @@ func StarHourAngle(jde, ra, lon, timezone float64) float64 {
return Limit360(st - ra)
}
// MeanSiderealTime 不含章动下的恒星时
// MeanSiderealTime 恒星时
func MeanSiderealTime(JD float64) float64 {
T := (JD - 2451545) / 36525
return (Limit360(280.46061837+360.98564736629*(JD-2451545.0)+0.000387933*T*T-T*T*T/38710000) / 15)
return MeanSiderealTime2006(JD)
}
// ApparentSiderealTime 视恒星时,计算章动
func ApparentSiderealTime(JD float64) float64 {
tmp := MeanSiderealTime(JD)
return tmp + HJZD(JD)*Cos(Sita(JD))/15
return ApparentSiderealTime2006(JD)
}
// MeanSiderealTime1982 不含章动下的恒星时
func MeanSiderealTime1982(JD float64) float64 {
T := (JD - 2451545) / 36525
return (Limit360(280.46061837+360.98564736629*(JD-2451545.0)+0.000387933*T*T-T*T*T/38710000) / 15)
}
// ApparentSiderealTime1982 视恒星时,计算章动
func ApparentSiderealTime1982(JD float64) float64 {
tmp := MeanSiderealTime1982(JD)
return tmp + Nutation2000Bi(JD)*Cos(Sita(JD))/15
}
// EarthRotationAngle 计算地球自转角 (ERA)
// jd_ut1: UT1 时间的儒略日
// 返回值: 地球自转角 (弧度)
func EarthRotationAngle(jd_ut1 float64) float64 {
t := jd_ut1 - 2451545.0
frac := math.Mod(jd_ut1, 1.0)
era := math.Mod(math.Pi*2*(0.7790572732640+0.00273781191135448*t+frac), math.Pi*2)
if era < 0 {
era += math.Pi * 2
}
return era
}
// MeanSiderealTime2006 计算格林尼治平恒星时 (GMST)
// jd_ut1: UT1 时间的儒略日
// jd_tt: TT 时间的儒略日
// 返回值: 格林尼治平恒星时 (弧度)
func MeanSiderealTime2006(jd_ut1 float64) float64 {
jd_tt := TD2UT(jd_ut1, true)
t := (jd_tt - 2451545.0) / 36525.0
era := EarthRotationAngle(jd_ut1)
// 公式 2.12
gmst := math.Mod(era+(0.014506+4612.15739966*t+1.39667721*t*t+
-0.00009344*t*t*t+0.00001882*t*t*t*t)/60/60*math.Pi/180, math.Pi*2)
if gmst < 0 {
gmst += math.Pi * 2
}
return gmst * deg / 15
}
// ApparentSiderealTime2006 视恒星时,计算章动
func ApparentSiderealTime2006(JD float64) float64 {
tmp := MeanSiderealTime2006(JD)
return tmp + Nutation2000Bi(JD)*Cos(Sita(JD))/15
}
func StarAngle(RA, DEC, JD, Lon, Lat, TZ float64) float64 {
//JD=JD-8/24+TZ/24;
calcjd := JD - TZ/24