astro/basic/coordinate.go
starainrt 3ffdbe0034
feat: 扩展天文计算能力
- 新增日食、月食、本地可见性、中心线、半影区域、SVG 图示与沙罗周期信息
- 新增行星冲合、留、方照、物理星历、视直径、相位、亮肢角、轨道节点等计算
- 新增木星伽利略卫星位置、现象与接触事件计算
- 新增恒星星表、星座判定、自行修正与观测辅助能力
- 新增 coord、formula、orbit、sundial、lite/sun、lite/moon 等扩展包
- 完善农历年号、月相英文别名、视差角、大气质量、折射、日晷与双星计算
- 增加 NASA、JPL Horizons、IMCCE 等回归测试数据与基线测试
- 重构基础算法文件组织,补充大量公开 API 注释和语义回归测试
- 更新中文和英文 README,补充示例、精度说明、SVG 配图
2026-05-01 22:38:44 +08:00

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package basic
import (
"math"
. "b612.me/astro/tools"
)
/*
* 坐标变换,黄道转赤道
*/
func LoToRa(jde, lo, bo float64) float64 {
ra := math.Atan2(Sin(lo)*Cos(TrueObliquity(jde))-Tan(bo)*Sin(TrueObliquity(jde)), Cos(lo))
ra = ra * 180 / math.Pi
if ra < 0 {
ra += 360
}
return ra
}
func BoToDec(jde, lo, bo float64) float64 {
dec := ArcSin(Sin(bo)*Cos(TrueObliquity(jde)) + Cos(bo)*Sin(TrueObliquity(jde))*Sin(lo))
return dec
}
func LoBoToRaDec(jde, lo, bo float64) (float64, float64) {
dec := ArcSin(Sin(bo)*Cos(TrueObliquity(jde)) + Cos(bo)*Sin(TrueObliquity(jde))*Sin(lo))
ra := math.Atan2(Sin(lo)*Cos(TrueObliquity(jde))-Tan(bo)*Sin(TrueObliquity(jde)), Cos(lo))
ra = ra * 180 / math.Pi
if ra < 0 {
ra += 360
}
return ra, dec
}
func RaDecToLoBo(jde, ra, dec float64) (float64, float64) {
//tan(λ) = (sin(α)*cos(ε) + tan(δ)*sin(ε)) / cos(α)
//sin(β)=sin(δ)*cos(ε)-cos(δ)*sin(ε)*sin(α)
eps := TrueObliquity(jde)
sinBo := Sin(dec)*Cos(eps) - Cos(dec)*Sin(eps)*Sin(ra)
lo := math.Atan2((Sin(ra)*Cos(eps) + Tan(dec)*Sin(eps)), Cos(ra))
lo = Limit360(lo * 180 / math.Pi)
return lo, ArcSin(sinBo)
}
func RaToLo(jde, ra, dec float64) float64 {
//tan(λ) = (sin(α)*cos(ε) + tan(δ)*sin(ε)) / cos(α)
//sin(β)=sin(δ)*cos(ε)-cos(δ)*sin(ε)*sin(α)
eps := TrueObliquity(jde)
lo := math.Atan2((Sin(ra)*Cos(eps) + Tan(dec)*Sin(eps)), Cos(ra))
lo = Limit360(lo * 180 / math.Pi)
return lo
}
func DecToBo(jde, ra, dec float64) float64 {
//tan(λ) = (sin(α)*cos(ε) + tan(δ)*sin(ε)) / cos(α)
//sin(β)=sin(δ)*cos(ε)-cos(δ)*sin(ε)*sin(α)
eps := TrueObliquity(jde)
sinBo := Sin(dec)*Cos(eps) - Cos(dec)*Sin(eps)*Sin(ra)
return ArcSin(sinBo)
}
/*
* 地心坐标转站心坐标,参数分别为,地心赤经赤纬 纬度经度jde离地心位置au
*/
func pcosi(lat, h float64) float64 {
b := 6356.755
a := 6378.14
u := ArcTan(b / a * Tan(lat))
//psin=b/a*Sin(u)+h/6378140*Sin(lat);
pcos := Cos(u) + h/6378140.0*Cos(lat)
return pcos
}
func psini(lat, h float64) float64 {
b := 6356.755
a := 6378.14
u := ArcTan(b / a * Tan(lat))
psin := b/a*Sin(u) + h/6378140*Sin(lat)
//pcos=Cos(u)+h/6378140*Cos(lat);
return psin
}
func TopocentricRaDec(ra, dec, lat, lon, jd, au, h float64) (float64, float64) {
sinpi := Sin(0.0024427777777) / au
pcosi := pcosi(lat, h)
psini := psini(lat, h)
tH := Limit360(TD2UT(ApparentSiderealTime(jd), false)*15 + lon - ra)
nra := math.Atan2(-pcosi*sinpi*Sin(tH), (Cos(dec)-pcosi*sinpi*Cos(tH))) * 180 / math.Pi
ndec := math.Atan2((Sin(dec)-psini*sinpi)*Cos(nra), (Cos(dec)-pcosi*sinpi*Cos(tH))) * 180 / math.Pi
return ra + nra, ndec
}
func TopocentricRa(ra, dec, lat, lon, jd, au, h float64) float64 { //jd为格林尼治标准时
sinpi := Sin(0.0024427777777) / au
pcosi := pcosi(lat, h)
tH := Limit360(TD2UT(ApparentSiderealTime(jd), false)*15 + lon - ra)
nra := math.Atan2(-pcosi*sinpi*Sin(tH), (Cos(dec)-pcosi*sinpi*Cos(tH))) * 180 / math.Pi
return ra + nra
}
func TopocentricDec(ra, dec, lat, lon, jd, au, h float64) float64 { //jd为格林尼治标准时
sinpi := Sin(0.0024427777777) / au
pcosi := pcosi(lat, h)
psini := psini(lat, h)
tH := Limit360(TD2UT(ApparentSiderealTime(jd), false)*15 + lon - ra)
nra := math.Atan2(-pcosi*sinpi*Sin(tH), (Cos(dec)-pcosi*sinpi*Cos(tH))) * 180 / math.Pi
ndec := math.Atan2((Sin(dec)-psini*sinpi)*Cos(nra), (Cos(dec)-pcosi*sinpi*Cos(tH))) * 180 / math.Pi
return ndec
}
func TopocentricLo(lo, bo, lat, lon, jd, au, h float64) float64 { //jd为格林尼治标准时
c := pcosi(lat, h)
s := psini(lat, h)
sinpi := Sin(0.0024427777777) / au
ra := LoToRa(jd, lo, bo)
tH := Limit360(TD2UT(ApparentSiderealTime(jd), false)*15 + lon - ra)
n := Cos(lo)*Cos(bo) - c*sinpi*Cos(tH)
nlo := math.Atan2(Sin(lo)*Cos(bo)-sinpi*(s*Sin(TrueObliquity(jd))+c*Cos(TrueObliquity(jd))*Sin(tH)), n) * 180 / math.Pi
return nlo
}
func TopocentricBo(lo, bo, lat, lon, jd, au, h float64) float64 { //jd为格林尼治标准时
c := pcosi(lat, h)
s := psini(lat, h)
sinpi := Sin(0.0024427777777) / au
ra := LoToRa(jd, lo, bo)
tH := Limit360(TD2UT(ApparentSiderealTime(jd), false)*15 + lon - ra)
n := Cos(lo)*Cos(bo) - c*sinpi*Cos(tH)
nlo := math.Atan2(Sin(lo)*Cos(bo)-sinpi*(s*Sin(TrueObliquity(jd))+c*Cos(TrueObliquity(jd))*Sin(tH)), n) * 180 / math.Pi
nbo := math.Atan2(Cos(nlo)*(Sin(bo)-sinpi*(s*Cos(TrueObliquity(jd))-c*Sin(TrueObliquity(jd))*Sin(tH))), n) * 180 / math.Pi
return nbo
}
func GXCLo(lo, bo, jd float64) float64 { //光行差修正
k := 20.49552
sunlo := SunTrueLo(jd)
e := Earthe(jd)
epi := EarthPI(jd)
tmp := (-k*Cos(sunlo-lo) + e*k*Cos(epi-lo)) / Cos(bo)
return tmp
}
func GXCBo(lo, bo, jd float64) float64 {
k := 20.49552
sunlo := SunTrueLo(jd)
e := Earthe(jd)
epi := EarthPI(jd)
tmp := -k * Sin(bo) * (Sin(sunlo-lo) - e*Sin(epi-lo))
return tmp
}