b612
044f2f4381
- 新增半解析、旧模型、自定义与多源堆叠星历实例，提供 Context、Instance、SPK 读取及状态与视位置计算 - 统一太阳、月球和行星实例接口，扩展黄经穿越、留、相位、最近角距、偕日可见、任意高度升落、轨道节点及凌日等天象查询 - 完善日月食、月掩与凌日的月缘剖面、有限盘面接触、站心修正、局地可见性、全球路径和地图输出 - 新增 SVG、GeoJSON、KML 天象输出及凌日、月掩和月缘地形相关缓存与几何求解 - 新增恒星星表导入与查询，支持 CSV、Hipparcos、BSC5、Stellarium 等格式及名称、交叉标识、锥面检索和星等过滤 - 补充 IAU 2006、地球定向、折射消光、大气观测、轨道传播及半解析行星/月球数据支持 - 将默认未来民用时标切换为 TimeScaleLeapHour，更新 2027–2400 农历速查表、中文日期解析和时区边界处理 - 增加事件基线、跨模型回归、几何边界、月缘地形和输出契约测试，完善中英文手册、示例资源、NOTICE 与忽略规则
108 lines
4.9 KiB
Go
108 lines
4.9 KiB
Go
package basic
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import (
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"math"
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"b612.me/astro/internal/ephem"
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"b612.me/astro/planet"
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. "b612.me/astro/tools"
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)
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func moonCalcNewNWithInstance(coordIndex int, jd float64, n int, inst *Instance) float64 {
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if inst == nil {
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return planet.WhereMoonN(coordIndex, jd, n)
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}
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if inst.Model() != ephem.Custom {
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return planet.WhereMoonModelN(inst.Model(), coordIndex, jd, n)
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}
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if lo, bo, distAU, ok := instanceStateEcliptic(ephem.Moon, jd, inst); ok {
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switch coordIndex {
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case 0:
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return lo * math.Pi / 180
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case 1:
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return bo * math.Pi / 180
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case 2:
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return distAU * astronomicalUnitKM
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}
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}
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return math.NaN()
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}
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// MoonCalcNewWithInstance 指定星历实例的月球几何量 / lunar geometry with an explicit ephemeris instance.
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func MoonCalcNewWithInstance(coordIndex int, jd float64, inst *Instance) float64 {
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return moonCalcNewNWithInstance(coordIndex, jd, -1, inst)
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}
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// MoonCalcNewNWithInstance 指定星历实例的月球几何量（n 变体） / n-parameterised lunar geometry with an explicit ephemeris instance.
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func MoonCalcNewNWithInstance(coordIndex int, jd float64, n int, inst *Instance) float64 {
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return moonCalcNewNWithInstance(coordIndex, jd, n, inst)
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}
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// HMoonTrueLoWithInstance 指定星历实例的月球真黄经 / true lunar longitude with an explicit ephemeris instance.
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func HMoonTrueLoWithInstance(jde float64, inst *Instance) float64 {
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return HMoonTrueLoNWithInstance(jde, -1, inst)
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}
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// HMoonTrueLoNWithInstance 指定星历实例的月球真黄经（n 变体） / n-parameterised true lunar longitude with an explicit ephemeris instance.
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func HMoonTrueLoNWithInstance(jde float64, n int, inst *Instance) float64 {
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return Limit360(moonCalcNewNWithInstance(0, jde, n, inst) * 180 / math.Pi)
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}
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// HMoonTrueBoWithInstance 指定星历实例的月球真黄纬 / true lunar latitude with an explicit ephemeris instance.
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func HMoonTrueBoWithInstance(jde float64, inst *Instance) float64 {
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return HMoonTrueBoNWithInstance(jde, -1, inst)
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}
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// HMoonTrueBoNWithInstance 指定星历实例的月球真黄纬（n 变体） / n-parameterised true lunar latitude with an explicit ephemeris instance.
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func HMoonTrueBoNWithInstance(jde float64, n int, inst *Instance) float64 {
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return moonCalcNewNWithInstance(1, jde, n, inst) * 180 / math.Pi
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}
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// HMoonAwayWithInstance 指定星历实例的月地距离 / lunar distance with an explicit ephemeris instance.
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func HMoonAwayWithInstance(jde float64, inst *Instance) float64 {
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return HMoonAwayNWithInstance(jde, -1, inst)
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}
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// HMoonAwayNWithInstance 指定星历实例的月地距离（n 变体） / n-parameterised lunar distance with an explicit ephemeris instance.
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func HMoonAwayNWithInstance(jde float64, n int, inst *Instance) float64 {
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return moonCalcNewNWithInstance(2, jde, n, inst)
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}
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// HMoonApparentLoWithInstance 指定星历实例的月球视黄经 / apparent lunar longitude with an explicit ephemeris instance.
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func HMoonApparentLoWithInstance(jde float64, inst *Instance) float64 {
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return HMoonApparentLoNWithInstance(jde, -1, inst)
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}
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// HMoonApparentLoNWithInstance 指定星历实例的月球视黄经（n 变体） / n-parameterised apparent lunar longitude with an explicit ephemeris instance.
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func HMoonApparentLoNWithInstance(jde float64, n int, inst *Instance) float64 {
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if lo, _, _, _, ok, err := vectorApparentWithInstance(ephem.Moon, jde, n, inst); err != nil {
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return math.NaN()
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} else if ok {
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return lo
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}
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return HMoonTrueLoNWithInstance(jde, n, inst) + Nutation2000Bi(jde)
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}
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// HMoonGeocentricApparentRaDecWithInstance 指定星历实例的月球地心视赤经纬 / apparent geocentric lunar right ascension and declination with an explicit ephemeris instance.
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func HMoonGeocentricApparentRaDecWithInstance(jde float64, inst *Instance) (float64, float64) {
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return HMoonGeocentricApparentRaDecNWithInstance(jde, -1, inst)
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}
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// HMoonGeocentricApparentRaDecNWithInstance 指定星历实例的月球地心视赤经纬（n 变体） / n-parameterised apparent geocentric lunar right ascension and declination with an explicit ephemeris instance.
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func HMoonGeocentricApparentRaDecNWithInstance(jde float64, n int, inst *Instance) (float64, float64) {
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return moonApparentRaDecN(jde, n, inst)
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}
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// HMoonTrueRaDecWithInstance 指定星历实例的月球真赤经纬 / true lunar right ascension and declination with an explicit ephemeris instance.
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func HMoonTrueRaDecWithInstance(jde float64, inst *Instance) (float64, float64) {
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return moonApparentRaDecN(jde, -1, inst)
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}
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// HMoonApparentRaDecWithInstance 指定星历实例的月球站心视赤经纬 / topocentric apparent lunar right ascension and declination with an explicit ephemeris instance.
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func HMoonApparentRaDecWithInstance(jd, lon, lat, tz float64, inst *Instance) (float64, float64) {
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jde := UTC2TT(jd) - tz/24
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ra, dec := HMoonTrueRaDecWithInstance(jde, inst)
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away := HMoonAwayWithInstance(jde, inst) / astronomicalUnitKM
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return TopocentricRaDec(ra, dec, lat, lon, jd-tz/24, away, 0)
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}
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