feat: 引入可切换星历模型并扩展天象观测链路
- 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
This commit is contained in:
+288
-245
@@ -3,20 +3,21 @@ package basic
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import (
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"math"
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"b612.me/astro/planet"
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. "b612.me/astro/tools"
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)
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// Exported N variants below keep the same jd semantics as the non-N APIs; n < 0 means full series.
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type planetDeclinationFuncN func(float64, int) float64
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func planetXYZN(planetIndex int, jde float64, n int) (float64, float64, float64) {
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l := planet.WherePlanetN(planetIndex, 0, jde, n)
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b := planet.WherePlanetN(planetIndex, 1, jde, n)
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r := planet.WherePlanetN(planetIndex, 2, jde, n)
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el := planet.WherePlanetN(-1, 0, jde, n)
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eb := planet.WherePlanetN(-1, 1, jde, n)
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er := planet.WherePlanetN(-1, 2, jde, n)
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func planetXYZN(planetIndex int, jde float64, n int, instances ...*Instance) (float64, float64, float64) {
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inst := instanceValue(instances)
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l := PlanetCoordinateNWithInstance(planetIndex, 0, jde, n, inst)
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b := PlanetCoordinateNWithInstance(planetIndex, 1, jde, n, inst)
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r := PlanetCoordinateNWithInstance(planetIndex, 2, jde, n, inst)
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el := PlanetCoordinateNWithInstance(-1, 0, jde, n, inst)
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eb := PlanetCoordinateNWithInstance(-1, 1, jde, n, inst)
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er := PlanetCoordinateNWithInstance(-1, 2, jde, n, inst)
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x := r*Cos(b)*Cos(l) - er*Cos(eb)*Cos(el)
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y := r*Cos(b)*Sin(l) - er*Cos(eb)*Sin(el)
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z := r*Sin(b) - er*Sin(eb)
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@@ -58,34 +59,6 @@ func planetEarthAwayN(planetIndex int, jd float64, n int) float64 {
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return planetEarthAwayExplicitN(planetIndex, jd, n)
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}
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func planetHeightN(localJD, lon, lat, timezone float64, n int, apparentRaDec func(float64, int) (float64, float64)) float64 {
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utcJD := localJD - timezone/24.0
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ra, dec := apparentRaDec(UTC2TT(utcJD), n)
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st := Limit360(ApparentSiderealTime(UTC2UT1(utcJD))*15 + lon)
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H := Limit360(st - ra)
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sinHeight := Sin(lat)*Sin(dec) + Cos(dec)*Cos(lat)*Cos(H)
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return ArcSin(sinHeight)
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}
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func planetAzimuthN(localJD, lon, lat, timezone float64, n int, apparentRaDec func(float64, int) (float64, float64)) float64 {
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utcJD := localJD - timezone/24.0
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ra, dec := apparentRaDec(UTC2TT(utcJD), n)
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st := Limit360(ApparentSiderealTime(UTC2UT1(utcJD))*15 + lon)
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H := Limit360(st - ra)
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tanAzimuth := Sin(H) / (Cos(H)*Sin(lat) - Tan(dec)*Cos(lat))
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azimuth := ArcTan(tanAzimuth)
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if azimuth < 0 {
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if H/15 < 12 {
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return azimuth + 360
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}
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return azimuth + 180
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}
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if H/15 < 12 {
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return azimuth + 180
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}
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return azimuth
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}
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func planetHourAngleN(jd, lon, timezone float64, n int, apparentRa func(float64, int) float64) float64 {
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siderealLongitude := Limit360(ApparentSiderealTime(UTC2UT1(jd-timezone/24))*15 + lon)
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hourAngle := siderealLongitude - apparentRa(UTC2TT(jd-timezone/24.0), n)
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@@ -181,548 +154,618 @@ func planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight floa
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return estimateJD - localTimezone/24 + timezone/24, nil
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}
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// MercuryApparentLoN 水星视黄经（截断版） / truncated apparent ecliptic longitude of Mercury.
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// MercuryApparentLoN 水星视黄经（n 变体） / n-parameterised apparent ecliptic longitude of Mercury.
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func MercuryApparentLoN(jd float64, n int) float64 {
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lo, _ := planetApparentLoBoN(1, jd, n)
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return lo
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}
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// MercuryApparentBoN 水星视黄纬（截断版） / truncated apparent ecliptic latitude of Mercury.
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// MercuryApparentBoN 水星视黄纬（n 变体） / n-parameterised apparent ecliptic latitude of Mercury.
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func MercuryApparentBoN(jd float64, n int) float64 {
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_, bo := planetApparentLoBoN(1, jd, n)
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return bo
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}
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// MercuryApparentLoBoN 水星视黄经黄纬（截断版） / truncated apparent ecliptic longitude and latitude of Mercury.
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// MercuryApparentLoBoN 水星视黄经黄纬（n 变体） / n-parameterised apparent ecliptic longitude and latitude of Mercury.
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func MercuryApparentLoBoN(jd float64, n int) (float64, float64) {
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return planetApparentLoBoN(1, jd, n)
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}
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// MercuryApparentRaN 水星视赤经（截断版） / truncated apparent right ascension of Mercury.
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// MercuryApparentRaN 水星视赤经（n 变体） / n-parameterised apparent right ascension of Mercury.
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func MercuryApparentRaN(jde float64, n int) float64 {
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lo, bo := MercuryApparentLoBoN(jde, n)
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return LoToRa(jde, lo, bo)
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}
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// MercuryApparentDecN 水星视赤纬（截断版） / truncated apparent declination of Mercury.
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// MercuryApparentDecN 水星视赤纬（n 变体） / n-parameterised apparent declination of Mercury.
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func MercuryApparentDecN(jde float64, n int) float64 {
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lo, bo := MercuryApparentLoBoN(jde, n)
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eps := TrueObliquity(jde)
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return ArcSin(Sin(bo)*Cos(eps) + Cos(bo)*Sin(eps)*Sin(lo))
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}
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// MercuryApparentRaDecN 水星视赤经赤纬（截断版） / truncated apparent right ascension and declination of Mercury.
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// MercuryApparentRaDecN 水星视赤经赤纬（n 变体） / n-parameterised apparent right ascension and declination of Mercury.
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func MercuryApparentRaDecN(jde float64, n int) (float64, float64) {
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lo, bo := MercuryApparentLoBoN(jde, n)
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return LoBoToRaDec(jde, lo, bo)
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}
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// EarthMercuryAwayN 地水距离（截断版） / truncated Earth-Mercury distance.
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// EarthMercuryAwayN 地水距离（n 变体） / n-parameterised Earth-Mercury distance.
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func EarthMercuryAwayN(jd float64, n int) float64 {
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return planetEarthAwayN(1, jd, n)
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}
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// MercuryMagN 水星视星等（截断版） / truncated apparent magnitude of Mercury.
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func MercuryMagN(jde float64, n int) float64 {
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awaySun := planet.WherePlanetN(1, 2, jde, n)
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awayEarth := EarthMercuryAwayN(jde, n)
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away := planet.WherePlanetN(-1, 2, jde, n)
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// MercuryMagNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
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func MercuryMagNWithInstance(jde float64, n int, inst *Instance) float64 {
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awaySun := PlanetCoordinateNWithInstance(1, 2, jde, n, inst)
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awayEarth := EarthMercuryAwayNWithInstance(jde, n, inst)
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away := PlanetCoordinateNWithInstance(-1, 2, jde, n, inst)
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i := (awaySun*awaySun + awayEarth*awayEarth - away*away) / (2 * awaySun * awayEarth)
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i = ArcCos(i)
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mag := -0.42 + 5*math.Log10(awaySun*awayEarth) + 0.0380*i - 0.000273*i*i + 0.000002*i*i*i
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return FloatRound(mag, 2)
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}
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// MercuryHeightN 水星高度角（截断版） / truncated altitude of Mercury.
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func MercuryHeightN(localJD, lon, lat, timezone float64, n int) float64 {
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return planetHeightN(localJD, lon, lat, timezone, n, MercuryApparentRaDecN)
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// MercuryHeightNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
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func MercuryHeightNWithInstance(localJD, lon, lat, timezone float64, n int, inst *Instance) float64 {
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return planetHeightN(1, localJD, lon, lat, timezone, n, inst)
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}
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// MercuryAzimuthN 水星方位角（截断版） / truncated azimuth of Mercury.
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func MercuryAzimuthN(localJD, lon, lat, timezone float64, n int) float64 {
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return planetAzimuthN(localJD, lon, lat, timezone, n, MercuryApparentRaDecN)
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// MercuryAzimuthNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
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func MercuryAzimuthNWithInstance(localJD, lon, lat, timezone float64, n int, inst *Instance) float64 {
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return planetAzimuthN(1, localJD, lon, lat, timezone, n, inst)
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}
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// MercuryHourAngleN 水星时角（截断版） / truncated hour angle of Mercury.
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func MercuryHourAngleN(jd, lon, timezone float64, n int) float64 {
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return planetHourAngleN(jd, lon, timezone, n, MercuryApparentRaN)
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// MercuryHourAngleNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
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func MercuryHourAngleNWithInstance(jd, lon, timezone float64, n int, inst *Instance) float64 {
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return planetHourAngleN(jd, lon, timezone, n, func(jde float64, n int) float64 { return MercuryApparentRaNWithInstance(jde, n, inst) })
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}
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// MercuryCulminationTimeN 水星中天时间（截断版） / truncated culmination time of Mercury.
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func MercuryCulminationTimeN(localJD, lon, timezone float64, n int) float64 {
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return planetCulminationTimeN(localJD, lon, timezone, n, MercuryHourAngleN)
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// MercuryCulminationTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
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func MercuryCulminationTimeNWithInstance(localJD, lon, timezone float64, n int, inst *Instance) float64 {
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return planetCulminationTimeN(localJD, lon, timezone, n, func(jd, lon, timezone float64, n int) float64 {
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return MercuryHourAngleNWithInstance(jd, lon, timezone, n, inst)
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})
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}
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// MercuryRiseTimeN 水星升起时间（截断版） / truncated rise time of Mercury.
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func MercuryRiseTimeN(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int) (float64, error) {
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return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, true, n, MercuryCulminationTimeN, MercuryHeightN, MercuryApparentDecN)
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// MercuryRiseTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
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func MercuryRiseTimeNWithInstance(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int, inst *Instance) (float64, error) {
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return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, true, n, func(localJD, lon, timezone float64, n int) float64 {
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return MercuryCulminationTimeNWithInstance(localJD, lon, timezone, n, inst)
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}, func(localJD, lon, lat, timezone float64, n int) float64 {
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return MercuryHeightNWithInstance(localJD, lon, lat, timezone, n, inst)
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}, func(jde float64, n int) float64 { return MercuryApparentDecNWithInstance(jde, n, inst) })
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}
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// MercurySetTimeN 水星落下时间（截断版） / truncated set time of Mercury.
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func MercurySetTimeN(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int) (float64, error) {
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return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, false, n, MercuryCulminationTimeN, MercuryHeightN, MercuryApparentDecN)
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// MercurySetTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
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func MercurySetTimeNWithInstance(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int, inst *Instance) (float64, error) {
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return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, false, n, func(localJD, lon, timezone float64, n int) float64 {
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return MercuryCulminationTimeNWithInstance(localJD, lon, timezone, n, inst)
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}, func(localJD, lon, lat, timezone float64, n int) float64 {
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return MercuryHeightNWithInstance(localJD, lon, lat, timezone, n, inst)
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}, func(jde float64, n int) float64 { return MercuryApparentDecNWithInstance(jde, n, inst) })
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}
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// VenusApparentLoN 金星视黄经（截断版） / truncated apparent ecliptic longitude of Venus.
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// VenusApparentLoN 金星视黄经（n 变体） / n-parameterised apparent ecliptic longitude of Venus.
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func VenusApparentLoN(jd float64, n int) float64 {
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lo, _ := planetApparentLoBoN(2, jd, n)
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return lo
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}
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// VenusApparentBoN 金星视黄纬（截断版） / truncated apparent ecliptic latitude of Venus.
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// VenusApparentBoN 金星视黄纬（n 变体） / n-parameterised apparent ecliptic latitude of Venus.
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func VenusApparentBoN(jd float64, n int) float64 {
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_, bo := planetApparentLoBoN(2, jd, n)
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return bo
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}
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// VenusApparentLoBoN 金星视黄经黄纬（截断版） / truncated apparent ecliptic longitude and latitude of Venus.
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// VenusApparentLoBoN 金星视黄经黄纬（n 变体） / n-parameterised apparent ecliptic longitude and latitude of Venus.
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func VenusApparentLoBoN(jd float64, n int) (float64, float64) {
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return planetApparentLoBoN(2, jd, n)
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}
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// VenusApparentRaN 金星视赤经（截断版） / truncated apparent right ascension of Venus.
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// VenusApparentRaN 金星视赤经（n 变体） / n-parameterised apparent right ascension of Venus.
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func VenusApparentRaN(jd float64, n int) float64 {
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return planetApparentRaManualN(2, jd, n)
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}
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// VenusApparentDecN 金星视赤纬（截断版） / truncated apparent declination of Venus.
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// VenusApparentDecN 金星视赤纬（n 变体） / n-parameterised apparent declination of Venus.
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func VenusApparentDecN(jd float64, n int) float64 {
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return planetApparentDecManualN(2, jd, n)
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}
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// VenusApparentRaDecN 金星视赤经赤纬（截断版） / truncated apparent right ascension and declination of Venus.
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// VenusApparentRaDecN 金星视赤经赤纬（n 变体） / n-parameterised apparent right ascension and declination of Venus.
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func VenusApparentRaDecN(jd float64, n int) (float64, float64) {
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return planetApparentRaDecManualN(2, jd, n)
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}
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// EarthVenusAwayN 地金距离（截断版） / truncated Earth-Venus distance.
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// EarthVenusAwayN 地金距离（n 变体） / n-parameterised Earth-Venus distance.
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func EarthVenusAwayN(jd float64, n int) float64 {
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return planetEarthAwayN(2, jd, n)
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}
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// VenusMagN 金星视星等（截断版） / truncated apparent magnitude of Venus.
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func VenusMagN(jde float64, n int) float64 {
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awaySun := planet.WherePlanetN(2, 2, jde, n)
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awayEarth := EarthVenusAwayN(jde, n)
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away := planet.WherePlanetN(-1, 2, jde, n)
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// VenusMagNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
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func VenusMagNWithInstance(jde float64, n int, inst *Instance) float64 {
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awaySun := PlanetCoordinateNWithInstance(2, 2, jde, n, inst)
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awayEarth := EarthVenusAwayNWithInstance(jde, n, inst)
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away := PlanetCoordinateNWithInstance(-1, 2, jde, n, inst)
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i := (awaySun*awaySun + awayEarth*awayEarth - away*away) / (2 * awaySun * awayEarth)
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i = ArcCos(i)
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mag := -4.40 + 5*math.Log10(awaySun*awayEarth) + 0.0009*i + 0.000239*i*i - 0.00000065*i*i*i
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return FloatRound(mag, 2)
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}
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// VenusHeightN 金星高度角（截断版） / truncated altitude of Venus.
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func VenusHeightN(localJD, lon, lat, timezone float64, n int) float64 {
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return planetHeightN(localJD, lon, lat, timezone, n, VenusApparentRaDecN)
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// VenusHeightNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
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func VenusHeightNWithInstance(localJD, lon, lat, timezone float64, n int, inst *Instance) float64 {
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return planetHeightN(2, localJD, lon, lat, timezone, n, inst)
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}
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// VenusAzimuthN 金星方位角（截断版） / truncated azimuth of Venus.
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func VenusAzimuthN(localJD, lon, lat, timezone float64, n int) float64 {
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return planetAzimuthN(localJD, lon, lat, timezone, n, VenusApparentRaDecN)
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// VenusAzimuthNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
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func VenusAzimuthNWithInstance(localJD, lon, lat, timezone float64, n int, inst *Instance) float64 {
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return planetAzimuthN(2, localJD, lon, lat, timezone, n, inst)
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}
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// VenusHourAngleN 金星时角（截断版） / truncated hour angle of Venus.
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func VenusHourAngleN(jd, lon, timezone float64, n int) float64 {
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return planetHourAngleN(jd, lon, timezone, n, VenusApparentRaN)
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// VenusHourAngleNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
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func VenusHourAngleNWithInstance(jd, lon, timezone float64, n int, inst *Instance) float64 {
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return planetHourAngleN(jd, lon, timezone, n, func(jd float64, n int) float64 { return VenusApparentRaNWithInstance(jd, n, inst) })
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}
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// VenusCulminationTimeN 金星中天时间（截断版） / truncated culmination time of Venus.
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func VenusCulminationTimeN(localJD, lon, timezone float64, n int) float64 {
|
||||
return planetCulminationTimeN(localJD, lon, timezone, n, VenusHourAngleN)
|
||||
// VenusCulminationTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func VenusCulminationTimeNWithInstance(localJD, lon, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetCulminationTimeN(localJD, lon, timezone, n, func(jd, lon, timezone float64, n int) float64 {
|
||||
return VenusHourAngleNWithInstance(jd, lon, timezone, n, inst)
|
||||
})
|
||||
}
|
||||
|
||||
// VenusRiseTimeN 金星升起时间（截断版） / truncated rise time of Venus.
|
||||
func VenusRiseTimeN(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, true, n, VenusCulminationTimeN, VenusHeightN, VenusApparentDecN)
|
||||
// VenusRiseTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func VenusRiseTimeNWithInstance(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int, inst *Instance) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, true, n, func(localJD, lon, timezone float64, n int) float64 {
|
||||
return VenusCulminationTimeNWithInstance(localJD, lon, timezone, n, inst)
|
||||
}, func(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return VenusHeightNWithInstance(localJD, lon, lat, timezone, n, inst)
|
||||
}, func(jd float64, n int) float64 { return VenusApparentDecNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// VenusSetTimeN 金星落下时间（截断版） / truncated set time of Venus.
|
||||
func VenusSetTimeN(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, false, n, VenusCulminationTimeN, VenusHeightN, VenusApparentDecN)
|
||||
// VenusSetTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func VenusSetTimeNWithInstance(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int, inst *Instance) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, false, n, func(localJD, lon, timezone float64, n int) float64 {
|
||||
return VenusCulminationTimeNWithInstance(localJD, lon, timezone, n, inst)
|
||||
}, func(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return VenusHeightNWithInstance(localJD, lon, lat, timezone, n, inst)
|
||||
}, func(jd float64, n int) float64 { return VenusApparentDecNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// MarsApparentLoN 火星视黄经（截断版） / truncated apparent ecliptic longitude of Mars.
|
||||
// MarsApparentLoN 火星视黄经（n 变体） / n-parameterised apparent ecliptic longitude of Mars.
|
||||
func MarsApparentLoN(jd float64, n int) float64 {
|
||||
lo, _ := planetApparentLoBoN(3, jd, n)
|
||||
return lo
|
||||
}
|
||||
|
||||
// MarsApparentBoN 火星视黄纬（截断版） / truncated apparent ecliptic latitude of Mars.
|
||||
// MarsApparentBoN 火星视黄纬（n 变体） / n-parameterised apparent ecliptic latitude of Mars.
|
||||
func MarsApparentBoN(jd float64, n int) float64 {
|
||||
_, bo := planetApparentLoBoN(3, jd, n)
|
||||
return bo
|
||||
}
|
||||
|
||||
// MarsApparentLoBoN 火星视黄经黄纬（截断版） / truncated apparent ecliptic longitude and latitude of Mars.
|
||||
// MarsApparentLoBoN 火星视黄经黄纬（n 变体） / n-parameterised apparent ecliptic longitude and latitude of Mars.
|
||||
func MarsApparentLoBoN(jd float64, n int) (float64, float64) {
|
||||
return planetApparentLoBoN(3, jd, n)
|
||||
}
|
||||
|
||||
// MarsApparentRaN 火星视赤经（截断版） / truncated apparent right ascension of Mars.
|
||||
// MarsApparentRaN 火星视赤经（n 变体） / n-parameterised apparent right ascension of Mars.
|
||||
func MarsApparentRaN(jd float64, n int) float64 {
|
||||
return planetApparentRaManualN(3, jd, n)
|
||||
}
|
||||
|
||||
// MarsApparentDecN 火星视赤纬（截断版） / truncated apparent declination of Mars.
|
||||
// MarsApparentDecN 火星视赤纬（n 变体） / n-parameterised apparent declination of Mars.
|
||||
func MarsApparentDecN(jd float64, n int) float64 {
|
||||
return planetApparentDecManualN(3, jd, n)
|
||||
}
|
||||
|
||||
// MarsApparentRaDecN 火星视赤经赤纬（截断版） / truncated apparent right ascension and declination of Mars.
|
||||
// MarsApparentRaDecN 火星视赤经赤纬（n 变体） / n-parameterised apparent right ascension and declination of Mars.
|
||||
func MarsApparentRaDecN(jd float64, n int) (float64, float64) {
|
||||
return planetApparentRaDecManualN(3, jd, n)
|
||||
}
|
||||
|
||||
// EarthMarsAwayN 地火距离（截断版） / truncated Earth-Mars distance.
|
||||
// EarthMarsAwayN 地火距离（n 变体） / n-parameterised Earth-Mars distance.
|
||||
func EarthMarsAwayN(jd float64, n int) float64 {
|
||||
return planetEarthAwayN(3, jd, n)
|
||||
}
|
||||
|
||||
// MarsMagN 火星视星等（截断版） / truncated apparent magnitude of Mars.
|
||||
func MarsMagN(jde float64, n int) float64 {
|
||||
awaySun := planet.WherePlanetN(3, 2, jde, n)
|
||||
awayEarth := EarthMarsAwayN(jde, n)
|
||||
away := planet.WherePlanetN(-1, 2, jde, n)
|
||||
// MarsMagNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func MarsMagNWithInstance(jde float64, n int, inst *Instance) float64 {
|
||||
awaySun := PlanetCoordinateNWithInstance(3, 2, jde, n, inst)
|
||||
awayEarth := EarthMarsAwayNWithInstance(jde, n, inst)
|
||||
away := PlanetCoordinateNWithInstance(-1, 2, jde, n, inst)
|
||||
i := (awaySun*awaySun + awayEarth*awayEarth - away*away) / (2 * awaySun * awayEarth)
|
||||
i = ArcCos(i)
|
||||
mag := -1.52 + 5*math.Log10(awaySun*awayEarth) + 0.016*i
|
||||
return FloatRound(mag, 2)
|
||||
}
|
||||
|
||||
// MarsHeightN 火星高度角（截断版） / truncated altitude of Mars.
|
||||
func MarsHeightN(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return planetHeightN(localJD, lon, lat, timezone, n, MarsApparentRaDecN)
|
||||
// MarsHeightNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func MarsHeightNWithInstance(localJD, lon, lat, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetHeightN(3, localJD, lon, lat, timezone, n, inst)
|
||||
}
|
||||
|
||||
// MarsAzimuthN 火星方位角（截断版） / truncated azimuth of Mars.
|
||||
func MarsAzimuthN(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return planetAzimuthN(localJD, lon, lat, timezone, n, MarsApparentRaDecN)
|
||||
// MarsAzimuthNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func MarsAzimuthNWithInstance(localJD, lon, lat, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetAzimuthN(3, localJD, lon, lat, timezone, n, inst)
|
||||
}
|
||||
|
||||
// MarsHourAngleN 火星时角（截断版） / truncated hour angle of Mars.
|
||||
func MarsHourAngleN(jd, lon, timezone float64, n int) float64 {
|
||||
return planetHourAngleN(jd, lon, timezone, n, MarsApparentRaN)
|
||||
// MarsHourAngleNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func MarsHourAngleNWithInstance(jd, lon, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetHourAngleN(jd, lon, timezone, n, func(jd float64, n int) float64 { return MarsApparentRaNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// MarsCulminationTimeN 火星中天时间（截断版） / truncated culmination time of Mars.
|
||||
func MarsCulminationTimeN(localJD, lon, timezone float64, n int) float64 {
|
||||
return planetCulminationTimeN(localJD, lon, timezone, n, MarsHourAngleN)
|
||||
// MarsCulminationTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func MarsCulminationTimeNWithInstance(localJD, lon, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetCulminationTimeN(localJD, lon, timezone, n, func(jd, lon, timezone float64, n int) float64 {
|
||||
return MarsHourAngleNWithInstance(jd, lon, timezone, n, inst)
|
||||
})
|
||||
}
|
||||
|
||||
// MarsRiseTimeN 火星升起时间（截断版） / truncated rise time of Mars.
|
||||
func MarsRiseTimeN(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, true, n, MarsCulminationTimeN, MarsHeightN, MarsApparentDecN)
|
||||
// MarsRiseTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func MarsRiseTimeNWithInstance(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int, inst *Instance) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, true, n, func(localJD, lon, timezone float64, n int) float64 {
|
||||
return MarsCulminationTimeNWithInstance(localJD, lon, timezone, n, inst)
|
||||
}, func(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return MarsHeightNWithInstance(localJD, lon, lat, timezone, n, inst)
|
||||
}, func(jd float64, n int) float64 { return MarsApparentDecNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// MarsSetTimeN 火星落下时间（截断版） / truncated set time of Mars.
|
||||
func MarsSetTimeN(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, false, n, MarsCulminationTimeN, MarsHeightN, MarsApparentDecN)
|
||||
// MarsSetTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func MarsSetTimeNWithInstance(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int, inst *Instance) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, false, n, func(localJD, lon, timezone float64, n int) float64 {
|
||||
return MarsCulminationTimeNWithInstance(localJD, lon, timezone, n, inst)
|
||||
}, func(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return MarsHeightNWithInstance(localJD, lon, lat, timezone, n, inst)
|
||||
}, func(jd float64, n int) float64 { return MarsApparentDecNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// JupiterApparentLoN 木星视黄经（截断版） / truncated apparent ecliptic longitude of Jupiter.
|
||||
// JupiterApparentLoN 木星视黄经（n 变体） / n-parameterised apparent ecliptic longitude of Jupiter.
|
||||
func JupiterApparentLoN(jd float64, n int) float64 {
|
||||
lo, _ := planetApparentLoBoN(4, jd, n)
|
||||
return lo
|
||||
}
|
||||
|
||||
// JupiterApparentBoN 木星视黄纬（截断版） / truncated apparent ecliptic latitude of Jupiter.
|
||||
// JupiterApparentBoN 木星视黄纬（n 变体） / n-parameterised apparent ecliptic latitude of Jupiter.
|
||||
func JupiterApparentBoN(jd float64, n int) float64 {
|
||||
_, bo := planetApparentLoBoN(4, jd, n)
|
||||
return bo
|
||||
}
|
||||
|
||||
// JupiterApparentLoBoN 木星视黄经黄纬（截断版） / truncated apparent ecliptic longitude and latitude of Jupiter.
|
||||
// JupiterApparentLoBoN 木星视黄经黄纬（n 变体） / n-parameterised apparent ecliptic longitude and latitude of Jupiter.
|
||||
func JupiterApparentLoBoN(jd float64, n int) (float64, float64) {
|
||||
return planetApparentLoBoN(4, jd, n)
|
||||
}
|
||||
|
||||
// JupiterApparentRaN 木星视赤经（截断版） / truncated apparent right ascension of Jupiter.
|
||||
// JupiterApparentRaN 木星视赤经（n 变体） / n-parameterised apparent right ascension of Jupiter.
|
||||
func JupiterApparentRaN(jd float64, n int) float64 {
|
||||
return planetApparentRaManualN(4, jd, n)
|
||||
}
|
||||
|
||||
// JupiterApparentDecN 木星视赤纬（截断版） / truncated apparent declination of Jupiter.
|
||||
// JupiterApparentDecN 木星视赤纬（n 变体） / n-parameterised apparent declination of Jupiter.
|
||||
func JupiterApparentDecN(jd float64, n int) float64 {
|
||||
return planetApparentDecManualN(4, jd, n)
|
||||
}
|
||||
|
||||
// JupiterApparentRaDecN 木星视赤经赤纬（截断版） / truncated apparent right ascension and declination of Jupiter.
|
||||
// JupiterApparentRaDecN 木星视赤经赤纬（n 变体） / n-parameterised apparent right ascension and declination of Jupiter.
|
||||
func JupiterApparentRaDecN(jd float64, n int) (float64, float64) {
|
||||
return planetApparentRaDecManualN(4, jd, n)
|
||||
}
|
||||
|
||||
// EarthJupiterAwayN 地木距离（截断版） / truncated Earth-Jupiter distance.
|
||||
// EarthJupiterAwayN 地木距离（n 变体） / n-parameterised Earth-Jupiter distance.
|
||||
func EarthJupiterAwayN(jd float64, n int) float64 {
|
||||
return planetEarthAwayN(4, jd, n)
|
||||
}
|
||||
|
||||
// JupiterMagN 木星视星等（截断版） / truncated apparent magnitude of Jupiter.
|
||||
func JupiterMagN(jde float64, n int) float64 {
|
||||
awaySun := planet.WherePlanetN(4, 2, jde, n)
|
||||
awayEarth := EarthJupiterAwayN(jde, n)
|
||||
away := planet.WherePlanetN(-1, 2, jde, n)
|
||||
// JupiterMagNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func JupiterMagNWithInstance(jde float64, n int, inst *Instance) float64 {
|
||||
awaySun := PlanetCoordinateNWithInstance(4, 2, jde, n, inst)
|
||||
awayEarth := EarthJupiterAwayNWithInstance(jde, n, inst)
|
||||
away := PlanetCoordinateNWithInstance(-1, 2, jde, n, inst)
|
||||
i := (awaySun*awaySun + awayEarth*awayEarth - away*away) / (2 * awaySun * awayEarth)
|
||||
i = ArcCos(i)
|
||||
mag := -9.40 + 5*math.Log10(awaySun*awayEarth) + 0.0005*i
|
||||
return FloatRound(mag, 2)
|
||||
}
|
||||
|
||||
// JupiterHeightN 木星高度角（截断版） / truncated altitude of Jupiter.
|
||||
func JupiterHeightN(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return planetHeightN(localJD, lon, lat, timezone, n, JupiterApparentRaDecN)
|
||||
// JupiterHeightNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func JupiterHeightNWithInstance(localJD, lon, lat, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetHeightN(4, localJD, lon, lat, timezone, n, inst)
|
||||
}
|
||||
|
||||
// JupiterAzimuthN 木星方位角（截断版） / truncated azimuth of Jupiter.
|
||||
func JupiterAzimuthN(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return planetAzimuthN(localJD, lon, lat, timezone, n, JupiterApparentRaDecN)
|
||||
// JupiterAzimuthNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func JupiterAzimuthNWithInstance(localJD, lon, lat, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetAzimuthN(4, localJD, lon, lat, timezone, n, inst)
|
||||
}
|
||||
|
||||
// JupiterHourAngleN 木星时角（截断版） / truncated hour angle of Jupiter.
|
||||
func JupiterHourAngleN(jd, lon, timezone float64, n int) float64 {
|
||||
return planetHourAngleN(jd, lon, timezone, n, JupiterApparentRaN)
|
||||
// JupiterHourAngleNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func JupiterHourAngleNWithInstance(jd, lon, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetHourAngleN(jd, lon, timezone, n, func(jd float64, n int) float64 { return JupiterApparentRaNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// JupiterCulminationTimeN 木星中天时间（截断版） / truncated culmination time of Jupiter.
|
||||
func JupiterCulminationTimeN(localJD, lon, timezone float64, n int) float64 {
|
||||
return planetCulminationTimeN(localJD, lon, timezone, n, JupiterHourAngleN)
|
||||
// JupiterCulminationTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func JupiterCulminationTimeNWithInstance(localJD, lon, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetCulminationTimeN(localJD, lon, timezone, n, func(jd, lon, timezone float64, n int) float64 {
|
||||
return JupiterHourAngleNWithInstance(jd, lon, timezone, n, inst)
|
||||
})
|
||||
}
|
||||
|
||||
// JupiterRiseTimeN 木星升起时间（截断版） / truncated rise time of Jupiter.
|
||||
func JupiterRiseTimeN(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, true, n, JupiterCulminationTimeN, JupiterHeightN, JupiterApparentDecN)
|
||||
// JupiterRiseTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func JupiterRiseTimeNWithInstance(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int, inst *Instance) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, true, n, func(localJD, lon, timezone float64, n int) float64 {
|
||||
return JupiterCulminationTimeNWithInstance(localJD, lon, timezone, n, inst)
|
||||
}, func(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return JupiterHeightNWithInstance(localJD, lon, lat, timezone, n, inst)
|
||||
}, func(jd float64, n int) float64 { return JupiterApparentDecNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// JupiterSetTimeN 木星落下时间（截断版） / truncated set time of Jupiter.
|
||||
func JupiterSetTimeN(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, false, n, JupiterCulminationTimeN, JupiterHeightN, JupiterApparentDecN)
|
||||
// JupiterSetTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func JupiterSetTimeNWithInstance(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int, inst *Instance) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, false, n, func(localJD, lon, timezone float64, n int) float64 {
|
||||
return JupiterCulminationTimeNWithInstance(localJD, lon, timezone, n, inst)
|
||||
}, func(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return JupiterHeightNWithInstance(localJD, lon, lat, timezone, n, inst)
|
||||
}, func(jd float64, n int) float64 { return JupiterApparentDecNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// SaturnApparentLoN 土星视黄经（截断版） / truncated apparent ecliptic longitude of Saturn.
|
||||
// SaturnApparentLoN 土星视黄经（n 变体） / n-parameterised apparent ecliptic longitude of Saturn.
|
||||
func SaturnApparentLoN(jd float64, n int) float64 {
|
||||
lo, _ := planetApparentLoBoN(5, jd, n)
|
||||
return lo
|
||||
}
|
||||
|
||||
// SaturnApparentBoN 土星视黄纬（截断版） / truncated apparent ecliptic latitude of Saturn.
|
||||
// SaturnApparentBoN 土星视黄纬（n 变体） / n-parameterised apparent ecliptic latitude of Saturn.
|
||||
func SaturnApparentBoN(jd float64, n int) float64 {
|
||||
_, bo := planetApparentLoBoN(5, jd, n)
|
||||
return bo
|
||||
}
|
||||
|
||||
// SaturnApparentLoBoN 土星视黄经黄纬（截断版） / truncated apparent ecliptic longitude and latitude of Saturn.
|
||||
// SaturnApparentLoBoN 土星视黄经黄纬（n 变体） / n-parameterised apparent ecliptic longitude and latitude of Saturn.
|
||||
func SaturnApparentLoBoN(jd float64, n int) (float64, float64) {
|
||||
return planetApparentLoBoN(5, jd, n)
|
||||
}
|
||||
|
||||
// SaturnApparentRaN 土星视赤经（截断版） / truncated apparent right ascension of Saturn.
|
||||
// SaturnApparentRaN 土星视赤经（n 变体） / n-parameterised apparent right ascension of Saturn.
|
||||
func SaturnApparentRaN(jd float64, n int) float64 {
|
||||
return planetApparentRaManualN(5, jd, n)
|
||||
}
|
||||
|
||||
// SaturnApparentDecN 土星视赤纬（截断版） / truncated apparent declination of Saturn.
|
||||
// SaturnApparentDecN 土星视赤纬（n 变体） / n-parameterised apparent declination of Saturn.
|
||||
func SaturnApparentDecN(jd float64, n int) float64 {
|
||||
return planetApparentDecManualN(5, jd, n)
|
||||
}
|
||||
|
||||
// SaturnApparentRaDecN 土星视赤经赤纬（截断版） / truncated apparent right ascension and declination of Saturn.
|
||||
// SaturnApparentRaDecN 土星视赤经赤纬（n 变体） / n-parameterised apparent right ascension and declination of Saturn.
|
||||
func SaturnApparentRaDecN(jd float64, n int) (float64, float64) {
|
||||
return planetApparentRaDecManualN(5, jd, n)
|
||||
}
|
||||
|
||||
// EarthSaturnAwayN 地土距离（截断版） / truncated Earth-Saturn distance.
|
||||
// EarthSaturnAwayN 地土距离（n 变体） / n-parameterised Earth-Saturn distance.
|
||||
func EarthSaturnAwayN(jd float64, n int) float64 {
|
||||
return planetEarthAwayN(5, jd, n)
|
||||
}
|
||||
|
||||
// SaturnMagN 土星视星等（截断版） / truncated apparent magnitude of Saturn.
|
||||
func SaturnMagN(jde float64, n int) float64 {
|
||||
awaySun := planet.WherePlanetN(5, 2, jde, n)
|
||||
awayEarth := EarthSaturnAwayN(jde, n)
|
||||
ringB, _, _, deltaU, _, _ := SaturnRingParametersN(jde, n)
|
||||
// SaturnMagNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func SaturnMagNWithInstance(jde float64, n int, inst *Instance) float64 {
|
||||
awaySun := PlanetCoordinateNWithInstance(5, 2, jde, n, inst)
|
||||
awayEarth := EarthSaturnAwayNWithInstance(jde, n, inst)
|
||||
ringB, _, _, deltaU, _, _ := SaturnRingParametersNWithInstance(jde, n, inst)
|
||||
ringB = math.Abs(ringB)
|
||||
mag := -8.68 + 5*math.Log10(awaySun*awayEarth) + 0.044*deltaU - 2.6*Sin(ringB) + 1.25*Sin(ringB)*Sin(ringB)
|
||||
return FloatRound(mag, 2)
|
||||
}
|
||||
|
||||
// SaturnHeightN 土星高度角（截断版） / truncated altitude of Saturn.
|
||||
func SaturnHeightN(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return planetHeightN(localJD, lon, lat, timezone, n, SaturnApparentRaDecN)
|
||||
// SaturnHeightNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func SaturnHeightNWithInstance(localJD, lon, lat, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetHeightN(5, localJD, lon, lat, timezone, n, inst)
|
||||
}
|
||||
|
||||
// SaturnAzimuthN 土星方位角（截断版） / truncated azimuth of Saturn.
|
||||
func SaturnAzimuthN(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return planetAzimuthN(localJD, lon, lat, timezone, n, SaturnApparentRaDecN)
|
||||
// SaturnAzimuthNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func SaturnAzimuthNWithInstance(localJD, lon, lat, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetAzimuthN(5, localJD, lon, lat, timezone, n, inst)
|
||||
}
|
||||
|
||||
// SaturnHourAngleN 土星时角（截断版） / truncated hour angle of Saturn.
|
||||
func SaturnHourAngleN(jd, lon, timezone float64, n int) float64 {
|
||||
return planetHourAngleN(jd, lon, timezone, n, SaturnApparentRaN)
|
||||
// SaturnHourAngleNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func SaturnHourAngleNWithInstance(jd, lon, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetHourAngleN(jd, lon, timezone, n, func(jd float64, n int) float64 { return SaturnApparentRaNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// SaturnCulminationTimeN 土星中天时间（截断版） / truncated culmination time of Saturn.
|
||||
func SaturnCulminationTimeN(localJD, lon, timezone float64, n int) float64 {
|
||||
return planetCulminationTimeN(localJD, lon, timezone, n, SaturnHourAngleN)
|
||||
// SaturnCulminationTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func SaturnCulminationTimeNWithInstance(localJD, lon, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetCulminationTimeN(localJD, lon, timezone, n, func(jd, lon, timezone float64, n int) float64 {
|
||||
return SaturnHourAngleNWithInstance(jd, lon, timezone, n, inst)
|
||||
})
|
||||
}
|
||||
|
||||
// SaturnRiseTimeN 土星升起时间（截断版） / truncated rise time of Saturn.
|
||||
func SaturnRiseTimeN(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, true, n, SaturnCulminationTimeN, SaturnHeightN, SaturnApparentDecN)
|
||||
// SaturnRiseTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func SaturnRiseTimeNWithInstance(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int, inst *Instance) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, true, n, func(localJD, lon, timezone float64, n int) float64 {
|
||||
return SaturnCulminationTimeNWithInstance(localJD, lon, timezone, n, inst)
|
||||
}, func(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return SaturnHeightNWithInstance(localJD, lon, lat, timezone, n, inst)
|
||||
}, func(jd float64, n int) float64 { return SaturnApparentDecNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// SaturnSetTimeN 土星落下时间（截断版） / truncated set time of Saturn.
|
||||
func SaturnSetTimeN(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, false, n, SaturnCulminationTimeN, SaturnHeightN, SaturnApparentDecN)
|
||||
// SaturnSetTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func SaturnSetTimeNWithInstance(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int, inst *Instance) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, false, n, func(localJD, lon, timezone float64, n int) float64 {
|
||||
return SaturnCulminationTimeNWithInstance(localJD, lon, timezone, n, inst)
|
||||
}, func(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return SaturnHeightNWithInstance(localJD, lon, lat, timezone, n, inst)
|
||||
}, func(jd float64, n int) float64 { return SaturnApparentDecNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// UranusApparentLoN 天王星视黄经（截断版） / truncated apparent ecliptic longitude of Uranus.
|
||||
// UranusApparentLoN 天王星视黄经（n 变体） / n-parameterised apparent ecliptic longitude of Uranus.
|
||||
func UranusApparentLoN(jd float64, n int) float64 {
|
||||
lo, _ := planetApparentLoBoN(6, jd, n)
|
||||
return lo
|
||||
}
|
||||
|
||||
// UranusApparentBoN 天王星视黄纬（截断版） / truncated apparent ecliptic latitude of Uranus.
|
||||
// UranusApparentBoN 天王星视黄纬（n 变体） / n-parameterised apparent ecliptic latitude of Uranus.
|
||||
func UranusApparentBoN(jd float64, n int) float64 {
|
||||
_, bo := planetApparentLoBoN(6, jd, n)
|
||||
return bo
|
||||
}
|
||||
|
||||
// UranusApparentLoBoN 天王星视黄经黄纬（截断版） / truncated apparent ecliptic longitude and latitude of Uranus.
|
||||
// UranusApparentLoBoN 天王星视黄经黄纬（n 变体） / n-parameterised apparent ecliptic longitude and latitude of Uranus.
|
||||
func UranusApparentLoBoN(jd float64, n int) (float64, float64) {
|
||||
return planetApparentLoBoN(6, jd, n)
|
||||
}
|
||||
|
||||
// UranusApparentRaN 天王星视赤经（截断版） / truncated apparent right ascension of Uranus.
|
||||
// UranusApparentRaN 天王星视赤经（n 变体） / n-parameterised apparent right ascension of Uranus.
|
||||
func UranusApparentRaN(jd float64, n int) float64 {
|
||||
return planetApparentRaManualN(6, jd, n)
|
||||
}
|
||||
|
||||
// UranusApparentDecN 天王星视赤纬（截断版） / truncated apparent declination of Uranus.
|
||||
// UranusApparentDecN 天王星视赤纬（n 变体） / n-parameterised apparent declination of Uranus.
|
||||
func UranusApparentDecN(jd float64, n int) float64 {
|
||||
return planetApparentDecManualN(6, jd, n)
|
||||
}
|
||||
|
||||
// UranusApparentRaDecN 天王星视赤经赤纬（截断版） / truncated apparent right ascension and declination of Uranus.
|
||||
// UranusApparentRaDecN 天王星视赤经赤纬（n 变体） / n-parameterised apparent right ascension and declination of Uranus.
|
||||
func UranusApparentRaDecN(jd float64, n int) (float64, float64) {
|
||||
return planetApparentRaDecManualN(6, jd, n)
|
||||
}
|
||||
|
||||
// EarthUranusAwayN 地天距离（截断版） / truncated Earth-Uranus distance.
|
||||
// EarthUranusAwayN 地天距离（n 变体） / n-parameterised Earth-Uranus distance.
|
||||
func EarthUranusAwayN(jd float64, n int) float64 {
|
||||
return planetEarthAwayN(6, jd, n)
|
||||
}
|
||||
|
||||
// UranusMagN 天王星视星等（截断版） / truncated apparent magnitude of Uranus.
|
||||
func UranusMagN(jde float64, n int) float64 {
|
||||
awaySun := planet.WherePlanetN(6, 2, jde, n)
|
||||
awayEarth := EarthUranusAwayN(jde, n)
|
||||
away := planet.WherePlanetN(-1, 2, jde, n)
|
||||
// UranusMagNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func UranusMagNWithInstance(jde float64, n int, inst *Instance) float64 {
|
||||
awaySun := PlanetCoordinateNWithInstance(6, 2, jde, n, inst)
|
||||
awayEarth := EarthUranusAwayNWithInstance(jde, n, inst)
|
||||
away := PlanetCoordinateNWithInstance(-1, 2, jde, n, inst)
|
||||
i := (awaySun*awaySun + awayEarth*awayEarth - away*away) / (2 * awaySun * awayEarth)
|
||||
i = ArcCos(i)
|
||||
mag := -7.19 + 5*math.Log10(awaySun*awayEarth) + 0.016*i
|
||||
return FloatRound(mag, 2)
|
||||
}
|
||||
|
||||
// UranusHeightN 天王星高度角（截断版） / truncated altitude of Uranus.
|
||||
func UranusHeightN(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return planetHeightN(localJD, lon, lat, timezone, n, UranusApparentRaDecN)
|
||||
// UranusHeightNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func UranusHeightNWithInstance(localJD, lon, lat, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetHeightN(6, localJD, lon, lat, timezone, n, inst)
|
||||
}
|
||||
|
||||
// UranusAzimuthN 天王星方位角（截断版） / truncated azimuth of Uranus.
|
||||
func UranusAzimuthN(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return planetAzimuthN(localJD, lon, lat, timezone, n, UranusApparentRaDecN)
|
||||
// UranusAzimuthNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func UranusAzimuthNWithInstance(localJD, lon, lat, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetAzimuthN(6, localJD, lon, lat, timezone, n, inst)
|
||||
}
|
||||
|
||||
// UranusHourAngleN 天王星时角（截断版） / truncated hour angle of Uranus.
|
||||
func UranusHourAngleN(jd, lon, timezone float64, n int) float64 {
|
||||
return planetHourAngleN(jd, lon, timezone, n, UranusApparentRaN)
|
||||
// UranusHourAngleNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func UranusHourAngleNWithInstance(jd, lon, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetHourAngleN(jd, lon, timezone, n, func(jd float64, n int) float64 { return UranusApparentRaNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// UranusCulminationTimeN 天王星中天时间（截断版） / truncated culmination time of Uranus.
|
||||
func UranusCulminationTimeN(localJD, lon, timezone float64, n int) float64 {
|
||||
return planetCulminationTimeN(localJD, lon, timezone, n, UranusHourAngleN)
|
||||
// UranusCulminationTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func UranusCulminationTimeNWithInstance(localJD, lon, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetCulminationTimeN(localJD, lon, timezone, n, func(jd, lon, timezone float64, n int) float64 {
|
||||
return UranusHourAngleNWithInstance(jd, lon, timezone, n, inst)
|
||||
})
|
||||
}
|
||||
|
||||
// UranusRiseTimeN 天王星升起时间（截断版） / truncated rise time of Uranus.
|
||||
func UranusRiseTimeN(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, true, n, UranusCulminationTimeN, UranusHeightN, UranusApparentDecN)
|
||||
// UranusRiseTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func UranusRiseTimeNWithInstance(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int, inst *Instance) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, true, n, func(localJD, lon, timezone float64, n int) float64 {
|
||||
return UranusCulminationTimeNWithInstance(localJD, lon, timezone, n, inst)
|
||||
}, func(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return UranusHeightNWithInstance(localJD, lon, lat, timezone, n, inst)
|
||||
}, func(jd float64, n int) float64 { return UranusApparentDecNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// UranusSetTimeN 天王星落下时间（截断版） / truncated set time of Uranus.
|
||||
func UranusSetTimeN(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, false, n, UranusCulminationTimeN, UranusHeightN, UranusApparentDecN)
|
||||
// UranusSetTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func UranusSetTimeNWithInstance(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int, inst *Instance) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, false, n, func(localJD, lon, timezone float64, n int) float64 {
|
||||
return UranusCulminationTimeNWithInstance(localJD, lon, timezone, n, inst)
|
||||
}, func(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return UranusHeightNWithInstance(localJD, lon, lat, timezone, n, inst)
|
||||
}, func(jd float64, n int) float64 { return UranusApparentDecNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// NeptuneApparentLoN 海王星视黄经（截断版） / truncated apparent ecliptic longitude of Neptune.
|
||||
// NeptuneApparentLoN 海王星视黄经（n 变体） / n-parameterised apparent ecliptic longitude of Neptune.
|
||||
func NeptuneApparentLoN(jd float64, n int) float64 {
|
||||
lo, _ := planetApparentLoBoN(7, jd, n)
|
||||
return lo
|
||||
}
|
||||
|
||||
// NeptuneApparentBoN 海王星视黄纬（截断版） / truncated apparent ecliptic latitude of Neptune.
|
||||
// NeptuneApparentBoN 海王星视黄纬（n 变体） / n-parameterised apparent ecliptic latitude of Neptune.
|
||||
func NeptuneApparentBoN(jd float64, n int) float64 {
|
||||
_, bo := planetApparentLoBoN(7, jd, n)
|
||||
return bo
|
||||
}
|
||||
|
||||
// NeptuneApparentLoBoN 海王星视黄经黄纬（截断版） / truncated apparent ecliptic longitude and latitude of Neptune.
|
||||
// NeptuneApparentLoBoN 海王星视黄经黄纬（n 变体） / n-parameterised apparent ecliptic longitude and latitude of Neptune.
|
||||
func NeptuneApparentLoBoN(jd float64, n int) (float64, float64) {
|
||||
return planetApparentLoBoN(7, jd, n)
|
||||
}
|
||||
|
||||
// NeptuneApparentRaN 海王星视赤经（截断版） / truncated apparent right ascension of Neptune.
|
||||
// NeptuneApparentRaN 海王星视赤经（n 变体） / n-parameterised apparent right ascension of Neptune.
|
||||
func NeptuneApparentRaN(jd float64, n int) float64 {
|
||||
return planetApparentRaManualN(7, jd, n)
|
||||
}
|
||||
|
||||
// NeptuneApparentDecN 海王星视赤纬（截断版） / truncated apparent declination of Neptune.
|
||||
// NeptuneApparentDecN 海王星视赤纬（n 变体） / n-parameterised apparent declination of Neptune.
|
||||
func NeptuneApparentDecN(jd float64, n int) float64 {
|
||||
return planetApparentDecManualN(7, jd, n)
|
||||
}
|
||||
|
||||
// NeptuneApparentRaDecN 海王星视赤经赤纬（截断版） / truncated apparent right ascension and declination of Neptune.
|
||||
// NeptuneApparentRaDecN 海王星视赤经赤纬（n 变体） / n-parameterised apparent right ascension and declination of Neptune.
|
||||
func NeptuneApparentRaDecN(jd float64, n int) (float64, float64) {
|
||||
return planetApparentRaDecManualN(7, jd, n)
|
||||
}
|
||||
|
||||
// EarthNeptuneAwayN 地海距离（截断版） / truncated Earth-Neptune distance.
|
||||
// EarthNeptuneAwayN 地海距离（n 变体） / n-parameterised Earth-Neptune distance.
|
||||
func EarthNeptuneAwayN(jd float64, n int) float64 {
|
||||
return planetEarthAwayN(7, jd, n)
|
||||
}
|
||||
|
||||
// NeptuneMagN 海王星视星等（截断版） / truncated apparent magnitude of Neptune.
|
||||
func NeptuneMagN(jde float64, n int) float64 {
|
||||
awaySun := planet.WherePlanetN(7, 2, jde, n)
|
||||
awayEarth := EarthNeptuneAwayN(jde, n)
|
||||
// NeptuneMagNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func NeptuneMagNWithInstance(jde float64, n int, inst *Instance) float64 {
|
||||
awaySun := PlanetCoordinateNWithInstance(7, 2, jde, n, inst)
|
||||
awayEarth := EarthNeptuneAwayNWithInstance(jde, n, inst)
|
||||
mag := -6.87 + 5*math.Log10(awaySun*awayEarth)
|
||||
return FloatRound(mag, 2)
|
||||
}
|
||||
|
||||
// NeptuneHeightN 海王星高度角（截断版） / truncated altitude of Neptune.
|
||||
func NeptuneHeightN(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return planetHeightN(localJD, lon, lat, timezone, n, NeptuneApparentRaDecN)
|
||||
// NeptuneHeightNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func NeptuneHeightNWithInstance(localJD, lon, lat, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetHeightN(7, localJD, lon, lat, timezone, n, inst)
|
||||
}
|
||||
|
||||
// NeptuneAzimuthN 海王星方位角（截断版） / truncated azimuth of Neptune.
|
||||
func NeptuneAzimuthN(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return planetAzimuthN(localJD, lon, lat, timezone, n, NeptuneApparentRaDecN)
|
||||
// NeptuneAzimuthNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func NeptuneAzimuthNWithInstance(localJD, lon, lat, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetAzimuthN(7, localJD, lon, lat, timezone, n, inst)
|
||||
}
|
||||
|
||||
// NeptuneHourAngleN 海王星时角（截断版） / truncated hour angle of Neptune.
|
||||
func NeptuneHourAngleN(jd, lon, timezone float64, n int) float64 {
|
||||
return planetHourAngleN(jd, lon, timezone, n, NeptuneApparentRaN)
|
||||
// NeptuneHourAngleNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func NeptuneHourAngleNWithInstance(jd, lon, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetHourAngleN(jd, lon, timezone, n, func(jd float64, n int) float64 { return NeptuneApparentRaNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// NeptuneCulminationTimeN 海王星中天时间（截断版） / truncated culmination time of Neptune.
|
||||
func NeptuneCulminationTimeN(localJD, lon, timezone float64, n int) float64 {
|
||||
return planetCulminationTimeN(localJD, lon, timezone, n, NeptuneHourAngleN)
|
||||
// NeptuneCulminationTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func NeptuneCulminationTimeNWithInstance(localJD, lon, timezone float64, n int, inst *Instance) float64 {
|
||||
return planetCulminationTimeN(localJD, lon, timezone, n, func(jd, lon, timezone float64, n int) float64 {
|
||||
return NeptuneHourAngleNWithInstance(jd, lon, timezone, n, inst)
|
||||
})
|
||||
}
|
||||
|
||||
// NeptuneRiseTimeN 海王星升起时间（截断版） / truncated rise time of Neptune.
|
||||
func NeptuneRiseTimeN(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, true, n, NeptuneCulminationTimeN, NeptuneHeightN, NeptuneApparentDecN)
|
||||
// NeptuneRiseTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func NeptuneRiseTimeNWithInstance(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int, inst *Instance) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, true, n, func(localJD, lon, timezone float64, n int) float64 {
|
||||
return NeptuneCulminationTimeNWithInstance(localJD, lon, timezone, n, inst)
|
||||
}, func(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return NeptuneHeightNWithInstance(localJD, lon, lat, timezone, n, inst)
|
||||
}, func(jd float64, n int) float64 { return NeptuneApparentDecNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
// NeptuneSetTimeN 海王星落下时间（截断版） / truncated set time of Neptune.
|
||||
func NeptuneSetTimeN(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, false, n, NeptuneCulminationTimeN, NeptuneHeightN, NeptuneApparentDecN)
|
||||
// NeptuneSetTimeNWithInstance 用指定星历实例求值；inst 为 nil 时用进程当前模型 / evaluation with an explicit instance; nil uses the process model.
|
||||
func NeptuneSetTimeNWithInstance(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, n int, inst *Instance) (float64, error) {
|
||||
return planetRiseDownN(jd, lon, lat, timezone, aeroCorrection, observerHeight, false, n, func(localJD, lon, timezone float64, n int) float64 {
|
||||
return NeptuneCulminationTimeNWithInstance(localJD, lon, timezone, n, inst)
|
||||
}, func(localJD, lon, lat, timezone float64, n int) float64 {
|
||||
return NeptuneHeightNWithInstance(localJD, lon, lat, timezone, n, inst)
|
||||
}, func(jd float64, n int) float64 { return NeptuneApparentDecNWithInstance(jd, n, inst) })
|
||||
}
|
||||
|
||||
Reference in New Issue
Block a user