package basic import ( "math" "b612.me/astro/planet" . "b612.me/astro/tools" ) func VenusL(jde float64) float64 { return planet.WherePlanet(2, 0, jde) } func VenusB(jde float64) float64 { return planet.WherePlanet(2, 1, jde) } func VenusR(jde float64) float64 { return planet.WherePlanet(2, 2, jde) } func AVenusX(jde float64) float64 { l := VenusL(jde) b := VenusB(jde) r := VenusR(jde) el := planet.WherePlanet(-1, 0, jde) eb := planet.WherePlanet(-1, 1, jde) er := planet.WherePlanet(-1, 2, jde) x := r*Cos(b)*Cos(l) - er*Cos(eb)*Cos(el) return x } func AVenusY(jde float64) float64 { l := VenusL(jde) b := VenusB(jde) r := VenusR(jde) el := planet.WherePlanet(-1, 0, jde) eb := planet.WherePlanet(-1, 1, jde) er := planet.WherePlanet(-1, 2, jde) y := r*Cos(b)*Sin(l) - er*Cos(eb)*Sin(el) return y } func AVenusZ(jde float64) float64 { //l := VenusL(jde) b := VenusB(jde) r := VenusR(jde) // el := planet.WherePlanet(-1, 0, jde) eb := planet.WherePlanet(-1, 1, jde) er := planet.WherePlanet(-1, 2, jde) z := r*Sin(b) - er*Sin(eb) return z } func AVenusXYZ(jde float64) (float64, float64, float64) { l := VenusL(jde) b := VenusB(jde) r := VenusR(jde) el := planet.WherePlanet(-1, 0, jde) eb := planet.WherePlanet(-1, 1, jde) er := planet.WherePlanet(-1, 2, jde) x := r*Cos(b)*Cos(l) - er*Cos(eb)*Cos(el) y := r*Cos(b)*Sin(l) - er*Cos(eb)*Sin(el) z := r*Sin(b) - er*Sin(eb) return x, y, z } func VenusApparentRa(jde float64) float64 { lo, bo := VenusApparentLoBo(jde) eps := TrueObliquity(jde) ra := math.Atan2((Sin(lo)*Cos(eps) - Tan(bo)*Sin(eps)), Cos(lo)) ra = ra * 180 / math.Pi return Limit360(ra) } func VenusApparentDec(jde float64) float64 { lo, bo := VenusApparentLoBo(jde) eps := TrueObliquity(jde) dec := ArcSin(Sin(bo)*Cos(eps) + Cos(bo)*Sin(eps)*Sin(lo)) return dec } func VenusApparentRaDec(jde float64) (float64, float64) { lo, bo := VenusApparentLoBo(jde) eps := TrueObliquity(jde) ra := math.Atan2((Sin(lo)*Cos(eps) - Tan(bo)*Sin(eps)), Cos(lo)) ra = ra * 180 / math.Pi dec := ArcSin(Sin(bo)*Cos(eps) + Cos(bo)*Sin(eps)*Sin(lo)) return Limit360(ra), dec } func EarthVenusAway(jd float64) float64 { return planetEarthAwayExplicitN(2, jd, -1) } func VenusApparentLo(jd float64) float64 { geo, _ := planetApparentGeocentricPositionN(2, jd, -1) return geo.lo } func VenusApparentBo(jd float64) float64 { geo, _ := planetApparentGeocentricPositionN(2, jd, -1) return geo.bo } func VenusApparentLoBo(jd float64) (float64, float64) { geo, _ := planetApparentGeocentricPositionN(2, jd, -1) return geo.lo, geo.bo } func VenusMag(jde float64) float64 { sunDistance := VenusR(jde) earthDistance := EarthVenusAway(jde) earthSunDistance := planet.WherePlanet(-1, 2, jde) i := (sunDistance*sunDistance + earthDistance*earthDistance - earthSunDistance*earthSunDistance) / (2 * sunDistance * earthDistance) i = ArcCos(i) mag := -4.40 + 5*math.Log10(sunDistance*earthDistance) + 0.0009*i + 0.000239*i*i - 0.00000065*i*i*i return FloatRound(mag, 2) } // VenusHeightWithInstance 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 VenusHeightWithInstance(localJD, lon, lat, timezone float64, inst *Instance) float64 { return planetHeightN(2, localJD, lon, lat, timezone, -1, inst) } // VenusAzimuthWithInstance 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 VenusAzimuthWithInstance(localJD, lon, lat, timezone float64, inst *Instance) float64 { return planetAzimuthN(2, localJD, lon, lat, timezone, -1, inst) } // VenusHourAngleWithInstance 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 VenusHourAngleWithInstance(jd, lon, tz float64, inst *Instance) float64 { startime := Limit360(ApparentSiderealTime(UTC2UT1(jd-tz/24))*15 + lon) timeangle := startime - VenusApparentRaWithInstance(UTC2TT(jd-tz/24.0), inst) if timeangle < 0 { timeangle += 360 } return timeangle } // VenusCulminationTimeWithInstance 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 VenusCulminationTimeWithInstance(localJD, lon, timezone float64, inst *Instance) float64 { // localJD 是本地民用日锚点(当地 0 时),不是力学时。 //ra,dec 瞬时天球座标,非J2000等时间天球坐标 localJD = math.Floor(localJD) + 0.5 estimateJD := localJD + Limit360(360-VenusHourAngleWithInstance(localJD, lon, timezone, inst))/15.0/24.0*0.99726851851851851851 limitHA := func(localJD, lon, timezone float64) float64 { ha := VenusHourAngleWithInstance(localJD, lon, timezone, inst) if ha < 180 { ha += 360 } return ha } var ok bool estimateJD, ok = eventNewtonRefine(estimateJD, 0.00001, func(prevJD float64) float64 { stDegree := limitHA(prevJD, lon, timezone) - 360 stDegreep := (limitHA(prevJD+0.000005, lon, timezone) - limitHA(prevJD-0.000005, lon, timezone)) / 0.00001 return stDegree / stDegreep }) if !ok { return math.NaN() } return estimateJD } // VenusRiseTimeWithInstance 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 VenusRiseTimeWithInstance(jd, lon, lat, tz, aeroCorrection, observerHeight float64, inst *Instance) (float64, error) { return venusRiseDown(jd, lon, lat, tz, aeroCorrection, observerHeight, true, inst) } // VenusSetTimeWithInstance 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 VenusSetTimeWithInstance(jd, lon, lat, tz, aeroCorrection, observerHeight float64, inst *Instance) (float64, error) { return venusRiseDown(jd, lon, lat, tz, aeroCorrection, observerHeight, false, inst) } func venusRiseDown(jd, lon, lat, tz, aeroCorrection, observerHeight float64, isRise bool, instances ...*Instance) (float64, error) { inst := instanceValue(instances) return planetRiseDown(jd, lon, lat, tz, aeroCorrection, observerHeight, isRise, func(localJD, lon, timezone float64) float64 { return VenusCulminationTimeWithInstance(localJD, lon, timezone, inst) }, func(localJD, lon, lat, timezone float64) float64 { return VenusHeightWithInstance(localJD, lon, lat, timezone, inst) }, func(jde float64) float64 { return VenusApparentDecWithInstance(jde, inst) }) }