b612
ccf5880269
- 基于平均下合周期与节点相位预筛候选，减少无效星历计算；跳过无法求解的单个会合周期，避免有限覆盖星历导致搜索提前终止 - 引入影轴 γ、半影半径及地球尺度几何判定，结合站心可见性识别地心无接触、仅部分地区可见的掠凌 - 添加金星 243 年、水星 46 年周期族编号，并明确编号适用范围及未分配时的零值语义 - 为 SVG、GeoJSON 和 KML 增加站心部分凌日可见区，适配接触等时线、几何元数据、图层样式及取景；为地心无接触凌日事件增加正射图，按可见区球面面积加权居中
68 lines
2.7 KiB
Go
68 lines
2.7 KiB
Go
package basic
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import "math"
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const (
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planetTransitEarthRadiusKM = 6378.137
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planetTransitEarthEccentricitySquared = 0.00669437999014
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)
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func planetTransitShadowGeometry(tt float64, cfg planetTransitConfig, inst *Instance) (float64, float64, Observer, bool) {
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sunRA, sunDec := HSunApparentRaDecNWithInstance(tt, -1, inst)
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planetRA, planetDec := cfg.apparentRaDecN(tt, -1)
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sunDistance := EarthAwayNWithInstance(tt, -1, inst) * angularDiameterAstronomicalUnitKM
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planetDistance := cfg.earthDistanceN(tt, -1) * angularDiameterAstronomicalUnitKM
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sun := eclipticCartesian(sunRA, sunDec, sunDistance)
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body := eclipticCartesian(planetRA, planetDec, planetDistance)
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axis, length := pn(Vector3{body[0] - sun[0], body[1] - sun[1], body[2] - sun[2]})
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projection := -(body[0]*axis[0] + body[1]*axis[1] + body[2]*axis[2])
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impact := Vector3{body[0] + projection*axis[0], body[1] + projection*axis[1], body[2] + projection*axis[2]}
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_, distance := pn(impact)
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planetRadius := venusEquatorialRadiusKM
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if cfg.planetIndex == 1 {
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planetRadius = mercuryEquatorialRadiusKM
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}
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sine := (sunEquatorialRadiusKM + planetRadius) / length
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cosine := math.Sqrt(1 - sine*sine)
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penumbra := (planetRadius + projection*sine) / cosine / planetTransitEarthRadiusKM
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gamma := math.Copysign(distance/planetTransitEarthRadiusKM, impact[2])
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sidereal := ApparentSiderealTime(TT2UT1(tt)) * 15
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seed := Observer{
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Longitude: normalizeLongitude180(math.Atan2(impact[1], impact[0])*180/math.Pi - sidereal),
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Latitude: math.Atan2(impact[2], math.Hypot(impact[0], impact[1])*(1-planetTransitEarthEccentricitySquared)) * 180 / math.Pi,
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}
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possible := isFiniteFloat(gamma) && isFiniteFloat(penumbra) && projection > 0 && planetDistance < sunDistance && math.Abs(gamma) <= penumbra+1/cosine
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return gamma, penumbra, seed, possible
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}
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func planetTransitSurfaceOverlap(transit PlanetTransitResult, seed Observer, inst *Instance) bool {
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snapshot, ok := buildPlanetTransitSnapshot(transit, inst)
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if !ok {
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return false
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}
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best := math.Inf(1)
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for step := 4.0; step > 0.0001; step /= 2 {
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center := seed
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for _, latitudeStep := range []float64{-step, 0, step} {
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for _, longitudeStep := range []float64{-step, 0, step} {
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observer := Observer{Longitude: normalizeLongitude180(center.Longitude + longitudeStep), Latitude: math.Max(-90, math.Min(90, center.Latitude+latitudeStep))}
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tt, valid := snapshot.localGreatestTT(UTC2TT(transit.Greatest), observer)
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state, stateOK := snapshot.stateAt(tt, observer)
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if !valid || !stateOK {
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continue
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}
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if state.external < 0 {
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local := snapshot.local(transit, observer)
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if local.Valid && local.Visible {
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return true
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}
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}
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if state.external < best {
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best, seed = state.external, observer
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}
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}
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}
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}
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return false
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}
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