feat: 完善日月食与月掩几何链路并扩展历法接口
- 新增日月食中心带、偏食带、阴影足迹、等时线、食分线及升落边界计算,支持极区与混合食拓扑 - 新增日食单时刻阴影求解器、站心状态查询、批量采样和 ΔT 覆盖接口 - 重构恒星与行星月掩路径,补充有限盘面接触、站心修正、掩带宽度、极区投影及升落边界 - 扩展 SVG 与 GeoJSON 输出,支持详细面板、全球/极区/地球投影、边界闭合、时间标记和拓扑签名 - 扩展日月食候选搜索、局地搜索、沙罗序列预计算与范围外推,补充系列锚点和成员一致性校验 - 补齐古历纪年、儒略历独有闰日、多公历候选、历法改革跨日及精确日期运算接口 - 优化 ΔT、章动、恒星时、月球地平线、事件根搜索和本地星历缓存,降低重复计算开销并提升边界稳定
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package basic
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import (
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"fmt"
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"math"
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"time"
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)
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// StarOccultationInstant 包含指定时刻的点源恒星月掩可见足迹;若接触锥在该时刻未到达可见地球,Footprint 为 nil。
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// StarOccultationInstant contains the visible point-source footprint at one requested instant; Footprint is nil when no part of the contact cone reaches the visible Earth.
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type StarOccultationInstant struct {
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Time time.Time
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TargetID string
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// DeltaTSeconds 本次实际使用的 ΔT / ΔT actually used.
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DeltaTSeconds float64
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// SublunarLongitude 与 SublunarLatitude 是该时刻月下点,用于声明地平闭合弧 / sublunar point for the horizon closure.
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SublunarLongitude float64
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SublunarLatitude float64
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Footprint *OccultationFootprint
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}
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// PlanetOccultationInstant 包含指定时刻的行星外接触和内接触可见足迹;相应接触锥未到达可见地球时,Partial 或 Total 为 nil。
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// PlanetOccultationInstant contains the visible outer- and inner-contact footprints at one requested instant; Partial or Total is nil when that contact cone does not reach the visible Earth.
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type PlanetOccultationInstant struct {
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Time time.Time
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Planet OccultationPlanet
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TargetID string
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// DeltaTSeconds 本次实际使用的 ΔT / ΔT actually used.
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DeltaTSeconds float64
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// SublunarLongitude 与 SublunarLatitude 是该时刻月下点,用于声明地平闭合弧 / sublunar point for the horizon closure.
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SublunarLongitude float64
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SublunarLatitude float64
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Partial *PlanetOccultationFootprint
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Total *PlanetOccultationFootprint
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}
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// StarOccultationFootprintAt 返回指定时刻的精确点源恒星月掩可见足迹;它采用与路径时间线相同的分辨率,并对完整接触弧执行站心校正。
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// StarOccultationFootprintAt returns the exact visible lunar-occultation footprint of a point-source star at one instant, using timeline resolution and station-centred correction of the complete contact arc.
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func StarOccultationFootprintAt(at time.Time, star StarCoordinate) (StarOccultationInstant, error) {
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result := StarOccultationInstant{Time: at, TargetID: star.ID}
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if at.IsZero() {
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return result, fmt.Errorf("%w: time is required", ErrInvalidOccultationInput)
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}
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if err := star.Validate(); err != nil {
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return result, err
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}
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cache := newStarOccultationEventCache(star)
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tt := occultationTimeToTT(at)
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result.DeltaTSeconds = DeltaT(tt, true)
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result.SublunarLongitude, result.SublunarLatitude = occultationSublunarPoint(tt, cache.frameAt)
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result.Footprint = occultationInstantFootprint(
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at, cache.frameAt, cache.riseSetContextAt, false,
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)
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return result, nil
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}
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// PlanetOccultationFootprintsAt 返回指定时刻有限行星盘面的精确外接触和内接触月掩可见足迹;它采用路径时间线分辨率,并对每条完整接触弧执行站心校正。
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// PlanetOccultationFootprintsAt returns the exact visible outer- and inner-contact lunar-occultation footprints of a finite planetary disk at one instant, using timeline resolution and station-centred correction of each complete contact arc.
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func PlanetOccultationFootprintsAt(at time.Time, planet OccultationPlanet) (PlanetOccultationInstant, error) {
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result := PlanetOccultationInstant{Time: at, Planet: planet, TargetID: planet.String()}
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if at.IsZero() {
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return result, fmt.Errorf("%w: time is required", ErrInvalidOccultationInput)
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}
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if err := planet.Validate(); err != nil {
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return result, err
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}
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config, _ := planetOccultationConfigFor(planet)
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cache := newPlanetOccultationEventCache(config)
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tt := occultationTimeToTT(at)
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result.DeltaTSeconds = DeltaT(tt, true)
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result.SublunarLongitude, result.SublunarLatitude = occultationSublunarPoint(tt, cache.outerFrameAt)
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result.Partial = occultationInstantFootprint(
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at, cache.outerFrameAt, cache.riseSetContextAt, false,
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)
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result.Total = occultationInstantFootprint(
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at, cache.totalFrameAt, cache.riseSetContextAt, true,
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)
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return result, nil
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}
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func occultationSublunarPoint(tt float64, frameAt occultationPathFrameFunc) (float64, float64) {
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frame, ok := frameAt(tt)
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if !ok {
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return math.NaN(), math.NaN()
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}
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distance := math.Sqrt(frame.moon.x*frame.moon.x + frame.moon.y*frame.moon.y + frame.moon.z*frame.moon.z)
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if distance == 0 {
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return math.NaN(), math.NaN()
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}
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rightAscension := math.Atan2(frame.moon.y, frame.moon.x) * 180 / math.Pi
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declination := math.Asin(math.Max(-1, math.Min(1, frame.moon.z/distance))) * 180 / math.Pi
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longitude := rightAscension - ApparentSiderealTime(TD2UT(tt, false))*15
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for longitude > 180 {
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longitude -= 360
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}
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for longitude < -180 {
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longitude += 360
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}
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return longitude, declination
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}
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func occultationInstantFootprint(
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at time.Time,
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frameAt occultationPathFrameFunc,
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contextAt occultationRiseSetContextFunc,
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total bool,
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) *OccultationFootprint {
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tt := occultationTimeToTT(at)
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footprint, ok := planetOccultationFootprintAtWithResolution(
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tt, frameAt, at.Location(),
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planetOccultationTimelineBoundaryPoints,
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planetOccultationTimelineHorizonPoints,
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planetOccultationTimelineTargetSpacingKM,
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)
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if !ok {
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return nil
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}
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// A one-element correction deliberately treats this instant as both ends of
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// the sequence, so every contact-arc sample receives the exact station solve.
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corrected := occultationStationCorrectFootprintEdges(
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[]PlanetOccultationFootprint{footprint}, frameAt, contextAt, total, at.Location(),
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)
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if len(corrected) != 1 {
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return nil
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}
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footprint = corrected[0]
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normalizeOccultationInstantTime(&footprint, at)
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return &footprint
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}
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func normalizeOccultationInstantTime(footprint *OccultationFootprint, at time.Time) {
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if footprint == nil {
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return
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}
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footprint.Time = at
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for _, polygons := range [][][]OccultationPathPoint{
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footprint.Polygons,
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footprint.InteriorPolygons,
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footprint.Boundaries,
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} {
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for polygonIndex := range polygons {
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for pointIndex := range polygons[polygonIndex] {
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polygons[polygonIndex][pointIndex].Time = at
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}
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}
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}
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}
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