044f2f4381
- 新增半解析、旧模型、自定义与多源堆叠星历实例,提供 Context、Instance、SPK 读取及状态与视位置计算 - 统一太阳、月球和行星实例接口,扩展黄经穿越、留、相位、最近角距、偕日可见、任意高度升落、轨道节点及凌日等天象查询 - 完善日月食、月掩与凌日的月缘剖面、有限盘面接触、站心修正、局地可见性、全球路径和地图输出 - 新增 SVG、GeoJSON、KML 天象输出及凌日、月掩和月缘地形相关缓存与几何求解 - 新增恒星星表导入与查询,支持 CSV、Hipparcos、BSC5、Stellarium 等格式及名称、交叉标识、锥面检索和星等过滤 - 补充 IAU 2006、地球定向、折射消光、大气观测、轨道传播及半解析行星/月球数据支持 - 将默认未来民用时标切换为 TimeScaleLeapHour,更新 2027–2400 农历速查表、中文日期解析和时区边界处理 - 增加事件基线、跨模型回归、几何边界、月缘地形和输出契约测试,完善中英文手册、示例资源、NOTICE 与忽略规则
220 lines
6.9 KiB
Go
220 lines
6.9 KiB
Go
package eclipse
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import (
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"math"
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"sync"
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"b612.me/astro/basic"
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"b612.me/astro/internal/ephem"
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)
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const (
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sarosExtendedStartTT = 625308.343824885320
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sarosExtendedEndTT = 3912880.500800740905
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sarosInexLunations = 358
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sarosLunationEpoch = 2451550.09765
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// Keep the acceptance interval below half a synodic month while allowing
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// the mean-phase seed to drift in remote eras.
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sarosEclipseSeedToleranceDays = 7.0
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// 表外外推按 ±90 个沙罗周期求值同一批朔望月,直映缓存让相邻序列成员复用结果。
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sarosEclipseMemoSlots = 4096
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)
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type sarosEclipseMemoEntry struct {
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key int64
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gen uint64
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maximum float64
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exists bool
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valid bool
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set bool
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}
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var (
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sarosEclipseMemoMu sync.RWMutex
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sarosEclipseMemoEntries [sarosEclipseMemoSlots]sarosEclipseMemoEntry
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)
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// 直接取模即可:外推窗口的步长 223 与槽数互质,±90 个回次落在互不相同的槽位上。
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func sarosEclipseMemoSlot(key int64) int {
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return int(uint64(key) % sarosEclipseMemoSlots)
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}
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func sarosEclipseLookup(k, phase int) (float64, bool, bool, bool) {
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key := int64(k)*2 + int64(phase)
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slot := sarosEclipseMemoSlot(key)
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sarosEclipseMemoMu.RLock()
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entry := sarosEclipseMemoEntries[slot]
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sarosEclipseMemoMu.RUnlock()
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if !entry.set || entry.key != key || entry.gen != ephem.Generation() {
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return 0, false, false, false
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}
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return entry.maximum, entry.exists, entry.valid, true
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}
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func sarosEclipseStore(k, phase int, maximum float64, exists, valid bool) {
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key := int64(k)*2 + int64(phase)
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slot := sarosEclipseMemoSlot(key)
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sarosEclipseMemoMu.Lock()
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sarosEclipseMemoEntries[slot] = sarosEclipseMemoEntry{
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key: key, gen: ephem.Generation(), maximum: maximum, exists: exists, valid: valid, set: true,
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}
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sarosEclipseMemoMu.Unlock()
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}
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// A span contains consecutive 223-month returns. Separate spans preserve gaps
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// in shallow series without counting the missing returns as eclipses.
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type sarosSpan struct {
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Series int
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First int
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Last int
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Member int
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Count int
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}
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func sarosLunation(ttJDE float64, phase int) (int, bool) {
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k := (ttJDE-sarosLunationEpoch)/solarEclipseSynodicMonthDays - float64(phase)/2
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if math.IsNaN(k) || math.IsInf(k, 0) || math.Abs(k) > 1e7 {
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return 0, false
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}
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return int(math.Round(k)), true
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}
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// 358*38 = 1 (mod 223). Select the Inex column whose Saros row is nearest
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// the catalog reference; neighboring solutions are 358 Saros rows apart.
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// See NASA SEperiodicity.html, sections 1.7 and 1.9 (also valid for lunar series).
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func sarosNumber(k, phase int) int {
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anchors, base := solarSarosAnchors[:], 0
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if phase == 1 {
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anchors, base = lunarSarosAnchors[:], 1
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}
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anchor := decodeSarosMagic(anchors[len(anchors)/2], base+len(anchors)/2)
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refTT := basic.JDCalc(int(anchor.Year), int(anchor.Month), float64(anchor.Day))
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refK, _ := sarosLunation(refTT, phase)
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delta := k - refK
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column := (38 * delta) % sarosCycleLunations
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column += sarosCycleLunations * int(math.Round((float64(delta)/sarosInexLunations-float64(column))/sarosCycleLunations))
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return int(anchor.Series) + column
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}
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func matchSarosSpans(spans []sarosSpan, k int) (SarosInfo, bool) {
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for _, span := range spans {
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if k < span.First || k > span.Last || (k-span.First)%sarosCycleLunations != 0 {
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continue
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}
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return SarosInfo{
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Series: span.Series,
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Member: span.Member + (k-span.First)/sarosCycleLunations,
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Count: span.Count,
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}, true
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}
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return SarosInfo{}, false
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}
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func extendedSarosInfo(ttJDE float64, phase int) (SarosInfo, bool) {
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return defaultModule.extendedSarosInfo(ttJDE, phase)
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}
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func (module *Eclipse) extendedSarosInfo(ttJDE float64, phase int) (SarosInfo, bool) {
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return extendedSarosInfoForModel(ttJDE, phase, module.model(), module.sarosEclipse)
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}
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func extendedSarosInfoForModel(ttJDE float64, phase int, model ephem.Model, evaluate func(int, int) (float64, bool, bool)) (SarosInfo, bool) {
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k, ok := sarosLunation(ttJDE, phase)
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if !ok {
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return SarosInfo{}, false
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}
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if ttJDE >= sarosExtendedStartTT && ttJDE < sarosExtendedEndTT {
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spans := sarosExtensionSpansForModel(phase, model)
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info, ok := matchSarosSpans(spans, k)
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if !ok {
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return SarosInfo{}, false
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}
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if anchor, known := sarosAnchorRangeFor(phase, info.Series); known {
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info.Count = anchor.count
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}
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return info, true
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}
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return extrapolateSarosWithEvaluator(k, phase, evaluate)
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}
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func sarosExtensionSpans(phase int) []sarosSpan {
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return sarosExtensionSpansForModel(phase, ephem.Active())
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}
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func sarosExtensionSpansForModel(phase int, model ephem.Model) []sarosSpan {
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if model == ephem.Semianalytic {
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if phase == 1 {
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return lunarSarosExtendedSemianalytic[:]
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}
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return solarSarosExtendedSemianalytic[:]
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}
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if phase == 1 {
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return lunarSarosExtendedLegacy[:]
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}
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return solarSarosExtendedLegacy[:]
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}
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func sarosEclipse(k, phase int) (float64, bool, bool) { return defaultModule.sarosEclipse(k, phase) }
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func (module *Eclipse) sarosEclipse(k, phase int) (float64, bool, bool) {
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if module.inst != nil {
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return sarosEclipseUncached(k, phase, module)
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}
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if maximum, exists, valid, ok := sarosEclipseLookup(k, phase); ok {
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return maximum, exists, valid
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}
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maximum, exists, valid := sarosEclipseUncached(k, phase, module)
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sarosEclipseStore(k, phase, maximum, exists, valid)
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return maximum, exists, valid
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}
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// Saros metadata uses the Split-K solar model and the union of Danjon and
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// Chauvenet lunar detections, independent of the observer or display model.
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func sarosEclipseUncached(k, phase int, modules ...*Eclipse) (float64, bool, bool) {
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module := &defaultModule
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if len(modules) > 0 {
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module = modules[0]
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}
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seed := sarosLunationEpoch + (float64(k)+float64(phase)/2)*solarEclipseSynodicMonthDays
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var maximum float64
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var exists bool
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if phase == 0 {
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result := basic.SolarEclipseNASABulletinSplitKWithInstance(seed, module.inst)
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maximum, exists = result.GreatestEclipse, result.Type != basic.SolarEclipseNone
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} else {
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result := basic.LunarEclipseDanjonWithInstance(seed, module.inst)
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if result.Type == basic.LunarEclipseNone {
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result = basic.LunarEclipseChauvenetWithInstance(seed, module.inst)
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}
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maximum, exists = result.Maximum, result.Type != basic.LunarEclipseNone
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}
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valid := !math.IsNaN(maximum) && !math.IsInf(maximum, 0) && math.Abs(maximum-seed) < sarosEclipseSeedToleranceDays
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return maximum, exists, valid
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}
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func extrapolateSaros(k, phase int) (SarosInfo, bool) {
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return extrapolateSarosWithEvaluator(k, phase, sarosEclipse)
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}
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func extrapolateSarosWithEvaluator(k, phase int, evaluate func(int, int) (float64, bool, bool)) (SarosInfo, bool) {
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info := SarosInfo{Series: sarosNumber(k, phase)}
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for offset := -sarosExtrapolationWindow; offset <= sarosExtrapolationWindow; offset++ {
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_, exists, valid := evaluate(k+offset*sarosCycleLunations, phase)
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if !valid || (offset == 0 && !exists) {
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return SarosInfo{}, false
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}
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if !exists {
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continue
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}
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if offset == -sarosExtrapolationWindow || offset == sarosExtrapolationWindow {
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return SarosInfo{}, false
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}
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info.Count++
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if offset <= 0 {
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info.Member++
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}
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}
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return info, true
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}
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