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
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@@ -3,6 +3,8 @@ package basic
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import (
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"math"
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"sort"
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"b612.me/astro/internal/geodata"
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)
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const (
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@@ -20,6 +22,8 @@ type LocalSolarEclipseDiagramOptions struct {
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StepDays float64
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// SunRadiusModel 太阳半径口径,零值为标准档 / solar radius convention, standard when zero.
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SunRadiusModel SolarEclipseSunRadiusModel
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// LunarLimb 月缘剖面,nil 为圆月面;修正接触时刻、站心食分与遮蔽率,食甚时刻不变,月盘仍按圆面采样 / lunar limb profile for contacts, magnitude and obscuration.
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LunarLimb LunarLimb
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}
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// LocalSolarEclipseDiagramFrame 表示一个时刻的站心日月视圆几何。
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@@ -80,28 +84,28 @@ func LocalSolarEclipseDiagram(seedJDE, lon, lat, height float64, options LocalSo
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return LocalSolarEclipseDiagramNASABulletinSplitK(seedJDE, lon, lat, height, options)
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}
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// LocalSolarEclipseDiagramIAUSingleK 计算站心日食视圆图几何数据,使用 IAU Single-K 模型。
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// LocalSolarEclipseDiagramIAUSingleK computes local solar eclipse disk diagram geometry with the IAU Single-K model.
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func LocalSolarEclipseDiagramIAUSingleK(seedJDE, lon, lat, height float64, options LocalSolarEclipseDiagramOptions) LocalSolarEclipseDiagramResult {
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return localSolarEclipseDiagram(seedJDE, lon, lat, height, SolarEclipseModelIAUSingleK, options)
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// LocalSolarEclipseDiagramIAUSingleKWithInstance 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 LocalSolarEclipseDiagramIAUSingleKWithInstance(seedJDE, lon, lat, height float64, options LocalSolarEclipseDiagramOptions, inst *Instance) LocalSolarEclipseDiagramResult {
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return localSolarEclipseDiagram(seedJDE, lon, lat, height, SolarEclipseModelIAUSingleK, options, inst)
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}
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// LocalSolarEclipseDiagramNASABulletinSplitK 计算站心日食视圆图几何数据,使用 NASA bulletin Split-K 模型。
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// LocalSolarEclipseDiagramNASABulletinSplitK computes local solar eclipse disk diagram geometry with the NASA bulletin Split-K model.
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func LocalSolarEclipseDiagramNASABulletinSplitK(seedJDE, lon, lat, height float64, options LocalSolarEclipseDiagramOptions) LocalSolarEclipseDiagramResult {
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return localSolarEclipseDiagram(seedJDE, lon, lat, height, SolarEclipseModelNASABulletinSplitK, options)
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// LocalSolarEclipseDiagramNASABulletinSplitKWithInstance 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 LocalSolarEclipseDiagramNASABulletinSplitKWithInstance(seedJDE, lon, lat, height float64, options LocalSolarEclipseDiagramOptions, inst *Instance) LocalSolarEclipseDiagramResult {
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return localSolarEclipseDiagram(seedJDE, lon, lat, height, SolarEclipseModelNASABulletinSplitK, options, inst)
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}
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func localSolarEclipseDiagram(
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seedJDE, lonDeg, latDeg, heightMeters float64,
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model SolarEclipseRadiusModel,
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options LocalSolarEclipseDiagramOptions,
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) LocalSolarEclipseDiagramResult {
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options LocalSolarEclipseDiagramOptions, instances ...*Instance) LocalSolarEclipseDiagramResult {
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inst := instanceValue(instances)
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options = normalizeLocalSolarEclipseDiagramOptions(options)
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eclipse := localSolarEclipse(seedJDE, lonDeg, latDeg, heightMeters, SolarEclipseOptions{
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RadiusModel: model,
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SunRadiusModel: options.SunRadiusModel,
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})
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LunarLimb: options.LunarLimb,
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}, inst)
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result := LocalSolarEclipseDiagramResult{
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Eclipse: eclipse,
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StepDays: options.StepDays,
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@@ -118,7 +122,7 @@ func localSolarEclipseDiagram(
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result.StepDays = stepDays
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result.Frames = make([]LocalSolarEclipseDiagramFrame, 0, len(times))
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for _, item := range times {
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frame := localSolarEclipseDiagramFrameAt(item.jde, lonRad, latRad, heightKM, params)
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frame := localSolarEclipseDiagramFrameAt(item.jde, lonRad, latRad, heightKM, params, inst)
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frame.Label = localSolarEclipseDiagramPrimaryLabel(item.labels)
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frame.Labels = append([]string(nil), item.labels...)
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result.Frames = append(result.Frames, frame)
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@@ -250,9 +254,10 @@ func localSolarEclipseDiagramLabelPriority(labels []string) int {
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func localSolarEclipseDiagramFrameAt(
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jdTT, lonRad, latRad, heightKM float64,
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params solarEclipseModelParameters,
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) LocalSolarEclipseDiagramFrame {
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sunEquatorial, moonEquatorial := solarEclipseSunMoonEquatorial(jdTT)
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params solarEclipseModelParameters, instances ...*Instance) LocalSolarEclipseDiagramFrame {
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inst := instanceValue(instances)
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sunEquatorial, moonEquatorial := solarEclipseSunMoonEquatorial(jdTT, inst)
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sunXYZ := solarEclipseLLRToXYZ(sunEquatorial[0], sunEquatorial[1], sunEquatorial[2])
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moonXYZ := solarEclipseLLRToXYZ(moonEquatorial[0], moonEquatorial[1], moonEquatorial[2])
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@@ -278,14 +283,14 @@ func localSolarEclipseDiagramFrameAt(
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)
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sunRadiusRad := math.Asin(localSolarEclipseClampUnit(
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solarEclipseEarthEquatorialRadiusKM * params.sunRadiusRatio / sunTopocentric[2],
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geodata.EarthEquatorialRadiusKM * params.sunRadiusRatio / sunTopocentric[2],
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))
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moonRadiusRad := math.Asin(localSolarEclipseClampUnit(
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solarEclipsePenumbralRadiusNumerator(params) / moonTopocentric[2],
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))
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if params.umbralK > params.penumbralK {
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moonRadiusRad = math.Asin(localSolarEclipseClampUnit(
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solarEclipseEarthEquatorialRadiusKM * params.umbralK * localSolarMoonRadiusScale / moonTopocentric[2],
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geodata.EarthEquatorialRadiusKM * params.umbralK * localSolarMoonRadiusScale / moonTopocentric[2],
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))
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}
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