Files
astro/basic/occultation_station_envelope.go
T
b612 044f2f4381 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
2026-10-15 23:54:15 +08:00

78 lines
3.0 KiB
Go

package basic
import (
"math"
"time"
"b612.me/astro/internal/geodata"
)
// occultationStationDensifyContours applies the map's projection metric after
// station correction. The correction can move adjacent geocentric samples by
// tens of kilometres, so a contour that was dense before correction can still
// contain a long Web Mercator chord. A spatial arclength plane selects the
// midpoint branch even where time reverses and a fixed-time solve is singular.
// The refined curve is split again at time folds for the public time contract.
func occultationStationDensifyContours(
contours [][]OccultationPathPoint,
cache *occultationRiseSetEvaluationCache,
location *time.Location,
) [][]OccultationPathPoint {
if len(contours) == 0 || cache == nil {
return contours
}
const (
targetSpacingKM = 30.0
maxDepth = 10
)
result := make([][]OccultationPathPoint, 0, len(contours))
for _, contour := range contours {
if len(contour) < 2 {
continue
}
var refine func(OccultationPathPoint, OccultationPathPoint, int, *[]OccultationPathPoint)
refine = func(start, end OccultationPathPoint, depth int, output *[]OccultationPathPoint) {
if depth >= maxDepth || occultationStationProjectedSpacingKM(start, end) <= targetSpacingKM {
*output = append(*output, end)
return
}
startTT, endTT := centerTimeTT(start.Time), centerTimeTT(end.Time)
chord := [3]float64{math.Remainder(end.Longitude-start.Longitude, 360), end.Latitude - start.Latitude,
(endTT - startTT) * occultationStationEnvelopeTimeScale}
length := math.Sqrt(dotSolarEclipse3(chord, chord))
if length <= 1e-12 {
*output = append(*output, end)
return
}
predictor := [3]float64{start.Longitude + chord[0]/2, start.Latitude + chord[1]/2, chord[2] / 2}
for index := range chord {
chord[index] /= length
}
midpoint, _, ok := occultationStationCorrectEnvelopeArc(predictor, chord, startTT, cache,
occultationStationEnvelopeModel{kind: occultationStationContactEnvelope}, (start.WidthKM+end.WidthKM)/2, location)
if ok && occultationPathDistanceKM(start, midpoint.point) < occultationPathDistanceKM(start, end) &&
occultationPathDistanceKM(midpoint.point, end) < occultationPathDistanceKM(start, end) {
refine(start, midpoint.point, depth+1, output)
refine(midpoint.point, end, depth+1, output)
return
}
// Leave a failed local solve untouched. Retrying with an unrelated
// branch would be less accurate than retaining the source sample.
*output = append(*output, end)
}
refined := []OccultationPathPoint{contour[0]}
for index := 1; index < len(contour); index++ {
refine(refined[len(refined)-1], contour[index], 0, &refined)
}
result = append(result, occultationStationSplitEnvelopeAtTimeFolds(refined)...)
}
return result
}
func occultationStationProjectedSpacingKM(first, second OccultationPathPoint) float64 {
return geodata.WebMercatorDistanceKM(
geodata.GeoPoint{Longitude: first.Longitude, Latitude: first.Latitude},
geodata.GeoPoint{Longitude: second.Longitude, Latitude: second.Latitude},
)
}