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
This commit is contained in:
2026-10-15 23:54:15 +08:00
parent 16c62a97d5
commit 044f2f4381
674 changed files with 62983 additions and 8396 deletions
+20 -14
View File
@@ -1,6 +1,8 @@
package basic
import "math"
import (
"math"
)
// SolarEclipseShadowKind 阴影类型 / shadow kind.
type SolarEclipseShadowKind int
@@ -125,6 +127,8 @@ func (instant SolarEclipseShadowInstant) Empty() bool {
// SolarEclipseShadowSolver 可复用的单时刻求解器;非并发安全,宿主每条 lane 各持一个 / reusable solver, one per lane.
type SolarEclipseShadowSolver struct {
inst *Instance
options SolarEclipseShadowSolverOptions
anchorSet bool
@@ -132,8 +136,8 @@ type SolarEclipseShadowSolver struct {
anchorSolver solarEclipseSolver
}
// NewSolarEclipseShadowSolver 构造单时刻求解器 / builds a single-instant solver.
func NewSolarEclipseShadowSolver(options SolarEclipseShadowSolverOptions) *SolarEclipseShadowSolver {
// NewSolarEclipseShadowSolverWithInstance 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.
func NewSolarEclipseShadowSolverWithInstance(options SolarEclipseShadowSolverOptions, inst *Instance) *SolarEclipseShadowSolver {
options.Model = normalizeSolarEclipseRadiusModel(options.Model)
options.SunRadiusModel = normalizeSolarEclipseSunRadiusModel(options.SunRadiusModel)
if options.BoundaryPoints <= 0 {
@@ -156,7 +160,7 @@ func NewSolarEclipseShadowSolver(options SolarEclipseShadowSolverOptions) *Solar
if options.TargetSpacingKM < 0 {
options.TargetSpacingKM = 0
}
return &SolarEclipseShadowSolver{options: options}
return &SolarEclipseShadowSolver{inst: inst, options: options}
}
// ShadowAtJDE 给定 TT 时刻的阴影足迹;不在地球上时返回 (零值, false) / footprint at one TT instant.
@@ -210,13 +214,13 @@ func (solver *SolarEclipseShadowSolver) solverFor(jdeTT float64) solarEclipseSol
if solver.anchorSet && math.Abs(jdeTT-solver.anchorJDE) <= solarEclipseShadowAnchorHalfWindowDays {
return solver.anchorSolver
}
anchor := CalcMoonSHByJDE(jdeTT, 0)
anchor := solarEclipseAnchorNewMoon(jdeTT, solver.inst)
solver.anchorSet = true
solver.anchorJDE = anchor
solver.anchorSolver = newSolarEclipseSolverWithOptions(anchor, SolarEclipseOptions{
RadiusModel: solver.options.Model,
SunRadiusModel: solver.options.SunRadiusModel,
})
}, solver.inst)
return solver.anchorSolver
}
@@ -228,7 +232,7 @@ func (solver *SolarEclipseShadowSolver) besselGeometryAt(
if solver.options.DeltaTSeconds <= 0 {
return inner.besselGeometryAt(jdeTT)
}
sunEquatorial, moonEquatorial := solarEclipseSunMoonEquatorial(jdeTT)
sunEquatorial, moonEquatorial := solarEclipseSunMoonEquatorial(jdeTT, solver.inst)
axis := solarEclipseBesselAxisFromEquatorialWithDeltaT(
jdeTT, sunEquatorial, moonEquatorial, deltaTSeconds,
)
@@ -311,7 +315,7 @@ func (solver *SolarEclipseShadowSolver) StationStateAtJDE(
heightKM := heightMeters / 1000
state := localSolarEclipseStateAtWithDeltaT(
jdeTT, deltaT, lonDeg*rad, latDeg*rad, heightKM,
solarEclipseModelParams(solver.options.Model, solver.options.SunRadiusModel),
solarEclipseModelParams(solver.options.Model, solver.options.SunRadiusModel), solver.inst,
)
contact := state.movingDiskContactState()
central := contact.internalContactGap() <= 0
@@ -361,17 +365,19 @@ func SolarEclipseStationStateAtJDE(
func localSolarEclipseStateAtWithDeltaT(
jdTT, deltaTSeconds, lonRad, latRad, heightKM float64,
params solarEclipseModelParameters,
) localSolarEclipseState {
context := newLocalSolarEclipseStateContextWithDeltaT(jdTT, deltaTSeconds, params)
params solarEclipseModelParameters, instances ...*Instance) localSolarEclipseState {
inst := instanceValue(instances)
context := newLocalSolarEclipseStateContextWithDeltaT(jdTT, deltaTSeconds, params, inst)
return context.stateAt(lonRad, latRad, heightKM)
}
func newLocalSolarEclipseStateContextWithDeltaT(
jdTT, deltaTSeconds float64,
params solarEclipseModelParameters,
) localSolarEclipseStateContext {
sunEquatorial, moonEquatorial := solarEclipseSunMoonEquatorial(jdTT)
params solarEclipseModelParameters, instances ...*Instance) localSolarEclipseStateContext {
inst := instanceValue(instances)
sunEquatorial, moonEquatorial := solarEclipseSunMoonEquatorial(jdTT, inst)
utJDE := jdTT - deltaTSeconds/86400
return localSolarEclipseStateContext{
sunXYZ: solarEclipseLLRToXYZ(sunEquatorial[0], sunEquatorial[1], sunEquatorial[2]),