54 lines
2.4 KiB
Go
54 lines
2.4 KiB
Go
|
|
package basic
|
|||
|
|
|
|||
|
|
import (
|
|||
|
|
"math"
|
|||
|
|
"testing"
|
|||
|
|
"time"
|
|||
|
|
)
|
|||
|
|
|
|||
|
|
// Axis 与 Gamma 是同一个量的两种刻度:Gamma × 月球处的地球视差 = Axis。
|
|||
|
|
func TestLunarEclipseShadowGeometryAxisMatchesGamma(t *testing.T) {
|
|||
|
|
for _, date := range []time.Time{
|
|||
|
|
time.Date(2025, time.March, 14, 0, 0, 0, 0, time.UTC),
|
|||
|
|
time.Date(2026, time.March, 3, 0, 0, 0, 0, time.UTC),
|
|||
|
|
time.Date(2028, time.July, 6, 0, 0, 0, 0, time.UTC),
|
|||
|
|
} {
|
|||
|
|
result := LunarEclipse(TD2UT(Date2JDE(date), true))
|
|||
|
|
geometry := LunarEclipseShadowGeometryAt(result.Maximum)
|
|||
|
|
// 影几何内部用的是小角近似的地球视差(R⊕/月距),这里必须用同一形式,否则二级差会露出来。
|
|||
|
|
earthParallaxDegrees := (1 / geometry.MoonDistanceEarthRadii) * 180 / math.Pi
|
|||
|
|
if delta := geometry.Gamma*earthParallaxDegrees - geometry.AxisDegrees; math.Abs(delta) > 1e-9 {
|
|||
|
|
t.Fatalf("%s: Gamma×parallax - Axis = %g", date.Format("2006-01-02"), delta)
|
|||
|
|
}
|
|||
|
|
}
|
|||
|
|
}
|
|||
|
|
|
|||
|
|
// 食分公式反解出的月心到影轴距离必须等于 Axis:这条把影几何与食分求解器对起来。
|
|||
|
|
// 食分 = (影半径 + 月视半径 − Axis) / (2 × 月视半径)。
|
|||
|
|
func TestLunarEclipseMagnitudeInvertsToAxis(t *testing.T) {
|
|||
|
|
for _, date := range []time.Time{
|
|||
|
|
time.Date(2025, time.March, 14, 0, 0, 0, 0, time.UTC),
|
|||
|
|
time.Date(2026, time.March, 3, 0, 0, 0, 0, time.UTC),
|
|||
|
|
time.Date(2028, time.July, 6, 0, 0, 0, 0, time.UTC),
|
|||
|
|
time.Date(2020, time.November, 30, 0, 0, 0, 0, time.UTC),
|
|||
|
|
} {
|
|||
|
|
result := LunarEclipse(TD2UT(Date2JDE(date), true))
|
|||
|
|
geometry := LunarEclipseShadowGeometryAt(result.Maximum)
|
|||
|
|
moonSemidiameter := MoonSemidiameter(result.Maximum) / 3600
|
|||
|
|
fromUmbral := geometry.UmbralRadiusDegrees + moonSemidiameter -
|
|||
|
|
2*moonSemidiameter*result.Magnitude
|
|||
|
|
fromPenumbral := geometry.PenumbralRadiusDegrees + moonSemidiameter -
|
|||
|
|
2*moonSemidiameter*result.PenumbralMagnitude
|
|||
|
|
t.Logf("%s %s: Axis=%.4f 本影反推=%.4f 半影反推=%.4f",
|
|||
|
|
date.Format("2006-01-02"), result.Type, geometry.AxisDegrees, fromUmbral, fromPenumbral)
|
|||
|
|
if math.Abs(fromUmbral-geometry.AxisDegrees) > 0.002 {
|
|||
|
|
t.Fatalf("%s: umbral magnitude implies axis %.4f, geometry gives %.4f",
|
|||
|
|
date.Format("2006-01-02"), fromUmbral, geometry.AxisDegrees)
|
|||
|
|
}
|
|||
|
|
if math.Abs(fromPenumbral-geometry.AxisDegrees) > 0.002 {
|
|||
|
|
t.Fatalf("%s: penumbral magnitude implies axis %.4f, geometry gives %.4f",
|
|||
|
|
date.Format("2006-01-02"), fromPenumbral, geometry.AxisDegrees)
|
|||
|
|
}
|
|||
|
|
}
|
|||
|
|
}
|