x p (t) = −f u(t)w(t) ,y p(t) = −f v(t)w(t)(3.40)where⎡⎢⎣u(t)v(t)w(t)⎤⎡⎥⎦ = R T ⎢(ω, ϕ, κ) ⎣X i (t) − X CY i (t) − Y CZ i (t) − Z C⎤⎥⎦Differentiating the collinearity equations <strong>with</strong> respect to parameter t leads to 2Dtangent direction in the image space.x ′ p(t) = −f u′ (t)w(t) − u(t)w ′ (t), y ′w 2 (t)p(t) = −f v′ (t)w(t) − v(t)w ′ (t)w 2 (t)(3.41)⎡⎢⎣u ′ (t)v ′ (t)w ′ (t)⎤⎡⎥⎦ = R T ⎢(ω, ϕ, κ) ⎣X i(t)′ ⎤Y i ′ ⎥(t) ⎦Z i(t)′⎡⎢⎣du ′ ⎤dv ′dw ′⎥⎦ = ∂RT∂ω⎡X ′ ⎤⎡iX ′ ⎤⎡⎢⎣ Y i′ ⎥⎦ dω + ∂RT iX ′ ⎤⎢⎣ Y ′ ⎥Z i′ i ⎦ dϕ + ∂RT i⎢⎣ Y ′ ⎥∂ϕZ i′ i ⎦ dκ∂κZ i′ ⎡ ⎤⎡ ⎤⎡12t3t 2 ⎤⎡+R T ⎢ ⎥⎣ 0 ⎦ da 1 + R T ⎢ ⎥⎣ 0 ⎦ da 2 + R T ⎢ ⎥⎣ 0 ⎦ da 3 + R T ⎢⎣000⎡ ⎤ ⎡ ⎤ ⎡ ⎤⎡+R T ⎢ ⎥⎣ ⎦ db 2 + R T ⎢ ⎥⎣ ⎦ db 3 + R T ⎢ ⎥⎣ ⎦ dc 1 + R T ⎢⎣+R T ⎡⎢⎣02t0⎤0⎥03t 2⎡⎦ dc 3 + R T ⎢⎣03t 202a 2 + 6a 3 t2b 2 + 6b 3 t2c 2 + 6c 3 t⎤001010002t⎤⎥⎦ db 1⎤⎥⎦ dc 2⎥⎦ dt j (3.42)tan(θ t ) = y′ px ′ p= v′ (t)w(t) − v(t)w ′ (t)u ′ (t)w(t) − u(t)w ′ (t)(3.43)where tan(θ t ) the tangent in terms of the angle θ t (0 ≤ θ t ≤ 2π)54
d tan(θ t ) = w′ (v ′ w − w ′ v)(u ′ w − w ′ u) 2 du − w(v′ w − w ′ v)(u ′ w − w ′ u) 2 du′ −w ′u ′ w − w ′ u dv +wu ′ w − w ′ u dv′+ v′ (u ′ w − w ′ u) − u ′ (v ′ w − v ′ w)(u ′ w − w ′ u) 2 dw − v(u′ w − w ′ u) − u(v ′ w − vw ′ )(u ′ w − w ′ u) 2 dw ′(3.44)Linear observation equation can be obtained <strong>with</strong> incremental values, dX C , dY C , dZ C ,dω, dϕ, dκ, da 0 , da 1 , da 2 , da 3 , db 0 , db 1 , db 2 , db 3 , dc 0 , dc 1 , dc 2 , dc 3 , dt j as (3.45).tan(θ t ) − v′0 w 0 − w ′0 v 0u ′0 w 0 − w ′0 u 0 = L 1 dX C + L 2 dY C + L 3 dZ C + L 4 dω + L 5 dϕ + L 6 dκ+L 7 da 0 + L 8 da 1 + L 9 da 2 + L 10 da 3 + L 11 db 0+L 12 db 1 + L 13 db 2 + L 14 db 3 + L 15 dc 0 + L 16 dc 1+L 17 dc 2 + L 18 dc 3 + L 19 dt j + e t (3.45)<strong>with</strong> tan(θ t ) the tangent direction of a point in the image space, u 0 , v 0 , w 0 , u ′0 , v ′0 , w ′0the approximate parameters by (XC, 0 YC, 0 ZC, 0 ω 0 , ϕ 0 , κ 0 , a 0 0, a 0 1, a 0 2, a 0 3, b 0 0, b 0 1, b 0 2, b 0 3,c 0 0, c 0 1, c 0 2, c 0 3, t 0 i ) and e t the stochastic error of tangent between two locations <strong>with</strong> zeroexpectation. L 1 , · · · , L 19 denote the partial derivatives of the tangent of a 3D <strong>natural</strong><strong>cubic</strong> spline. Detailed derivations are in Appendix A.3.55
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c○ Copyright byWon Hee Lee2008
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ACKNOWLEDGMENTSThanks be to God, my
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3. BUNDLE BLOCK ADJUSTMENTWITH 3D N
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CHAPTER 1INTRODUCTION1.1 OverviewOn
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+2f( t [1 + t 2) − 1 22s 12 (Y i
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+Du ′ ( t 1 + t 22)2r 11 t + Dv
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A 17 = t [2 − t 1 16 2 f(t 1) −
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1−u ′ w − w ′ u {w′ [s 21
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BIBLIOGRAPHY[1] Ackerman, F., and V
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[24] Haala, N., and G. Vosselman. 1
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[49] Parian, J.A., and A. Gruen. 20
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[73] Vosselman, G., and H. Veldhuis