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Precise Orbit Determination of Global Navigation Satellite System of ...

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Chapter 6 Algorithms <strong>of</strong> <strong>Orbit</strong> <strong>Determination</strong> <strong>of</strong> IGSO, GEO and MEO <strong>Satellite</strong>s<br />

ϖ ϖ ∂O<br />

ϖ ∂O<br />

ϖ 1 ∂ O ϖ 2 1 ∂ O ϖ 2<br />

yk<br />

= y′<br />

k + ( ) ′ ∆xk<br />

+ ( ) ′ ∆z<br />

k + ( ) ′ ( ∆x<br />

) + ( ) ′ ( ∆ ) + ...<br />

2 2 k<br />

z<br />

2 2 k<br />

∂x<br />

∂z<br />

∂x<br />

∂z<br />

where „ ´ “ means related terms are computed by approximate ρ xk ′ at epoch tk .<br />

Neglecting the second and higher order terms and supposing<br />

∂f<br />

∂O<br />

�<br />

Fk<br />

= ( ) ′ k, Hk<br />

= ( ) ′ k �<br />

∂x<br />

∂x<br />

�<br />

ϖ ϖ ϖ ϖ ϖ ϖ<br />

∆xk′= xk − xk′ , ∆z<br />

= zk − zk′<br />

�<br />

�<br />

the linear dynamic and observation equations can be expressed as<br />

ϖ<br />

∆&x ϖ ϖ<br />

′= ∆ ′+ �<br />

k Fk xk wk<br />

�<br />

ϖ ϖ ϖ ϖ �<br />

yk = Hk∆xk + Gk∆zk + ε k��<br />

2<br />

72<br />

2<br />

(6-40)<br />

(6-41)<br />

(6-42)<br />

where ρ wk is the dynamic noise and ρ ε is the measurement noise and we can further assume that<br />

ϖ ϖ<br />

Ew ( ) = 0, E(<br />

ε ) = 0.<br />

k k<br />

The satellite dynamic system equation becomes<br />

ϖ ϖ ϖ<br />

∆x = Φ ∆x + Γ w<br />

k k, k−1 k−1 k, k−1 k−1<br />

(6-43)<br />

where Φ kk , −1 is a solution <strong>of</strong> following differential equation<br />

dΦ<br />

dt<br />

= FΦ<br />

(6-44)<br />

Eq.(6-44) shows that if the dimension <strong>of</strong> state vector is 6, actually 36 differential equations in Eq.(6-44) must be<br />

solved. In the orbit computation, the dimension <strong>of</strong> state vector is more than 6, so the solution <strong>of</strong> Eq.(6-44) is a<br />

time-consuming task for computer. Eq.(6-44) can only be rigorously solved using numerical integration method.<br />

For actually application, some approximation approach may be used. From Kalman filter algorithm, ϖ xk ′ should<br />

be first computed using numerical integration, ϖ xk ′ is also called reference value (or ϖ ϖ Λ ϖ<br />

x0′ , x1′ , , xk′ series called<br />

reference orbit) and should be precisely computed, as the errors <strong>of</strong> the reference orbit will affect the accuracy <strong>of</strong><br />

orbit determination; for computation <strong>of</strong> ∆ ϖ x k and Pkk-1, Φ kk , −1 may not be so precise as for the computation <strong>of</strong><br />

ϖ<br />

xk ′ . Therefore approximation approach can be used to compute Φ kk , −1 for ∆ ϖ x k and Pkk-1. The computation<br />

burden will be significantly reduced and the accuracy <strong>of</strong> orbit determination will be kept.<br />

The approximation approach <strong>of</strong> the solution <strong>of</strong> Eq.(6-44) in the stationary system can be expressed as<br />

Φ( t) e Ft<br />

= (6-45)<br />

Supposing t=h, Φ is a system transition matrix, then according to Tarlor series<br />

Fh<br />

1 1<br />

Φ( h) = e = I + Fh+ Fh* Fh+ Fh* Fh* Fh+<br />

....<br />

2!<br />

3!<br />

where<br />

I an identity matrix.<br />

Referring to Eq.(6-11) to Eq.(6-13), F in Eq.(6-46) may be written as<br />

(6-46)

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