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

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Chapter 9 S<strong>of</strong>tware and Simulation Results<br />

Difference (meter)<br />

10<br />

10<br />

8<br />

6<br />

4<br />

2<br />

0<br />

-2<br />

-4<br />

-6<br />

-8<br />

-10<br />

0 24 48 72 96 120 144 168 192 216 240<br />

8<br />

6<br />

4<br />

2<br />

0<br />

-2<br />

-4<br />

-6<br />

-8<br />

-10<br />

Tim e (hour)<br />

Figure 9-19 Accuracy <strong>of</strong> <strong>Orbit</strong> <strong>Determination</strong> <strong>of</strong> a GEO <strong>Satellite</strong> Located at λ=20°<br />

0 24 48 72 96 120 144 168 192 216 240<br />

Figure 9-20 Accuracy <strong>of</strong> <strong>Orbit</strong> <strong>Determination</strong> <strong>of</strong> a GEO <strong>Satellite</strong> Located at λ=60<br />

The accuracy <strong>of</strong> x, y, z coordinates <strong>of</strong> dynamic orbit determination <strong>of</strong> a GEO satellite located at λ=-10° are<br />

±0.09, ±0.09 and ±0.13 meters respectively. The accuracy <strong>of</strong> a GEO satellite located at λ= 20° are ±0.15, ±0.16<br />

and ±0.13 meters respectively. The accuracy <strong>of</strong> a GEO satellite located at λ=60° are ±0.24, ±0.25 and ±0.14<br />

meters respectively.<br />

Also considering the unmodeling errors in the satellite dynamic models, the propagation and some unknown<br />

errors, 1-10 m accuracy-level <strong>of</strong> dynamic orbit determination <strong>of</strong> GEO satellites can be achieved using range<br />

observations with 1 m errors.<br />

Obviously, the accuracy <strong>of</strong> dynamic orbit determination <strong>of</strong> GEO satellites is better than that <strong>of</strong> IGSO satellites.<br />

This is related to satellite visibility, refer to Figure 9-5 to Figure 9-8.<br />

9.3 Simulation Results using Carrier Observations<br />

In order to carry out the simulation <strong>of</strong> dynamic orbit determination <strong>of</strong> IGSO and GEO satellite using carrier<br />

phase observation, a theoretical error-free orbit is produced using a numerical integration method. Four major<br />

122<br />

dx<br />

dy<br />

dz<br />

dx<br />

dy<br />

dz

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