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

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Chapter 2 Observations <strong>of</strong> <strong>Orbit</strong> <strong>Determination</strong><br />

∂r(<br />

t4)<br />

∂r<br />

( t4)<br />

∂p(<br />

t4)<br />

δ r( t4)<br />

= δr(<br />

t0)<br />

+<br />

δp(<br />

t0)<br />

∂r<br />

( t0)<br />

∂p(<br />

t4)<br />

∂p(<br />

t0)<br />

(2-93)<br />

r&<br />

( t1)<br />

r&<br />

∂<br />

δ ( t1)<br />

= r&<br />

( t0)<br />

r&<br />

δ<br />

∂ ( t0)<br />

(2-94)<br />

r&<br />

( t4<br />

)<br />

r&<br />

∂<br />

δ ( t4<br />

) = δr&<br />

( t0<br />

)<br />

∂r&<br />

( t )<br />

(2-95)<br />

0<br />

∂S<br />

( t2)<br />

δ S ( t2)<br />

= δS<br />

( t0)<br />

(2-96)<br />

∂S<br />

( t )<br />

0<br />

∂S<br />

( t3)<br />

δ S ( t3)<br />

= δS<br />

( t0)<br />

(2-97)<br />

∂S<br />

( t0)<br />

where<br />

p satellite dynamical model parameters<br />

2.2.2.2 Error Budget<br />

Like two way range observations, for the two-way Doppler observation, the atmosphere errors are increased<br />

twice. Using error propagation law, the accuracy <strong>of</strong> two-way Doppler observation can be given by<br />

2<br />

ion<br />

2<br />

trop<br />

2<br />

multi<br />

2<br />

r<br />

2<br />

noise<br />

md = 2m<br />

+ 2m<br />

+ m + 2m<br />

+ 2m<br />

≈ 2mo<br />

(2-98)<br />

where<br />

md two way Doppler error<br />

one way Doppler error<br />

m o<br />

2.3 Conclusion<br />

In this chapter the major observations <strong>of</strong> one-way and two-way systems such as ranges, range rates (Doppler),<br />

carrier phases and laser ranges were discussed. One-way observations require two clocks, one in the receiver and<br />

another on-board the satellite. This introduces clock synchronization errors to the observations. Two-way<br />

observations do not have such a problem. Another advantage <strong>of</strong> two-way observations is that for time transfer no<br />

accurate position coordinates <strong>of</strong> satellite and ground station are needed to compute the signal propagation delays<br />

<strong>of</strong> the mainly reciprocal paths and the clock <strong>of</strong>fset respectively (Hahn, 1996). Significant drawbacks <strong>of</strong> two-way<br />

observations are that atmospheric errors are introduced twice due to the signal traveling around the propagation<br />

path.<br />

As an orbit tracking system for GNSS-2, range observations are one <strong>of</strong> the best choices for orbit determination,<br />

because a range observation is simple in mathematical form, easily processed and well modeled for the various<br />

error sources. It is very important that range observations can be used in real time. If SLR is used for orbit<br />

determination <strong>of</strong> GNSS-2 satellites, in addition to the advantages mentioned above, there is another advantage,<br />

high accuracy. The disadvantage is that SLR is strongly dependent on the weather, which can not be used in<br />

routine operation.<br />

Carrier phase observations are highly accurate measurements, but they are complicated to process due to initial<br />

ambiguity and cycle slips, especially in real-time applications. If two L-band frequencies just like the GPS<br />

system are used, it is difficult to determine GEO satellite orbits using carrier phase observations because the<br />

initial ambiguity is not sensitive to GEO satellite.<br />

Doppler measurement is also a good choice due to its high accuracy. It can also be used in real time applications.<br />

For GEO satellite orbit determination, the problem is that the position change <strong>of</strong> GEO satellite related to the<br />

earth is so small that the accuracy <strong>of</strong> Doppler measurement will not be good.<br />

16

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