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

where<br />

n total number <strong>of</strong> parameters to be solved<br />

6 number <strong>of</strong> coordinate components <strong>of</strong> position and velocity <strong>of</strong> satellite<br />

m number <strong>of</strong> tracking stations<br />

For example, if eight tracking stations are tracking one satellite at the same time, at least 6+8=14 parameters<br />

should be solved. For one epoch, only 8 observations are available. That means in order to solve the orbit<br />

determination problem using carrier-phase observations, from the theoretical point <strong>of</strong> view, at least two epochs<br />

<strong>of</strong> observation are necessary.<br />

2.1.3.2 Error Budget<br />

For dual frequency carrier phase observations, ionospheric error will be significantly decreased. Another<br />

advantage <strong>of</strong> carrier phase observations is that the receiver noise is much smaller due to high resolution <strong>of</strong> carrier<br />

phase measurement.<br />

The carrier phase processed in the receiver is mainly affected by following error sources<br />

• Observation resolution<br />

• Variation <strong>of</strong> the antenna phase center<br />

• Variation <strong>of</strong> phase delay in the receiver<br />

• Instability <strong>of</strong> the oscillator<br />

• Interchannel bias<br />

Interchannel bias for each hardware channel can be <strong>of</strong> order <strong>of</strong> ±2.5 mm r.m.s. Phase delay variations depend on<br />

the satellite signal strength. The influence can be reduced by processing observations from many satellites.<br />

Oscillator instabilities play only a minor role in carefully designed receivers if the timing signal is taken from the<br />

satellite clock or a well-behaved atomic clock. The phase center variation is minimized and reproducible for<br />

well-designed antenna. For a modern microstrip antenna the variation is a few mm (Seeber, 1993). Observation<br />

resolution depends on the signal to noise ratio from the satellite signals. Currently, the observation resolution is<br />

about 1% <strong>of</strong> the signal wavelength according to rule <strong>of</strong> thumb.<br />

Using GPS as an example, the error budget <strong>of</strong> one-way carrier phase measurements are listed in Table 2-3.<br />

Table 2-3 Error Budget <strong>of</strong> One-Way Carrier Phase Measurements (GPS, L1)<br />

Error Source Error (m)<br />

Ionosphere 0.1<br />

Troposphere 2.0*<br />

Multipath 0.1<br />

<strong>Satellite</strong> Clock 3.0*<br />

Receiver Error 0.002<br />

Total (1σ) 3.6<br />

* based on Table 2-1<br />

From Table 2-3, the accuracy <strong>of</strong> a carrier phase observation is not much better than that <strong>of</strong> a range observation.<br />

Usually a carrier phase observation is used in differential way. Under this situation, the accuracy <strong>of</strong> the carrier<br />

phase observation is much higher than that <strong>of</strong> the range observation. See Chapter 7 for details. Another problem<br />

for carrier phase observations are initial ambiguities. It is difficult to solve initial ambiguites in real-time<br />

applications such as navigaion.<br />

2.2 Two-Way <strong>System</strong><br />

In a two-way system, the signal is transmitted and received by the same station. A typical two-way system is<br />

satellite laser ranging (SLR). Supposing that the signal is transmitted by the ground station at ti-1 and is reflected<br />

by the satellite at t = t + ∆ t . The same signal is returned and received at the ground station at<br />

i i−1<br />

1<br />

11

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