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

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Chapter 3 <strong>Orbit</strong> Tracking <strong>System</strong> and Their Error Budgets<br />

(1) the space segment, a small self-contained hardware unit <strong>of</strong> dimensions 400x250x180 mm with a mass <strong>of</strong> 20<br />

kg, a power consumption <strong>of</strong> 32 W and host satellite independent communication links,<br />

(2) the ground segment, a network <strong>of</strong> 29 small autonomously transportable operating ground tracking stations,<br />

which can be installed at any site that is connected to a power line, for generation <strong>of</strong> tracking data,<br />

(3) the control segment consisting <strong>of</strong> a command station (Stuttgart), which is responsible for space segment<br />

control and data dumping; a master station (Oberpfaffenh<strong>of</strong>en) which is responsible for station network<br />

management, user support, and data preprocessing, quality control and distribution; and a calibration station<br />

(Potsdam), where a third generation laser system is operated to produce simultaneous laser ranging observations<br />

for periodic system calibration.<br />

Two PRARE signals (X and S-Bands) are emitted from space segment to earth. Both signals are modulated with<br />

PN-codes (10 MChips/s for X band and 1 Mchips/s for S-Band) and spread-spectrum binary data. They are all<br />

generated inside the space segment derived from its central ultra-stable oscillator and permanently disseminated<br />

by two dipole antennas.<br />

As PRARE has four independent receiver channels, up to four preselected stations can be handled<br />

simultaneously. The transportable and automatically operating ground stations receive the X-band downlink<br />

signal and demodulate the PN-code. Then the PN-sequence is remodulated on the X-band that is retransmitted to<br />

the space segment (regenerative transponders) containing ground station measurement data used for the<br />

preprocessing <strong>of</strong> the data. The PRARE space segment measures both two-way range and the received two-way<br />

Doppler-shifted signals very precisely by comparing the phase <strong>of</strong> the received signal to the phase <strong>of</strong> the on-board<br />

clock. The overall accuracy stems mainly from this two-way configuration <strong>of</strong> the system that eliminates the most<br />

clock errors <strong>of</strong> one-way systems.<br />

Ranging data is acquired by determination <strong>of</strong> the signal delay between outgoing and incoming signal (PN-code<br />

correlation method, 91 averaged measurements per second), range-rate by counting <strong>of</strong> the microwave cycles and<br />

the phase shift <strong>of</strong> the return signal (1 measurement per second). The high data precision is based on the full<br />

coherent two-way principle <strong>of</strong> the system, the high signal frequencies, and the appropriate resolution <strong>of</strong> the space<br />

segment receiver counters.<br />

S(t 2 )<br />

S(t 3 )<br />

S 2<br />

S 1<br />

23<br />

r(t 4 )<br />

r(t 1 )<br />

Figure 3-3 PRARE Two-Way Range Measurement<br />

S(t 4 )<br />

S(t 1 )<br />

The basic observation can be written as follows<br />

(1)Two-way range observation:<br />

Assuming the signal is transmitted from the satellite. From Figure 3-3, two-way range observation is<br />

L cF(<br />

t − t ) = S + S + ε<br />

(3-2)<br />

= 4 1 1 2<br />

where<br />

c speed <strong>of</strong> light in vacuum.<br />

F conversion factor from seconds <strong>of</strong> PRARE time to UTC units

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