Full text: XVIIIth Congress (Part B1)

amic noise 
ect to code 
n vector is 
31) 
32) 
33) 
assumed. 
ponents are 
dentical in 
ito the three 
S: 
4) 
15, and j=1, 
g and 
uniformly, 
completely 
uniformly, 
In other 
asymptotic 
I'he longer 
e the state 
itions (30) 
nce of the 
n X(j) can 
olution X, 
f filtering 
n be seen 
rate while 
ble. This 
mparison 
moothing 
ted to the 
-hievable. 
Figure 1 shows the convergence of the filtering variance 
with filtering time and the effects of different noise levels of 
the code solutions onto this resulting accuracy. However, 
this theoretical accuracy model has only limited validity 
because both code position vector X(k) and delta- position 
vector X(k,k-1) are affected by systematic error sources such 
as un-modelled troposphere errors, GPS orbital errors and 
multipath. The magnitude of these effects depends on the 
user's receiver and the measurement environment. 
  
  
  
  
  
  
  
  
  
  
  
(3 
10r 
P 
1 
B sj 
U 
g 
= 
DOES 
ù 0 20 40 60 80 100 
€ i Filtering Time in Epochs(1-100) 
5 T T T T 
© 
a 
E 0.5} = 
oO ae u... 
€ ; U—— RS —— 
E 0 500 1000 1500 2000 2500 
Filtering Time in Epochs(100-2500) 
Figure 1 The Convergence of Filtering Accuracy with 
Time, where the standard deviations of the code position 
are assumed as 10 m ( dot line ), 5 m (Solid line) and 2 m 
(broken line). 
From this figure we learn that this method allows under 
good conditions for real-time positioning with decimetre 
accuracy or better. Also, the method is suitable for any 
ranges and dynamic environments as no assumptions where 
necessary relating to the baseline length and receiver's 
dynamics. 
4. AIRBORNE TEST RESULTS AND ANALYSIS 
4.1 Description Of The Long-Range Dynamic (LRD) GPS 
Processing System 
The LRD system processes the measurements from both 
base and mobile receivers epoch by epoch. First, cycle slip 
detection and removal for one-way phase measurements is 
performed on the basis of combined phase measurements 
Ni, and N.;s. Next, the accepted integer candidates are 
used to compute the residuals of ionosphere-free double 
69 
difference measurements and then form a Fisher test 
statistic for selecting correct integer cycle slips (Han, 1995). 
After this, ionosphere-free double differenced phase and 
code ranges are jointly used to create delta-position vectors 
and position vectors, followed by the described on-line 
filtering and off-line smoothing processes, which require 
only 4 satellites for initialisation and maintenance and are 
therefore suitable for the environments with large mask 
angles; of course the use of more satellites are advantageous. 
4.2 Testing Results For Cycle Slip Detection And Repair 
Airborne DGPS kinematic data were collected on June 4 
1992 from two Trimble Geodesist IIP GPS receivers. Ll 
and L2 carrier phase and C/A code and P2 code data were 
available for use. The base station was located some 57 
meters from the take-off and touch-down site of the 
aeroplane. The data were logged every second for 2.5 hours, 
including static tracking periods of 4-5 minutes before take- 
off and after landing. Figure 1 shows the 2D trajectory of 
the aeroplane, whose height was 4500 metres during the en 
route phase of the flight. To demonstrate our method's 
efficiency for cycle slip detection and repair, the real-valued 
cycle estimates of DN; and DN; of PRN 23 for the 
airborne receiver are plotted in Figure 3a and b, where a 
moving time window of ten seconds of data was used to fit 
the ionosphere variation while the prediction time is set to 
one second. It can be seen that the noise of DN, is 
normally bounded within the range of +0.20cycles (1 cycle 
= 14.653m), thus the integer CS;s can be uniquely 
determined. The DN; noise sometimes exceeds 0.5 cycle 
(1 cycle= .864m). The CS, variable may therefore have 
two integer solutions, and the test procedure proposed in 
Han (1995) is applied to select an unique integer candidate. 
In order to test the method's ability for data gap removal, 
the prediction time was set to 60 seconds and the moving 
time window was set to 1 minute. Figure 4a,b show the 
real-valued cycle estimates of DN, (k+60) and DN. 
79(k+60) for the same satellite. The figure shows the 
significant increase in the noise level of the DN(k+60) 
estimates. Also in this example, correct integer cycles have 
been determined by the same test procedure. 
4.3 Experimental Results for the Filtering Solutions 
Four types of positioning solutions were obtained: the phase 
delta-position solution, the code position solution, the 
filtered solution and smoothing solution. In addition, as the 
initial baseline vector has been determined by an external 
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B1. Vienna 1996 
 
	        
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