Full text: Proceedings, XXth congress (Part 5)

   
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The state vector model typically used to process IMU data is 
made up of two sets of parameters. The first set contains the 
errors resulting from the Newtonian model, ie. errors in 
position, velocity, and orientation. The second set contains the 
sensor errors, such as accelerometer and gyro biases. While the 
models for the first set of variables are given by the physics of 
the problem, the models for the second set are rather arbitrary. 
They are usually chosen by looking for a structure that makes 
state space modeling simple. Typical models of this type are 
random ramp, random walk, or first-order Gauss-Markov 
processes. Often a combination of these models is used to fit a 
specific error distribution, but in general model identification 
techniques are not applied to verify the model itself. Since most 
of the terms to be determined are long-wavelength features, an 
AR model can be used to determine what type of model 
structure would best fit the data. This idea was recently studied 
by Nassar et al (2003). Results are quite encouraging, especially 
if de-noising is applied first. The data sets studied so far all 
show significant second- order effects, and in some cases small 
third-order effects. When they are included in the state-space 
model, results improve by about 30%. However, if the order of 
the model is further increased, results get worse. Thus, it may 
be efficient and advisable to determine the optimal model order 
for typical classes of IMUs in advance and incorporate them 
into the state vector. 
Post-mission processing, when compared to real-time filtering, 
has the advantage that data of the whole mission can be used to 
estimate the trajectory. This is not possible when using filtering 
because only part of the data is available at each trajectory 
point, except the last. When filtering has been used in a first 
step, one of the optimal smoothing methods, such as the Rauch 
et al (1965) algorithm can be applied. It uses the filtered results 
and their covariances as a first approximation. This 
approximation is improved by using the additional data that 
were not used in the filtering process. Depending on the type of 
data used, the improvement obtained by optimal smoothing can 
be considerable. This improvement comes at a price, however. 
The price is in terms of storage requirement and computation 
time. It is not only necessary to store all estimated state vectors, 
but also their complete covariance matrices before and after 
updates. 
In cases where the IMU is mainly used to bridge GPS-outages, 
such as in land-vehicle applications in urban centers, a simple 
algorithm can be used very effectively. It calculates the 
difference between the IMU position and the GPS position at 
the beginning and the end of the outage. The resulting 
difference is attributed to a C-error. The choice of this simple 
error mode resulted from an analysis of the complete INS error 
model for short-time periods up to a few minutes; see Nassar 
and Schwarz (2002) for details. This model has been tested in 
both airborne and land-vehicle applications and has consistently 
modeled between 9094-9594 of the accumulated error (ibid). 
Requirements in terms of storage and time are minimal and the 
algorithm is very simple. The error graph for a 85 second 
outage and its model fit is shown in Figure 8. . 
  
International Archives of the Photogrammetry, Remote Sensing and Spatial [Information Sciences, Vol XXXV, Part B5. Istanbul 2004 
  
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Q 17 34 51 68 85 
Outage Interval At (sec) 
Figure 8: SINS (a navigation-grade - Honeywell LRF-III) 
Positioning Errors during DGPS Outage 
6. CURRENTLY ACHIEVABLE ACCURACIES AND 
ONGOING DEVELOPMENTS 
The tables of results shown in the following are not based on a 
comprehensive analysis of published results. They are rather 
samples of results achieved with specific imaging systems and 
have been taken from company brochures and technical 
publications. The authors think that they are representative for 
the systems that have been discussed previously. The following 
will include three examples of post-mission systems, one 
airborne, one van based, and one portable, and one airborne 
real-time system. 
The accuracy specifications for the Applanix family of 
POS/AV™ airborne direct georeferencing systems are listed in 
Table 2 (Mostafa et al, 2000). The primary difference in system 
performance between the POS/AV'" 310 and POS/AV™ 510 
systems is the orientation accuracy, which is directly a function 
of the IMU gyro drifts and noise characteristics. For example, 
the gyro drifts for the POS/AV™ 310 and POS/AV™ 510 
systems are 0.5deg/h and 0.ldeg/h, respectively. While the 
corresponding gyro noises are 0.15 and 0.02 deg/sqrt(h), 
respectively. 
  
  
  
  
  
  
  
  
  
  
  
  
  
  
ESO Accuracy | possav"" 240 | POS/AV"" 310 | POS/AV"" 410 | POS/AV™ 510 
Position (m) 0.05 - 0.30 0.05 - 0.30 0.05 - 0.30 0.05 - 0.30 
Velocity (m/s) 0.010 0.010 0.005 0.005 
Roll & Pitch (Deg) 0.040 0.013 0.008 0.005 
True Heading (Deg) 0.080 0.035 0.015 0.008 
  
  
  
Table 2: Post-processed POS/AV ™ navigation parameter 
accuracy (Mostafa et al, 2000] 
The second example is for land MMS. Accuracies achieved 
with many land MMS systems, such as the VISAT system (El- 
Sheimy, 1996) are suitable for all but the most demanding 
cadastral and engineering applications. Accuracies in this case 
mainly depend on availability of GPS and how long the INS 
systems can work independently in stand-alone mode. If GPS is 
available, the positioning accuracy is uniform at a level of 3-5 
cm (rms). If GPS is not available, the positional accuracy 
depends on the length of the outage, see Table 3. It lists the 
stand-alone accuracy of a strapdown navigation-grade system 
  
  
   
  
  
  
  
  
  
  
   
  
  
  
  
   
	        
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