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On the Availability of Fault Detection and Exclusion in GNSS Receiver Autonomous Integrity Monitoring

Published online by Cambridge University Press:  12 March 2009

Jinling Wang
Affiliation:
(The University of New South Wales)
Pieter B. Ober
Affiliation:
(The University of New South Wales)
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Abstract

Global Navigation Satellite System (GNSS) Receiver Autonomous Integrity Monitoring (RAIM) is essential for safety-of-life and liability critical applications. This paper discusses two fundamentally different ways to assess the integrity risk of an operation with RAIM, based on a different amount of information available: the expected (or average) performance that is computed using the GNSS models only and the real-time (or actual) performance, which also uses information on the internal status of a GNSS receiver. It is shown both theoretically and by simulation that the real-time integrity risk significantly exceeds the expected risk after the detection and exclusion of a failing satellite. Therefore, while most published RAIM algorithms base their performance assessment on the expected performance only, this is only correct when the requirements allow the risk evaluation to be averaged over multiple operations. However, when the GNSS integrity requirement is to be applied on a ‘per operation’ basis, real-time integrity measures are more appropriate.

Information

Type
Research Article
Copyright
Copyright © The Royal Institute of Navigation 2009
Figure 0

Table 1. Signal-In-Space Integrity Requirements from ICAO (2006).

Figure 1

Figure 1. The operation of RAIM FDE. When a failure is detected, the satellite that is most likely to have failed is removed from the position solution. Navigation can only continue successfully when the remaining system performance is still adequate.

Figure 2

Figure 2. The estimated integrity risk after the exclusion of a satellite for 504 locations on a grid on the earth (latitudes: −65,−55,−45, …, 55,65, latitudes −180,−170,−160, …, 170) for a single point in time (GPS Week 703, 344 064 seconds).

Figure 3

Figure 3. The number of geometries for which a certain integrity risk was found after the exclusion of a satellite – for failures in a random satellite and failures in the worst-case satellite respectively.

Figure 4

Table 2. Number of geometries with observed missed detection and no exclusion fractions.

Figure 5

Table 3. Number of geometries with observed integrity risks after an exclusion.