Wide-Sense CDF Overbounding for GNSS Integrity

  • NAVIGATION: Journal of the Institute of Navigation
  • June 2025,
  • 72
  • (2)
  • navi.697;
  • DOI: https://doi.org/10.33012/navi.697

Abstract

The need for highly reliable positioning in safety-of-life applications has led to the development of global navigation satellite system (GNSS) augmentation systems such as satellite-based augmentation systems and advanced receiver autonomous integrity monitoring. These systems rely on a transfer of integrity from the range to the position domain through concepts such as cumulative distribution function (CDF) overbounding and the more recent two-step overbounding. Here, we propose a new approach, wide-sense CDF overbounding, which offers more flexibility and robustness than existing methods by accommodating biased distributions and relaxing stringent assumptions of symmetry and unimodality while retaining the original simplicity of CDF overbounding. This method combines CDF and paired overbounding, adjusting protection volumes with a formula to compensate for weaker assumptions. We perform numerical analyses using real GNSS data that demonstrate the enhanced flexibility of wide-sense CDF overbounding and show its potential to improve the robustness and performance of GNSS-based safety solutions in various applications.

Keywords

1 INTRODUCTION

The growing number of use cases for global navigation satellite system (GNSS) technology related to safety-of-life applications, ranging from rail transport and drones to maritime and automotive systems, accompanied by the deployment of associated new operational systems, requires increasingly demanding performance in terms of precision and integrity.

For location applications, the notion of integrity refers to the level of confidence that a user can assign to a position estimation based on measurements from one or multiple sensors. The integrity concept was originally developed in the field of civil aviation for safety-related applications, such as commercial aircraft landing according to performance-based navigation approach procedures.

For GNSS users, this concept has been embodied in the emergence and operationalization of safety-of-life augmentation systems, such as ground-based augmentation systems, satellite-based augmentation systems (SBASs), receiver autonomous integrity monitoring (RAIM), and its updated variant, advanced RAIM (ARAIM). These systems are designed to provide bounds that cover unmodeled residual errors to a specified integrity risk. The integrity risk is the probability that the actual position error exceeds the bound that is assumed for that error for a specific duration.

Even if integrity is required for the user position, it is generally convenient to demonstrate and monitor integrity in the range domain, with a separate focus on each contributor of pseudorange errors: thermal noise, multipath, residual errors on GNSS satellites orbit and clocks, ionospheric and tropospheric delays, etc.

Consequently, demonstrating and maintaining integrity generally involves three distinct stages. The first stage identifies all contributors to the residual measurement errors and characterizes their probability distributions. The second stage calculates and provides the user a distribution maintaining measurement-level integrity. This distribution is simpler than the real distribution so that the user can manipulate it for computation. The final stage ensures that measurement integrity implies positional integrity, which is referred as an integrity transfer from the range to position domain.

The transfer of integrity from the range domain to the position domain is currently the subject of intensive research, as this transfer enables integrity demonstrations and subsequently the generalization of SBASs to safety-of-life applications beyond aviation.

According to the single point positioning algorithm in the Minimal Operational Performance Standard (MOPS) (EUROCAE, 2021; RTCA, 2016), positioning errors are linear combinations of range errors. If we assume that range errors have a centered independent Gaussian distribution, then the positional errors also have a centered Gaussian distribution. Consequently, in this case, integrity transfer from range to position is straightforward. However, the distributions of range errors are not clearly centered Gaussian: in practice, they could be biased, asymmetric, or even heavy-tailed.

DeCleene (2000) introduced the cumulative distribution function (CDF) overbounding concept to transfer integrity from the range domain to the position domain when the range errors are not Gaussian. The aim is to overbound the CDF of the range errors, up to a quantile related to the specified integrity risk. DeCleene (2000) showed that CDF overbounding guarantees position integrity, on condition that the true distribution of the range errors is symmetric and unimodal. Rife et al. (2006) and Blanch et al. (2018) generalized this concept to multimodal and asymmetric distributions via, respectively, paired overbounding and two-step overbounding, with an additional bias parameter and increased complexity.

The purpose of this article is to introduce a new integrity concept called wide-sense CDF overbounding, which relies on milder assumptions than original CDF overbounding, at the cost of an increased standard deviation for the overbound in the position domain. This new concept appears to be particularly relevant when the symmetry of the range error distribution is unrealistic or difficult to show and two-step overbounding is challenging to implement. The remainder of this article is organized as follows. Section 2 describes the state of the art in overbounding concepts. Section 3 describes the wide-sense CDF overbounding concept and provides a demonstration of integrity transfer from range to position, even if the range errors are neither symmetric nor unimodal. Section 4 generalizes the wide-sense CDF overbounding concept to biased distributions. Section 5 provides a numerical illustration of this new concept on real range errors. Finally, Section 6 presents conclusions.

2 STATE OF THE ART IN OVERBOUNDING CONCEPTS

This section describes the existing overbounding concepts, as illustrated in Figure 1.

FIGURE 1

Graphical illustration of overbounding concepts for X: CDF overbounding (left), paired overbounding (middle), two-step overbounding (right)

The overbounding condition requires that the CDF FX of X lie in the shaded green region. In addition, for the two-step overbounding (right), the first-step overbounds (in blue) must lie in the blue area.

2.1 CDF Overbounding

The CDF overbounding concept was proposed and developed by DeCleene (2000). The main aim is to overbound the empirical measurement error distribution, in the field of the CDF, by a simpler distribution that allows better control over the integrity risk, primarily at the tails. The use of a simplified distribution enables both analytical manipulation of the error distributions and the establishment of margins on the true error distributions, which are only partially known.

In the following, the CDF of a random variable X is denoted by FX. According to DeCleene, the random variable OX is a CDF overbound of the random variable X. We note that XOX if the following holds:

x0,FX(x)FOX(x)x0,FX(x)FOX(x)1

The CDF overbound concept is preserved by convolution: if XOX and YOY, if X and Y are independent, and if all the distributions are unimodal and symmetric, then α,β, αX+βYαOX+βOY. This mathematical result demonstrates that the integrity risk associated with the sum Ox+Oy serves as an upper bound for the integrity risk of the sum X+Y.

Consequently, each real empirical measurement error distribution is replaced by its overbound distribution, and as the position errors are obtained as a linear combination of the residual measurement errors, the positional errors are also overbounded by a symmetric, unimodal distribution. This property guarantees that integrity in the pseudorange domain implies integrity in the positional domain.

The CDF overbound concept, however, requires that the distributions of error components be centered, meaning that they should be unimodal and symmetric, with no bias. Yet, the verification of hypotheses of zero mean and symmetry for residual measurement errors is never perfectly met. Systematic errors (including tropospheric delays, multipath effects, interchannel biases, etc.) inevitably introduce biases into the residual errors. Furthermore, there is no guarantee that the empirical distributions are indeed unimodal.

These errors are composed of a random part, a noise ϵi along the lines of sight, and an additional bias μi. If these biases were known, they would be integrated into, for instance, the SBAS corrections and the distributions of the residual errors would be centered, which is not the case. Even if these biases are poorly understood, it is generally assumed that an upper limit of their absolute values is known. It then becomes possible to introduce this upper limit into the variance σi of the overbound distributions by applying an inflation factor ξn,K, which depends on an integrity factor K and the number n of lines of sight (DeCleene, 2000; Rife et al., 2006):

ξn,K=1+maxi=1,,n|μi|σinK2

However, this approach is highly conservative and often leads to excessively large protection volumes, which limits service availability.

The concept of the CDF overbound requires that the tails of the overbound cover the tails of the empirical distribution. In the case of a Gaussian overbound (which is generally the case), we know that the tails of Gaussian distributions are very light; thus, we will eventually find a quantile (however large) beyond which the tail of the Gaussian falls below the tail of the empirical distribution. For this reason, in practice, we set a quantile q, beyond the specified integrity risk (IR), q > F–1(IR/2), within which, over the interval [–q, q], the overbound property exists. This approach can be justified by applying core overbounding (Rife, Walter et al., 2004).

2.2 Paired Overbounding

The paired overbounding concept of Rife et al. (2006) is designed to dispense with the hypotheses of CDF overbounding other than the independence of the random variables, namely, that the distributions of the residual error components must all be centered, unimodal, and symmetrical.

We suppose that the random variables X and X provide a paired overbound for the random variable X, and we denote X[X,X] if the following hold:

x,FX(x)FX(x)x,FX(x)FX(x)3

The random variable X is called the left overbound, and X is called the right overbound of the variable X.

The paired overbounding property is preserved by convolution if X and X are symmetric (X=X): if X[X,X] and Y[y,y], then α,β, αX+βY[|α|X|β|Y,|α|X+|β|Y]. Only independence is needed for the result to hold, and no specific assumptions on the distributions are necessary to demonstrate their stability by convolution. Consequently, if the distribution of each measurement residual error is paired-overbounded, then the positional errors are also paired-overbounded and integrity in the pseudorange domain implies integrity in the positional domain. This approach is very useful when accounting for residual biases and developing an overbound concept that can accommodate any residual distribution shape.

In practice for GNSS integrity, the pair of overbounds are set as two Gaussian distributions with identical standard deviation σ, with mean –μ for the left overbound and +μ for the right overbound. However, although the paired overbounding concept brings generality to range overbounding, the search for left and right limits may lead to conservatism, especially when considering symmetrical overbounding distributions. This issue arises because Equation (3) implies that the tail of X is heavier on the right than that of X, but also lighter on the left. For Gaussian overbounds with only two degrees of freedom, this situation often leads to an excessive inflation of the μ parameter and over-conservatism.

This specific problem has been addressed by the excess mass CDF overbounding method presented by Rife, Pullen et al. (2004). The main idea is to apply paired overbounding by using distributions in which the total mass is allowed to be greater than unity. This method leverages the fact that only the left tail of the left overbound and the right tail of the right overbound are used to build the protection levels. Furthermore, the properties of paired overbounding do not depend on the fact that the total probability is normalized to unity. Thus, the excess mass method allows one to build an overbounding pair closer to the distribution of interest by relaxing the conditions on the right tail of the left overbound and on the left tail of the right overbound. In practice, the paired overbounding method is very rarely used without excess mass.

An alternative way to deal with the excessive conservatism of paired overbounding with symmetrical overbounds is to consider non-symmetrical (and thus non-Gaussian) overbounding distributions. This approach is taken, for example, by Rife and Pervan (2012); in that work, the authors propose a numerically defined distribution for the right overbound with a light tail on the left side and a heavy tail on the right side. Their left overbound is the mirror reflection of the right overbound. This approach enables one to reduce conservatism at the price of an increased computation load, as no analytical expression is available for the position domain protection level, which must be computed numerically.

To further improve on the excess mass overbounding method, the two-step overbounding method was introduced by Blanch et al. (2018).

2.3 Two-Step Overbounding

Blanch et al. (2018) cleverly blended the last two concepts, the CDF overbound and the paired overbound, taking advantage of the less conservative property of the first concept and the robustness of the second. The purpose is to frame the empirical distribution X of an unmodeled residual error with Gaussian overbounds.

Their approach starts with the construction of left and right overbounds that are symmetrical and unimodal around their medians. Because these distributions do not need to be Gaussian, they are not strongly affected by the issue presented in the section above. Each distribution is then CDF-overbounded by a Gaussian distribution. The result is a pair of biased Gaussian distributions that can be used as a paired overbound for protection-level computation. Because the intermediate paired overbound is symmetrical and unimodal, the integrity demonstration is obtained naturally by applying the CDF and paired overbound stability with convolution. The first step of paired overbounding can also be combined with the excess mass method in order to obtain an overbounding distribution closer to the original distribution.

This construction enables a transfer of integrity from the measurement domain to the positional domain without specific assumptions of symmetry, centering, or unimodality for the empirical error distribution. The approach is less conservative than the paired overbound method. In return, the construction of the paired overbounding (first step) requires a complex optimization algorithm that is not straightforward to implement. In addition, it is not easy to verify whether a distribution is a two-step overbound of another distribution, as this necessitates to exhibit a first step paired overbound that is compatible with the final overbound.

3 WIDE-SENSE CDF OVERBOUNDING FOR UNBIASED DISTRIBUTIONS

In this section, we introduce a new overbounding method that combines the simplicity of CDF overbounding and the robustness of paired overbounding. We start by describing the method for unbiased distributions, but without the classical assumptions of symmetry and unimodality. We first take a Gaussian CDF overbound of the real distribution and work directly with the overbounding Gaussian for integrity and protection volume calculations. To account for asymmetry and possible multimodality, we multiply the variance of the overbounding Gaussian by a suitable inflation factor, with values provided in Table 1. Because the new property demands fewer hypotheses than the original CDF overbound, but requires a knowledge of a possible range of the number of error sources and integrity risks considered at the position level, we call this overbound a wide-sense CDF overbound.

View this table:
TABLE 1

Upper Bounds of the Inflation Factor An,K*

To compute a factor An,K for n, K values not included in this table, we recommend taking the column entry corresponding to a larger n and a row entry corresponding to a smaller K in order to remain conservative in the protection level.

*Conservative bound because of numerical instabilities with the accurate evaluation

3.1 Overview of the Problem and Proposed Method

In this section, we consider a user of a GNSS with an augmentation system for positioning. The receiver uses measurements with n independent error sources for its positioning. The error sources can be, for example, orbit determination and time synchronization errors or errors in the estimate of the ionosphere delay or some local effect such as multipath. n will a priori be a multiple of the number of lines of sight in view of the receiver. We will suppose that the user has access to a Gaussian CDF overbound of the range errors for the different error sources via the augmentation system. We assume that the errors are unbiased and independent from each other, but without any further hypotheses on the true range error distributions. The case of biased errors will be developed in Section 4.

In our method for constructing a position protection level for an integrity risk IR, we first compute the usual Gaussian-associated K-factor (K = Φ−1 (1 – IR/2), where Φ is the CDF of the normal centered distribution) and then multiply it by an inflation factor An,K to account for the asymmetry and possible multimodality of the range error distribution. The origin and calculation of the factor An,K are presented in Section 3.2. The inflation factor An,K depends only on the number of independent errors n and the integrity risk; thus, this factor can be taken from a table or pre-computed once and for all for a particular integrity context (see Section 3.2.6 for how n may be reduced in specific cases). To this end, numerical values of the inflation factor An,K are provided in Table 1. Thus, the complexity of our method is equivalent to the complexity of finding the Gaussian CDF overbound of the range errors.

Here, we provide a few definitions and notations that will be used throughout the remainder of this paper. We state that a Gaussian random variable with standard deviation σ provides a wide-sense CDF overbound of the centered random variable X if the following hold:

x0,FX(x)Φσ(x)x0,FX(x)Φσ(x)4

The only difference between this case and conventional CDF overbounding is that we drop the unimodality and symmetry hypotheses on the distribution of X.

We now suppose that for each error source Xi, the user has access to a Gaussian wide-sense CDF overbound of Xi with variance σi2. From these overbounds, we obtain the associated reduced error Yi=Xi/σi. To determine its position, the user performs a (possibly weighted) least-square algorithm, so that the position domain error ℰ is a linear combination of the range-level errors (here, ℰ denotes a one-dimensional component of the position error, for example, the vertical error), i.e., (si)n so that =isiXi=isiσiYi. We note that σpos2=isi2σi2 (the variance of the position-level CDF overbound that we would obtain if using the CDF overbound concept), and ε=/σpos (the reduced position error). We have the following:

ε=iYi×siσiσpos=iαiYiwhereαi=siσiσpos5

(Note that by construction, the vector of αi is a Euclidean unit vector, i.e., ||(αi)||2 = 1).

The main result of this section is that a knowledge of the Gaussian wide-sense CDF overbounds of each error sources is sufficient to construct a protection level associated with an integrity risk IR. The protection level is given as follows:

PL=An,K×σpos×K6

where K=Φ1(1IR2) and An,K is a suitable inflation factor whose origin is detailed in Section 3.2 and whose value is presented in Table 1.

Compared with conventional CDF overbounding, our method can deal with error distributions that are not symmetric or unimodal, which is the case for most error sources in practice. The trade-off is reflected in an inflation factor An,K that leads to a larger protection volume, to account for the loss of stability by a linear combination of CDF overbounding. The factor An,K is specific to the target integrity risk and depends on the number of contributors entering the user’s position determination. However, for a given integrity context, this factor (or a table of factors with different values of n) only has to be computed once and can be broadcast to the user or saved in an integrity algorithm. Consequently, the wide-sense CDF overbound method is very simple to use and is more robust to assumptions on the error distribution.

3.2 Justification of the Method and Integrity Proof

In this section, we justify the origin of the inflation factor An,K. The main idea of the wide-sense CDF overbounding method is based on the observation that the condition in Equation (4) is equivalent to having a paired overbound with half-Gaussian distributions. Unlike Equation (4), the paired overbounding is preserved by linear combination, which allows us to obtain an explicit paired overbound of the user position error. The inflation factor An,K is then determined by considering the worst sums of half-Gaussian distributions (from the viewpoint of position error) compared with typical sums of Gaussian distributions. In the last part, we prove that our protection level formula is conservative for the considered integrity risk.

3.2.1 From CDF Overbounding to Paired Overbounding

Let us first consider one reduced error source, Yi=Xi/σi, which has an unknown distribution with density fi and CDF Fi. By assumption, its distribution is CDF-overbounded by a standard normal distribution (whose probability distribution function and CDF are denoted as ϕ and Φ, respectively):

x0,Fi(x)Φ(x)x0,Fi(x)Φ(x)7

However, in general, Fi does not respect the other hypotheses from the CDF overbound, in particular, the symmetry and unimodality hypotheses (but it is centered, because Equation (7) implies that the median of Fi is 0). Notably, this means that Equation (7) will not be preserved per summation (and linear combination) in the general case.

We note (ϕl, Φl) and (ϕr, Φr) as the density and CDF of the two half-Gaussian distributions, defined as follows:

Φl(x)=1[,0[(x)Φ(x)+1[0,[(x)andΦr(x)=1[0,[(x)Φ(x)8

As illustrated in Figure 2, Equation (7) is equivalent to Fi being overbounded on the left by Φl and overbounded on the right by Φr :

Φr(x)F(x)Φl(x)x9

FIGURE 2

Graphical illustration of the equivalence between the CDF overbounding condition in Equation (7) by a normal centered Gaussian distribution (panel (a)) and the paired overbounding condition in Equation (9) by left and right half-Gaussian distributions (panel (b)) for the distribution with CDF FX

The two overbounding conditions cause FX to fall within the shaded green region.

In contrast to Equation (7), the property in Equation (9) is preserved by summation and linear combination with positive coefficients without additional assumptions on Fi. Because the left and right overbounding distributions are reflections of each other about the vertical axis, i.e., ϕl(x) = ϕr(–x), the property is also preserved under linear combination with real coefficients.

3.2.2 Paired Overbound of Any Linear Combination with n Terms

When the receiver calculates its position, it achieves a reduced position error according to Equation (5). As discussed above, we can use the stability through linear combination of Equation (9) to obtain a right overbound of ε, denoted as (αi). The right overbound (αi) with CDF R(αi) is explicitly given by (αi)=|αi|Zi, where the (Zi)i1..n are n independent identically distributed (i.i.d.) variables with CDF Φr. The symmetrical left overbound is obtained via the same calculation, by replacing Φr with Φl. Note that throughout this paper, curly letters are used to design random variables and straight letters indicate CDFs.

At this point, we have defined a paired overbound of the user’s position error. Yet, the two overbounding distributions require manipulations of the half-Gaussian Φr and Φl and are thus not easy to compute numerically. Moreover, the resulting CDF is dependent on the geometry matrix of the receiver, via αi. We would like to construct a more general overbounding pair that covers all cases, regardless of the user’s particular position. To this aim, we introduce the following definition:

Definition 1 For fixed n, we define Rn*(t) as the best possible right overbound of all R(αi) for any unit vector α:

Rn*(t)=infα2=1R(αi)(t)=infα2=1(i|αi|Zit)10

where Zi are n i.i.d. random variables following a right Gaussian of CDF Φr.

This function Rn*(t) can be viewed as the CDF of a random variable1, which we will denote as n*. n* is a distribution that right-overbounds the distribution of the reduced error ε for any user with n error sources, regardless of the geometry matrix or weight chosen by the receiver. A similar left overbound n* is defined in the same way by replacing “right” with “left” in the definition and taking the supremum. Note that the infimum is taken for each value of t ; thus, there is not a priori an αi vector that realizes the infimum for all t. In other terms, Rn*(t) cannot possibly be expressed as iαiZi.

3.2.3 Sigma Inflation Factor for Wide-Sense CDF Overbounding

The last step is to determine the protection volume by using the paired overbounding distributions n* and n*. Instead of working with the quantiles of these distributions, we compare these quantiles to the quantiles of the more typical Gaussian distribution, and we interpret the quantiles of the former as the quantiles of the Gaussian times an inflation factor.

For an integrity risk IR, the protection volume is given by (Rn*)1(1IR/2), the point from which the right tail of the right-overbounding distribution weighs less than IR/2. For a standard normal Gaussian, this point would be given by Φ−1(1 – IR/2) = K, usually called the K-factor (K = 5.33 for IR = 10−7 is used in the MOPS, for example). To use the correct protection volume, we should multiply the Gaussian quantile K by the following factor:

An,K*:=(Rn*)1(1IR/2)K=(Rn*)1(Φ(K))K11

3.2.4 Upper Bound on the Inflation Factor

In practice, we will only be able to compute an upper bound of the inflation factor An,K*, which we denote as An,K. We stress that this factor needs only to be computed once for a particular integrity requirement. The user does not need to compute this factor in each protection volume calculation, but only needs to store one or several values of the inflation factor. Furthermore, the upper bound presented in this paper is not optimal; some margin of improvement of the wide-sense CDF overbounding method is still possible.

The upper bound of the inflation factor An,K is obtained by constructing an explicit right overbound of the distribution n*. The method used to evaluate An,K is discussed in Appendix A. Table 1 presents numerical values of the inflation factor for different integrity risks and numbers of contributors.

For a practical case with specific values for K and the number of contributors n, the value of An,K can be either computed by applying the method described in Appendix A or taken from Table 1. If values not in the table are needed, a higher value of n can be used because the inflation factor grows with n. For the factor K, numerical evidence suggests that An,K decreases with K; thus, we recommend taking a smaller value of K present in the table.

3.2.5 Integrity Proof

In this section, we prove the integrity condition below:

(||An,KKσpos)1IR12

where ℰ is the position error, n is the number of contributors to positioning errors, and K is the Gaussian K-factor. The proof is only an application of the paired CDF overbound theorem and of our previous definitions and is given here as a summary of the arguments detailed above:

(||>An,KKσpos)=(ε>An,KK)+(ε<An,KK)(|α|>An,KK)+(|α|<An,KK)(n*>An,KK)+(n*<An,KK)(n*>An,K*K)+(n*<An,K*K)=2(1Rn*(An,K*K))=2(1Φ(K))=2(1(1IR2))=IR13

Step-by-step, we have the following:

  • From line 1 to line 2, we use the fact that the paired overbound is preserved by linear combinations to build an overbounding pair of ε, |α| and |α|, which depend on the user.

  • From line 2 to line 3, we use the paired overbound n* and n* defined in Definition (1) independent of αi.

  • From line 3 to line 4, we use the fact that An,K is an upper bound of the inflation factor An,K*.

  • From line 4 to line 5, we use the definition of the CDF and the symmetry of the overbounding pair, Rn*(x)=1Ln*(x).

  • From line 5 to line 6, we leverage the fact that An,K* is defined so that Rn*(An,K*K)=Φ(K).

This concludes the proof that our method builds a conservative protection volume.

3.2.6 Discussion on the Choice of n

The main limitation of the proposed approach is that the inflation factor An,K increases with n. In this section, we show that n does not have to include all error contributors for the case in which some of the contributors respect the conditions of the classical CDF overbound theorem (unimodality, symmetry). In this case, it is sufficient to consider n = k +1, where k is the number of independent range errors that are not known to follow the conditions of the CDF overbounding theorem.

We consider a case in which we have m independent range errors Xi with respective Gaussian wide-sense CDF overbounds with standard deviation σi. As before, the corresponding reduced range errors are written as Yi. Among these errors, mk follow a symmetrical and unimodal distribution (thus, their wide-sense CDF overbound is also a proper CDF overbound), and k have no specific conditions on their distribution. Here, we consider the case with k < m (for k = m, we simply take n = m).

Without a loss of generality, we can consider that the errors that comply to the CDF overbound theorem are the last errors. Using the same notation as in Section 3.1, the position error is expressed as =i=1ksiXi+i=k+1msiXi. Because the errors in the second sum respect the hypothesis of the CDF overbound theorem, i=k+1msiXi is CDF-overbounded by a Gaussian distribution with variance i=k+1msi2σi2.

Because a CDF overbound is also a wide-sense CDF overbound, Xk+1^=i=k+1msiXi can be treated as a single random variable in the derivation of the final position error overbound (with =i=1ksiXi+Xk+1^). This does not impact the computation of σpos, but it shows that it is sufficient to consider n = k +1 for the inflation factor An,K in Equation (6).

4 WIDE-SENSE CDF OVERBOUNDING FOR BIASED DISTRIBUTIONS

The aim of this section is to develop the wide-sense CDF overbounding concept for biased error distributions. In practice, such biases are not unusual, and two strategies has been developed to treat them.

The first strategy, initially proposed by DeCleene (2000), is to increase the standard deviation of errors to cover for the bias, as detailed by Equation (2), where bi is a bound on the bias of the range errors. This strategy makes sense when it is not possible to broadcast an additional bias parameter, as for operational SBASs. DeCleene (2000) showed that this strategy guarantees integrity when the true distribution of errors is symmetric about its mean.

The second strategy is to transmit to the user a bound on the nominal bias of each error contributor. This approach is utilized by ARAIM, which relies on an integrity support message with parameters ±bnom and σURA to model the bias and standard deviation of the left and right Gaussian overbounds of GNSS orbit and clock errors. This strategy guarantees integrity if the bias and standard deviations of the overbounds are compliant with paired overbounding, as shown by Rife et al. (2006), or two-step overbounding, as shown by Blanch et al. (2018), even if the true distribution is not symmetric.

Both of these strategies suffer some limitations. As detailed earlier, the symmetry assumption required by the first strategy may be unrealistic or difficult to justify. The second strategy may be over-conservative or difficult to implement in practice, as explained in Section 2.

Wide-sense CDF overbounding is attractive in both cases. The following section describes the generalization of the wide-sense overbounding concept to biased distributions. Section 4.2 demonstrates the transfer from wide-sense CDF overbounding at the range level to integrity at the user level.

4.1 Proposed Method

Wide-sense CDF overbounding of a potentially biased random variable X is defined as follows. The Gaussian random variables GX+ and GX with identical variance σ2 and mean ±b provide a paired wide-sense CDF overbound for an error contributor X to positioning error, if the following hold:

xb,FX(x)FGX(x)x+b,FX(x)FGX+(x)14

where b is at least larger than the absolute value of the median of X.

The main idea of the wide-sense CDF overbounding concept is based on the observation that the conditions in Equation (14) allow us to build an overbounding pair X and X as two half-Gaussian random variables defined as follows. X has CDF FX(x)=FGX¯(x) for x ≤ –b and FX(x)=1 for x > –b, and X is symmetrically defined as Fx(x)=FGx+(x) for xb and FX(x)=0 for x < b.

We consider a GNSS user that computes a position with measurements that have n error contributors Xi. We assume that each contributor Xi has a wide-sense CDF overbound with standard deviation σi and bias bi (noting that the bias is positive). For an integrity risk IR, the user computes a protection level as follows:

PL=An,K×K×σpos+i=1n|si|bi15

where An,K is the inflation factor defined in the previous section and listed in Table 1, K is the Gaussian K-factor, and σpos is given by σpos2=isi2σi2.

If the strategy of DeCleene (2000) is preferred, the biases can be integrated in an additional inflation factor, leading to the following protection level formula:

PL=ξn,K×An,K×K×σpos16

where ξn,K is provided by Equation (2).

In addition to its simplicity, a major advantage of wide-sense CDF overbounding over paired and two-step overbounding is that it does not require majoration of the distribution on the entire x-axis. In regard to CDF overbounding, the main asset of wide-sense CDF overbounding is the guarantee of integrity without the assumption of symmetry, as demonstrated below.

4.2 Integrity Proof

The aim of this section is to show that wide-sense CDF overbounding of a biased distribution and the use of the protection level formulas in Equation (15) or (16) imply position integrity, as follows:

(||>PL)IR

where ℰ is the position error, PL is the protection level computed according to the definition of wide-sense CDF overbounding, and IR is the integrity risk. As in Section 3.2.5, this proof is simply an application of the paired overbounding theorem and of our previous definitions and is presented here to summarize the arguments stated above.

For the protection level defined in Equation (15), the proof consists of the following steps:

(||>PL)=(i=1nsiXi<An,KKσposi=1n|si|bi)+(i=1nsiXi>An,KKσpos+i=1n|si|bi)(i=1n|si|Xi<An,KKσposi=1n|si|bi)+(i=1n|si|Xi>An,KKσpos+i=1n|si|bi)=(i=1n|si|σiσpos(Xi+biσi)<An,KK)+(i=1n|si|σiσpos(Xibiσi)>An,KK)(n*<An,KK)+(n*>An,KK)IR2+IR2=IR17

Step-by-step, we have the following:

  • In line 1, we apply the definition of the position error ℰ and protection level from Equation (15).

  • For line 2, we use the fact that all Xi are paired-overbounded by Xi and Xi and that paired overbounding is preserved by linear combination.

  • Line 3 is a rearrangement of terms to make apparent the normal centered half-Gaussians Xi+biσi and Xibiσi that were considered in Section 3.

  • Line 4 uses the fact that αi=|si|σiσpas forms a Euclidean unit vector, reducing to the case treated in Section 3.

For the protection level defined in Equation (16), an additional step must be added to demonstrate that the overbounding bias can be integrated in the inflation factor of the standard deviation ξ. This demonstration is identical to that provided by DeCleene (2000).

5 ILLUSTRATION ON GNSS DATA

The proposed method is illustrated here on real GNSS data from the International GNSS Service (IGS) station TLSE (France), for 5 days (from 2021/06/01 to 2021/06/05). We consider GPS and Galileo constellations and dual-frequency measurements: L1/L2 for the Global Positioning System (GPS) and E1/E5a for Galileo. Every 30 s, the range errors Xi are computed based on:

  • the final products from the Center for Orbit Determination in Europe and IGS ANTEX and SINEX BIAS files for the reference GNSS’s orbits and clocks

  • the IGS ANTEX and SINEX antenna files for the precise position of the TLSE station.

These range errors include all error sources: signal-in-space errors (due to errors in GNSS orbits and clocks in IGS final products), propagation errors (due to residual troposphere and ionosphere errors), and local errors (multipath, receiver noise).

The overbounding is applied on Xi/σMOPS,i with σMOPS,i being the standard deviation of range errors described in the MOPS (EUROCAE, 2021; RTCA, 2016). Even if σMOPS,i has not been designed for IGS ground stations (but for airborne SBAS receivers), it appears relevant to reduce the correlation with elevation and consider identically distributed Xi/σMOPS,i for all epochs and lines of sight per constellation.

For each GPS and Galileo constellation, a sample of reduced range errors is constructed with the pseudorange errors for all satellites and epochs such that the elevation is greater than 5°.

For the two constellations, the reduced range errors display a small, yet significant, bias in the median:

  • −0.23 for GPS

  • −0.16 for Galileo

Consequently, we apply the overbounding methods dedicated to biased distributions: the Gaussian paired and two-step overbounding methods with excess mass, as state-of-the-art references, and the wide-sense CDF overbounding, as an illustration of the new method. Even though the computed empirical distribution is only an approximation of the true distribution, we consider that the true error distribution is known and equal to the empirical distribution in this application for illustration purposes.

For the paired overbounding, the excess mass is fixed to 2.5×10−3, as proposed by Blanch et al. (2018). For each constellation, Gaussian paired overbounding is attempted with increasing bias, starting from the median of the reduced range errors. As expected, high biases appeared necessary to obtain a suitable pair of overbounds: 4.9 for GPS, 1.6 for Galileo. These high bias parameters well illustrate the conservatism of paired overbounding with symmetrical overbounds mentioned in Section 2.2 – even with excess mass.

For two-step overbounding, as for paired overbounding, the excess mass is fixed to 2.5× 10 3, and the first step of the overbounding is attempted with increasing bias, starting from the median of the reduced range errors without a trade-off between μ and Σ. The first-step overbound is implemented in accordance with the work by Blanch et al. (2021). The empirical CDF of Xi/σMOPS,i is discretized with a step of 0.01, which leads to an optimization problem with a size below 2500 for each constellation. For the Galileo constellation, a solution is found with μ equal to 0.2, which is slightly higher than the absolute median (0.16). For the GPS constellation, no solution is found until the bias has been increased to μ = 1.6. As for the paired overbounding, we consider a Gaussian two-step overbound in this numerical application.

For the wide-sense CDF overbounding, no excess mass or discretization is applied. The bias μ is arbitrarily fixed to the absolute median: 0.23 for GPS and 0.16 for Galileo.

Figures 3 and 4 illustrate the overbounding performed on the range errors of GPS and Galileo. More precisely, these figures display the folded CDF, defined as the CDF before the median and the survival function (1-CDF) after the median, in order to present a clear view of the tails, which generally drive the overbounding. For the two-step overbounding, we can verify the following:

  • The empirical folded CDF lies between the left and right first-step overbounds both before and after μ.

  • The folded CDF of the left second-step overbound is above the folded CDF of the left first-step overbound before μ (the left second-step overbound is not plotted after μ).

  • The folded CDF of the right second-step overbound is above the folded CDF of the right first-step overbound after Bnom (the right second-step overbound is not plotted before μ).

FIGURE 3

Overbounding of Xi/σMOPS,i for GPS satellites: Gaussian paired overbounding (left), Gaussian two-step overbounding (middle), wide-sense CDF overbounding (right)

FIGURE 4

Overbounding of Xi/σMOPS,i for Galileo satellites: Gaussian paired overbounding (left), Gaussian two-step overbounding (middle), wide-sense CDF overbounding (right)

Figure 5 displays the probability density functions of the first-step overbounds in order to verify that the symmetry and unimodality constraints are satisfied. Indeed, symmetry cannot be verified in Figures 3 and 4 because they take into account excess mass (in order to check overbounding) whereas symmetry applies without excess mass.

FIGURE 5

First-step overbound probability density function of Xi/σMOPS,i for GPS (left) and Galileo (right) satellites

We see that the first-step overbounding is generally very close to the empirical distribution in the core of the distribution. Unfortunately, the second-step overbound is driven by the tails of the distribution, where the first-step overbound is significantly higher than the empirical distribution. Note that the performance of the two-step overbound can most likely be improved at the expense of a fine tuning of the algorithm parameters (such as constraint tolerance, discretization step, etc.) and/or an optimization of the cost function.

Table 2 reports the overbounding mean μ and standard deviation Γ resulting from the different overbounding methods. As expected, the bias and standard deviation of the overbound are higher for the two-step overbounding than for the wide-sense CDF overbounding before inflation. Figure 6 displays the standard deviation of the overbound achieved by two-step overbounding and wide-sense CDF overbounding, including the inflation factor. The inflation factor has been fixed according to the number of contributors to positioning errors n (which is equal to 20) because, in our modeling, the number of contributors is equal to the number of satellites in view. In this example, there is only one contributor per line of sight, which is unlikely to be the case in general. However, we show in Section 3.2.6 how one can remove some contributors from n if they are known to meet the asumptions of the CDF overbounding theorem. The standard deviation Γ obtained by wide-sense CDF overbounding is generally higher than that obtained with the other methods, even if it is close to the value obtained with the two-step overbound for high K-factors (integrity risk below 10−9 per second). The standard deviation obtained for paired overbounding is far below that obtained with two-step overbounding and wide-sense CDF overbounding, but at the price of a high bias μ.

FIGURE 6

Standard deviation of the Yi overbound with respect to integrity for GPS (left) and Galileo (right) constellations

View this table:
TABLE 2

Overbounding Parameters Obtained by Two-Step Overbounding and Wide-Sense CDF Overbounding

To compare the overbounding methods that consider both the bias μ and standard deviation Γ, vertical protection levels (VPLs) for an integrity risk of 10−7 per second are displayed in Figure 7. Every 30 s, the VPL is computed by the Snapshot Positioning Accurate Ranging Kit software, according to Equation (15) with σi = Γ× σMOPS,i.

FIGURE 7

VPL with respect to time for different overbounding methods

The VPLs obtained for the three overbounding methods are very close. The wide-sense CDF overbounding provides a slightly lower VPL than the paired and two-step overbounding, most likely because of the lower bias μ and reasonable increase with Γ. Even if this application is not generalized, this result demonstrates that, despite its simplicity, the wide-sense CDF overbounding method can achieve an availability similar to that of state-of-the-art overbounding methods, especially when the integrity risk and number of contributors to range errors are low.

6 CONCLUSION

This article has proposed a new method for overbounding that smartly combines CDF and paired overbounding in order to relax the unimodality and symmetry assumptions required by CDF overbounding, which are difficult to satisfy in practice. This new method is called wide-sense CDF overbounding, as it relies on milder assumptions than CDF overbounding and leads to less general overbounding properties. More precisely, wide-sense CDF overbounding permits us to discard the unimodality and symmetry assumptions required by CDF overbounding. For a user, the only practical difference between the proposed method and CDF overbounding is the application of an inflation factor in the computation of the protection level, which can be obtained from a table as a function of the number of independent measurements and of the target integrity risk. This method can be extended to biased distributions if necessary. While CDF overbounding is applicable to any integrity risk above the target and any decomposition of pseudorange errors, wide-sense CDF overbounding applies to a fixed integrity risk and number of contributors in range errors. The gain in generality comes at the cost of possible over-conservatism of the overbound. The main advantages of the proposed method are its simplicity of use, robustness, and verifiability.

In practice, wide-sense CDF overbounding consists of the second step of two-step overbounding, which is a simple Gaussian overbound before and after the median, followed by an inflation of the overbounding standard deviation. The inflation factor depends on:

  • the integrity risk

  • the number of contributors to pseudorange, i.e., the number of lines of sight multiplied by the number of errors per line of sight (for instance, 4 if we are separately considering the errors due to GNSS orbits and clocks, troposphere, multi-path, and thermal noise). More precisely, the inflation factor depends on the number of error sources that do not follow the hypotheses of the classical CDF overbound, as discussed in Section 3.2.6.

A table of inflation factors could be hard-coded in the receiver in order to set the correct inflation factor for any integrity risk and number of contributors.

In exchange for the relaxation of assumptions, wide-sense CDF overbounding may be overly conservative, especially when the integrity risk and number of contributors to pseudorange errors are high. Hopefully, future work can reduce this conservatism by providing a tighter bound of the inflation factor.

Usability is most likely the main advantage of wide-sense CDF overbounding over two-step overbounding, which is the state-of-the-art method for handling potential multimodal or asymmetric distributions. Indeed, two-step overbounding requires discretization of the CDF and linear optimization under a constraint in high dimensions.

Robustness is also an asset of wide-sense CDF overbounding. More precisely, the wide-sense CDF overbound always exists as soon as the overbounding bias is greater than or equal to the absolute value of the median. In contrast, a two-step overbound may not exist for some overbounding biases above the median, when the linear optimization problem involved in the first step is infeasible because of the constraints. An increase in overbounding bias and/or excess mass permits one to reach a feasible first step, but this approach has several drawbacks. First, an increase in overbounding bias or excess mass could degrade availability, as illustrated in Section 5. Second, the excess mass must remain low enough to have a negligible impact on the K-factor when the user algorithm does not take excess mass into account in the protection level computation, which drastically limits the degrees of freedom in the first-step overbound. Consequently, wide-sense CDF overbounding could present a good back-up approach for two-step overbounding.

A last advantage of wide-sense CDF overbounding is its verifiability. For an external observer, it would be straightforward to verify that wide-sense CDF overbounding is suitable based on the overbounding bias and standard deviation. In contrast, verifying two-step overbounding without knowing the internal tuning parameters (discretization step, excess mass) and steps of computation (first-step overbound) presents a challenge. Thus, wide-sense CDF overbounding seems to be relevant for monitoring purposes.

Future research could explore the benefits of wide-sense CDF overbounding for the generation or monitoring of integrity parameters, typically for SBASs or ARAIM.

HOW TO CITE THIS ARTICLE

Maliet, O., Mimouni, K., Antic, J., & Trilles, S. (2025). Wide-Sense CDF overbounding for GNSS integrity. NAVIGATION, 72(2). https://doi.org/10.33012/navi.697

APPENDICES

A NUMERICAL UPPER BOUND OF THE SIGMA INFLATION FACTOR

A.1 Constructing a Right Overbound of n*

In this section, we want to construct an explicit right overbound of n* and obtain an upper bound of the inflation factor An,K* that one can use in practical integrity applications. To this end, we will use the following theorem:

Theorem 1 Let (Zi)i1..n be n i.i.d. variables on + with density f such that the function log f(x1/2) is concave. Let a, b be two vectors of +n of equal Euclidean norm ||a||2 = ||b||2. Furthermore, if we have the following condition for all k, 1 ≤ k ≤ n:

i=knb(i)2i=kna(i)218

where a(i) denote the elements of a sorted in ascending order, then we have the following for all t >0:

(aiZit)(biZit)

In other words, biZi is a right overbound of the distribution aiZi.

This theorem is a direct rephrasing of the theorem presented by Yu (2011), also mentioned by Pan et al. (2013) and earlier by Karlin and Rinott (1983) for the case of p = q = 2. The proof of this theorem is beyond the scope of this paper; thus, we refer the reader to these references for further details. In particular, for the specific choice bi=1/n for all i, the condition in Equation (18) is verified for all a of unit norm2, and we determine that 1/nZi is a right overbound of aiZi for all a.

In our case of interest, we want to construct a right overbound of αiZi with α of unit norm. The random variable Zi follows the right half-Gaussian distribution of CDF Φr and does not follow the conditions of Theorem 1 (in particular, the log-concavity condition is not met). Thus, we cannot affirm that the linear combination with equal weights is a right overbound of the other combinations. Actually, this is not the case, as shown by the counter example represented in Figure 8(b).

FIGURE 8

(a) Representation of the CDF R˜n(t) for a few n values; (b) representation of the folded CDF of αiZi for two vectors (αi) of unitary norm: αi=1/5×(1,1,1,1,1) and αi = (0.89,0.24,0.24,0.23,0.21)

However, we can view Zi as a composite random variable that takes a value of 0 with probability 12 and follows a folded Gaussian distribution with probability 12 (the folded Gaussian can be defined as the absolute value of a normal standard Gaussian). In contrast, the folded Gaussian distribution does follow the hypothesis of Theorem 13. Hence, we can set a condition on the number of Zi=0 and then use Theorem 1 for the remaining linear combination of folded Gaussian distributions.

As the number of non-zero Zi follows a binomial distribution, we have the following:

(i=1nαiZit)=k=0n(knon0Zi)(i=1nαiZitknon0Zi)=k=0n12nCkn(i=1nαi𝟙Zi>0Yitknon0Zi)12n+k=1n12nCkn(i=1k1kYit)19

To proceed from line 1 to line 2, we use the explicit value of ℙ(k non-zero Zi) and the fact that Zi follows the same distribution as Yi when conditioned on being strictly positive. The passage from line 2 to line 3 is the application of Theorem 1 for the sum of k i.i.d. Yi random variables, based on the fact that the subsets of elements of vector αi always have a Euclidean norm less than 1.

Definition 2 We define the following function R˜n(t):

R˜n(t)=12n+k=1n12nCkn(1ki=1kYit)20

where Yi are i.i.d. random variables following a right folded Gaussian distribution.

Figure 8(a) shows the CDF R˜n(t) for different values of n. From the argument above, R˜n(t) is a right overbound of n*, and the factor An,K defined as follows:

An,K=R˜n1(Φ(K))K21

is an upper bound of the inflation factor An,K*. This term corresponds to the upper bound shown in Table 1.

We stress that our proposed overbound by R˜n(t) is not optimal and a tighter bound of n* might be proposed in the future, improving the table of inflation factors An,K. This non-optimality is primarily due to the fact that Theorem 1 is applied term by term in the sum after conditioning by the number of non-zero Zi values in Equation (19). Thus, the worst-case coefficients in the final expression depend on which Zi are non-zero and different coefficients are considered in each term of the sum. Consequently, there is no (αi) vector for which R˜n is the CDF of αiZi, and the inequality is strict for any (αi). This non-optimality is illustrated in Figure 8(b).

A.2 Evaluation of the Function R˜n

One way to evaluate the CDF R˜n(t) is to use its characteristic function. The characteristic function of a random variable is the Fourier transform of its probability density function, which, when it exists, entirely defines its probability distribution. The Fourier transform is a classical tool for evaluating sums of random variables and has been used in the context of overbounding, for example, by Yan et al. (2024) to compute position-level overbounding by non-Gaussian range-level overbounds.

The characteristic function of the folded Gaussian distribution is as follows:

φy(k)=12πexp(k22)[1ierfi(k2)]

Because the characteristic function of the sum is the product of the characteristic functions, we can evaluate the CDF of i=1nYi as the inverse Fourier transform of the function:

12πikexp(nk22)[1ierfi(k2)]n

Then, R˜n(t) is obtained as a linear combination and rescaling of the intermediate CDFs.

Footnotes

  • 1 For t2t1, we have α,(Σi|αi|Zit2)(Σi|αi|Zit1); hence, by taking the infimum, we have Rn*(t2)Rn*(t1). Thus, Rn*(t) is an increasing function, with limits 0 and 1.

  • 2 We want to prove that ∀k, nkni=kna(i)2. Because a(i) is ranked in ascending order, there is a rank k0 for which ∀kk0, a(i)1/n and ∀k < k0, a(i)1/n. For k = 0, this property holds because a has a unit norm, and for kk0, the proof is obtained by induction, with i=kna(i)2=i=k1na(i)2a(k1)2nk+1n1n. For kk0, the inequality is true because all terms are larger than or equal to 1/n.

  • 3 For the folded Gaussian, log f(x1/2) = –x/2 + c (where c is a constant), which is a concave function.

This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.

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