This subsection is focused on the horizontal potential conflicts between the pattern pair 1–1 of the flow pair F4–F24, where the second flight belongs to F24 (i.e., the flight of F4 is already within LECMBDP).
The CD performance is evaluated from two perspectives. Firstly, the HTP performance impact assessment considers the two differently modeled HTPs, alongside a selection of , which are selected as they represent different levels of uncertainty. Secondly, the examination of the effects of dynamic thresholds involves the , which sets the notification threshold, and , which influences the estimation of encounter probability.
3.2.1. System Dynamic Range
The estimated probability, and consequently the CD performance, are intimately related to the performance of the trajectory predictors used in the detection process. This dependency can be observed in the SDR graphs, which compare the predicted time separation and the estimated encounter probability.
Figure 11 presents the SDR graphs of the pair F4–F24 using different HTPs, time difference thresholds, and evaluation arc-lengths. It contains four graphs. The figures of column A are obtained using MLP-HTPs whereas those for column B are obtained using XGB-HTPs. The two upper graphs show the SDR curves across
when
= 60 s, and the lower two show the variation in
when
= −108 NM (entry point at LECMBDP).
In the four graphs, each point represents a flight pair whose encounter probability is greater than zero. Points of the same colour form the SDR distribution of the same evaluation arc-length or threshold . Each distribution has its corresponding logistic fit in the same colour.
Regarding the variation by
, all logistic fits intersect with the black step function, which represents the ideal CD performance, around a midpoint. At this intersection, the
is approximately
and the encounter probability is about 0.5. Due to the characteristic of the probability estimation formula, Equation (
2) simplifies when
, as shown in Equation (
10), as follows:
As error function is bounded within the range of −1 and 1 and is positive, the resulting probability is 0.5 at this point in the distribution. Therefore, the transition area is centred around this midpoint; as increasingly deviates from , the resulting probabilities asymptotically approach the extremities of zero and one.
In addition, the prediction uncertainty diminishes as increases, because the flights are approaching the critical point. Consequently, the SDR distribution progressively approximates ideal behaviour, characterised by a steeper slope.
Regarding the variation by
, it is noteworthy that the maximum probability of the SDR escalates with increasing
until it reaches 1. The maximum encounter probability occurs when
0 s, where the probability estimation (Equation (
2)) simplifies to the following form:
As result, the encounter probability will equal the error function of . The ideal result will be P = 1 for 0 s. Given the characteristics of the error function, the larger is, the closer to one the output of the error function will be. Therefore, the maximum probability achievable is determined by the selected threshold and the performance of the predictor and is a necessary condition to approach optimum performance.
To check the condition, the highest
of both flows for the first critical point are selected, which correspond to the prediction errors at their corresponding entry point (see
Table 5). The
of MLP-HTPs for F4 and F24 are 20.78 and 17.73 s, respectively, resulting in a
(using Equation (
4)) of 27.31 and
. On the other side, the
of XGB-HTPs are 21.15 and 15.56 s, respectively, resulting in
. Thus, the results of both predictors reached a probability of one when the time separation equals 60 s. However, for a
of 10 and 30 s, the maximum probability achievable is less than one, because
, resulting in a distribution with a reduced maximum value.
Although the overall deviation of the predictors is slightly lower in MLP-HTPs for F4 for low
and
, the low
in XGB-HTPs for F24 compensates for the error and leads to a set of lower
, as reflected in
Table 5. As a result, the XGB-HTPs’ distributions exhibit a more pronounced slope than those of the MLP-HTPs.
The analysis of the SDR graphs is further detailed by examining the parameters of the logistic functions (see
Figure 12). The values that lead to a optimum SDR are:
In
Figure 12, the optimal values of L, k, and b are achieved in the CD tool for the
values of 60, 90, and 120 s, and they remain constant. This constancy is because they all satisfy the condition of
for any given
, whereas for
values of 10 s and 30 s, the parameters are far away from optimal. As uncertainty decreases with increasing
, the parameters of these curves approach the optimal. Specifically, for 30 s, the SDR curve meets the optimal values for L, k, and b at −28 NM. For the same reason, the logistic parameters of CD using XGB-HTPs reach the optimal values earlier than those using MLP-HTPs.
As result, the SDR and its associated logistic parameters facilitate setting the performance requirements for the trajectory predictors used in the detection process. By selecting the appropriate logistic parameters, the SDR curve that aligns with the expected CD output distribution and performance (to be analysed in
Section 3.2.2) can be constructed, and the key points of the SDR will delineate the required TP accuracy. In the adaptive CD tool, where the dynamic parameters are adjustable during operation, the TP requirements may vary accordingly, to sustain CD performance across various CD configurations. This approach ensures flexibility in selecting the CD configuration while consistently upholding CD performance.
3.2.2. System Tuning Envelope
For the variable STE, the CD performance variations, mainly the accuracy, arising from HTP performance and dynamic thresholds are examined.
The resulting STE curves are presented in
Figure 13. Each curve is composed of several points, which represent the proportion of nuisances and missed alerts for a given
. The two graphs on the first row present the variation of the STE curves by
for a fixed
= 30 s, and the other two illustrate the variation by
for a fixed
= −108 NM. In this subsection, the selected
is 30 s to visualise distinct variations, because it is the closest value to the maximum
, as presented in
Section 3.2.1.
In general, despite the fluctuations in the curves, the STE curves exhibit a clear trend across , where the proportion of nuisances and missed alerts decreases as increases, approaching the critical point. This phenomenon is due to the reduction in the size of the sample of potential conflicts; as increases, many flights have already flown over the critical point, and the potential interaction is cleared.
Regarding the HTP-induced variation, XGB-HTPs generally exhibit a higher proportion of FAs, whereas MLP-HTPs show a greater proportion of MAs. This phenomenon, taking into account the smaller standard deviation of XGB-HTPs’ residuals, is caused by the use of the error function (
and
) in the probability estimation, using Equation (
2). The error function is a sigmoid function in nature, whose slope depends on
. A lower
in XGB-HTPs causes the function to have a steep slope, leading to a rapid transition to extreme values as the predicted time separation deviates from
, resulting in a sharp probability transition and thereby an increase in notified positives and FAs. In contrast, MLP-HTPs, with higher
values, induce a gradual slope in the error function, manifesting a slower probability transition over the predicted separation range and a tendency towards more MAs due to a less pronounced probability change.
The CD performance variation due to the larger disparity of the predictors’ accuracy is assessed by comparing results at different evaluation points. As presented in
Figure 13, the FA and MA proportions both decrease with an increase in
. This reduction is caused by two factors. Firstly, a higher
leads many flights to overfly the critical point, making the interaction impossible and consequently reducing the interaction sample size. Second, the uncertainty diminishes as
increases, enhancing the accuracy of probability estimations and resulting in higher rates of True Positive (TP) and True Negative (TN).
Figure 14 provides two flight pair examples, showcasing significant probability variation over
, converting what initially appear as FAs and MAs into TNs and TAs, respectively. In the blue one, although it is a conflict-free flight pair, whose
lies above
= 30 s, the estimated probability at
= −108 NM is relatively high at 0.61, making it possible to be notified and then classified as an FA. However, as the uncertainty decreases, this probability decreases to zero when
reaches −28 NM, allowing the tool to accurately identify this case as conflict-free. The second flight pair presents the opposite case: a RP with an initial low estimated probability of 0.2 that escalates to 0.84 at
= −8 NM, close to the sector boundary of PAU.
Concerning the variation by
at
−108 NM, the observed trend is inconsistent. The FA and MA proportions initially decrease with increasing
up to 60 s, followed by a slight increase at 90 s and 120 s. The sample sizes and the error function again influence the results. RP and CD notifications are both dependent on
; the size of both samples increases with less strict
. In terms of the error function, unlike the variation by
, changing the
does not affect the overall steepness of the curve; it changes the point along the existing sigmoid curve. Given the same
and predicted separation, the difference between
and the predicted separation increases with
, where the estimated point is likely to be located at the extreme steep regions.
Table 6 shows an example, illustrating changes in analysis sample size with different
.
These graphs could assist the user in selecting the most appropriate CD operating point for the operation, depending on LAT, by choosing suitable dynamic thresholds. First, this involves selecting the most appropriate that exhibits the lowest proportions of FAs and MAs.
Secondly, the selection of determines the notification of predicted alerts, representing the trade-off between FAs and MAs. The dynamic nature of is beneficial during the operation. A low implies a higher proportion of nuisances and fewer missed alerts, while a high implies fewer nuisances and more missed alerts. The trade-off is tailored to the specific roles and tasks of the executive and planner controller, as well as to the look-ahead time.
On one hand, a large LAT allows for the consideration of a low rate of MAs and a reduction in the number of missed alerts. This is considering the greater TP prediction error and more available time for the controller to further evaluate the situation at a large LAT. Consequently, this implies selecting a low .
On the other hand, as flights approach the critical point, a higher operating point that prioritises highly probable encounters becomes more appropriate. This is aimed at short LATs, to reduce false alerts by notifying interactions that require immediate actions and thus avoiding overwhelming the controllers.
Hence, the STE facilitates the selection of different operating points for the adaptive CD tool, depending on the corresponding LAT.
CD Stability
The stability of the estimated probability cannot be directly discerned from the previous figures of merit; it requires the examination of specific instances. The analysis, based on the two flight pairs selected in
Section 3.1, demonstrates that CD stability is influenced by the stability of the predictions, as depicted in
Figure 15. Moderate fluctuations in the predictions result in smooth variation in the estimated probability with
, while large irregularities result in high-frequency fluctuations.