The GNSS integer ambiguities: estimation and validation
The GNSS integer ambiguities: estimation and validation
The GNSS integer ambiguities: estimation and validation
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in order to guarantee a low fail rate the critical value should somehow depend on the<br />
distance to all <strong>integer</strong> vectors in the neighborhood of â, where the distance is measured<br />
in the metric of Qâ.<br />
2-D examples<br />
By comparing 2-D aperture pull-in regions of the RTIA, DTIA <strong>and</strong> OIA estimators, it is<br />
possible to get a better idea of the differences in performance of the three estimators.<br />
<strong>The</strong>refore three aperture pull-in regions for are plotted for different vc-matrices in figure<br />
5.25. <strong>The</strong> following vc-matrices are considered:<br />
2<br />
3 Qˆz 02 01, Qˆz 02 01, 4Qˆz 02 01, Qˆz 02 01 +<br />
<strong>The</strong> regions correspond to the following three situations:<br />
<br />
0.8 0<br />
0 0<br />
a : µ chosen such that for each estimator the fail rate is obtained for which the percentage<br />
of RTIA / DTIA solutions identical to the OIA solution, Pid, is minimum;<br />
b : Ratio Test with fixed critical value of µ = 0.5,<br />
µ for DTIA <strong>and</strong> OIA chosen such that fail rates of all estimators are equal<br />
c : all estimators with fixed fail rate of Pf = 0.025<br />
It follows that the first situation, smallest Pid for the same fail rate, in general occurs<br />
when the OIA pull-in region just touches the ILS pull-in region, <strong>and</strong> thus the aperture<br />
parameter is large. <strong>The</strong> reason is that for a large aperture parameter the shape of the<br />
RTIA <strong>and</strong> DTIA pull-in regions start to resemble the shape of the ILS pull-in region<br />
<strong>and</strong> is larger in the direction of the corner points of the ILS pull-in regions where little<br />
probability mass is located. <strong>The</strong> OIA pull-in region, on the other h<strong>and</strong>, touches the<br />
ILS pull-in regions there where more probability mass is located in Sa, since the PDF<br />
of â is elliptically shaped. <strong>The</strong> smallest Pid is not obtained for a large aperture pull-in<br />
region when the precision is so high that the PDF of â is peaked since then there is little<br />
probability mass close to the boundaries of the ILS pull-in region.<br />
If the aperture pull-in regions are chosen even larger than shown in figure 5.25, the OIA<br />
pull-in region is cut off by the ILS pull-in region. So, if µ is increased the OIA pull-in<br />
region cannot exp<strong>and</strong> in all directions, <strong>and</strong> therefore the fail rate will not change much.<br />
<strong>The</strong> aperture pull-in regions of the RTIA <strong>and</strong> DTIA estimators are especially different<br />
from those of the OIA estimator in the direction of the vertices of the ILS pull-in region.<br />
That is because in those directions there are two <strong>integer</strong>s, ǎ2 <strong>and</strong> ǎ3 with the same<br />
distance to â, but only â − ǎ22 is considered by the ratio test <strong>and</strong> difference test,<br />
Qâ<br />
whereas with OIA <strong>estimation</strong> the likelihood of all <strong>integer</strong>s is considered.<br />
Using a fixed critical value for the ratio test (b) results in very different <strong>and</strong> sometimes<br />
large fail rates, depending on the vc-matrix. <strong>The</strong> reason is that the size of the aperture<br />
pull-in regions is not adjusted if the precision changes. This can be seen for the first<br />
128 Integer Aperture <strong>estimation</strong>