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The GNSS integer ambiguities: estimation and validation

The GNSS integer ambiguities: estimation and validation

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µ<br />

200<br />

100<br />

10<br />

2<br />

1<br />

1 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.81.9 2<br />

p<br />

f<br />

µ<br />

2<br />

1.9<br />

1.8<br />

1.7<br />

1.6<br />

1.5<br />

1.4<br />

1.3<br />

1.2<br />

1.1<br />

1<br />

1 2 10 100 200<br />

p<br />

f<br />

Figure 5.14: µ as function of the penalty pf with ps = 0 <strong>and</strong> pu = 1. Left: pf = 1, . . . , 2;<br />

Right: pf = 2, . . . , 200.<br />

2-D example<br />

In order to get an idea of the shape of the aperture space, Qˆz 02 01 from appendix B<br />

is chosen as the vc-matrix, the corresponding PDFs of the float <strong>ambiguities</strong> <strong>and</strong> the<br />

ambiguity residuals are determined, <strong>and</strong> then the inequality (5.48) is used to find Ω0 as<br />

function of µ.<br />

Figure 5.15 shows the results. Furthermore, figure 5.14 shows µ as function of the<br />

penalty pf > 1, where ps = 0 <strong>and</strong> pu = 1. In this case µ → 1 for pf ↓ pu. <strong>The</strong><br />

reasoning behind this choice is that it seems realistic that no penalty is assigned in<br />

the case of correct <strong>integer</strong> ambiguity resolution, <strong>and</strong> also that the penalty in the case<br />

of incorrect <strong>integer</strong> ambiguity <strong>estimation</strong> is larger than the penalty in the case of ’no<br />

decision’ (undecided). This implies that in order to minimize the average penalty E{p},<br />

the fail rate Pf should be as small as possible in all cases, <strong>and</strong> the probability of no<br />

decision Pu should also be small, especially if pf ↓ pu. Thus the success rate should be<br />

as large as possible in all cases, which is the case if the PDF of â is peaked. However,<br />

for very small values of µ (close to one), the undecided rate will become large since then<br />

the aperture space will be small. This results in lower success rates.<br />

It can be seen that the shape of Ω0 is a mixture of an ellipse <strong>and</strong> the shape of the pull-in<br />

region. <strong>The</strong> reason is that the contour lines of fâ(x) (see top panel of figure 5.15) are<br />

ellipse-shaped, but those of fˇɛ(x) (center panels) are not. It is clear that for larger µ<br />

the aperture space becomes larger.<br />

Penalized Integer Aperture <strong>estimation</strong> 109

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