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The GNSS integer ambiguities: estimation and validation

The GNSS integer ambiguities: estimation and validation

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Integer Aperture <strong>estimation</strong> 5<br />

In section 3.2 the success rate was introduced. This probability is a valuable measure<br />

for deciding whether one can have enough confidence in the fixed solution. As soon<br />

as the success rate is close enough to one, a user can fix the <strong>ambiguities</strong>, so that the<br />

precise carrier phase measurements start to contribute to the solution. However, when<br />

the success rate is considered too low with respect to a given threshold, it will not yet be<br />

possible to benefit from the precise phase observations. This also means that there is a<br />

probability that the user unnecessarily sticks to the float solution just because the fail rate<br />

is too high. In practice, not only the success rate is considered to decide on acceptance<br />

or rejection of the <strong>integer</strong> solution. <strong>The</strong> <strong>integer</strong> solution is also validated using one of<br />

the methods described in section 3.5. Since no sound <strong>validation</strong> criterion exists yet, in<br />

this chapter a new class of <strong>integer</strong> estimators is defined, the class of <strong>integer</strong> aperture<br />

estimators. Within this class estimators can be defined such that the acceptance region<br />

of the fixed solution is determined by the probabilities of success <strong>and</strong> failure.<br />

<strong>The</strong> new class of <strong>integer</strong> estimators is defined in section 5.1. <strong>The</strong>n different examples<br />

of <strong>integer</strong> aperture estimators are presented. First, the ellipsoidal aperture estimator in<br />

section 5.2, for which the aperture space is built up of ellipsoidal regions. <strong>The</strong>n in section<br />

5.3 it is shown that <strong>integer</strong> <strong>estimation</strong> in combination with the ratio test, difference test,<br />

or the projector test belongs to the class of <strong>integer</strong> aperture estimators. When the<br />

aperture space is chosen as a scaled pull-in region, the <strong>integer</strong> aperture bootstrapping<br />

<strong>and</strong> least-squares estimators can be defined. This will be shown in section 5.4. Finally,<br />

the penalized <strong>integer</strong> aperture estimator <strong>and</strong> optimal <strong>integer</strong> aperture estimator are<br />

presented in sections 5.5 <strong>and</strong> 5.6. Section 5.7 deals with implementation aspects. A<br />

comparison of all the different estimators is given in section 5.8, <strong>and</strong> examples in order<br />

to show the benefits of the new approach are given in section 5.9.<br />

In order to illustrate the principle of IA <strong>estimation</strong>, throughout this chapter a twodimensional<br />

(2-D) example will be used. Simulations were carried out to generate<br />

500,000 samples of the float range <strong>and</strong> <strong>ambiguities</strong>, see appendix B, for the following<br />

vc-matrix:<br />

Q =<br />

Qˆ b<br />

Q â ˆ b<br />

Qˆ bâ<br />

Qâ<br />

Note that Qâ = Qˆz 02 01.<br />

<br />

⎛<br />

0.1800 −0.1106<br />

⎞<br />

0.0983<br />

= ⎝−0.1106<br />

0.0865 −0.0364⎠<br />

0.0983 −0.0364 0.0847<br />

87

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