Global Positioning System Reference
In-Depth Information
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7.7.4 Ambiguity Function
Th e least-squares techniques discussed above require partial derivatives and the min-
im ization of v T Pv , with v and P being the double-difference residuals and double-
di fference weight matrix. The derivatives and the discrepancy terms depend on the
as sumed approximate coordinates of the stations. The least-squares solution is iter-
ate d until the solution converges. In the case of the ambiguity function technique,
we search for station coordinates that maximize the cosine of the residuals. Consider
ag ain the double-difference observation equation
f
c ρ
v pq
km
ϕ pq
km,a
ϕ pq
km,b
pq
km,a
N pq
km,a
ϕ pq
km,b
=
=
+
(7.103)
In usual adjustment notation, the subscripts a and b denote the adjusted and the
observed values, respectively. In (7.103) we have neglected again the residual double-
difference ionospheric and tropospheric terms, as well as the signal multipath term.
The residuals in units of radians are
[26
Lin
5 ——
Lon
PgE
pq
km
v pq
km
ψ
=
2
π
(7.104)
The key idea of the ambiguity function technique is to realize that a change in the
integer N pq
pq
km by a multiple 2
km changes the function
ψ
π
and that the cosine of this
function is not affected by such a change because
cos ψ
km,L =
cos 2
km,L =
cos 2
π v pq
km,L (7.105)
pq
v pq
N pq
π
km,L + ∆
[26
N pq
where
km,L denotes the arbitrary integer. The subscript L , denoting the frequency
id entifier, has been added for the purpose of generality.
There are 2 (R
1 ) double differences available for dual-frequency ob-
se rvations . If we further assume that all observations are equally weighted, then the
su m of the squared residuals becomes, with the help of (7.104),
1 )(S
2
R
1
S
1
2
R
1
S
1
v T Pv x m ,N pq
km,L =
v pq
km,L 2
ψ
km,L 2
1
pq
=
(7.106)
4
π
2
L
=
1
m
=
1
q
=
1
L
=
1
m
=
1
q
=
1
If the station coordinates x k are known, the function could be minimized by varying
the coordinates x m and the ambiguities using least-squares estimation. The ambiguity
function is defined as
2
R 1
S 1
cos ψ
km,L
pq
AF ( x m )
L
=
1
m
=
1
q
=
1
cos 2
f L
c
2
R
1
S
1
pq
km,a
N pq
km,L,a
ϕ pq
km,L,b
=
π
ρ
+
L
=
1
m
=
1
q
=
1
 
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