Global Positioning System Reference
In-Depth Information
I ijk
I i jk
L k
I i
j k
I
L i
L j
I i
jk
I ij k
L j
O k
O i
L i
I ij k
O j
L k
I ijk
Fig. 5. Refining the locus of the receiver position under noisy measurement conditions.
Fig. 5 shows the ideal scenario where the position of the receiver to be determined,
, and the
three respective planar form LOPs O i , O j and O k are obtained from any three arbitrary satellite
pairs
ρ
P k .
The equation for L i , L j , L k can be found using (8).
P i ,
P j and
ξ
is constant due to identical receiver clock bias and exposure to similar atmospheric noise.
Hence, L i , L j , L k vary from the ideal noise free LOPs O i , O j , O k by the extra constant terms of
2
For specific measurement instance
r 2 respectively. Crucially their slopes remain unchanged
(Left hand side of (8)), and these are shown by the solid planes L i , L j , L k parallel to O i , O j and
O k in Fig. 5. For non co-planar satellite pairs, L i , L j and L k will have a physical intersection
point
r i 1
r i 2 ,2
r j
r 2 and 2
r 1
ξ
ξ
1
ξ
x ijk , y ijk , z ijk .
I ijk =
r i 1
r i 2 with
Another plane L i
parallel to L i can be found as follows by modifying the term 2
ξ
q r i 1
r i 2 , where q is an arbitrary positive constant.
x i 2
x i 1 x
y i 2
y i 1 y
z i 2
z i 1 z
+
+
=
2
r i 2
r i 1 2
r i 2 2
q r i 1
(34)
i 2
2
i
1
2
p
p
+
The original LOP O i will then pass between the planes L i and L i as the constants have opposite
signs. A similar argument applies to L j , L k so that the parallelopiped bounded by the planes
O i , L i , O j , L j , O k , L k will have an aspect ratio AR
r i 1
r 2 as L i , L j , L k are
: r j
r j
2
r i 2
: r 1
=
1
r i 1
r i 2 ,2
r j
2 and 2
r 1
r 2 distances away from O i , O j and O k respectively as they
r j
2
ξ
ξ
1
ξ
di
er only by the constant terms in (8). The AR of the parallelopiped bounded by the planes
O i , L i , O j , L j , O k , L k will have exactly the same aspect ratio so indicating
ff
ijk and
I ijk ,
I
I
to be the
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