Global Positioning System Reference
In-Depth Information
ε s
S'
S
d m
d m
d u
d u
α
S - Satellite position
S' - Estimated satellite position
M - Reference station position
U - User position
φ m
φ m
M
U
User
p
Reference
station
Figure 8.2
Variation of broadcast ephemeris errors with viewing angle.
d m , and neglecting
the higher order terms in the binomial expansion of the square root in each of these
equations, we obtain
Solving the first equation for
d mu and the second for d u
′ −
1
2
p
d
1
2
dd
′− ′≈− ⋅
pp
+⋅
cos
φα
+′ ⋅
p
sin
φ
+⋅
α⋅⋅
2
p
cos
φ
m
u
m
m
m
m
1
2
p
d
dd
−≈+⋅
pp
−⋅
cos
φ
u
m
m
m
Adding these two equations, we find that the difference between the errors,
ε u
=
dd
′ −
and
ε mmm
=
dd
′ −
, is
u
u
1
2
(
)
(
)
ε
−=′ −′
ε
dd
+
d d
=′ ⋅
α
p
sin
φ
+⋅
α
2
p
cos
φ
mu
u
m
m u
m
m
or
1
2
(
)
(
)
2
ε
ε
=
dd
′−′ +
d d
≤ ⋅⋅
α
p
sin
φ
+ ⋅
α
⋅⋅
p
cos
φ
mu
u
m
m u
m
m
where the equality holds if the estimated satellite position lies in the plane defined
by the user position, reference station position, and true satellite position.
The difference
is the error introduced by the pseudorange correction at
the user. To simplify the expression, assume that the angle
εε
mu
φ m is greater than 5º, that
the separatio n be tween the user and referenc e sta tion is less than 1,000 km, and that
the direction SS
is parallel to the direction MU . Then
ε
sin
φ
=
ε
S
m
S
sin 2
ε
−≤⋅
ε
α
p
sin
φ
⋅⋅
p
sin
φ
⋅⋅
p
φ
(8.1)
mu
m
m
m
d
d
m
m
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