Global Positioning System Reference
In-Depth Information
where
x
,
y
,
z
and
x
u
,
y
u
,
z
u
are the coordinates of the satellite and the user,
respectively,
c
is the speed of light. Use this transit time to modify the angle
er
in Equation (4.49) as
˙
ie
t
t
er
⇒
er
−
(
9
.
23
)
Use this new
er
in the first portion of Equation (9.19) to calculate the satellite
position
x
,
y
,
z
in the new coordinate system. From these satellite positions, the
user position
x
u
,
y
u
,
z
u
will be calculated again from Equation (9.21).
These four equations (9.19), (9.21), (9.22), and (9.23) can be used in an iter-
ative way until the changes in
x
,
y
,
z
(or
x
u
,
y
u
,
z
u
) are below a predetermined
value. The final position will be the desired user position
x
u
,
y
u
,
z
u
.
9.14 CHANGING USER POSITION TO COORDINATE SYSTEM
OF THE EARTH
Once the user position
x
u
,
y
u
,
z
u
in Cartesian coordinate system is found, it
should be converted into a spherical coordinate system, because the user position
on the surface of the earth is given in geodetic latitude
L
, longitude
l
, and altitude
h
as shown in Equations (2.17) - (2.19):
x
u
+
r
=
y
u
+
z
u
tan
−
1
z
u
L
c
=
x
u
+
y
u
tan
−
1
y
u
x
u
=
l
(9.24)
where
L
c
is the geocentric latitude. However, the surface of the earth is not
a perfect sphere; the shape of the earth must be taken into consideration. The
geodetic latitude
L
is used in maps and should be calculated from
L
c
through
Equations (2.50) or (2.51) as
L
=
L
c
+
e
p
sin 2
L
or
L
i
+
1
=
L
c
+
e
p
sin 2
L
i
(9.25)
where
e
p
is the ellipticity. The second portion of the above equation is written
in iterative form. The altitude can be found from Equation (2.57) as
x
u
+
y
u
+
z
u
−
a
e
(
1
−
e
p
sin
2
L)
h
=
(
9
.
26
)
These last three values, latitude
L
, longitude
l
, and altitude
h
, are the desired
user position. The latitude and longitude are often expressed in degrees, minutes,
and seconds or in degrees and minutes.
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