Global Positioning System Reference
In-Depth Information
The distance from satellite to the center of the earth r can be found as
r = a s ( 1 e s cos E)
( 4 . 40 )
The true anomaly ν can be found from the following equations as
cos 1 cos E e s
1
ν 1 =
e s cos E
sin 1 1 e s sin E
1
ν 2 =
(4.41)
e s cos E
ν
=
ν 1 sign(ν 2 )
The definition of φ is
φ ν + ω
( 4 . 42 )
The er can be found as
ž (t GPS
ž ie t GPS
er =
e +
t oe )
( 4 . 46 )
where t is replaced by t GPS .
The position of the satellite can be found as
x
y
z
r cos er cos φ
r sin er cos i sin φ
=
r sin er cos φ
r cos er cos i sin φ
r sin i sin φ
+
( 4 . 47 )
The satellite position obtained is in earth-center, earth-fixed (ECEF) coordination.
This approach is used to calculate the positions of all the satellites.
Step3. Coordinatetransform . In this operation, three coordinate systems are
included. The user position is usually given in latitude ( L c ), longitude ( l ), and
altitude ( h ). The satellite position is in ECEF system. The final satellite position is
referenced to the user position in east, north, and height. The following coordinate
transform can achieve this goal:
The user position is changed from L c , l ,and h into ECEF system to have the
same coordinate with the satellite position through
a e sin l
x 0 =
1 +
e e ) tan L c + h × cos l × cos L c
( 1
a e cos l
1 + ( 1 e e ) tan L c +
y 0 =
h
×
sin l
×
sin L c
(12.25)
e e ) sin L c
a e ( 1
z 0 =
1
+
h
×
sin L c
e e sin 2 L c
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