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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