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Thesis - Leigh Moody.pdf - Bad Request - Cranfield University

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Chapter 3 / Sensors / NAVSTAR GPS<br />

_ _<br />

The universal navigation constant (G), and the Earth mass (M) define the<br />

WGS 84 gravitational constant (µG),<br />

µ<br />

G<br />

: = G ⋅ M : =<br />

3.11-7<br />

3.<br />

986005 x<br />

10<br />

14<br />

Equation 3.11-11<br />

Transmission quantisation errors and the use of 2 nd order satellite clock<br />

corrections, introduces a pseudorange error of < 0.1 m in the first 1.5 hrs<br />

after a navigation message up-link. Thereafter, the degradation reaches<br />

90 m after 3.5 hrs, Dierendonck (D.17) .<br />

3.11.4 Reference Pseudo-Data<br />

From Kepler’s laws, the satellite period (TS) is related to its orbital rate (ωS),<br />

T<br />

S<br />

: =<br />

2 ⋅ π<br />

ω<br />

S<br />

: =<br />

2 ⋅ π<br />

P<br />

µ<br />

3<br />

r,<br />

s<br />

G<br />

Equation 3.11-12<br />

The satellite period is revised using the correction for the computed orbital<br />

rate (∆ωS) in the Ephemeris data. For simplicity, 24 satellites are modelled<br />

travelling in circular orbits about the Earth centre at a radius (Pr,s) of<br />

20_183 km with an orbital speed (ωS) of 0.00833333 rad/s. The position of<br />

the j’th satellite in the i’th orbital plane is defined by the Mean Anomaly<br />

with respect to the rising node (κij),<br />

∀<br />

( i , j ) : i = [ 1 ( 1 ) 6 ] ; j = [ 1 ( 1 ) 4 ]<br />

κ<br />

ij<br />

: =<br />

ω<br />

S<br />

⋅ t<br />

m<br />

π<br />

+ ⋅<br />

6<br />

( 2 ⋅ i + 3 ⋅ j − 5 )<br />

⇒<br />

Equation 3.11-13<br />

(tm) is the time after midnight General Mean Time (GMT). The position of<br />

a particular satellite in the Orbital frame,<br />

O<br />

r,<br />

s<br />

r,<br />

s<br />

( ) T<br />

cos κ , sin , 0<br />

P : = P ⋅<br />

κ<br />

Equation 3.11-14<br />

A satellite's position with respect to the Celestial frame is therefore,<br />

C<br />

s<br />

C<br />

O<br />

P : = T ⋅ P<br />

The position of the receiver with respect to the Celestial frame is,<br />

O<br />

s<br />

Equation 3.11-15

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