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

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Chapter 3 / Inertial Navigation<br />

_ _<br />

ZA<br />

o<br />

YA<br />

EQUATORIAL<br />

PLANE<br />

XA<br />

ZC ; ZE<br />

r<br />

q<br />

IMU-1<br />

d<br />

3.3-3<br />

YG<br />

u<br />

ZB<br />

ZG<br />

YB<br />

XB<br />

XG<br />

n<br />

ZW<br />

XC<br />

c<br />

ω E<br />

CE<br />

XW<br />

XP<br />

m<br />

YW<br />

YP<br />

XE<br />

CELESTIAL<br />

REFERENCE<br />

Figure 3-22 : Transfer Alignment Frames of Reference<br />

3.3.1.1 IMU-1 Input Derived From External LGA Data<br />

IMU-2<br />

Suppose that the position of point (u) is defined by 3D geodetically<br />

referenced way-points. Its geodetic velocity, acceleration and piecewise<br />

constant jerk can then be obtained at the IMU reference frequency (fR) of<br />

800 Hz (a sub-frame interval ∆R of 1.25 ms) from cubic splines passing<br />

through the way-points. The inertial angular rate expressed in the Body<br />

frame comprises the Earth’s Siderial rate, tilt rate and the rate of rotation of<br />

the missile with respect to East-North-Up (ENU) LGA,<br />

ω<br />

B<br />

C,<br />

B<br />

B<br />

G<br />

G<br />

C,<br />

G<br />

B<br />

G,<br />

B<br />

B<br />

G<br />

G E G B<br />

( T ⋅ ω + ω ) +<br />

: = T ⋅ ω + ω : = T ⋅<br />

ω<br />

E<br />

C,<br />

E<br />

E,<br />

G<br />

The Earth rate and the tilt rate of (G) over the Earth are respectively,<br />

G<br />

C,<br />

G<br />

G<br />

E<br />

E<br />

C,<br />

E<br />

G,<br />

B<br />

XM<br />

Equation 3.3-1<br />

( ) T<br />

− λ&<br />

, µ & ⋅ cos λ , µ ⋅ sin<br />

ω : = T ⋅ ω +<br />

& λ<br />

d<br />

d<br />

d<br />

d<br />

d<br />

Equation 3.3-2

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