14.02.2013 Views

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

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

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

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

Chapter 3 / Inertial Navigation<br />

_ _<br />

3.3.1.3 IMU-2 Kinematics<br />

Extending the dynamic analysis of the Master IMU to the angular rate of the<br />

Missile Body frame (M) in a flexible missile attached to a pylon on the wing<br />

of an aircraft,<br />

ω<br />

M<br />

C,<br />

M<br />

M<br />

P<br />

P P W W B<br />

M<br />

( ω + T ⋅ ( ω + T ⋅ ω ) ) +<br />

: = T ⋅<br />

ω<br />

W,<br />

P<br />

3.3-8<br />

W<br />

B,<br />

W<br />

B<br />

C,<br />

B<br />

P,<br />

M<br />

Equation 3.3-30<br />

Wing motion with respect to the fuselage comprises wing bending and low<br />

frequency wing flexure in the frequency range < 1 Hz and 5-15 Hz; these<br />

are complex functions of fuel and armament load, aircraft speed, turn rate,<br />

buffet and vortex shedding. Pylon motion with respect to the wing has a<br />

spectral content of typically 30-50 Hz. Missile vibration is constrained by<br />

its supports, stiffness, and the mode of vibration, a function of the number<br />

of supports and the distance between them. The effect of these static and<br />

dynamic components is twofold. Low frequency motion effects target<br />

designation performance and the ability of the weapon system to keep the<br />

target in the seeker field-of-view. High frequency motion causes the energy<br />

falling on the seeker detector to be smeared when using IR staring arrays<br />

reducing the acquisition range and accuracy. When studying the effect of<br />

this motion on the seeker smear it must be modelled, not at the highest<br />

modal frequency within the seeker bandwidth (70-100 Hz), but at a<br />

frequency commensurate with the internal gimbal dynamics and the detector<br />

stare time, typically > 2 kHz.<br />

These models are derived from instrumented wing, pylon and missile data<br />

and it is extremely difficult to isolate the individual noise components<br />

comprising the overall spectra and the cross coupling between axes. Data<br />

reduction invariably results in separate, none co-ordinated roll-pitch-yaw<br />

spectra that are a function of the operating conditions. Flexure models are<br />

thus partitioned into a static elements associated with the wing, pylon<br />

attachment, missile supports and missile body misalignment. Thus the<br />

orientation of the Missile Body frame with respect to the Launcher Body<br />

frame comprises a nominal orientation, onto which is superimposed small<br />

angle transforms representing the quasi-static and flexure components<br />

denoted by “N”, “S” and “F” respectively,<br />

M<br />

B<br />

M<br />

DTB<br />

M<br />

STB<br />

M P W<br />

( T ⋅ T T )<br />

T : = ⋅ ⋅<br />

⋅<br />

N<br />

P<br />

N<br />

W<br />

N<br />

B<br />

Equation 3.3-31<br />

The various static misalignments, such as the residual harmonisation angle<br />

of the pylon and missile, are modelled as initial zero mean, Gaussian errors.<br />

Wing bending is treated as a quasi-static misalignment that is a function of<br />

say speed and turn rate. When designating targets it is this component of<br />

structural motion that some aircraft attempt to compensate for, not the<br />

higher frequency pylon noise that invariably requires a small scan pattern.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!