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guidance, flight mechanics and trajectory optimization

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with the rocket motor which is to supply the braking thrust. Data taking<br />

<strong>and</strong> processing requirements could also place a particular requirement on .<br />

For a generalization to finite thrusts, see below Section 2.3.1 <strong>and</strong> the work<br />

of Tschauner <strong>and</strong> Hempel (Reference 1.k).<br />

2.2.4.3 Extension to Non-Circular Orbits<br />

The state transition matrix used in the derivation of the required<br />

velocity in the last section was limited to circular orbit . If the<br />

transition .matrix of Equation (1.58) is replaced by the symbolic notation<br />

--pi $1 ,<br />

the technique of the previous section can be'applied to any orbit. In the<br />

case of a circular orbit, the transition matrix has been given (Equation 1.58<br />

or Figure 1.58). For other orbits, the matrix is available in an analytic<br />

form (Reference 1.1, 1.5, 1.6, 1.9). References 1.1 <strong>and</strong> 1.9 gives ex-<br />

'pressions for transition matrices for elliptic <strong>and</strong> hyperbolic orbits. For<br />

extension to finite thrust, see the work of Tschanner (Reference 1.5 <strong>and</strong> 1.6)<br />

Very little use appears to have been made of the results for elliptic<br />

target orbits <strong>and</strong> it is suggested here that they should be of significant use.<br />

For example, possibly the use of the long set of approximate equations for<br />

orbits of small eccentricity developed by Anthony <strong>and</strong> Sasaki (Reference 1.2<br />

<strong>and</strong> Section 2.2.4.5 below) could be replaced entirely <strong>and</strong> with no limitation<br />

on eccentricity.<br />

2.2.4.4. Multiple Impulse Rendezvous<br />

A modification of the previous scheme developed by Shapiro (Reference 2.11)<br />

employs several velocity corrections <strong>and</strong> drives the range rate to zero by the<br />

successive application of velocity pulses rather than by a single impulse at<br />

zero range. This technique achieves a degree of flexibility over the previous<br />

scheme in that it is also applicable to targets in an elliptical orbit.<br />

The first velocity correction is computed from Equation (2.11) based on<br />

a fictitious time to rendezvous r . Subsequent velocity corrections are<br />

computed on the basis of a time to rendezvous equal to ( f - kt) where t is<br />

the time elapsed since the initiation of the .rendezvous'maneuver <strong>and</strong> k is a<br />

constant. The desired velocity magnitude decreases at each computation<br />

period because of the dilated<br />

see that this is so, consider<br />

the approximations &ir-g~!)<br />

are valid <strong>and</strong> Equation (2.2.1)<br />

time scale <strong>and</strong> approaches zero as t --c 74 .<br />

the solution (2.11) as t -G T/J . Inn $$-$y,<br />

c fi(-r-dt) <strong>and</strong> Eaon (-r-At) =<br />

reduces to<br />

2<br />

"<br />

‘20<br />

43

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