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guidance, flight mechanics and trajectory optimization

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The velocity correction, SVtO) represent the corrections which must be<br />

added to the "first order" require: velocity so that the miss distance at<br />

rendezvous will be reduced to zero.<br />

Figures 2.9 <strong>and</strong> 2.10 (taken from Reference 2.12) illustrate a comparison<br />

of the first <strong>and</strong> second order scheme described above.<br />

KcyfaFlg5to9<br />

lo = 50 NM<br />

A: With fint-whr AV1<br />

m mldsouna correctIon.<br />

5: WI”, fint-dar AV,<br />

ona mld-cms comestIm.<br />

0<br />

1 I<br />

m<br />

I I<br />

40<br />

I I<br />

M)<br />

I I1<br />

80<br />

R.n&zrun Tlfw, 1, Mln<br />

Figure 2.9<br />

Figure 2.10<br />

As can be seen in these figures, the effectiveness of the improvement depend<br />

upon the initial separation distance <strong>and</strong> rendezvous time r . As a consequence<br />

of reducing the number of midcourse corrections, the second order<br />

technique requires a smaller total A V to perform the rendezvous maneuver.<br />

This difference<br />

times.<br />

becomes more significant for large initial separations <strong>and</strong><br />

2.2.4.6 Direct Calculation using Two-Body Orbits<br />

Perhaps the most straightforward method of determining the impulsive<br />

velocity required for rendezvous is obtained by using the equations of<br />

absolute motion of the two vehicles. The relative notion can then be de-<br />

termined as the difference of the respective absolute motions. However, since<br />

the relative positions <strong>and</strong> velocities will be several orders of magnitude<br />

smaller than their absolute counterparts, it is seen that great computational<br />

precision is required. Furthermore, the errors in the knowledge of the orbits<br />

of the two vehicles must be small in order to maintain acceptably small errors<br />

in the relative motion. The method has the advantage, however, of providing<br />

48<br />

10-S<br />

E /

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