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ESA Document - Emits - ESA

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s<br />

Inclination (deg)<br />

47.5<br />

47<br />

46.5<br />

46<br />

45.5<br />

The total dV is143.5 m/s.<br />

Master and Flyer Inclination Evolution<br />

Master<br />

Flyer<br />

45<br />

0 2000 4000 6000<br />

Time (s)<br />

8000 10000 12000<br />

4.5.2.4.1.1 Intermediate rendezvous<br />

Figure 4-109: Inclination evolution<br />

HMM<br />

Assessment Study<br />

Report: CDF-20(A)<br />

February 2004<br />

page 373 of 422<br />

After any plane change, the chaser is at 50 km below the target and at 140 km behind it. A<br />

Hohmann transfer is executed to move the Orbiter towards the MAV, from a point 20 km behind<br />

the target and in V-bar (see Figure 4-110).<br />

For the intermediate rendezvous, a trade-off was mad between several substrategies:<br />

• To place the MAV above and ahead drifts backwards towards the target<br />

• To place the MAV below and behind drifts in front of the target<br />

• To place the MAV below and ahead drifts the MAV in from of the orbiter<br />

Finally, the last substrategy was selected: To place the MAV below and ahead. It is a quick<br />

transfer based on Shuttle guidance to ISS docking port that has very good manual backup<br />

features.<br />

After the Hohmann manoeuvre, a tangential transfer in V-bar is executed to place the chaser 1<br />

km ahead of the target maintaining it still in V-bar.<br />

At that point a station keeping is commanded and a series of test start. These hold points will<br />

allow the astronauts to verify the authorisation to proceed for the next phase. The hold point is<br />

expensive in terms of fuel. It accounts for for the following tasks:<br />

• Checking out subsystems.<br />

• Occurrence for the sub-solar angle: Earth-orbiter-Sun angle more than 5 degrees.<br />

• Communication with Earth for the ATPs (Authorisation to Proceed) to the next point.

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