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ESA Document - Emits - ESA

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s<br />

5 Reduce 2dB pointing precision to 2µrad.<br />

6 Problems when angular distance between Sun- G/S – Spacecraft is low.<br />

HMM<br />

Assessment Study<br />

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

February 2004<br />

page 209 of 422<br />

The development of space-qualified cavity dump lasers [RD51] is expected to solve the two first<br />

problems. As regards the third problem, adaptative optics for downlink in G/S are expensive, but<br />

are considered state of the art.<br />

One of the main problems for laser links is the high pointing accuracy needed (around 2 µrad in<br />

this case). The approach is based on using high bandwidth inertial sensors to compensate for<br />

jitter excursions caused by spacecraft vibrations. This use of high bandwidth inertial sensors,<br />

together with a fine pointing mirror (see Figure 3-57), would enable the implementation of laser<br />

communication links by achieving submicro radian-pointing precision [RD45]. As a reference,<br />

<strong>ESA</strong>-Artemis is obtaining 3 µrad of pointing accuracy.<br />

In this report, a minimum SEM angle of 10° for laser communications feasibility was taken,<br />

which is a conservative value. A lower minimum SEM angle (3°) is considered in [RD47].<br />

Two laser transmitter options have been considered, the first is a 30.5 cm telescope transmitting<br />

5W, and the second is a 50cm telescope transmitting 20W. See Table 3-41 for details.<br />

The 30.5 cm telescope with a 5W laser is enough from the point of view of data rate (it covers<br />

the average downlink data rate shown in Table 3-40) and the pointing precision needed is lower.<br />

Nowadays, a maximum power of approximately 1.5W is achievable, 5W is a more realistic<br />

option than the 20W. Therefore, the 30.5 cm and 5W option has been selected.<br />

Mirror diameter Transmitted power Expected data rate Pointing accuracy<br />

2.7 A.U. - 0.7 A.U. (3dB beamwidth)<br />

30.5cm 5W 10 Mbps-250Mbps 6 µrad.<br />

50cm 20W 100 Mbps-1Gbps 2.5 µrad<br />

Table 3-41: Laser transmitter considered options.<br />

Figure 3-57: Pointing detector system. It is used together an inertial sensor.<br />

3.3.7.4 Communications continuity<br />

An analysis of communications during solar superior conjunction is done in section 3.3.7.2.5

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