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OLSG Report_Final_06_05_12 - Interagency Operations Advisory ...

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Optical Link Study Group (<strong>OLSG</strong>) <strong>Final</strong> <strong>Report</strong><br />

IOAG.T.<strong>OLSG</strong>.20<strong>12</strong>.V1<br />

• The data rate is 10 Gb/s.<br />

• Data are transmitted only above 20° elevation.<br />

• An example set of nine globally located ground terminals may provide optical<br />

communications to the satellite<br />

From these assumptions we deduce:<br />

• The average amount of data dumped per contact is 3 Tbit (= 5 min x 10 Gb/s).<br />

• With 15 orbits/day, the satellite shall dump, on average, 800 Gbit per orbit (= [<strong>12</strong><br />

Tbit/day]/[15 orbits/day]) with a high probability. Thus, 80s (= [800 Gb/orbit]/[10<br />

Gb/s]) of contact time per orbit is required.<br />

Table 7 summarizes the ConOps parameters for the LEO Scenario.<br />

Table 7: LEO Scenario Concept of <strong>Operations</strong> Parameters<br />

LEO Scenario<br />

Onboard Data<br />

Collection Rate<br />

Onboard Storage<br />

Capacity<br />

Hours of CFLOS<br />

Required per Day<br />

Data Rate used<br />

for Link Budget<br />

<strong>12</strong> Tb/day 2.3 Tb 0.3 10 Gbps<br />

3.1.2 Space Terminal<br />

In this section, five different concepts for LEO flight terminals are presented: DLR-IKN’s<br />

Optical Space Infrared Downlink System (OSIRIS), the DLR/Tesat Laser Communication<br />

Terminal (LCT), the Optel-µ terminal, NASA JPL’s 10-Gb/s terminal, and the Small Optical<br />

Transponder (SOTA) from Japan’s National Institution of Information and Communication<br />

Technology (NICT).<br />

The space terminal must provide the functions described in the ConOps:<br />

• Optical head<br />

• Communication system<br />

• PAT system<br />

• Onboard storage<br />

The electro-optics box includes lasers, laser amplifiers, encoder and modulator, data<br />

formatting and spacecraft electrical interfaces. For most LEO satellites, the laser terminal<br />

should possess its own coarse pointing assembly (CPA), which typically takes the form of a<br />

periscope. Additionally, a fine pointing assembly (FPA) and optical tracking sensor should<br />

both operate with an angular error that is much smaller than the downlink beam<br />

divergence. A point-ahead angle (PAA) around 50 µrad should be implemented.<br />

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