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OLSG Report_Final_06_05_12 - Interagency Operations Advisory ...

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3.2 Highly Elliptical Earth Orbit (HEO) Scenario<br />

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 HEO Scenario is not elaborated as it is considered similar to the Lunar Scenario with<br />

shorter distances.<br />

3.3 Geostationary Earth Orbit (GEO) Scenario<br />

This scenario is discussed in section 4.1.1.2.3 Earth Relay Optical Feeder Link and section 4.2<br />

Telecom Mission Optical Feeder Uplink.<br />

3.4 Lunar Scenario<br />

3.4.1 Concept of <strong>Operations</strong><br />

3.4.1.1 Basic Concept of <strong>Operations</strong><br />

The Lunar Scenario refers to a system providing optical communications from a lunar<br />

orbiting satellite to a ground station on the Earth’s surface. This scenario is of particular<br />

interest since the NASA LLCD is currently in preparation for a 2013 launch. Much of this<br />

scenario description is drawn from LLCD experience, as well as extrapolation to potential<br />

future lunar missions. The space terminal of LLCD is called the Lunar Lasercomm Space<br />

Terminal (LLST) and the dedicated ground terminal is called the Lunar Lasercomm Ground<br />

Terminal (LLGT).<br />

The first criterion for a free space optical link is geometric line of site from the spacecraft to<br />

a ground terminal. As with other scenarios, the optical link quality is affected by the ground<br />

station elevation angle, with lower elevations reducing the link capabilities. For all lunar<br />

orbiting spacecraft, the first obvious requirement is line of sight to the Moon itself; thus,<br />

lunar elevation angles will be consistent for all missions in this scenario analysis. Orbitspecific<br />

information further refines the scenario, though this information will vary from<br />

mission to mission.<br />

LLCD will be launched on LADEE. This science mission will fly a relatively low altitude (250<br />

km) retrograde lunar orbit. Due to the specific orbit, the satellite regularly passes behind<br />

the Moon and loses contact with the ground station. For LADEE, the passes with geometric<br />

line of sight vary between 40 and 80 minutes in duration. Lunar polar orbits that do not<br />

pass behind the Moon (from perspective of the ground site) would have more continuous<br />

geometric access when the Moon is in the sky.<br />

Under current plans, LLCD will be able to communicate with two ground stations. One—the<br />

LLGT—is a transportable terminal currently slated to be located on Mount Haleakala, on<br />

Maui, Hawaii. The second ground site is the OCTL, located on Table Mountain, California;<br />

this site is referred to as the Lunar Lasercomm OCTL Terminal (LLOT).<br />

The geometry from LADEE to the two ground sites illustrates several general features of<br />

lunar missions. These features are particularly relevant for interoperability, as multiple<br />

ground sites would be a major benefit of interoperability. While California and Hawaii are<br />

not at the same longitude, the fact that they are in the same hemisphere means that the<br />

Moon is visible simultaneously to both sites much of the time. Consider Figure 29, which<br />

shows the access times to the LLST from the two ground sites over a one-month period<br />

beginning July 1, 2013. Access is plotted at the given elevation angle. From the figure, one<br />

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