2005
DOI: 10.1117/12.600832
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Uplink beacon laser for Mars laser communication demonstration (MLCD)

Abstract: The requirements and design concepts for a ground-based laser assembly for transmitting an uplink beacon to a Mars bound spacecraft, carrying a laser communications terminal, are reported. The effects of the atmosphere are analyzed and drive the multi-beam design.

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Cited by 13 publications
(3 citation statements)
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“…Increased additive background noise when SPE angles are small further limits beacon-assisted acquisition, tracking, and pointing. Current studies that have analyzed beaconassisted acquisition and tracking from Mars farthest range with SPE angles of 2 -3 using 22-30-cm diameter space terminal aperture diameters suggest this to be viable [28], [29]. In these cases, the beacon is modulated and temporal acquisition is utilized in order to discriminate against background noise (see Section IV).…”
Section: B Deep-space Linksmentioning
confidence: 99%
See 1 more Smart Citation
“…Increased additive background noise when SPE angles are small further limits beacon-assisted acquisition, tracking, and pointing. Current studies that have analyzed beaconassisted acquisition and tracking from Mars farthest range with SPE angles of 2 -3 using 22-30-cm diameter space terminal aperture diameters suggest this to be viable [28], [29]. In these cases, the beacon is modulated and temporal acquisition is utilized in order to discriminate against background noise (see Section IV).…”
Section: B Deep-space Linksmentioning
confidence: 99%
“…Since the ground transmitted lasers propagate through the atmosphere without adaptive optics corrections, multi-beaming [28], [77] is used to mitigate scintillation effects. Multibeaming is accomplished by transmitting multiple mutually incoherent, coaligned beamlets.…”
Section: B Ground Subsystemmentioning
confidence: 99%
“…Ground-to-space laser uplinks to Earth-orbiting satellites and deep space probes serve both as a beacon and an uplink command channel for deep space probes and Earth-orbiting satellites. 1 An acquisition and tracking point design to support a high bandwidth downlink from a 20-cm optical terminal on an orbiting Mars spacecraft typically calls for 2.5 kW of 1030-nm uplink optical power in 40 microradians divergent beams. 2 The NOHD (nominal ocular hazard distance) of the 1030nm uplink is in excess of 2E5 km, approximately half the distance to the moon.…”
Section: High Power Lasers For Interplanetary Communicationsmentioning
confidence: 99%