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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 />

falls below the MPE. In line 9 of the table, the NOHD is calculated based on the method<br />

specified by the ICAO. This calculation, however, makes a far-field assumption that is not<br />

accurate for all of the scenarios of interest. A more refined calculation including near-field<br />

effects (following methods outlined in the ANSI standard Z136.1) is illustrated in line 10 and<br />

shows the LEO and GEO Relay uplinks are eye-safe using 1550 nm. The Lunar scenario could<br />

also be designed to be eye-safe with minor modifications to the scenario assumptions, thus<br />

avoiding a requirement for a laser safety system. All other scenarios (under the current<br />

assumptions) will require a laser safety system.<br />

Laser uplinks from Earth are traditionally protected by local onsite occupational health and<br />

safety standards, coordination with air traffic control authorities, and automated airspace<br />

monitoring. While onsite occupational health and safety measures vary by region, control<br />

measures to ensure coordination with air traffic control authorities have been identified in<br />

the Manual on Laser Emitters and Flight Safety published by ICAO. To protect the safety of<br />

aircraft against the hazardous effects of laser emitters, protected zones should be<br />

established around the affected airspace within the laser-beam free flight zone (up to 600<br />

meters above ground), critical flight zone (up to 3,<strong>05</strong>0 meters), and sensitive flight zone<br />

(above 3,<strong>05</strong>0 meters). Within the laser-beam free flight zone, the intensity of laser light is<br />

restricted to a level that is unlikely to cause any visual disruption, where irradiance is not to<br />

exceed 50nW/cm 2 unless some form of mitigation is applied. Within the critical flight zone,<br />

irradiance is not to exceed 5 µW/cm 2 and within the sensitive flight zone, it is not to exceed<br />

100 µW/cm 2 . According to ICAO, these restrictions refer to visible laser beams only. But in<br />

all navigable airspace, the irradiance level of any laser beam, visible or invisible, is expected<br />

to be less than or equal to the MPE, unless the prior permission has been obtained by the<br />

proper authority. Physical, procedural, and automated control measures established to<br />

ensure that aircraft operations will not be exposed to levels of illumination greater than the<br />

maximum acceptable irradiance level should meet one or more of the operator control<br />

measures:<br />

<br />

<br />

<br />

<br />

<br />

<br />

Ability to physically block the laser beam to prevent light from being directed into<br />

protected airspace<br />

Ability to adjust the laser beam divergence and output power or pulse energy<br />

emitted through the system aperture to meet exposure levels<br />

Redirection of beam in a specific area<br />

Manual operation of a shutter or beam-termination system, used in conjunction with<br />

airspace observers<br />

Scanning the laser beam to reduce the level of illumination<br />

Automated system designed to detect aircraft and terminate or redirect the beam or<br />

shutter the system<br />

2.3.2.3 Interference and Backscattering<br />

A further concern to be dealt with by optical ground communications terminals located in<br />

close proximity to astronomical telescopes is the issue of optical interference. The uplink<br />

beacon always suffers some losses from Mie scattering and scattering by dust and water<br />

droplets or ice crystals suspended in the air. An astronomical telescope pointing in the<br />

direction of the beacon will image the beacon as a line emanating from the ground terminal<br />

and extending to the position of the space terminal (see Figure 5).<br />

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