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THE LGSF LASER SYSTEM - Thirty Meter Telescope

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TMT.AOS.DRD.09.003.DRF05 Page 9 of 30REQUIREMENTS DOCUMENT FOR <strong>THE</strong> <strong>LGSF</strong> <strong>LASER</strong> <strong>SYSTEM</strong> August 25, 20092. OVERALL DESCRIPTION2.1 PERSPECTIVEThe <strong>LGSF</strong> is composed of 3 main sub-systems:(i)(ii)(iii)The Laser System (LAS), which includes the lasers and all associated controlsystems. The Laser System is located within the (-X ACRS , -Y ACRS ) quadrant of thetelescope azimuth structure (see Figure 3). The Laser System provides the lightsources for generating the artificial stars in the sodium layer at 90 – 110 kmaltitude. The Laser System is the subject of this requirement document.The Beam Transfer Optics (BTO) and Laser Launch <strong>Telescope</strong> (LLT) System,which is responsible for taking the beams from the output of the Laser System andtransferring them across the telescope azimuth structure, up the telescopeelevation structure and then launching them from the LLT located behind the TMTsecondary mirror. The BTO/LLT System is composed of two principal systems: (1)the BTO Optical Path and (2) the <strong>LGSF</strong> Top End, which consists of BTO and LLTcomponents located behind the TMT secondary mirror.The Laser Safety System (LSS), which is itself composed of several sub-systemsdedicated to:a. Protecting people and observatory systems from laser light,b. Protecting aircraft from laser illumination,c. Protecting neighboring telescopes (if any) from laser beams within their field ofview, when necessary.The <strong>LGSF</strong> optical block diagram is given in Figure 1:

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