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The GMT enclosure detail engineering design has been consolidated to confidently face the future construction phase. This final detailed design phase has focused on delivering a cost-effective reliable enclosure that can be efficiently built in Las Campanas remote location providing a resilient integrated system that will house and protect GMT telescope against adverse environmental and seismic conditions. A seamless integration of a wide variety of disciplines including concrete and steel structures, mechanisms, mechanical-electrical-plumbing (MEP), telescope specific utilities, control systems and architectural has been vital to comply with the strict requirements of the project.
Besides, a thorough validation plan has been produced comprising analytical verification, early prototypes, factory and site assembly and testing plans (FAT & SAT), to guarantee performance and reliability of all subsystems at the site. Furthermore, construction procedures, techniques and logistics have been reviewed and considered when developing design key features together with assembly specifications so that the enclosure is constructed at the site in a safe and effective manner.
The design of the GMT lower enclosure is driven by equipment storage and access requirements but also directly impacts the origin and quality of the air entering the enclosure aperture. To ensure the highest quality GMT optical performance, Computational Fluid Dynamics (CFD) models and specialized analyses are utilized to evaluate several lower enclosure designs for their ability to limit the amount of ground-layer air entering the enclosure aperture. Lower enclosure designs with traditional solid outer walls promote the formation of “necklace” vortices, which tend to direct near-surface air, containing steep thermal gradients, into the enclosure aperture, potentially reducing image quality. Modifications to the lower enclosure, such as perforating the outer walls, are shown to suppress these necklace vortices at the expense of added structural complexity and/or reduced internal storage space. Initial isothermal CFD simulations defined the minimum height above terrain reached by the flow-path upwind of the observatory as a proxy to characterize the quality of air entering the enclosure, with lower heights associated with steeper thermal gradients. Based on these results, the most promising designs are further refined and subjected to additional higher fidelity CFD analyses, which includes a terrestrial thermal boundary layer. These simulations are also surveyed to quantify the aero-thermal environment along telescope optical paths, permitting evaluation and comparison of the predicted optical performance of the final candidate enclosure designs. Results from preliminary water tunnel testing of select lower-enclosure designs have increased our confidence in the CFD simulations.
High-fidelity Reynolds-Averaged Navier Stokes (RANS) Computational Fluid Dynamics (CFD) analysis of the GMT, enclosure, and LCO terrain is performed to study (a) the impact of either an open or closed enclosure base soffit external shape design, (b) the effect of telescope/enclosure location on the mountain summit, and (c) the effect of enclosure venting patterns. Details on the geometry modeling, grid discretization, and flow solution are first described. Then selected computational results are shown to quantify the quality of the airflow entering the GMT enclosure based on soffit, site location, and venting considerations. Based on the results, conclusions are provided on GMT soffit design, site location, and enclosure venting. The current work is not used to estimate image quality but will be addressed in future analyses as described in the conclusions.
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