LIDAX is developing the Laser Launch Telescope for the Gran Telescopio de Canarias (GTC) located at the Roque de los Muchachos Observatory on the island of La Palma, Canary Islands, Spain. This unique beam expander will be part of the GTC Adaptive Optics System (GTCAO) facility, managed by the IAC (Instituto de Astrofísica de Canarias), and will allow the creation of laser guide stars to feed the Adaptive Optics System of the GTC, removing the atmospheric turbulence to obtain high quality images of the stellar objects observed. This paper describes the opto-mechanical design and shows how the design- analysis process is performed to meet the performance requirements, explaining the STOP analysis carried out together with INTA-LINES. Such a process includes the initial mechanical design, the elaboration of both thermal and FEM models to analyze the behavior in terms of temperatures distribution, stiffness, and thermo-elastic effects, and of course the of lenses’ displacements and deformations under the different load cases and boundary conditions, which are transformed into Zernike Polynomials to evaluate the WFE of the Telescope, which allows to obtain, closing the loop, the best optical performance.
J. Moreno, E. Vielba, A. Manjón, A. Motos, E. Vázquez, E. Rodríguez, D. Saez, M. Sengl, J. Fernández, G. Campos, D. Muñoz, M. Mas, A. Balado, G. Ramos, C. Cerruti, M. Pajas, I. Catalán, M. Alcacera, A. Valverde, P. Pflueger, I. Vera
This paper describes the thermo-mechanical design of the Focal Plane Assembly (FPA) of the PLAnetary Transits and Oscillations of stars (PLATO) Instrument, developed by INTA and LIDAX. This is an ESA program with OHB as industry prime. In terms of assembly, alignment, and operational stability very demanding needs are required by a huge focal plane composed of four CCDs to assure the proper performance. This is translated into a complex thermomechanical design which shall be also focused on the correct production approach of the main parts involved, including several processes, and taking into account the number of cameras, and therefore Focal Plane Assemblies, to be produced (26). Part of these challenges, and their associated risks, are mitigated by means of the development of a totally representative prototype, which is currently finishing the integration phase and facing the test campaign.
The Meteosat Third Generation (MTG) Programme is being realised through the well established and successful Cooperation between EUMETSAT and ESA. It will ensure the future continuity of MSG with the capabilities to enhance nowcasting, global and regional numerical weather prediction, climate and atmospheric chemistry monitoring data from Geostationary Orbit.
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