Beyond Conventional Adaptive Optics, Venice().Lithography Technology Options at 100nm and Beyond Schumacher, A., Montoya, L., Devaney, N., Dohlen, K., Dierickx, P., 2001, Phasing ELTs for Adaptive Optics: preliminary results of a comparison of techniques, ESO Conf. Mountain, M., 1996, What is beyond the current generation of ground-based 8-m to 10-m class telescopes and the VLT-I?, SPIE 2871, 597 Meinel, A.B., 1978, An overview of the Technological Possibilities of Future Telescopes, ESO 23, 13 Marchetti, E., Hubin, N., Fedrigo, E., Brynnel, J., Delabre, B., Donaldson, R., Franza, F., Conan, R., Le Louarn, M., Cavadore, C., Balestra, A., Baade, D., Lizon, J.L., Gilmozzi, R., Monnet, G., Ragazzoni, R., Arcidiacono, C., Baruffolo, A., Diolaiti, E., Farinato, J., Viard, E., Butler, D., Hippler, S., Amorim, A., 2002, MAD the ESO multi-conjugate adaptive optics demonstrator, SPIE Adaptive Optical System Technologies II Gilmozzi, R., Delabre, B., Dierickx, P., Hubin, N., Koch, F., Monnet, G., Quattri, M., Rigaut, F., Wilson, R.N., 1998, The Future of Filled Aperture Telescopes: is a 100m Feasible?, SPIE 3352, 778 Beyond Conventional Adaptive Optics, Venice, ()ĭierickx, P., Beletic, J., Delabre, B., Ferrari, M., Gilmozzi, R., Hubin, N., 2000, The Optics of the OWL 100-m Adaptive Telescope, Proceedings Bäckaskog Workshop on Extremely Large Telescopes, p97ĭierickx, P., Delabre, B., Noethe, L., 2000, OWL optical design, active optics and error budget, SPIE 4003, 2000 et al, 1994, Performance and potential applications of replica technology up to the 1-m range, SPIE 2199, 870īarr, L.D., 1979, Factors Influencing Selection of a Next Generation Telescope Concept, SPIE 172, 8Ĭhanan, G., Troy, M., Ohara, C., 2000, “Phasing the primary mirror segments of the Keck telescopes: a comparison of different techniques”, SPIE 4003, 188ĭierickx, P., 2001, Optical design and adaptive optics properties of the OWL 100-m telescope ESO Conf. This process is experimental and the keywords may be updated as the learning algorithm improves.Īrdeberg, A., Andersen, T., Lindberg, B., Owner-Petersen, M., Korhonen, T., S⊘ndergård, P., 1992, Breaking the 8m Barrier - One Approach for a 25m Class Optical Telescope, ESO Conf.
These keywords were added by machine and not by the authors. We elaborate on the design of ESO's concept for a 100-m class, diffraction-limited telescope.
#Optical telescope 100nm full#
A crucial assumption is that giant telescopes could take full benefit of adaptive optics, a technique currently under rapid development. Novel design approaches taking full benefit of such evolution will, therefore, enable the design, construction and operation of facilities hugely more powerful than currently available. We argue that such limitations have recently shifted from the realm of poorly reliable glassmaking and opto-mechanical alignment to that of predictable control systems and large-scale mechanical structures.
Traditional design approaches, and above all technology limitations, have limited gains in size to a mere factor 2 between successive generations.
Astronomers having very few other ways to perform experimentation, this quest has closely followed the path of technology development, and even promoted it more than once. The quest for larger telescopes is a never-ending story.
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