Bibcode
Bettonvil, F. C. M.; Codina, R.; Gómez Merchán, A.; Hammerschlag, R. H.; Hartman, J. J. M.; Hernández Suárez, E.; Jägers, A. P. L.; Murga Llano, G.; Pelser, J. W.; Sliepen, G.
Referencia bibliográfica
Ground-based and Airborne Telescopes III. Edited by Stepp, Larry M.; Gilmozzi, Roberto; Hall, Helen J. Proceedings of the SPIE, Volume 7733, pp. 773334-773334-12 (2010).
Fecha de publicación:
7
2010
Número de citas
0
Número de citas referidas
0
Descripción
EST (European Solar Telescope) is a 4-m class solar telescope, which is
currently in the conceptual design phase. EST will be located in the
Canary Islands and will aim at high spectral, spatial and temporal
resolution observations in the photosphere and chromosphere, using a
suite of instruments that can produce efficiently two-dimensional
spectropolarimetric information of the thermal, dynamic and magnetic
properties of the plasma over many scale heights. The pier is defined as
the construction that supports the telescope and the enclosure. It needs
a certain height to minimize daytime ground turbulence. At the bottom of
the pier a large instrument lab is located, 16 m in diameter and 10 m
high. To the pier is attached a service building that accommodates all
auxiliary services, possibly together with a separate building. Solid
concrete- and open framework piers are compared, in terms of stability,
thermal properties and flow characteristics and building structures in
terms of construction issues. FE and CFD analysis are used to give
qualitative insight in the differences between the alternatives. The
preferred alternative is a cone shaped pier surrounded by an open
framework.