LAMOST enclosure and its wind load analysis

Details LAMOST enclosure and its wind load analysis LAMOST enclosure and its wind load analysis

Aug 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000spie.4004..164y&link_type=abstract

Proc. SPIE Vol. 4004, p. 164-172, Telescope Structures, Enclosures, Controls, Assembly/Integration/Validation, and Commissioning

Computer Science

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Scientific paper

LAMOST is a reflecting Schmidt telescope that lies on the ground. It is consists of three main parts: Schmidt plate- MA, spherical primary mirror MB and focal plane unit. Its optical axis is on the meridian plane with a 25- degree inclination to the horizontal that is different to traditional telescope. Therefore LAMOST enclosure will be consists of two parts accordant: the dome enclosure of MA and the tunnel enclosure from focus to MB. This paper describes the major design consideration of the LAMOST enclosures, that featured with a better seeing performance, a good wind buffet function and an acceptable optical baffle, its structure are more simple with good operability and maintainability.

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