Paper
23 July 2008 Design of MB sub-mirror handling manipulator for LAMOST
Author Affiliations +
Abstract
LAMOST is a quasi-meridian reflecting Schmidt telescope, which consists of a reflecting Schmidt corrector MA, a spherical primary mirror MB and a focal plane. The telescope with its optical axis tilted by an angle of 25° to the horizon tracks the celestial objects by the movements of MA to make the light throughout aim at MB, and MB mirror consists of 37 spherical segments hanged upside down on the truss which tilted by about 25° to the horizon. This paper presents a design of MB sub-mirror segment handling manipulator for LAMOST, carries out a simulation analysis, presents an engineering program and describes the program's design principles and ideas. The manipulator including grab, declutch, elevation, stretch, pitching, rotation, automatic control and several other parts, and the control system can coordinate all these movements so that each segment can be located installed and handled precisely. In the structural design process the stiffness and positioning accuracy problems have been taken full account of.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Heng Zuo, Guoping Li, and Fanghua Jiang "Design of MB sub-mirror handling manipulator for LAMOST", Proc. SPIE 7018, Advanced Optical and Mechanical Technologies in Telescopes and Instrumentation, 70183I (23 July 2008); https://doi.org/10.1117/12.786900
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Mirrors

Telescopes

Spherical lenses

Reflector telescopes

Astronomical telescopes

Astronomical imaging

Astronomy

RELATED CONTENT

The pre research of the deploy technology for the large...
Proceedings of SPIE (September 25 2012)
LAMOST control system: past and future
Proceedings of SPIE (August 04 2010)
Performance introduction of a 2.5m telescope mount
Proceedings of SPIE (September 17 2012)
Introduction of a 2.5m telescope mount and its performance
Proceedings of SPIE (August 05 2010)
A new calculation of LAMOST optical vignetting
Proceedings of SPIE (September 25 2012)
2-m LAMOST-type telescope for the Antarctic
Proceedings of SPIE (June 23 2006)

Back to Top