Share Email Print
cover

Proceedings Paper

The active surface control system for the Tian Ma Telescope
Author(s): Jian Dong; Huiliang Jin; Qian Ye; Zhiqiang Shen; Qinghui Liu; Li Fu
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper Abstract

The Tian Ma Telescope (TM) is the largest fully steerable radio telescope in Asia. It has a primary reflector of 65-m in diameter with a shaped Cassegrain configuration. The primary reflector of the TM is an active surface with 1104 actuators for the 1008 surface panels. The panels of the telescope are divided into 18 rings, and 24 fan sections. Each section includes three sub-sections. The active surface system adopts TCP/IP Ethernet network and RS-485 bus as a dominating mode of communication. The control software works on the Windows system, and adopts the object-oriented technology. The photogrammetry and phase-coherent holography has been used to set the surface to about 0.3mm at the rigging angle. The FEM model is testing now. The Out-of-Focus holography and other techniques will be used to modify the dynamic surface deformation.

Paper Details

Date Published: 26 July 2016
PDF: 6 pages
Proc. SPIE 9913, Software and Cyberinfrastructure for Astronomy IV, 991306 (26 July 2016); doi: 10.1117/12.2230560
Show Author Affiliations
Jian Dong, Shanghai Astronomical Observatory (China)
Huiliang Jin, Shanghai Jiao Tong Univ. (China)
Qian Ye, Shanghai Jiao Tong Univ. (China)
Zhiqiang Shen, Shanghai Astronomical Observatory (China)
Qinghui Liu, Shanghai Astronomical Observatory (China)
Li Fu, Shanghai Astronomical Observatory (China)


Published in SPIE Proceedings Vol. 9913:
Software and Cyberinfrastructure for Astronomy IV
Gianluca Chiozzi; Juan C. Guzman, Editor(s)

© SPIE. Terms of Use
Back to Top