18 July 2014 New developments in rotating and linear motion mechanisms used in contamination sensitive space telescopes
Author Affiliations +
Abstract
We have been developing a rotating mechanism and a linear motion mechanism for their usage in contamination sensitive space telescopes. They both are needed for ~1.4 meter optical telescope and its focal plane instrument onboard SOLAR-C, the next-generation spaceborne solar observatory following Hinode. Highly reliable long life performance, low outgassing properties, and low level of micro-vibration are required along with their scientific performance. With the proto-type mechanisms, the long life performance and outgassing properties of the mechanisms have been evaluated in vacuum chambers. The level of micro-vibration excited during the operations of the rotating mechanism was measured by operating it on the Kestler table. This paper provides the overall descriptions of our mechanism developments.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Toshifumi Shimizu, Toshifumi Shimizu, Kyoko Watanabe, Kyoko Watanabe, Satoshi Nakayama, Satoshi Nakayama, Takao Tajima, Takao Tajima, Shingo Obara, Shingo Obara, Shinsuke Imada, Shinsuke Imada, Naoto Nishizuka, Naoto Nishizuka, Shin-nosuke Ishikawa, Shin-nosuke Ishikawa, Hirohisa Hara, Hirohisa Hara, } "New developments in rotating and linear motion mechanisms used in contamination sensitive space telescopes", Proc. SPIE 9151, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation, 915138 (18 July 2014); doi: 10.1117/12.2055664; https://doi.org/10.1117/12.2055664
PROCEEDINGS
7 PAGES


SHARE
RELATED CONTENT

SIMBOL X a formation flying mission for hard x...
Proceedings of SPIE (September 10 2005)
The challenges posed by future far IR and sub mm...
Proceedings of SPIE (July 12 2008)
The Solar Optical Telescope onboard the Solar-B
Proceedings of SPIE (October 12 2004)
Vacuum BRDF Measurements Of Cryogenic Optical Surfaces
Proceedings of SPIE (January 02 1990)

Back to Top