Translator Disclaimer
16 August 2000 Mosaic array cameras for NEO and space debris
Author Affiliations +
The recent interest in detecting asteroids and Reentrant Space Debris has developed a need for large field of view, high-resolution focal pane array cameras to provide for mapping and tracking of these object. Ideally, a number of these cameras would be used around the world to provide a complete sky map. The Japan Space Forum is currently constructing one such facility in Japan. This paper describes the construction and features of two cameras to be used at the Japanese facility. One camera will be used in conjunction with a half-meter telescope and the second camera will be used with a one meter telescope. Features of the camera included radiative cooling of the focal pane array to minimize stress on the detector assembly, a specially designed focal pane array mount to maintain flatness, a 24 hour hold time liquid nitrogen dewar, and high speed fiber optic readout. The cameras feature arrays of up to ten SITe ST002 2048 by 4096 backthinned CCDs for high performance and wide field of view.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Scott P. Way, Archie M. Barter, Joseph J. Imamura, Morley M. Blouke, George Tylinski, Chuck Gilman, and Syuzo Isobe "Mosaic array cameras for NEO and space debris", Proc. SPIE 4008, Optical and IR Telescope Instrumentation and Detectors, (16 August 2000);


Mosaic array cameras for NEO and space debris an...
Proceedings of SPIE (May 15 2001)
Optimal placing CCD-TDI in focal plane
Proceedings of SPIE (August 28 1992)
Cooling the Dark Energy Camera instrument
Proceedings of SPIE (July 09 2008)
Assembly of the Dark Energy Survey CCD Imager
Proceedings of SPIE (July 26 2010)
Phoenix Telescope at AMOS return of the Baker Nunn...
Proceedings of SPIE (December 24 2002)

Back to Top