Paper
5 August 2010 Monitoring of the environmental conditions inside the dome of the 4m Blanco Telescope at CTIO
Author Affiliations +
Abstract
Between February and April 2009 a number of ultrasonic anemometers, temperature probes and dust sensors were operated inside the CTIO Blanco telescope dome. These sensors were distributed in a way that temperature and 3 dimensional wind speeds were monitored along the line of sight of the telescope. During telescope operations, occasional seeing measurements were obtained using the Mosaic CCD imager and the CTIO site monitoring MASS-DIMM system. In addition, also a Lunar Scintillometer (LuSci) was operated over the course of a few nights inside the dome. We describe the instrumental setup and first preliminary results on the linkage of the atmospheric conditions inside the dome to the overall image quality.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
S. G. Els, T. M. C. Abbott, E. B. Bustos, J. Seguel, D. E. Walker, A. Berdja, R. Riddle, M. Schöck, W. Skidmore, and T. Travouillon "Monitoring of the environmental conditions inside the dome of the 4m Blanco Telescope at CTIO", Proc. SPIE 7733, Ground-based and Airborne Telescopes III, 77333X (5 August 2010); https://doi.org/10.1117/12.856297
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Domes

Environmental monitoring

Sensors

3D metrology

Atmospheric monitoring

Charge-coupled devices

RELATED CONTENT

RHESSI aspect system and in-flight calibration
Proceedings of SPIE (February 11 2003)
Increasing the productivity of the WHT
Proceedings of SPIE (July 25 2000)
Balloon-borne electron telescope with scintillating fibers
Proceedings of SPIE (October 18 1996)
Euclid Mission: assessment study
Proceedings of SPIE (August 26 2009)

Back to Top