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Proceedings Paper

The thermal control of the new solar telescope at Big Bear Observatory
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Paper Abstract

We present the basic design of the THermal Control System (THCS) for the 1.6-meter New Solar Telescope (NST) at the Big Bear Solar Observatory (BBSO), California. The NST is an off-axis Gregorian telescope with an equatorial mount and an open support structure. Since the telescope optics is exposed to the air, it is imperative to control the local/dome seeing, i.e., temperature fluctuations along the exposed optical path have to be minimized. To accomplish this, a THCS is implemented to monitor the dome environment and interact with the louver system of the dome to optimize instrument performance. In addition, an air knife is used to minimize mirror seeing. All system components have to communicate with the Telescope Control System (TCS), a hierarchical system of computers linking the various aspects of the entire telescope system, e.g., the active mirror control, adaptive optics, dome and telescope tracking, weather station, etc. We will provide an initial thermal model of the dome environment and first measurements taken in the recently replaced BBSO dome.

Paper Details

Date Published: 23 June 2006
PDF: 8 pages
Proc. SPIE 6267, Ground-based and Airborne Telescopes, 62670M (23 June 2006); doi: 10.1117/12.671777
Show Author Affiliations
Angelo P. Verdoni, New Jersey Institute of Technology (United States)
Carsten Denker, New Jersey Institute of Technology (United States)


Published in SPIE Proceedings Vol. 6267:
Ground-based and Airborne Telescopes
Larry M. Stepp, Editor(s)

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