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Proceedings Paper

Instrumentation for the Advanced Technology Solar Telescope
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Paper Abstract

The 4-m aperture Advanced Technology Solar Telescope (ATST) is the next generation ground based solar telescope. In this paper we provide an overview of the ATST post-focus instrumentation. The majority of ATST instrumentation is located in an instrument Coude lab facility, where a rotating platform provides image de-rotation. A high order adaptive optics system delivers a corrected beam to the Coude lab facility. Alternatively, instruments can be mounted at Nasmyth or a small Gregorian area. For example, instruments for observing the faint corona preferably will be mounted at Nasmyth focus where maximum throughput is achieved. In addition, the Nasmyth focus has minimum telescope polarization and minimum stray light. We describe the set of first generation instruments, which include a Visible-Light Broadband Imager (VLBI), Visible and Near-Infrared (NIR) Spectropolarimeters, Visible and NIR Tunable Filters, a Thermal-Infrared Polarimeter & Spectrometer and a UV-Polarimeter. We also discuss unique and efficient approaches to the ATST instrumentation, which builds on the use of common components such as detector systems, polarimetry packages and various opto-mechanical components.

Paper Details

Date Published: 30 September 2004
PDF: 14 pages
Proc. SPIE 5492, Ground-based Instrumentation for Astronomy, (30 September 2004); doi: 10.1117/12.551853
Show Author Affiliations
Thomas R. Rimmele, National Solar Observatory (United States)
Robert P. Hubbard, National Solar Observatory (United States)
K. S. Balasubramaniam, National Solar Observatory (United States)
Tom Berger, Lockheed Martin Solar and Astrophysics Lab. (United States)
David Elmore, High Altitude Observatory (United States)
G. Allen Gary, NASA Marshall Space Flight Ctr. (United States)
Don Jennings, NASA Goddard Space Flight Ctr. (United States)
Christoph Keller, National Solar Observatory (United States)
Jeff Kuhn, Institute for Astronomy/Univ. of Hawaii (United States)
Haosheng Lin, Institute for Astronomy/Univ. of Hawaii (United States)
Don Mickey, Institute for Astronomy/Univ. of Hawaii (United States)
Gilberto Moretto, National Solar Observatory (United States)
Hector Socas-Navarro, High Altitude Observatory (United States)
Jan O. Stenflo, ETH Zurich (Switzerland)
Haimin Wang, New Jersey Institute of Technology (United States)


Published in SPIE Proceedings Vol. 5492:
Ground-based Instrumentation for Astronomy
Alan F. M. Moorwood; Masanori Iye, Editor(s)

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