Solar site testing for the advanced technology solar telescope
Document Type
Conference Proceeding
Publication Date
12-24-2004
Abstract
The location of the Advanced Technology Solar Telescope (ATST) is a critical factor in the overall performance of the telescope. We have developed a set of instrumentation to measure daytime seeing, sky brightness, cloud cover, water vapor, dust levels, and weather. The instruments have been located at six sites for periods of one to two years. Here we describe the sites and instrumentation, discuss the data reduction, and present some preliminary results. We demonstrate that it is possible to estimate seeing as a function of height near the ground with an array of scintillometers, and that there is a distinct qualitative difference in daytime seeing between sites with or without a nearby lake.
Identifier
10444265165 (Scopus)
Publication Title
Proceedings of SPIE the International Society for Optical Engineering
External Full Text Location
https://doi.org/10.1117/12.551812
ISSN
0277786X
First Page
122
Last Page
129
Issue
PART 1
Volume
5489
Recommended Citation
Hill, F.; Beckers, J.; Brandt, P.; Briggs, J.; Brown, T.; Brown, W.; Collados, M.; Denker, C.; Fletcher, S.; Hegwer, S.; Horst, T.; Komsa, M.; Kuhn, J.; Lecinski, A.; Lin, H.; Oncley, S.; Penn, M.; Rimmele, T.; Socas-Navarro, H.; and Streander, K., "Solar site testing for the advanced technology solar telescope" (2004). Faculty Publications. 19994.
https://digitalcommons.njit.edu/fac_pubs/19994
