Solar site testing for the advanced technology solar telescope

F. Hill; J. Beckers; P. Brandt; J. Briggs; T. Brown; W. Brown; M. Collados; C. Denker; S. Fletcher; S. Hegwer; T. Horst; M. Komsa; J. Kuhn; A. Lecinski; H. Lin; S. Oncley; M. Penn; T. Rimmele; H. Socas-Navarro; K. Streander

doi:10.1117/12.551812

Solar site testing for the advanced technology solar telescope

F. Hill
, J. Beckers
, P. Brandt
, J. Briggs
, T. Brown
, W. Brown
, M. Collados
, C. Denker
, S. Fletcher
, S. Hegwer
, T. Horst
, M. Komsa
, J. Kuhn
, A. Lecinski
, H. Lin
, S. Oncley
, M. Penn
, T. Rimmele
, H. Socas-Navarro
, K. Streander

Earth Observing Lab

National Solar Observatory
The University of Chicago
Leibniz-Institut fuer Sonnenphysik (KIS)
National Solar Observatory Sacramento Peak
National Center for Atmospheric Research
Instituto de Astrofisica de Canarias
New Jersey Institute of Technology
University of Hawai'i at Mānoa

Research output: Contribution to journal › Conference article › peer-review

17 Scopus citations

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.

Original language	English
Pages (from-to)	122-129
Number of pages	8
Journal	Proceedings of SPIE - The International Society for Optical Engineering
Volume	5489
Issue number	PART 1
DOIs	https://doi.org/10.1117/12.551812
State	Published - 2004
Event	Ground-based Telescopes - Glasgow, United Kingdom Duration: Jun 21 2004 → Jun 25 2004

Keywords

Atmospheric turbulence
Seeing
Site testing

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10.1117/12.551812

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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., & Streander, K. (2004). Solar site testing for the advanced technology solar telescope. Proceedings of SPIE - The International Society for Optical Engineering, 5489(PART 1), 122-129. https://doi.org/10.1117/12.551812

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title = "Solar site testing for the advanced technology solar telescope",

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.",

keywords = "Atmospheric turbulence, Seeing, Site testing",

author = "F. Hill and J. Beckers and P. Brandt and J. Briggs and T. Brown and W. Brown and M. Collados and C. Denker and S. Fletcher and S. Hegwer and T. Horst and M. Komsa and J. Kuhn and A. Lecinski and H. Lin and S. Oncley and M. Penn and T. Rimmele and H. Socas-Navarro and K. Streander",

year = "2004",

doi = "10.1117/12.551812",

language = "English",

volume = "5489",

pages = "122--129",

journal = "Proceedings of SPIE - The International Society for Optical Engineering",

issn = "0277-786X",

publisher = "SPIE",

number = "PART 1",

note = "Ground-based Telescopes ; Conference date: 21-06-2004 Through 25-06-2004",

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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 & Streander, K 2004, 'Solar site testing for the advanced technology solar telescope', Proceedings of SPIE - The International Society for Optical Engineering, vol. 5489, no. PART 1, pp. 122-129. https://doi.org/10.1117/12.551812

TY - JOUR

T1 - Solar site testing for the advanced technology solar telescope

AU - Hill, F.

AU - Beckers, J.

AU - Brandt, P.

AU - Briggs, J.

AU - Brown, T.

AU - Brown, W.

AU - Collados, M.

AU - Denker, C.

AU - Fletcher, S.

AU - Hegwer, S.

AU - Horst, T.

AU - Komsa, M.

AU - Kuhn, J.

AU - Lecinski, A.

AU - Lin, H.

AU - Oncley, S.

AU - Penn, M.

AU - Rimmele, T.

AU - Socas-Navarro, H.

AU - Streander, K.

PY - 2004

Y1 - 2004

N2 - 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.

AB - 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.

KW - Atmospheric turbulence

KW - Seeing

KW - Site testing

UR - https://www.scopus.com/pages/publications/10444265165

U2 - 10.1117/12.551812

DO - 10.1117/12.551812

M3 - Conference article

AN - SCOPUS:10444265165

SN - 0277-786X

VL - 5489

SP - 122

EP - 129

JO - Proceedings of SPIE - The International Society for Optical Engineering

JF - Proceedings of SPIE - The International Society for Optical Engineering

IS - PART 1

T2 - Ground-based Telescopes

Y2 - 21 June 2004 through 25 June 2004

ER -

Solar site testing for the advanced technology solar telescope

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Keywords

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