Chromospheric Helium Imaging Photometer (an Instrument for High Time Cadence 1083-nm Wavelength Solar Observations)
The scientific motivation, design criteria, and specifications for a new ground-based instrument to observe the Sun in the He i 1083-nm spectral line is described. The instrument employs a liquid-crystal tunable Lyot-type spectral filter and an array detector that allows the full solar disk to be ob...
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Veröffentlicht in: | Applied Optics 1998-07, Vol.37 (19), p.4270-4276 |
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container_title | Applied Optics |
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creator | Elmore, D F Card, G L Chambellan, C W Hassler, D M Hull, H L Lecinski, A R Macqueen, R M Streander, K V Streete, J L White, O R |
description | The scientific motivation, design criteria, and specifications for a new ground-based instrument to observe the Sun in the He i 1083-nm spectral line is described. The instrument employs a liquid-crystal tunable Lyot-type spectral filter and an array detector that allows the full solar disk to be observed with a time cadence of minutes. We describe the telescope's optical and mechanical features and discuss computer interface and data-reduction procedures employed. Instrument performance during the initial year of operation of the telescope at its high-altitude site is summarized. |
doi_str_mv | 10.1364/AO.37.004270 |
format | Article |
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title | Chromospheric Helium Imaging Photometer (an Instrument for High Time Cadence 1083-nm Wavelength Solar Observations) |
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