
Proceedings Paper
Near infrared (NIR) achromatic phase retarderFormat | Member Price | Non-Member Price |
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Paper Abstract
The tunable near InfraRed Lyot filter (TNIRLF) is one of the focal plane instruments for Advanced Technology Solar Telescope (ATST) project of the National Solar Observatory (NSO). Achromatic half waveplate and quarter waveplates working from 1000 nm to 1700 nm will be used in this filter. In this paper, we give a description of the design and development for the synthesized achromatic waveplates using quartz plates. The retardance variation is within 1% over the full spectral range and we discuss the variance of optical axis.
Paper Details
Date Published: 14 October 2004
PDF: 9 pages
Proc. SPIE 5523, Current Developments in Lens Design and Optical Engineering V, (14 October 2004); doi: 10.1117/12.557652
Published in SPIE Proceedings Vol. 5523:
Current Developments in Lens Design and Optical Engineering V
Pantazis Z. Mouroulis; Warren J. Smith; R. Barry Johnson, Editor(s)
PDF: 9 pages
Proc. SPIE 5523, Current Developments in Lens Design and Optical Engineering V, (14 October 2004); doi: 10.1117/12.557652
Show Author Affiliations
Jun Ma, New Jersey Institute of Technology (United States)
Jingshan Wang, New Jersey Institute of Technology (United States)
W. Cao, New Jersey Institute of Technology (United States)
Jingshan Wang, New Jersey Institute of Technology (United States)
W. Cao, New Jersey Institute of Technology (United States)
Carsten Denker, New Jersey Institute of Technology (United States)
Big Bear Solar Observatory (United States)
Haimin Wang, New Jersey Institute of Technology (United States)
Big Bear Solar Observatory (United States)
Big Bear Solar Observatory (United States)
Haimin Wang, New Jersey Institute of Technology (United States)
Big Bear Solar Observatory (United States)
Published in SPIE Proceedings Vol. 5523:
Current Developments in Lens Design and Optical Engineering V
Pantazis Z. Mouroulis; Warren J. Smith; R. Barry Johnson, Editor(s)
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