EUV multilayers for solar physics

David L. Windt; S. Donguy; John F. Seely; Benjawan Kjornrattanawanich; Eric M. Gullikson; C. C. Walton; L. Golub; E. DeLuca

doi:10.1117/12.506175

29 January 2004 EUV multilayers for solar physics

David L. Windt, S. Donguy, John F. Seely, Benjawan Kjornrattanawanich, Eric M. Gullikson, C. C. Walton, L. Golub, E. DeLuca

Author Affiliations +

Proceedings Volume 5168, Optics for EUV, X-Ray, and Gamma-Ray Astronomy; (2004) https://doi.org/10.1117/12.506175
Event: Optical Science and Technology, SPIE's 48th Annual Meeting, 2003, San Diego, California, United States

Abstract

We present an overview of currently available EUV multilayer coatings that can be used for the construction of solar physics instrumentation utilizing normal-incidence optics. We describe the performance of a variety of Si-based multilayers, including Si/B₄C and new Si/SiC films that provide improved performance in the wavelength range from 25 n 35 nm, as well as traditional Si/Mo multilayers, including broad-band coatings recently developed for the Solar-B/EIS instrument. We also outline prospects for operation at both longer and shorter EUV wavelengths, and also the potential of ultra-short-period multilayers that work near normal incidence in the soft X-ray region.

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David L. Windt, S. Donguy, John F. Seely, Benjawan Kjornrattanawanich, Eric M. Gullikson, C. C. Walton, L. Golub, and E. DeLuca "EUV multilayers for solar physics", Proc. SPIE 5168, Optics for EUV, X-Ray, and Gamma-Ray Astronomy, (29 January 2004); https://doi.org/10.1117/12.506175

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