Poster + Presentation + Paper
13 December 2020 Mirrors for improved FUV space observations
N. Gutiérrez-Luna, P. López-Reyes, Carlos Honrado-Benítez, L. Espinosa-Yáñez, Á. Ríos-Fernández, L. V. Rodríguez-de Marcos, M. A. Quijada, J. I. Larruquert
Author Affiliations +
Conference Poster
Abstract
Future space missions require more efficient coatings with high stability over time. The Far-UV (FUV) (100-200 nm) and Extreme-UV (EUV) (10-100 nm) spectral ranges are of great interest to various scientific communities dedicated to the exploration and understanding of the universe. GOLD laboratory is a scientific research group that investigates on the development of coatings tuned in the FUV and EUV spectral ranges. In this proceeding, we present coatings that address different targets: 1) broadband mirrors based on Al/MgF2 and Al/AlF3, 2) narrowband mirrors peaked at wavelengths longer than ~120 nm based on (MgF2/LaF3)n multilayers, and 3) mirrors with high reflectance at Lyman β (102.6 nm) spectral line with strong rejection at the ubiquitous and intense H Lyman α(121.6 nm).
Conference Presentation
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
N. Gutiérrez-Luna, P. López-Reyes, Carlos Honrado-Benítez, L. Espinosa-Yáñez, Á. Ríos-Fernández, L. V. Rodríguez-de Marcos, M. A. Quijada, and J. I. Larruquert "Mirrors for improved FUV space observations", Proc. SPIE 11444, Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray, 1144478 (13 December 2020); https://doi.org/10.1117/12.2563351
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KEYWORDS
Mirrors

Space mirrors

Thin film coatings

Optical coatings

Astrophysics

Far ultraviolet

Gold

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