AI Article Synopsis
- The He-II (λ=30.4 nm) emission line is utilized to study the solar corona, providing important insights into solar activity.
- Researchers have developed innovative beryllium (Be)/magnesium multilayer coatings that enhance the reflective properties of these spectral channels.
- These coatings, when paired with a protective aluminum/Be bilayer, achieve reflection coefficients up to 56% and exhibit impressive spectral and temporal stability.
Article Abstract
The He-II (λ=30.4 nm) emission line is one of the spectral channels chosen to study solar corona. This Letter reports on investigations of novel beryllium (Be)/magnesium multilayer coatings which, when incorporated beneath a protective bilayer of aluminium and Be, ensure particularly high-reflection coefficients of up to 56%, a spectral width of Δλ=1.6 nm (λ/Δλ≈20), and high temporal stability.
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| http://dx.doi.org/10.1364/OL.44.000263 | DOI Listing |
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View Article and Find Full Text PDFArticle Synopsis
- The He-II (λ=30.4 nm) emission line is utilized to study the solar corona, providing important insights into solar activity.
- Researchers have developed innovative beryllium (Be)/magnesium multilayer coatings that enhance the reflective properties of these spectral channels.
- These coatings, when paired with a protective aluminum/Be bilayer, achieve reflection coefficients up to 56% and exhibit impressive spectral and temporal stability.
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