Author:
Wu Jiali,Qi Runze,Zhang Zhong,Wang Zhanshan
Abstract
The Ne VII line is an intense solar line emitted from the solar transition region located at 46.5 nm with a temperature of approximately 0.5 MK. The observation of a Ne VII line is important to deepen the understanding of solar physics. For observing the Ne VII line at 46.5 nm, we have proposed a narrowband Sc/Si multilayer that could avoid the other solar emission lines going to the observatory instrument. In this article, Sc/Si multilayers with a Sc thickness ratio of 0.35 (conventional design) and 0.65 (narrowband design) were deposited. The microstructures of both multilayers were measured by grazing incidence X-ray reflectometry, X-ray diffraction, and transmission electron microscopy. The results showed that the interdiffusion at the Si-on-Sc interface was more significant than that at the Sc-on-Si interface in both multilayer. Compared with the conventional multilayer, the narrowband multilayer had a thinner Si-on-Sc interface width. The measured reflectivity of the Sc/Si multilayer with a Sc thickness ratio of 0.65 was 37.9% at 45.5 nm with a near-normal incident angle of 4.60°. The bandwidth was 3.68 nm, which is narrow enough to observe the Ne VII solar line.
Funder
National Natural Science Foundation of China
Subject
Physical and Theoretical Chemistry,General Physics and Astronomy,Mathematical Physics,Materials Science (miscellaneous),Biophysics
Cited by
3 articles.
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