Wenjuan Wu, Jingtao Zhu, Fengli Wang, Zhong Zhang, Hongchang Wang, Shumin Zhang, Zhanshan Wang, Lingyan Chen, Hongjun Zhou, et al.
Proceedings Volume Seventh International Conference on Thin Film Physics and Applications, 79950Z (2011) https://doi.org/10.1117/12.888159
Mutilayers are important optical elements and widely used for extreme ultraviolet astronomical observation. For
selecting the emission line multilayers should have high reflectivity and narrow spectral bandwidth. In this paper, six
different multilayers including Si/C, Si/B4C, Si/Mo/B4C, Si/SiC, Mg/SiC and Mo/Si were designed for normal incidence
angle of 5° at He-IIemission line(λ=30.4 nm). These multilayers have been fabricated using a direct current magnetron
sputtering system. The period of multilayers were measured by X-ray diffractometer(XRD) and the reflectivities were
measured on National Synchrotron Radiation Facility in Hefei, China. Then the reflectivities and the spectral bandwidth
of these multilayers were compared respectively. It shows that the spectral bandwidth of multilayers of low Z materials is
narrower than that of the normal Mo/Si multiayer, the reflectivity of Si/Mo/B4C multilayer is higher than that of Si-based
multilayers of two kinds of materials. And Mg/SiC multilayer has the highest reflectivity of 43.81% and the narrowest
spectral bandwidth of 1.44nm, which proves that Mg/SiC multilayer is more potential for selecting the emission line in
extreme ultraviolet solar physics.