Author Affiliations
Abstract
1 Department of Astronomy, Beijing Normal University, Beijing100875, China
2 College of Physics and Electronic Engineering, Qilu Normal University, Jinan250200, China
3 CAS Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing100101, China
4 School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing101408, China
5 Graduate School of China Academy of Engineering Physics, Beijing100196, China
6 Collaborative Innovation Center of IFSA (CICIFSA), Shanghai Jiao Tong University, Shanghai200240, China
In this paper, we present a reanalysis of the silicon He-$\mathrm{\alpha}$ X-ray spectrum emission in Fujioka et al.’s 2009 photoionization experiment. The computations were performed with our radiative-collisional code, RCF. The central ingredients of our computations are accurate atomic data, inclusion of satellite lines from doubly excited states and accounting for the reabsorption of the emitted photons on their way to the spectrometer. With all these elements included, the simulated spectrum turns out to be in good agreement with the experimental spectrum.
high-energy-density physics laboratory astrophysics laser–plasma interaction 
High Power Laser Science and Engineering
2021, 9(1): 010000e9

关于本站 Cookie 的使用提示

中国光学期刊网使用基于 cookie 的技术来更好地为您提供各项服务,点击此处了解我们的隐私策略。 如您需继续使用本网站,请您授权我们使用本地 cookie 来保存部分信息。
全站搜索
您最值得信赖的光电行业旗舰网络服务平台!