KMS National Astronomical Observatories, CAS
Emission mechanism for the silicon He-alpha lines in a photoionization experiment | |
Han, Bo1,2; Wang, Feilu3,4,5![]() | |
2021-02-11 | |
Source Publication | HIGH POWER LASER SCIENCE AND ENGINEERING
![]() |
ISSN | 2095-4719 |
Volume | 9Pages:8 |
Abstract | In this paper, we present a reanalysis of the silicon He-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. |
Keyword | high-energy-density physics laboratory astrophysics laser-plasma interaction |
Funding Organization | Science Challenge Project ; Science Challenge Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Science Challenge Project ; Science Challenge Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Science Challenge Project ; Science Challenge Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Science Challenge Project ; Science Challenge Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences |
DOI | 10.1017/hpl.2020.49 |
Language | 英语 |
Funding Project | Science Challenge Project[TZ2016005] ; National Natural Science Foundation of China[11903006] ; National Natural Science Foundation of China[12073043] ; National Natural Science Foundation of China[U1930108] ; Strategic Priority Research Program of Chinese Academy of Sciences[XDA25030700] |
Funding Organization | Science Challenge Project ; Science Challenge Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Science Challenge Project ; Science Challenge Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Science Challenge Project ; Science Challenge Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Science Challenge Project ; Science Challenge Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences |
WOS Research Area | Optics |
WOS Subject | Optics |
WOS ID | WOS:000620167500001 |
Publisher | CHINESE LASER PRESS & CAMBRIDGE UNIV PRESS |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.bao.ac.cn/handle/114a11/79390 |
Collection | 中国科学院国家天文台 |
Corresponding Author | Wang, Feilu |
Affiliation | 1.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China 2.Qilu Normal Univ, Coll Phys & Elect Engn, Jinan 250200, Peoples R China 3.Chinese Acad Sci, CAS Key Lab Opt Astron, Natl Astron Observ, Beijing 100101, Peoples R China 4.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 101408, Peoples R China 5.China Acad Engn Phys, Grad Sch, Beijing 100196, Peoples R China 6.Shanghai Jiao Tong Univ, Collaborat Innovat Ctr IFSA CICIFSA, Shanghai 200240, Peoples R China |
Recommended Citation GB/T 7714 | Han, Bo,Wang, Feilu,Salzmann, David,et al. Emission mechanism for the silicon He-alpha lines in a photoionization experiment[J]. HIGH POWER LASER SCIENCE AND ENGINEERING,2021,9:8. |
APA | Han, Bo,Wang, Feilu,Salzmann, David,Zhong, Jiayong,&Zhao, Gang.(2021).Emission mechanism for the silicon He-alpha lines in a photoionization experiment.HIGH POWER LASER SCIENCE AND ENGINEERING,9,8. |
MLA | Han, Bo,et al."Emission mechanism for the silicon He-alpha lines in a photoionization experiment".HIGH POWER LASER SCIENCE AND ENGINEERING 9(2021):8. |
Files in This Item: | There are no files associated with this item. |
Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Edit Comment