TY - JOUR
T1 - Measurement and analysis of K-shell lines of silicon ions in laser plasmas
AU - Han, Bo
AU - Wang, Feilu
AU - Zhong, Jiayong
AU - Liang, Guiyun
AU - Wei, Huigang
AU - Yuan, Dawei
AU - Zhu, Baojun
AU - Li, Fang
AU - Liu, Chang
AU - Li, Yanfei
AU - Zhao, Jiarui
AU - Zhang, Zhe
AU - Wang, Chen
AU - Xiong, Jun
AU - Jia, Guo
AU - Hua, Neng
AU - Zhu, Jianqiang
AU - Li, Yutong
AU - Zhao, Gang
AU - Zhang, Jie
N1 - Publisher Copyright:
© The Author(s) 2018.
PY - 2018
Y1 - 2018
N2 - We present laboratory measurement and theoretical analysis of silicon K-shell lines in plasmas produced by Shenguang II laser facility, and discuss the application of line ratios to diagnose the electron density and temperature of laser plasmas. Two types of shots were carried out to interpret silicon plasma spectra under two conditions, and the spectra from 6.6 Å to 6.85 Å were measured. The radiative-collisional code based on the flexible atomic code (RCF) is used to identify the lines, and it also well simulates the experimental spectra. Satellite lines, which are populated by dielectron capture and large radiative decay rate, influence the spectrum profile significantly. Because of the blending of lines, the traditional G value and R value are not applicable in diagnosing electron temperature and density of plasma. We take the contribution of satellite lines into the calculation of line ratios of He-α lines, and discuss their relations with the electron temperature and density.
AB - We present laboratory measurement and theoretical analysis of silicon K-shell lines in plasmas produced by Shenguang II laser facility, and discuss the application of line ratios to diagnose the electron density and temperature of laser plasmas. Two types of shots were carried out to interpret silicon plasma spectra under two conditions, and the spectra from 6.6 Å to 6.85 Å were measured. The radiative-collisional code based on the flexible atomic code (RCF) is used to identify the lines, and it also well simulates the experimental spectra. Satellite lines, which are populated by dielectron capture and large radiative decay rate, influence the spectrum profile significantly. Because of the blending of lines, the traditional G value and R value are not applicable in diagnosing electron temperature and density of plasma. We take the contribution of satellite lines into the calculation of line ratios of He-α lines, and discuss their relations with the electron temperature and density.
KW - High energy density physics
KW - Laser plasmas interaction
KW - Plasmas astrophysics
UR - https://www.scopus.com/pages/publications/85100790709
U2 - 10.1017/hpl.2018.25
DO - 10.1017/hpl.2018.25
M3 - 文章
AN - SCOPUS:85100790709
SN - 2052-3289
VL - 6
JO - High Power Laser Science and Engineering
JF - High Power Laser Science and Engineering
M1 - e31
ER -