A simulation package for soft X-ray and EUV spectroscopy of astrophysical and laboratory plasmas in different environments

28th International Conference on Photonic, Electronic and Atomic Collisions

Liang, G.Y.^1 ; Li, F.^1 ; Wang, F.L.^1 ; Wu, Y.^2 ; Zhong, J.Y.^1 ; Zhao, G.^1

Key Laboratory of Optical Astronomy, National Astronomical Observatories, CAS, Beijing, China^1

Institute of Applied Physics and Computational Mathematics, Beijing, China^2

关键词: Astrophysical objects;    Astrophysical phenomena;    Laboratory astrophysics;    Research communities;    Self consistent modeling;    Spectroscopic research;    Theoretical modelling;    Visualized simulation;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/488/15/152008/pdf
DOI  :  10.1088/1742-6596/488/15/152008

来源: IOP

【 摘 要 】

Spectroscopic researches in astronomy are significantly dependent on theoretical modelling methods, such as Chianti, Xstar, Cloudy etc. Recently, a different research community - Laboratory Astrophysics tries to benchmark these theoretical models or simulate the astrophysical phenomenon directly in conditions accessed in ground laboratory. Those unavoidable differences between the astrophysical objects and laboratory provide a need for a self-consistent model to make a bridge for the two cases. So we setup a visualized simulation package for soft X-ray and EUV spectroscopy in astrophysical and laboratory plasmas.