NAOC Open IR
A simulation package-SASAL for X-ray and EUV spectroscopy of astrophysical and laboratory plasmas
Liang Guiyun1; Li Fang1; Wang Feilu1; Wu Yong2; Zhong Jiayong1; Zhao Gang1
2014
Source PublicationResearch in Astronomy and Astrophysics
ISSN1674-4527
Volume14Issue:10Pages:1351
AbstractFor the laboratory astrophysics community, those spectroscopic modeling codes extensively used in astronomy, e.g. Chianti, AtomDB, Cloudy and Xstar, cannot be directly applied to analyzing laboratory measurements due to their discrepancies from astrophysical cases. For example, plasma from an electron beam ion trap has an electron energy distribution that follows a Gaussian profile, instead of a Maxwellian one. The laboratory miniature for a compact object produced by a laser-driven implosion shows a departure from equilibrium, that often occurs in celestial objects, so we setup a spectral analysis system for astrophysical and laboratory (SASAL) plasmas to act as a bridge between them, which benefits the laboratory astrophysical community.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/52909
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.Data Center for High Energy Density Physics, Institute of Applied Physics and Computational Mathematics
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Liang Guiyun,Li Fang,Wang Feilu,et al. A simulation package-SASAL for X-ray and EUV spectroscopy of astrophysical and laboratory plasmas[J]. Research in Astronomy and Astrophysics,2014,14(10):1351.
APA Liang Guiyun,Li Fang,Wang Feilu,Wu Yong,Zhong Jiayong,&Zhao Gang.(2014).A simulation package-SASAL for X-ray and EUV spectroscopy of astrophysical and laboratory plasmas.Research in Astronomy and Astrophysics,14(10),1351.
MLA Liang Guiyun,et al."A simulation package-SASAL for X-ray and EUV spectroscopy of astrophysical and laboratory plasmas".Research in Astronomy and Astrophysics 14.10(2014):1351.
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