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作者: Feng Hua* & Jiamin Yangb 文题: Plasma effect on the Kα group emission of He-like molybdenum 期刊名,年份,卷(期),起止页码: Radiation Effects and Defects in Solids: Incorporating Plasma Science and Plasma Technology Volume 168, Issue 10, 2013 全文链接: http://www.tandfonline.com/doi/a ... 832251#.UqlmhWfUOVU 数据库名称: tandfonline.com |
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baiyuefei
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hf6391964: 金币+5, ★★★★★最佳答案, 非常感谢~~~~~ 2013-12-15 19:16:03
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恭喜，EI收录了，SCI暂未收录 Accession number: 20134316877520 Title: Plasma effect on the K α group emission of He-like molybdenum Authors: Hu, Feng1 ; Yang, Jiamin2 Author affiliation: 1School of Mathematic and Physical Science, Xuzhou Institute of Technology, Xuzhou 221400, China 2Research Center of Laser Fusion, China Academy of Engineering Physics, Mianyang 621900, China Corresponding author: Hu, F. (hufengscu@139.com) Source title: Radiation Effects and Defects in Solids Abbreviated source title: Radiat Eff Defects Solids Volume: 168 Issue: 10 Issue date: October 1, 2013 Publication year: 2013 Pages: 858-865 Language: English ISSN: 10420150 E-ISSN: 10294953 CODEN: REDSEI Document type: Journal article (JA) Publisher: Taylor and Francis Inc., 325 Chestnut St, Suite 800, Philadelphia, PA 19106, United States Abstract: The intercombination line (1s2p(3P1)-1s2) and the resonance line (1s2p(1P1)-1s2) of He-like Mo, which are the two electronic dipole transitions in the Kα group emissions, are studied under dense plasma conditions by using the ion-sphere model combined with the multi-configuration Dirac-Fock model. The results show that the two electronic dipole transitions red shift nearly linearly with the increase in plasma electron density. Moreover, the red-shift energy becomes more sensitive to the plasma electron density, when the plasma electron temperature is lower. It is worth to note that the energy discrepancy between these two spectral lines is equal to the exchange energy of state 1s2p (3P1). This result may be useful to dense plasma diagnosis in connection with variation of the relative position and the spectral fine structure splitting in high-density plasmas. © 2013 Taylor & Francis. |
2楼2013-12-13 10:30:51
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