SULFUR IX TO XIII SPECTRAL MEASURMENTS BETWEEN 170 AND 500 angstrom

doi:10.1088/0004-6256/137/4/4020

	SULFUR IX TO XIII SPECTRAL MEASURMENTS BETWEEN 170 AND 500 angstrom
	Du, S. B.2; Yang, Z. H.1; Cai, X. H.1; Yu, D. Y.1; Wang, W.1 ; Zhang, B. L.1; Chang, H. W.2; Zeng, X. T.2
刊名	ASTRONOMICAL JOURNAL
	2009-04-01
卷号	137 页码:4020-4023
关键词	atomic data line: identification methods: laboratory ultraviolet: general
ISSN号	0004-6256
DOI	10.1088/0004-6256/137/4/4020
英文摘要	This paper reports laboratory measurements of the spectrum of highly ionized sulfur. The spectrum of S IX - S XIII has been observed in the wavelength range 170 - 500 angstrom. A total of 54 lines have been measured. Forty-two of them have been classified as 2s(2)2p(k)-2s(2)p(k+) 1 and 2s2p(k)-2p(k+1) transitions. Twelve other lines have been ascribed to 2s-2p, 4p-5s, 5p6s, 5d-6p, and 6p-8d transitions. These spectral lines have been identified, among which 22 are new and accurately measured. The analysis of the spectra was based on a comparison with other experimental results and calculated values.
资助项目	National Natural Science Foundation of China[10774149]
WOS关键词	SOLAR-FLARE ; WAVELENGTHS ; XIV ; CLASSIFICATIONS ; EMISSION ; REGION ; LINES ; XVI
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	IOP PUBLISHING LTD
WOS记录号	WOS:000264046100028
资助机构	National Natural Science Foundation of China
内容类型	期刊论文
源URL	[http://119.78.100.186/handle/113462/30865]
专题	近代物理研究所_实验物理中心
通讯作者	Yang, Z. H.
作者单位	1.Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China 2.China Inst Atom Energy, Dept Nucl Phys, Beijing 102413, Peoples R China
推荐引用方式 GB/T 7714	Du, S. B.,Yang, Z. H.,Cai, X. H.,et al. SULFUR IX TO XIII SPECTRAL MEASURMENTS BETWEEN 170 AND 500 angstrom[J]. ASTRONOMICAL JOURNAL,2009,137:4020-4023.
APA	Du, S. B..,Yang, Z. H..,Cai, X. H..,Yu, D. Y..,Wang, W..,...&Zeng, X. T..(2009).SULFUR IX TO XIII SPECTRAL MEASURMENTS BETWEEN 170 AND 500 angstrom.ASTRONOMICAL JOURNAL,137,4020-4023.
MLA	Du, S. B.,et al."SULFUR IX TO XIII SPECTRAL MEASURMENTS BETWEEN 170 AND 500 angstrom".ASTRONOMICAL JOURNAL 137(2009):4020-4023.