ATOMIC DATA AND SPECTRAL-LINE INTENSITIES FOR O-VIII AND FE-XVII RESONANCE LINES AS WELL AS THEIR O-VII AND FE-XVI SATELLITE LINES

被引：0
作者：
CORNILLE, M
DUBAU, J
FAUCHER, P
BELYDUBAU, F
BLANCARD, C
机构：
[1] OBSERV COTE AZUR,CNRS,URA 1362,F-06304 NICE 4,FRANCE
[2] CTR ETUD LIMEIL VALENTON,F-94195 VILLENEUVE ST GEO,FRANCE
来源：
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1994年 / 105卷 / 01期
关键词：
ATOMIC DATA; LINES; IDENTIFICATION; SUN; CORONA; X-RAYS; GENERAL;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The atomic data required to analyse low density coronal plasmas have been calculated and used to interpret X-ray spectra observed by the Flat Crystal Spectrometer of the SMM/NASA satellite in the 14 - 19 angstrom wavelength range. The emission lines correspond mainly to Fe XVI, Fe XVII, Fe XVIII and some ones to O VII, O VIII.
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页码：77 / 90
页数：14
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