首页> 外文期刊>The Astrophysical journal >THE OPTICALLY THICK Fe XVII SPECTRUM: X-RAY, EXTREME-ULTRAVIOLET, AND FORBIDDEN LINE RATIOS
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THE OPTICALLY THICK Fe XVII SPECTRUM: X-RAY, EXTREME-ULTRAVIOLET, AND FORBIDDEN LINE RATIOS

机译:光学上较厚的Fe XVII光谱:X射线,极端超视距和禁忌线比例

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摘要

Level populations, X-ray line fluxes, and extreme-ultraviolet (EUV) line intensities are calculated for a 37 level model of the Fe XVII ion, as functions of the column density of Fe XVII, in slab geometry and cylindrical geometry. The resonance lines at 15.02 and 15.25 A are found to exhibit initial increases in fluxes relative to the forbidden line at 17.10 A and the usual reference resonance line at 16.78 A as optical thickness increases. Eleven EUV lines and the forbidden 2p~53s(~3P_o-~3p_1) transition near 1154 A are also found to be relatively enhanced by opacity.
机译:对于37级Fe XVII离子模型,根据平板几何形状和圆柱几何形状中Fe XVII离子的柱密度,计算出了水平填充,X射线线通量和极紫外(EUV)线强度。发现随着光学厚度的增加,相对于在17.10 A处的禁止线和在16.78 A处的通常参考共振线,在15.02和15.25 A处的共振线表现出通量的初始增加。还发现11条EUV线和1154 A附近的禁止2p〜53s(〜3P_o-〜3p_1)跃迁由于不透明而相对增强。

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