CLASSIFICATION OF SPECTRA OF K, CA, SC, TI, V AND CR AND EXTRAPOLATION TO FE SOLAR-FLARE LINES

被引：72

作者：

FAWCETT, BC ^{[1
]}

HAYES, RW ^{[1
]}

机构：

[1] SCI RES COUNCIL,APPLETON LAB,ASTROPHYS RES DIV,CULHAM LAB,ABINGDON,OXFORDSHIRE,ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1975年 / 170卷 / 01期

关键词：

Astrophysics; -; NASA;

D O I：

10.1093/mnras/170.1.185

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Potassium, calcium, scandium, titanium, vanadium and chromium emission lines are classified in the same isoelectronic sequences as Fe XIX to Fe XXIII. Most of the lines identified belong to the zpn-zpn-13d or zs2zpk-zszpk+l transition arrays. The data presented permit the calculation of the wavelengths of Fe XIX to Fe XXIII emission lines which are emitted from solar flares. Experimental data are based on spectral observations of plasmas generated when the output of a 4 GW laser is focused on to solid targets. © Royal Astronomical Society • Provided by the NASA Astrophysics Data System.

引用

页码：185 / 197

页数：13

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