ON SOLAR EMISSION-LINES

被引：13

作者：

MALIK, GP ^{[1
]}

PANDE, LK ^{[1
]}

VARMA, VS ^{[1
]}

机构：

[1] JAWAHARLAL NEHRU UNIV,SCH ENVIRONM SCI,NEW DELHI 110067,INDIA

来源：

ASTROPHYSICAL JOURNAL | 1991年 / 379卷 / 02期

关键词：

ATOMIC PROCESSES; LINE FORMATION; SUN CORONA; SUN SPECTRA;

D O I：

10.1086/170554

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We draw attention to the large number of unidentified solar emission lines and the various ingenious ideas that have been proposed from time to time to resolve the problem. An attempt is made to tackle the problem on the basis of one fundamental system consisting of an electron and a proton, the Coulomb potential between which is regulated by temperature. Use is made of an equation which has recently been given for the description of such a system.

引用

页码：788 / 795

页数：8

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