THEORETICAL EMISSION-LINE STRENGTHS FOR THE BERYLLIUM-LIKE ION S-XIII COMPARED TO XUV OBSERVATIONS OF SOLAR-FLARES

被引：9

作者：

KEENAN, FP ^{[1
]}

MCCANN, SM ^{[1
]}

WIDING, KG ^{[1
]}

机构：

[1] USN,RES LAB,EO HULBURT CTR SPACE RES,WASHINGTON,DC 20375

来源：

SOLAR PHYSICS | 1988年 / 117卷 / 01期

关键词：

D O I：

10.1007/BF00148573

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：69 / 75

页数：7

共 36 条

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