INTENSITY OSCILLATIONS OF THE FE XIV (LAMBDA=530.3 NM) SOLAR CORONA - DISTURBANCES DUE TO THE WAVE PROCESSES IN THE EARTHS ATMOSPHERE

被引：3

作者：

DERMENDJIEV, VN

KOLAROV, GV

MITSEV, TA

机构：

[1] BULGARIAN ACAD SCI,NAO,BU-1784 SOFIA,BULGARIA

[2] BULGARIAN ACAD SCI,INST ELECTR,BU-1784 SOFIA,BULGARIA

来源：

SOLAR PHYSICS | 1992年 / 137卷 / 01期

关键词：

D O I：

10.1007/BF00146584

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The short period oscillations of the earth's atmosphere transparency for the spectral line lambda = 510.6 nm are studied using lidar data. The results obtained are discussed in connection with the problem of the reliability of short period intensity oscillations of the Fe XIV (lambda = 530.3 nm) solar coronal emission line. The main conclusion is that the green coronal oscillations with periods shorter than 60 s are realistic.

引用

页码：199 / 202

页数：4

共 11 条

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[2]

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[3]

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