Variation in the 160.010 m period of the solar relative difference brightness

YNAO OpenIR > 其他

	Variation in the 160.010 m period of the solar relative difference brightness
	Li RF(李如凤); KOTOV, VA; DIDKOVSKY, LV; LI, RF
发表期刊	SCIENCE IN CHINA SERIES A-MATHEMATICS PHYSICS ASTRONOMY
	1990-09
卷号	33 期号:9 页码:1100-1105
产权排序	第1完成单位
收录类别	SCI
摘要	Two photoelectric diode arrays (16 x 16 and 32 x 32 pixels, respectively) were used to measure the difference brightness of the center of the sun with respect to the limb of the solar disk in 1986 at wavelengths of 0.7-0.8 micron. The results indicate a period of 160 m and an average amplitude of 0.00008 solar relative intensity unit. A refined value of the oscillation period of 160.0099 m is obtained from the periodic values of the difference brightness observed for 358 days (1870 hr) over the period 1976-1986 at the Crimean Astrophysical Observatory. This is in good agreement with the IR observed value of 160.0100 m (+ or - 6) and a value of 160.010 m (+ or - 1) obtained at the Doppler difference velocity.
语种	英语
学科领域	Mathematics
文章类型	Article
ISSN	1001-6511
URL	查看原文
WOS记录号	WOS:A1990ED28100008
WOS研究方向	Mathematics
WOS类目	Mathematics, Applied ; Mathematics
引用统计
文献类型	期刊论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/4074
专题	其他
通讯作者	LI, RF
推荐引用方式 GB/T 7714	Li RF,KOTOV, VA,DIDKOVSKY, LV,et al. Variation in the 160.010 m period of the solar relative difference brightness[J]. SCIENCE IN CHINA SERIES A-MATHEMATICS PHYSICS ASTRONOMY,1990,33(9):1100-1105.
APA	李如凤,KOTOV, VA,DIDKOVSKY, LV,&LI, RF.(1990).Variation in the 160.010 m period of the solar relative difference brightness.SCIENCE IN CHINA SERIES A-MATHEMATICS PHYSICS ASTRONOMY,33(9),1100-1105.
MLA	李如凤,et al."Variation in the 160.010 m period of the solar relative difference brightness".SCIENCE IN CHINA SERIES A-MATHEMATICS PHYSICS ASTRONOMY 33.9(1990):1100-1105.

条目包含的文件
文件名称/大小	文献类型	版本类型	开放类型	使用许可
VARIATIONINTHE16_省略_（286KB）	期刊论文	作者接受稿	开放获取	CC BY-NC-SA	浏览请求全文