气候变化领域集成服务门户(CCPortal): Excitation of the venus night airglow

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DOI	10.1126/science.195.4278.573
	Excitation of the venus night airglow
	Lawrence G.M.; Barth C.A.; Argabright V.
发表日期	1977
ISSN	0036-8075
起始页码	573
结束页码	574
卷号	195 期号:4278
英文摘要	The strongest spectral features in the Venus night airglow between 3000 and 8000 angstroms are identified as the Herzberg II (c1Σ u- - X3Σg- bands of molecular oxygen. These bands have been produced in a laboratory afterglow by the recombination of oxygen atoms in the presence of carbon dioxide molecules. It is hypothesized that the same mechanism produces this emission in the upper atmosphere of Venus.
语种	英语
来源期刊	Science
文献类型	期刊论文
条目标识符	http://gcip.llas.ac.cn/handle/2XKMVOVA/244469
作者单位	Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder 80309
推荐引用方式 GB/T 7714	Lawrence G.M.,Barth C.A.,Argabright V.. Excitation of the venus night airglow[J],1977,195(4278).
APA	Lawrence G.M.,Barth C.A.,&Argabright V..(1977).Excitation of the venus night airglow.Science,195(4278).
MLA	Lawrence G.M.,et al."Excitation of the venus night airglow".Science 195.4278(1977).