气候变化领域集成服务门户(CCPortal): Mariner 6: Origin of Mars ionized carbon dioxide ultraviolet spectrum

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DOI	10.1126/science.167.3924.1490
	Mariner 6: Origin of Mars ionized carbon dioxide ultraviolet spectrum
	Dalgarno A.; Degges T.C.; Stewart A.I.
发表日期	1970
ISSN	0036-8075
起始页码	1490
结束页码	1491
卷号	167 期号:3924
英文摘要	The predicted intensities of the ionized carbon dioxide (CO2+) emission feature at 2890 angstroms and the Fox-Duffendack-Barker bands are 5.2 and 19.9 kilorayleighs, respectively, for a vertical column. Direct photo-ionization of carbon dioxide by solar radiation contributes 3.5 and 4.1 kilorayleighs, respectively, and fluorescent scattering by CO2+, 1.6 and 15.3 kilorayleighs, respectively. Photoelectron impacts are less important.
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/243452
作者单位	Harvard College Observatory, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, United States; Technology Division, GCA Corporation, Bedford, MA 01730, United States; Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80302, United States
推荐引用方式 GB/T 7714	Dalgarno A.,Degges T.C.,Stewart A.I.. Mariner 6: Origin of Mars ionized carbon dioxide ultraviolet spectrum[J],1970,167(3924).
APA	Dalgarno A.,Degges T.C.,&Stewart A.I..(1970).Mariner 6: Origin of Mars ionized carbon dioxide ultraviolet spectrum.Science,167(3924).
MLA	Dalgarno A.,et al."Mariner 6: Origin of Mars ionized carbon dioxide ultraviolet spectrum".Science 167.3924(1970).