Absorption and photoionization cross sections of CO 2 , CO, Ar, and He at intense solar emission lines
1965; American Geophysical Union; Volume: 70; Issue: 1 Linguagem: Inglês
10.1029/jz070i001p00099
ISSN2156-2202
AutoresRobert B. Cairns, James A. R. Samson,
Tópico(s)Laser Design and Applications
ResumoJournal of Geophysical Research (1896-1977)Volume 70, Issue 1 p. 99-104 Absorption and photoionization cross sections of CO2, CO, Ar, and He at intense solar emission lines R. B. Cairns, R. B. CairnsSearch for more papers by this authorJames A. R. Samson, James A. R. SamsonSearch for more papers by this author R. B. Cairns, R. B. CairnsSearch for more papers by this authorJames A. R. Samson, James A. R. SamsonSearch for more papers by this author First published: 1 January 1965 https://doi.org/10.1029/JZ070i001p00099Citations: 76AboutPDF ToolsRequest permissionExport citationAdd to favoritesTrack citation ShareShare Give accessShare full text accessShare full-text accessPlease review our Terms and Conditions of Use and check box below to share full-text version of article.I have read and accept the Wiley Online Library Terms and Conditions of UseShareable LinkUse the link below to share a full-text version of this article with your friends and colleagues. Learn more.Copy URL Abstract Photoionization and total absorption cross sections have been measured for CO2, CO, Ar, and He at the wavelengths in the region 1040 A to 300 A which correspond to intense solar emission lines. The wavelength resolution, determined from the measured width of each of the spectral lines generated within the light sources, was in the range 0.04 to 0.1 A. Citing Literature Volume70, Issue11 January 1965Pages 99-104 RelatedInformation
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