Artigo Revisado por pares

Intensity of the first negative band system of nitrogen in the night sky over Arecibo

1977; American Geophysical Union; Volume: 82; Issue: 13 Linguagem: Inglês

10.1029/ja082i013p01855

ISSN

2156-2202

Autores

J. W. Meriwether, James C. G. Walker,

Tópico(s)

Solar and Space Plasma Dynamics

Resumo

Journal of Geophysical Research (1896-1977)Volume 82, Issue 13 p. 1855-1858 Intensity of the first negative band system of nitrogen in the night sky over Arecibo John W. Meriwether Jr., John W. Meriwether Jr.Search for more papers by this authorJames C. G. Walker, James C. G. WalkerSearch for more papers by this author John W. Meriwether Jr., John W. Meriwether Jr.Search for more papers by this authorJames C. G. Walker, James C. G. WalkerSearch for more papers by this author First published: 1 May 1977 https://doi.org/10.1029/JA082i013p01855Citations: 10AboutPDF 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 Share a linkShare onEmailFacebookTwitterLinkedInRedditWechat Abstract The 0–1 band (4278 Å) of the first negative system of nitrogen has been measured in the spectrum of the night sky with a 1-m Ebert-Fastie spectrophotometer at the Arecibo Observatory. Integration periods of approximately 4 hours were needed to provide an adequate ratio of signal to noise. The measured spectra were corrected for blending with the 2–9 Herzberg band of oxygen at 4281 Å. The intensity of the 4278-Å radiation measured on 6 nights in late March 1976 was about 0.1 R. Little variation in the intensity was observed from night to night. We suggest that most of the observed emission was produced not by charged particle bombardment of the atmosphere but by photoionization of N2 by scattered solar radiation at 304 and 584 Å. References Banks, P. M., G. Kockarts, Aeronomy, Part B, Academic, New York, 1973. Borst, W. L., E. C. 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