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Volumn 278, Issue 5341, 1997, Pages 1276-1278

Mechanism for the green glow of the upper ionosphere

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; ATMOSPHERE; ATMOSPHERIC TRANSPORT; CHEMICAL ANALYSIS; DISSOCIATION; ELECTRON TRANSPORT; EMISSION TOMOGRAPHY; ENERGY BALANCE; OXYGEN AFFINITY; PRIORITY JOURNAL; THEORY;

EID: 0030680118     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.278.5341.1276     Document Type: Article
Times cited : (46)

References (39)
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    • note
    • g, the excitation energy differences are 0.06 eV (29) and 0.1636 eV (28), respectively. These energy differences are accounted for in the rate coefficient uncertainties.
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    • note
    • MOLPRO is a package of ab initio programs written by H.-J. Werner and P. J. Knowles, with contributions from J. Almlöf, R. D. Amos, M. J. O. Deegan, S. T. Elbert, C. Hampel, W. Meyer, K. Peterson, R. Pitzer, A. J. Stone, P. R. Taytor, and R. Lindh. Contact molpro-request@tc.bham.ac.uk
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    • Supported by NASA grants NAG5-4316 and NAG5-4286 and NSF grant ATM-9503224
    • Supported by NASA grants NAG5-4316 and NAG5-4286 and NSF grant ATM-9503224.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.