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• W2138828360 startingPage "2511" @default.
• W2138828360 abstract "Rocket measurements of the O I ‘green line’ (¹ S ‐¹ D ) at 5577 Å and the O 2 (0, 0) atmospheric band at 7620 Å were made in a steady IBC II + aurora, simultaneously with measurements of N 2 emissions and the auroral electron flux. An empirical model based on these data demonstrates that the principal excitation source of O 2 ( b ¹Σ g + ) is energy transfer from O(¹ D ), with direct electron impact of O 2 contributing less than 5%. The altitude profile of the green line emission, taking into account quenching of O(¹ S ) by O(³ P ) near the lower border of the aurora, resembles what would be produced by electron impact excitation of O 2 but would require a dissociative excitation cross section of 10 −16 cm². None of the other known O(¹ S ) excitation mechanisms are capable of producing the observed emission rate." @default.
• W2138828360 created "2016-06-24" @default.
• W2138828360 creator A5010120800 @default.
• W2138828360 date "1978-06-01" @default.
• W2138828360 modified "2023-09-26" @default.
• W2138828360 title "Auroral excitation of optical emissions of atomic and molecular oxygen" @default.
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• W2138828360 doi "https://doi.org/10.1029/ja083ia06p02511" @default.
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