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• W2083351043 abstract "Abstract The variation of the intensities of the visible and vacuum ultraviolet emissions from the Lewis-Rayleigh afterglow of nitrogen is studied with the variation of nitrogen pressure. It has been found that the intensity of the visible emission is directly proportional to the intensity of the vacuum ultraviolet emission for nitrogen pressures below 0.25 torr. At higher pressures, the relative intensity of vacuum-ultraviolet radiation is smaller. This has been interpreted as due to the self-quenching of the N 2 (a 1 £ g ) molecules, which emit the LBH system in the vacuum ultraviolet region. The observations are utilized to obtain the quenching cross-section of N 2 a 1 £ g state by N2, which is found to be about 10-18 cm2." @default.
• W2083351043 created "2016-06-24" @default.
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• W2083351043 date "1972-12-01" @default.
• W2083351043 modified "2023-09-25" @default.
• W2083351043 title "The mechanism of vacuum ultraviolet emission from the Lewis-Rayleigh nitrogen afterglow" @default.
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• W2083351043 doi "https://doi.org/10.1016/0022-4073(72)90105-7" @default.
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