1968
DOI: 10.1016/0032-0633(68)90136-0
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New measurements of the fluorescence efficiency of air under electron bombardment

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1968
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Cited by 46 publications
(9 citation statements)
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“…1,2 These have mainly focused on emission from excited nitrogen and air 3,4 and from atmospheric nuclear weapons 5 testing, as well as upper atmosphere studies. 6 However, the development of powerful gasphase, e-beam-pumped exciplex lasers over the past 20 years has stimulated further investigations in this field, with reported determinations of the total and component process yields in some rare gas systems. 7 In several recent experimental investigations 8,9 absolute fluorescence yields of pulse electron-irradiated rare gas/halogen source gas mixtures (R/AX) for the RX* (B,C) states of XeBr* (Xe/CF 3 Br), 8 KrF* (Kr/SF 6 ), 9 and XeF* (Xe/SF 6 ) 9 have been measured.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…1,2 These have mainly focused on emission from excited nitrogen and air 3,4 and from atmospheric nuclear weapons 5 testing, as well as upper atmosphere studies. 6 However, the development of powerful gasphase, e-beam-pumped exciplex lasers over the past 20 years has stimulated further investigations in this field, with reported determinations of the total and component process yields in some rare gas systems. 7 In several recent experimental investigations 8,9 absolute fluorescence yields of pulse electron-irradiated rare gas/halogen source gas mixtures (R/AX) for the RX* (B,C) states of XeBr* (Xe/CF 3 Br), 8 KrF* (Kr/SF 6 ), 9 and XeF* (Xe/SF 6 ) 9 have been measured.…”
Section: Introductionmentioning
confidence: 99%
“…+ AX f X -+ A thermal electron capture(3)R* + AX f RX* + A rare gas excited-state reaction (+ R f RX* + 2R three-body ionic recombination(6) …”
mentioning
confidence: 99%
“…The fluorescent light is produced mostly in the near UV and 9 1995 American Institute of Physics 839 blue region. [1] Oda and others [2] pointed out that a cosmic ray cascade (known as an" extensive air shower) in the atmosphere would cause the air to glow along the path of the cascade. A detector made to observe the air glow induced by cosmic ray showers would be able to observe, event by event, the entire longitudinal cascade being developed in the atmosphere, a feat that ground arrays are unable to achieve.…”
Section: Introductionmentioning
confidence: 99%
“…[2][3][4][5][6][7][8][9] In laboratory experiments here, Hartman 8 has obtained spectra of the emission of air at 70-p. pressure excited by 850-eV electrons and has measured efficiencies for some of the nitrogen bands, including the important 3914-A (0, 0) N 2 + first negative band. [2][3][4][5][6][7][8][9] In laboratory experiments here, Hartman 8 has obtained spectra of the emission of air at 70-p. pressure excited by 850-eV electrons and has measured efficiencies for some of the nitrogen bands, including the important 3914-A (0, 0) N 2 + first negative band.…”
Section: Introductionmentioning
confidence: 99%