1972
DOI: 10.1088/0022-3700/5/12/026
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Dissociative recombination at elevated temperatures. IV. N2+dominated afterglows

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Cited by 35 publications
(13 citation statements)
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“…No uncertainty is given with respect to the power-law exponent, but an error of 20% seems reasonable. A theoretical work by Guberman (2003) concluded that the electron temperature dependence is slightly different for 600 K T e 3000 K. Considering now the absolute rate constant k, analysis of the literature shows that several experiments (Canosa et al 1991;Cunningham & Hobson 1972;Geoghegan et al 1991;Mehr & Biondi 1969) …”
Section: (±30%)mentioning
confidence: 98%
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“…No uncertainty is given with respect to the power-law exponent, but an error of 20% seems reasonable. A theoretical work by Guberman (2003) concluded that the electron temperature dependence is slightly different for 600 K T e 3000 K. Considering now the absolute rate constant k, analysis of the literature shows that several experiments (Canosa et al 1991;Cunningham & Hobson 1972;Geoghegan et al 1991;Mehr & Biondi 1969) …”
Section: (±30%)mentioning
confidence: 98%
“…They have observed only dissociative charge transfer products with branching ratios (T e /300) −0.39 cm 3 s −1 (±25%). The dissociative recombination of N + 2 has been extensively studied, both experimentally (Canosa et al 1991;Cunningham & Hobson 1972;Geoghegan et al 1991;Kasner 1967;Kella et al 1996;Mahdavi et al 1971;Mehr & Biondi 1969;Mul & McGowan 1979;Noren et al 1989;Oddone et al 1997;Peterson et al 1998;Queffelec et al 1985;Sheehan & St. Maurice 2004;Zipf 1980) and theoretically (Guberman 1991(Guberman , 2003(Guberman , 2012Guberman et al 1993). The interest in the reaction arises because of its involvement in Earth's atmosphere photochemistry (Fox & Dalgarno 1985;Torr & Torr 1979), and more generally in the chemistry of terrestrial planet ionospheres (Fox 1992(Fox , 1993Fox et al 1993).…”
Section: (±30%)mentioning
confidence: 99%
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“…The rate coefficient k DR for this rapid process had been obtained by Cunningham and Hobson 35 and is given by k DR = 1.47 ϫ 10 −12 ͑T e ͓K͔͒ −0.37 m 3 s −1 . ͑9͒…”
Section: A the Modelmentioning
confidence: 99%