The excitation of the O(1S) state by the dissociative recombination of O2(+) ions - Electron temperature dependence
The rate coefficient for the excitation of the O(1S) state due to the dissociative recombination of O2(+) (v of not greater than 3) ions has been determined as a function of the electron temperature from 300-3500 K. In agreement with the work of Guberman (1987), the results suggest that the absolute...
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Veröffentlicht in: | Planetary and space science 1988-06, Vol.36, p.621-628 |
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description | The rate coefficient for the excitation of the O(1S) state due to the dissociative recombination of O2(+) (v of not greater than 3) ions has been determined as a function of the electron temperature from 300-3500 K. In agreement with the work of Guberman (1987), the results suggest that the absolute magnitude of alpha(1S) is nearly the same for a wide variety of O2(+) vibrational distributions over the electron temperature range normally encountered in the nocturnal F-region. It is noted that previous studies which modeled 5577-A airglow data using a fixed value for f(1S) may be misleading. |
doi_str_mv | 10.1016/0032-0633(88)90030-X |
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In agreement with the work of Guberman (1987), the results suggest that the absolute magnitude of alpha(1S) is nearly the same for a wide variety of O2(+) vibrational distributions over the electron temperature range normally encountered in the nocturnal F-region. It is noted that previous studies which modeled 5577-A airglow data using a fixed value for f(1S) may be misleading.</description><identifier>ISSN: 0032-0633</identifier><identifier>DOI: 10.1016/0032-0633(88)90030-X</identifier><language>eng</language><publisher>Legacy CDMS</publisher><subject>Geophysics</subject><ispartof>Planetary and space science, 1988-06, Vol.36, p.621-628</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Zipf, Edward C.</creatorcontrib><title>The excitation of the O(1S) state by the dissociative recombination of O2(+) ions - Electron temperature dependence</title><title>Planetary and space science</title><description>The rate coefficient for the excitation of the O(1S) state due to the dissociative recombination of O2(+) (v of not greater than 3) ions has been determined as a function of the electron temperature from 300-3500 K. In agreement with the work of Guberman (1987), the results suggest that the absolute magnitude of alpha(1S) is nearly the same for a wide variety of O2(+) vibrational distributions over the electron temperature range normally encountered in the nocturnal F-region. 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In agreement with the work of Guberman (1987), the results suggest that the absolute magnitude of alpha(1S) is nearly the same for a wide variety of O2(+) vibrational distributions over the electron temperature range normally encountered in the nocturnal F-region. It is noted that previous studies which modeled 5577-A airglow data using a fixed value for f(1S) may be misleading.</abstract><cop>Legacy CDMS</cop><doi>10.1016/0032-0633(88)90030-X</doi><tpages>8</tpages></addata></record> |
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ispartof | Planetary and space science, 1988-06, Vol.36, p.621-628 |
issn | 0032-0633 |
language | eng |
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source | Elsevier ScienceDirect Journals Complete; NASA Technical Reports Server |
subjects | Geophysics |
title | The excitation of the O(1S) state by the dissociative recombination of O2(+) ions - Electron temperature dependence |
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