2019
DOI: 10.1134/s0030400x19110110
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On the Selectivity of Population of the Neon Excited Levels in the Decaying He–Ne Plasma

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Cited by 6 publications
(6 citation statements)
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“…On the one hand, this deionization mechanism determines the properties of a wide range of laboratory plasma objects and is a necessary link in models of stellar and planetary atmospheres [2]. On the other hand, despite the long history of studying the process, previously unknown manifestations of DR are found even in the case of the simplest molecular ions, such as H + 2 [3] or HeNe + [4], which stimulates the development of new approaches to the calculation of its main characteristics i.e. cross-sections and rate constants [5].…”
Section: Introductionmentioning
confidence: 99%
“…On the one hand, this deionization mechanism determines the properties of a wide range of laboratory plasma objects and is a necessary link in models of stellar and planetary atmospheres [2]. On the other hand, despite the long history of studying the process, previously unknown manifestations of DR are found even in the case of the simplest molecular ions, such as H + 2 [3] or HeNe + [4], which stimulates the development of new approaches to the calculation of its main characteristics i.e. cross-sections and rate constants [5].…”
Section: Introductionmentioning
confidence: 99%
“…For example, it was demonstrated in [8,9] that the afterglow of a discharge in a He−Ne mixture is formed under certain conditions as a result of recombination of heteronuclear HeNe + ions ans electrons. The effect of concentration of emission of the 2p 5 4p shell of a neon atom, which is represented by a set of 30 spectral lines of comparable intensity in pure neon plasma, into a single line at 352.0 nm emitted from the upper 3p 1 level (in the Paschen notation) at higher helium pressures was described in [10]. This phenomenon was discovered in studies of the evolution of the afterglow spectrum of a barrier discharge with a low neon content (several mTorr) under a total pressure of 0.1−20 Torr of the mixture.…”
Section: Introductionmentioning
confidence: 99%
“…С одной стороны, этот механизм деионизации определяет свойства широкого круга лабораторных плазменных объектов и является необходимым звеном в моделях звездной и планетной атмосфер [2]. С другой стороны, несмотря на долгую историю изучения процесса, обнаруживаются ранее неизвестные проявления DR даже в случае простейших молекулярных ионов, таких как H + 2 [3] или HeNe + [4], что стимулирует развитие новых подходов к расчету его основных характеристик-сечений и констант скорости [5]. Наиболее подробно обсуждаемый процесс изучен в плазме инертных газов, а наибольшее количество работ посвящено рекомбинации ионов Ne + 2 .…”
Section: Introductionunclassified