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• W3105606483 abstract "In this paper, the influence of chemi-ionization processes in $H^*(n ge 2) + H(1s)$ collisions, as well as the influence of inverse chemi-recombination processes on hydrogen atom excited-state populations in solar photosphere, are compared with the influence of concurrent electron-atom and electron-ion ionization and recombination processes. It has been found that the considered chemi-ionization/recombination processes dominate over the relevant concurrent processes in almost the whole solar photosphere. Thus, it is shown that these processes and their importance for the non-LTE modeling of the solar atmosphere should be investigated further." @default.
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• W3105606483 date "2011-01-18" @default.
• W3105606483 modified "2023-10-11" @default.
• W3105606483 title "CHEMI-IONIZATION IN SOLAR PHOTOSPHERE: INFLUENCE ON THE HYDROGEN ATOM EXCITED STATES POPULATION" @default.
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• W3105606483 doi "https://doi.org/10.1088/0067-0049/193/1/2" @default.
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