期刊
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
卷 193, 期 1, 页码 -出版社
IOP Publishing Ltd
DOI: 10.1088/0067-0049/193/1/2
关键词
atomic processes; Sun: atmosphere
资金
- Ministry of Science and Technological Development of Serbia [176002]
In this paper, the influence of chemi-ionization processes in H*(n >= 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-local thermodynamic equilibrium modeling of the solar atmosphere should be investigated further.
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