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- W2279891995 abstract "Ionization processes and the generation of plasmas are critical elements in a holistic understanding of substellar atmospheres. We propose Alfven ionization as a mechanism for producing localized pockets of ionized gas in the atmosphere, having sufficient degrees of ionization (>10-7) that they constitute plasmas. This paper outlines the criteria required for Alfven ionization to occur and demonstrate its applicability in Brown Dwarf atmospheres. Our results show that degrees of ionization ranging from 10-6-1 can be obtained. Furthermore, Alfven ionization alters the atmospheric chemistry via the creation of new ionic species not normally available in contemporary, thermally-driven atmospheric models. Observable consequences include continuum Bremsstrahlung emission superimposed with spectral lines from the plasma ion species. The presence of an atmospheric plasma opens the door to a multitude of plasma and chemical processes not yet considered in current atmospheric models." @default.
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- W2279891995 date "2013-01-01" @default.
- W2279891995 modified "2023-09-26" @default.
- W2279891995 title "Alfvén ionization in the atmospheres of brown dwarfs" @default.
- W2279891995 hasPublicationYear "2013" @default.
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