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• W2091673876 abstract "Using curve of growth methods the variation of apparent excitation temperature, |$theta^starenspace(=5040/T^star)$| , with excitation potential of lines used is compared for the iron group atoms. No significant differences were detected, contrary to recent investigations by Pecker and his collaborators. The curves of growth for all iron group atoms are similar. A theory is developed explaining quantitatively the observed difference between θ⋆ and the electron temperature, θ . This difference occurs because of the stratified nature of the solar atmosphere, not because of non-LTE conditions; in fact θ⋆ does not have any physical reality as a temperature. We conclude that any non-LTE phenomena in the photosphere produce insignificant errors in the abundance determinations." @default.
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• W2091673876 date "1964-06-01" @default.
• W2091673876 modified "2023-09-23" @default.
• W2091673876 title "On Departures from Local Thermodynamic Equilibrium in the Solar Atmosphere" @default.
• W2091673876 doi "https://doi.org/10.1093/mnras/128.1.63" @default.
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