Summary of the wavelength dependencies of the flux derived for simplified models for the chromosphere and the ionised wind.
|Optically thin||Optically thick|
|chromosphere||λ4Fλ ∝ λ2.1||λ4Fλ ∝ λ0|
|ionised wind||λ4Fλ ∝ λ2.1||λ4Fλ ∝ λ1.4|
Notes. The table gives the wavelength dependence for an optically thick ionised wind with a density distribution ne ∝ r−β with β = 2. For β = 1.5 we have λ4Fλ ∝ λ2.1 and for β → ∞ we have λ4Fλ ∝ λ0.
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