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Table 7
Summary of the wavelength dependencies of the flux derived for simplified models for the chromosphere and the ionised wind.
| Optically thin | Optically thick | |
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|
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| 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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