Fig. 2
CLVI (left panel) and CLVP (right panel) for the exact solution (crosses) given by Chandrasekhar (1960) and our calculation of the radiative transfer equation for polarised light for pure scattering atmosphere (solid line). The same solid line is obtained for all wavelengths from 4000 Å to 8000 Å and for different solar and stellar atmospheres assuming pure scattering as described in the text.
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