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Fig. 6

image

The importance of Compton scattering over the bremsstrahlung at the base of corona as a function of τcor (Eq. (38)). Solid lines in each package are computed for various values of χ = 0.18,0.26,0.40,0.57,0.67 and 0.86. Each package is calculated for three different values of magnetic pressure: βm = 0,10 and 100. The horizontal dashed line represents the case where ΛC/ ΛB = 1, while vertical dotted lines mark values of coronal optical depth for which it happens.

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