Fig. 10
Comparison of observed MW intensity in solar flux units (sfu) (top plot) and degree of polarization (bottom plot) with results of the simulations with CEB2 model for a magnetic field convergence of 2 (dotted line curves) and CEB3 model with convergence of 3 (solid line curves) and the model presented by Altyntsev et al. (2008) (dash-dotted line). In both plots asterisks mark the observed spectra.
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