Intensity (Eq. (10)) in solar flux units (sfu) (upper plots) and degree of polarization (Eq. (11)) (lower plots) of the MW emission spectra calculated for different precipitation models and propagation directions: for the viewing angles of 110° (left column plots), 140° (middle column plots), and 170° (right column plots). Numbers in the model abbreviations define the factor of magnetic field convergence, e.g CB2 or CEB3 while the number in brackets for CE(3) denotes simulations for DF calculated for CE model with magnetic field added in the MW intensity calculations. Propagation direction indicates the viewing angle for the observer looking from the top and varies from 0 to 90° for downwards emission and from 90° to 180° for upwards emission.