To study of preflare plasma.
Formation frequency domain with weak polarization.
Fig. 12   Another example of preflare plasma at microwaves. On the multiwaves scans two AR’s are
presented. Near the solar meridian the stable AR and near the West-limb the FPAR  9393 are located.
The microwave emission of FPAR demonstrates the frequency domain (the wavelengths from 2.47
cm to 3.21 cm) with low polarization degree, which shown on the right in big scale also. The sharp
structural changes one can see in narrow frequency band. The powewrful flare X 14.0 occured at
April 15, 2001 in  13h50m UT.