  Two flocculent galaxies NGC 3521 and NGC 5055 has been observed at 10.55GHz
with the Effelsberg 100m telescope. In both cases polarized emission reveals
substantial radial component of regular magnetic field - similar to that in
grand-designed spirals. Comparison with H_alpha distribution obtained at Lowell
Observatory is presented. Polarization models discussed, support modern
non-standard dynamo concepts for magnetic field generation in galaxies.
