The results of observations of a complete sample of radio sources with spec
tral indices alpha > -0.5 (S proportional to nu(alpha)) are presented. The
sample was selected from the Zelenchuk Survey at 3.9 GHz and contains all s
ources with declinations 4 degrees-6 degrees, Galactic latitudes /b/ > 10 d
egrees, and 3.9-GHz fluxes > 200 mJy. Spectra at 0.97-21.7 GHz were obtaine
d for all 69 sample sources. The spectra were classified, and a correlation
between variability amplitude and spectrum shape was found. The spectra we
re separated into extended and compact components. The distribution of spec
tral indices a for the extended components coincides with the distribution
for sources with power-law spectra. The correlation between the luminosity
and frequency of the peak flux density is confirmed. This correlation is du
e to the fact that the distribution of source linear dimensions does not de
pend on luminosity. (C) 2000 MAIK "Nauka/Interperiodica".