The Ondrejov radiospectrograph operating in the 0.8-2.0 GHz frequency range
recorded in recent years (1998-2000), three (August 10, 1998; August 17, 1
999; June 27, 2000) unique bursts with rapid frequency variations (lace bur
sts) lasting for several minutes. On August 17, 1999, the same burst was re
corded simultaneously by the Brazilian Solar Spectroscope in the 1.0-2.5 GH
z frequency range. The frequency variations of these bursts in four time in
tervals were analyzed by the Fourier method and power-law spectra with powe
r-law indices close to -2 were found. The Fourier spectra show the presence
of frequency variations in the 0.01-3.0 Hz interval which indicate fast ch
anges of plasma parameters in the radio source. Due to the similarities in
the line features of these bursts with zebra pattern lines, a model similar
to that of the zebra pattern was suggested. The model radio spectra, compu
ted using this model with a turbulent state of the solar are atmosphere, ar
e similar to those observed by the radiospectrographs.