  Three types of observations: the daily values of the solar radio flux at 7
frequencies, the daily international sunspot number and the daily Stanford mean
solar magnetic field were processed in order to find all the periodicities
hidden in the data. Using a new approach to the radio data, two time series
were obtained for each frequency examined, one more sensitive to spot magnetic
fields, the other to large magnetic structures not connected with sunspots.
Power spectrum analysis of the data was carried out separately for the minimum
(540 days from 1 March 1996 to 22 August 1997) and for the rising phase (708
days from 23 August 1997 to 31 July 1999) of the solar cycle 23. The Scargle
periodograms obtained, normalized for the effect of autocorrelation, show the
majority of known periods and reveal a clear difference between the
periodicities found in the minimum and the rising phase. We determined the
rotation rate of the `active longitudes' in the rising phase as equal to 444.4
$\pm$ 4 nHz ($26\fd0 \pm 0\fd3$). The results indicate that appropriate and
careful analysis of daily radio data at several frequencies allows the
investigation of solar periodicities generated in different layers of the solar
atmosphere by various phenomena related to the periodic emergence of diverse
magnetic structures.
