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Using wavelet analysis and Fourier analysis, the temporal behavior of ≈156 day quasi periodicity (Rieger quasi periodicity, RQ) is investigated for series of daily solar indices: Wolf numbers W for 161 years (from 1849), the flux F 10.7 of the Sun's radio emission at a frequency of 2800 MHz for 63 years (from 1947), the number of X ray flares N X for 29 years (from 1981), and the number of optical flares N α for 11 years in cycle 21. The N α series are studied for four quadrants of the solar disk. It is found for the W series that there is no stable dependence of the amplitude RQ on the cycle phase and the W value. It is associated with the fact that, cor responding to a period of around eight years, in the power spectrum changes in the amplitude of the Rieger quasi periodicity of the index W are dominated by the peak. Moreover, the peaks corresponding to the 11 year cyclicity are also significant. The comparative study of the temporal behavior of the Rieger quasi periodicity ampli tude of the indices W, F 10.7 , and N X has shown that the quasi periodicity covers the processes, occurring in active regions on the Sun at different altitudes, almost simultaneously. It is found that for N α , the lag of vari ations of the Rieger quasi periodicity amplitude for series of the Sun's western hemisphere, relative to those for series of the eastern hemisphere, is on average less than for the flare series. Thus, if the flare occurrence is modulated by the Rieger quasi periodicity process as a wave propagating over the Sun's disc, then the wave is not a retrograde one. Different interpretations of the nature of the Rieger quasi periodicity are discussed including the hypothesis of Rossby waves.