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A spectral analysis of the vertical positions and velocities of 374 open starclusters (OSCs) was carried out. We took these OSCs from the Hunt, Reffertcatalog; they have an average age of about 10 million years, and are located onthe galactic plane XY in a narrow zone inclined by 25 degrees to the galacticaxis Y. The following estimates of the parameters of the Radcliffe wave wereobtained: a) the maximum value in periodic perturbations of verticalcoordinates $Z_{max}=92\pm10$ pc with the wavelength of these perturbations$\lambda_z=4.82\pm0.09$ kpc; b)~maximum value of the velocity of verticaldisturbances $W_{max}=4.36\pm0.12$ km s$^{-1}$ with disturbance wavelength$\lambda_W=1.78\pm0.02$ kpc. Note that the results of the vertical velocityanalysis are first-class in accuracy and completely new.

The Radcliffe wave parameters from data on open star clusters