  The kinematic information of the Radcliffe Wave (RW) is essential for
determining its existence and gaining insights into its origin and evolution.
In this work, we present an accurate measurement of the vertical velocity
($V_Z$) of RW by incorporating the radial velocity (RV) measures through two
methods, which is crucial but was neglected previously. First, the velocities
are measured towards young stars, using their RV measurements from APOGEE-2 and
proper motion measurements from Gaia DR3. Second, we combine RV measurements
toward clouds with proper motion measurements of associated Young Stellar
Objects (YSOs) to determine the vertical velocities of the clouds. The results
reveal that the oscillations in $V_Z$ are not synchronous with the vertical
coordinate $Z$, which differs from the conclusions of previous studies.
Instead, we find a 5 km$\cdot$s$^{-1}$$\cdot$kpc$^{-1}$ gradient in $V_Z$ along
the RW, exhibiting a dipole-like pattern. Consequently, the kinematic
arrangement does not show a corresponding coherence with the spatial
arrangement, bringing the Radcliffe Wave model into question.
