We present the first stereoscopic and Doppler observations of simultaneous transverse oscillations of a prominence and a filament and longitudinal oscillation of another filament launched by a single shock wave .
Using H \alpha Doppler observations , we derive the three-dimensional oscillation velocities at different heights along the prominence axis .
The results indicate that the prominence has a larger oscillation amplitude and damping time at higher altitude , but the periods at different heights are the same ( i.e. , 13.5 minutes ) .
This suggests that the prominence oscillates like a linear vertical rigid body with one end anchored on the Sun .
One of the filaments shows weak transverse oscillation after the passing of the shock , which is possibly due to the low altitude of the filament and the weakening ( due to reflection ) of the shock wave before the interaction .
Large amplitude longitudinal oscillation is observed in the other filament after the passing of the shock wave .
The velocity amplitude and period are about 26.8 km s ^ { -1 } and 80.3 minutes , respectively .
We propose that the orientation of a filament or prominence relative to the normal vector of the incoming shock should be an important factor for launching transverse or longitudinal filament oscillations .
In addition , the restoring forces of the transverse prominence are most likely due to the coupling of gravity and magnetic tension of the supporting magnetic field , while that for the longitudinal filament oscillation is probably the resultant force of gravity and magnetic pressure .