  We have obtained H$\alpha$ high spatial and time resolution observations of
the upper solar chromosphere and supplemented these with multi-wavelength
observations from the Solar Dynamic Observatory (SDO) and the {\it Hinode}
ExtremeUltraviolet Imaging Spectrometer (EIS). The H$\alpha$ observations were
conducted on 11 February 2012 with the Hydrogen-Alpha Rapid Dynamics Camera
(HARDcam) instrument at the National Solar Observatory's Dunn Solar Telescope.
Our H$\alpha$ observations found large downflows of chromospheric material
returning from coronal heights following a failed prominence eruption. We have
detected several large condensations ("blobs") returning to the solar surface
at velocities of $\approx$200 km s$^{-1}$ in both H$\alpha$ and several SDO AIA
band passes. The average derived size of these "blobs" in H$\alpha$ is 500 by
3000 km$^2$ in the directions perpendicular and parallel to the direction of
travel, respectively. A comparison of our "blob" widths to those found from
coronal rain, indicate there are additional smaller, unresolved "blobs" in
agreement with previous studies and recent numerical simulations. Our observed
velocities and decelerations of the "blobs" in both H$\alpha$ and SDO bands are
less than those expected for gravitational free-fall and imply additional
magnetic or gas pressure impeding the flow. We derived a kinetic energy
$\approx$2 orders of magnitude lower for the main eruption than a typical CME,
which may explain its partial nature.
