  We identify coronal mass ejections (CMEs) associated with magnetic clouds
(MCs) observed near Earth by the Wind spacecraft from 2008 to mid-2012, a time
period when the two STEREO spacecraft were well positioned to study
Earth-directed CMEs. We find 31 out of 48 Wind MCs during this period can be
clearly connected with a CME that is trackable in STEREO imagery all the way
from the Sun to near 1 AU. For these events, we perform full 3-D
reconstructions of the CME structure and kinematics, assuming a flux rope
morphology for the CME shape, considering the full complement of STEREO and
SOHO imaging constraints. We find that the flux rope orientations and sizes
inferred from imaging are not well correlated with MC orientations and sizes
inferred from the Wind data. However, velocities within the MC region are
reproduced reasonably well by the image-based reconstruction. Our kinematic
measurements are used to provide simple prescriptions for predicting CME
arrival times at Earth, provided for a range of distances from the Sun where
CME velocity measurements might be made. Finally, we discuss the differences in
the morphology and kinematics of CME flux ropes associated with different
surface phenomena (flares, filament eruptions, or no surface activity).
