  We present ALFALFA HI observations of a well studied region of the Leo Cloud,
which includes the NGC 3227 group and the NGC 3190 group. We detect optically
dark HI tails and plumes with extents potentially exceeding 600 kpc, well
beyond the field of view of previous observations. These HI features contain
approximately 40% of the total HI mass in the NGC~3227 group and 10% in the
NGC~3190 group. We also present WSRT maps which show the complex morphology of
the extended emission in the NGC~3227 group. We comment on previously proposed
models of the interactions in these groups and the implications for the scale
of group processing through interactions. Motivated by the extent of the HI
plumes, we place the HI observations in the context of the larger loose group,
demonstrating the need for future sensitive, wide field HI surveys to
understand the role of group processing in galaxy evolution.
