Putman, Mary EBland-Hawthorn, JossVeilleux, SylvainGibson, Bradley KFreeman, KennethMaloney, P2015-12-130004-637Xhttp://hdl.handle.net/1885/87081We present deep Ha spectroscopy toward several high-velocity clouds (HVCs), which vary in structure from compact HVCs (CHVCs) to the Magellanic Stream. The clouds range from being bright (∼640 mR) to having upper limits on the order of 30-70 mR. The HαKeywords: Diffuse radiation; Galaxies: individual (Magellanic Stream); Galaxies: ISM; Galaxy: halo; Intergalactic medium200310.1086/3785552015-12-12