In order to study the magnetic topology of coronal streamers and coronal holes, the first WSM workshop proposes to model 1) the August 17 west limb equatorial streamer, 2) the August 20 SE quadrant streamer, and 3) the August 24 northern polar hole. We produce magnetic topologies for these ``solar minimum'' features using the self-consistent horizontal current-current sheet model. For comparison both MDI and WSO data are used.