Time-Dependent Model: disk and synoptic images of source surface. These images show the radial magnetic field (normalized to 1 AU) of the source surface on (insert delay time here). To the left is a view of the surface from Earth; the sub-Earth location is marked at disk center. The center of the disk and the visible solar pole, (north or south) are marked with plus signs. The solid line from pole to pole is the meridian at zero degrees heliographic longitude; the dashed line is the 180 degree meridian (only one of these is visible at any time). To the right is a Carrington map plot of the surface. The maps are derived from a time-dependent model of the solar wind that is fit to interplanetary scintillation (IPS) velocities and g-levels obtained daily from ISEE, Japan. The model is updated every time new data arrive from Japan, most recently at (insert t3d_time here). The display is updated hourly. The animations run in (insert movie time step here) steps from (insert begin movie here) before, to (insert end movie here) after the last time data were received.