Time-Dependent Model: full-disk image at source surface. These images show the density (normalized to 1 AU) and velocity at the source surface projected against the plane of the sky on (insert delay time here), (insert time delay here). The size of the visible solar disk is show as also shown. 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). The maps are derived from a tomographic time-dependent model of the solar wind that is fit to interplanetary scintillation (IPS) velocities and g-levels obtained daily from STELab, Japan. The model is updated every time new data arrive from Japan, most recently at (insert t3d_time here). The display is update 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.