Corotating Model: Real-time forecast of the solar wind at STEREO A Shown are time series of solar wind parameters at STEREO A derived from the corotating tomography model. Velocity is to the left; density derived from interplanetary scintillation (IPS) g-level is to the right. The display is updated hourly, most recently at (insert system time here) as indicated by the vertical dashed line. The corotating model forecasts several days past this time into the future. The model is updated every time new data are received from STELab, Japan (most recently at (insert t3d_time here)) and is the same curve as shown at the bottom of the corotating model synoptic forecast map plotted with time increasing left to right. 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.