Time-Dependent Model: Remote View from Deep Space 3-D files Shown are remote views of the inner heliosphere derived from a corotating tomographic reconstruction of the solar wind. The heliosphere is shown from the perspective of an observer at (insert heliocentric distance here), (insert ecliptic latitude here) the ecliptic and at the same ecliptic longitude as Earth, looking back at the Sun. The field of view is (insert fov size here) edge-to-edge. Velocity is to the left, density derived from interplanetary scintillation (IPS) g-level is to the right. Structures are plotted against a white background. The display is updated hourly, most recently at (insert system time here). The tomographic model is updated every time new data are received from STELab, Japan, most recently at (insert t3d_time here). 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.