Video slate image reads "High Resolution Two Dimensional Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere M.L. Rilee(NRC/GSFC) D. Spicer(GSFC) and R. Sudan(Cornell Univ.) June 1996".
Descriptive image reads, "Ideal MHD in a model photosphere/corona: Structured spatial mesh: resolution (nx, ny) = (300, 500) Flux-Corrected-Transport, 4th order spatial differences. Predictor-Corrector time advance. Periodic in x, hard wall at bottom. Characteristic outflow-no inflow at top. Initial condition: A sheet of magnetic flux suffers a velocity perturbation; the ratio of specific heasts is 1.05, (ct. Shibata et al., 1989 APJ 345 584)."