+ Visit NASA.gov + Advanced Search   + About the Server   + Animation List   + How to Use the Server   + RSS Feeds   + Podcasts   + Opportunities Previous Animation Next Animation Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density Gradient This animation is one of a series depicting the results of a two-dimensional ideal magnetohydrodynamic simulation of magnetic flux emerging through a solar atmosphere. The simulation has a resolution of 300x500 cells and a length scale of 16 Mm x 6.8 Mm. The simulation depicts 1730 seconds in the evolution of the model.    A animation of the evolution of the density gradient in the solar atmosphere model Duration: 10.0 seconds Available formats:   352x240 (29.97 fps) MPEG-1   1 MB   160x80       PNG           8 KB   80x40         PNG           2 KB   320x238     JPEG         6 KB How to play our movies Animation Number: 112 Completed: 1996-12-12 Animators: Liam Krauss (Hughes STX) (Lead)   Andy Acuna (Hughes STX) Scientists: Dan Spicer (NASA/GSFC)   M. L. Rilee (NASA/GSFC)   R. Sudan (Cornell University) Series: Solar Atmosphere Video: SVS1996-0011 * Keywords: DLESE >> Space science SVS >> Sun     Please give credit for this item to: NASA/Goddard Space Flight Center Scientific Visualization Studio *Please note: the SVS does not fulfill requests for copies of the tapes in our library. On some of our animation pages, there is a direct link to a video distribution service from which tapes, handled by the Public Affairs Office (PAO)/Goddard TV, including some of our animations may be ordered. General information on this service can be found here. Back to Top + Privacy Policy and Important Notices + Reproduction Guidelines NASA Official: Content Contact: Curator: