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Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density
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 in the solar atmosphere model    A animation of the evolution of the density in the solar atmosphere model
Duration: 10.0 seconds
Available formats:
  352x240 (29.97 fps) MPEG-1   1 MB
  160x80       PNG           14 KB
  80x40         PNG           4 KB
  320x238     JPEG         6 KB
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Animation Number:111
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.


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