Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density
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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.
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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 |
| Animators: | Liam Krauss (Lead) |
| | Andy Acuna |
| Studio: | SVS |
| Completed: | 1996-12-12 |
| 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
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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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