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High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere
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This series of animations (animations 107, 1416, 1417, and 1418) show sheets of magnetic flux undergoing velocity perturbations. The conditions for each simulation are outlined within the video.
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Density and magnetic flux surfaces from a simulation of magnetic flux in the solar atmosphere undergoing velocity perturbations. This run has a vertical scale height of 6.8 million meters.
Duration: 15.0 seconds
Available formats:
352x240 (29.97 fps)
MPEG-1
2 MB
320x238
JPEG
6 KB
80x40
PNG
3 KB
How to play our movies
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| Animation Number: | 1418 |
| Animator: | Liam Krauss (Lead) |
| Studio: | SVS |
| Completed: | 1996-05-21 |
| Scientists: | Dan Spicer (NASA/GSFC) |
| | M. L. Rilee (NASA/GSFC) |
| | R. Sudan (Cornell University) |
| Series: | Solar Atmosphere |
| Video: | SVS1996-0007 * |
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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