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Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density Gradient, Magnetic Field, and Mach Number
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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 gradient, the magnetic field, and the mach number in the solar atmosphere model. Magnetic field contours are shown in magenta and mach number contours are shown in green.
Duration: 9.0 seconds
Available formats:
352x240 (29.97 fps)
MPEG-1
1 MB
160x80
PNG
23 KB
80x40
PNG
6 KB
320x238
JPEG
12 KB
How to play our movies
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| Animation Number: | 114 |
| 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 visualization 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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