Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density, Magnetic Field, and Mach Number (1996)

Synopsis

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. Note: A animation of the evolution of the density, the magnetic field, and the mach number in the solar atmosphere model. Magnetic field contours are shown in black and mach…

Uploader's description on archive.org

More like this

• Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density (1996)
• Zoom Around the Sun using TRACE Imagery (1998)
• Pan around the Limb of the Sun with TRACE Imagery (1998)
• Zoom and Fade to Animation of Solar Flare using TRACE Imagery (1998)
• Irrigation in the Heart of the Sahara: Image of the Day (1999)
• Irrigation in the Heart of the Sahara (2002)