Solar magnetism simulation

Solar magnetism simulation


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Solar magnetism simulation. Supercomputer simulation of magnetic structures formed by a turbulent dynamo on the Sun. In the Sun, highly turbulent hot plasma flows stretch, twist, and fold magnetic field lines, resulting in magnetoconvection. Here, magnetic field lines form a 'carpet' of magnetic loops at a temperature of 6400 degrees Kelvin. This simulation is one of several Large-Eddy Simulations produced with the parallel 3D radiative magnetohydrodynamic code SolarBox, using NASA's Pleiades supercomputer. The simulation was featured at the SC13 supercomputing conference in November 2013.

Release details

Model release not required. Property release not required.

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