The Dynamic Evolution of Quiet Sun Magnetic Fields

Statistics – Computation

Scientific paper

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Scientific paper

We present the latest in a series of numerical simulations of quiet Sun magnetic fields. The upper convection zone, photosphere, chromosphere, transition region, and corona are all included within a single computational domain that is sufficiently large to encompass a typical active region. We introduce a simplified treatment of the physics of optically-thick radiative transfer throughout the surface layers, and compare these results with an earlier, non-physics based parameterized treatment of radiative cooling.

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