The Dynamic Evolution of Quiet Sun Magnetic Fields

Details The Dynamic Evolution of Quiet Sun Magnetic Fields The Dynamic Evolution of Quiet Sun Magnetic Fields

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.0903a&link_type=abstract

American Astronomical Society, SPD meeting #40, #9.03; Bulletin of the American Astronomical Society, Vol. 41, p.817

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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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