The Dynamic Evolution of Active Region Magnetic Fields in the Solar Atmosphere

Details The Dynamic Evolution of Active Region Magnetic Fields in the Solar Atmosphere The Dynamic Evolution of Active Region Magnetic Fields in the Solar Atmosphere

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsh31a..08a&link_type=abstract

American Geophysical Union, Spring Meeting 2008, abstract #SH31A-08

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7509 Corona, 7524 Magnetic Fields, 7529 Photosphere, 7546 Transition Region

Scientific paper

We present the latest results from a series of three-dimensional MHD simulations of active region magnetic fields. The computational domain extends from the upper convection zone out into the corona, and includes the highly-stratified layers of the photosphere, chromosphere, and transition region. We characterize the effects of convective turbulence on large-scale magnetic structures, the magnetic connectivity between sub-surface and coronal fields, and the energetics of the low atmosphere and corona.

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