MHD Modeling of the Solar Corona through Differential Rotation of the Magnetic Flux

Details MHD Modeling of the Solar Corona through Differential Rotation of the Magnetic Flux MHD Modeling of the Solar Corona through Differential Rotation of the Magnetic Flux

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsh51a1456l&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #SH51A-1456

Physics

7509 Corona, 7524 Magnetic Fields

Scientific paper

We model the evolution of the coronal magnetic field for several solar rotation using our 3D MHD algorithm in spherical coordinates. After imposing an initial magnetic flux distribution extracted from a magnetogram, we relax the system to steady state. We then evolve the magnetic flux distribution through differential rotation. The response of the coronal and heliospheric magnetic field is analyzed.

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