Coronal ejections from convective spherical shell dynamos

Details Coronal ejections from convective spherical shell dynamos Coronal ejections from convective spherical shell dynamos

2011-11-07

arxiv.org/abs/1111.1763v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

4 pages, 3 figures, proceedings of IAU Symposium 286: Comparative Magnetic Minima

Scientific paper

We present a three-dimensional model of rotating convection combined with a
simplified corona in spherical coordinates. The motions in the convection zone
generate a large-scale magnetic field that gets sporadically ejected into the
outer layers above. Our model corona is approximately isothermal, but it
includes density stratification due to gravity.

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